midgard.math
midgard.math.constant
Midgard library module defining an assortment of constants
Description:
This module provides constants that are used within the Midgard project. The actual constants are defined in the
constants.conf
file (see the file list for location). See that file for references and for adding or changing
constants.
The constants are stored as module variables so they can be used simply as constant.c
as in the example above. Some
models use particular values for constants that are different from the conventional ones. This is handled by the source
parameter. For instance, the EGM 2008 gravity field is calculated with a value for GM different from the IERS
Conventions value, using::
constant.get('GM', source='egm_2008')
instead of simply constant.GM
.
Example:
>>> from midgard.math.constant import Constant
>>> print(f"The speed of light is {constant.c:0.2f}")
The speed of light is 299792458.00
Todo:
Rewrite as a class instead of a module, to have somewhat cleaner code (and be more consistent with things like lib.unit).
Constant
Full name: midgard.math.constant.Constant
Signature: () -> None
constant (Constant)
constant = Constant('/home/kirann/miniconda3/envs/where/lib/python3.10/site-packages/midgard/math/constant.txt')
midgard.math.ellipsoid
Midgard library module for handling Earth ellipsoids
Description:
Ellipsoid
Full name: midgard.math.ellipsoid.Ellipsoid
Signature: (name: str, a: float, f_inv: float, description: str) -> None
Ellipsoid(name: str, a: float, f_inv: float, description: str)
GRS80 (Ellipsoid)
GRS80 = Ellipsoid(name='GRS80', a=6378137, f_inv=298.257222101, description='Used by ITRS')
IERS2003 (Ellipsoid)
IERS2003 = Ellipsoid(name='IERS2003', a=6378136.6, f_inv=298.25642, description='IERS conventions 2003, p. 12')
IERS2010 (Ellipsoid)
IERS2010 = Ellipsoid(name='IERS2010', a=6378136.6, f_inv=298.25642, description='IERS conventions 2010, p. 18')
WGS72 (Ellipsoid)
WGS72 = Ellipsoid(name='WGS72', a=6378135, f_inv=298.26, description='WGS72')
WGS84 (Ellipsoid)
WGS84 = Ellipsoid(name='WGS84', a=6378137, f_inv=298.257223563, description='Used by GPS')
get()
Full name: midgard.math.ellipsoid.get
Signature: (ellipsoid: str) -> 'Ellipsoid'
Get an ellipsoid by name
sphere (Ellipsoid)
sphere = Ellipsoid(name='sphere', a=6371008.8, f_inv=inf, description='Regular sphere, mean radius')
midgard.math.interpolation
Methods for interpolating in numpy arrays
Description:
Different interpolation methods are decorated with @register_interpolator
and will then become available for use as
kind
in interpolate
and moving_window
.
Example:
>>> import numpy as np
>>> np.set_printoptions(precision=3, suppress=True)
>>> x = np.linspace(-1, 1, 11)
>>> y = x**3 - x
>>> y
array([ 0. , 0.288, 0.384, 0.336, 0.192, 0. , -0.192, -0.336,
-0.384, -0.288, 0. ])
>>> x_new = np.linspace(-0.8, 0.8, 11)
>>> interpolate(x, y, x_new, kind='cubic')
array([ 0.288, 0.378, 0.369, 0.287, 0.156, -0. , -0.156, -0.287,
-0.369, -0.378, -0.288])
Developer info:
To add your own interpolators, you can simply decorate your interpolator functions with @register_interpolator
. Your
interpolator function should have the signature
(x: np.ndarray, y: np.ndarray) -> Callable
For instance, the following would implement a terrible interpolation function that sets all values to zero:
from midgard.math.interpolation import register_interpolator
@register_interpolator
def zero(x: np.ndarray, y: np.ndarray) -> Callable:
def _zero(x_new: np.ndarray) -> np.ndarray:
return np.zeros(y.shape)
return _zero
This function would then be available as an interpolator. For instance, one could do
>>> interpolate(x, y, x_new, kind='zero') # doctest: +SKIP
array([0., 0., 0., 0., 0., 0., 0., 0., 0., 0., 0.])
barycentric_interpolator()
Full name: midgard.math.interpolation.barycentric_interpolator
Signature: (x: numpy.ndarray, y: numpy.ndarray, **ipargs: Any) -> Callable
The interpolating polynomial through the given points
Uses the scipy.interpolate.BarycentricInterpolator function behind the scenes.
Args:
x
: 1-dimensional array with original x-values.y
: Array with original y-values.ipargs
: Keyword arguments passed on to the scipy-interpolator.
Returns:
Barycentric interpolation function
cubic()
Full name: midgard.math.interpolation.cubic
Signature: (x: numpy.ndarray, y: numpy.ndarray, **ipargs: Any) -> Callable
Cubic spline interpolation through the given points
Uses the scipy.interpolate.interp1d function with kind='cubic' behind the scenes.
Args:
x
: 1-dimensional array with original x-values.y
: Array with original y-values.ipargs
: Keyword arguments passed on to the interp1d-interpolator.
Returns:
Cubic spline interpolation function
get_interpolator()
Full name: midgard.math.interpolation.get_interpolator
Signature: (name: str) -> Callable
Return an interpolation function
Interpolation functions are registered by the @register_interpolator-decorator. The name-parameter corresponds to the function name of the interpolator.
Args:
name
: Name of interpolator.
Returns:
Interpolation function with the given name.
interpolate()
Full name: midgard.math.interpolation.interpolate
Signature: (x: numpy.ndarray, y: numpy.ndarray, x_new: numpy.ndarray, *, kind: str, **ipargs: Any) -> numpy.ndarray
Interpolate values from one x-array to another
See interpolators()
for a list of valid interpolators.
Args:
x
: 1-dimensional array with original x-values.y
: Array with original y-values.x_new
: 1-dimensional array with new x-values.kind
: Name of interpolator to use.ipargs
: Keyword arguments passed on to the interpolator.
Returns:
Array of interpolated y-values.
interpolate_with_derivative()
Full name: midgard.math.interpolation.interpolate_with_derivative
Signature: (x: numpy.ndarray, y: numpy.ndarray, x_new: numpy.ndarray, *, kind: str, dx: float = 0.5, **ipargs: Any) -> numpy.ndarray
Interpolate values from one x-array to another as well as find derivatives
See interpolators()
for a list of valid interpolators.
Args:
x
: 1-dimensional array with original x-values.y
: Array with original y-values.x_new
: 1-dimensional array with new x-values.kind
: Name of interpolator to use.dx
: Values at x ± dx are used to determine derivative.ipargs
: Keyword arguments passed on to the interpolator.
Returns:
Tuple with array of interpolated y-values and array of derivatives.
interpolated_univariate_spline()
Full name: midgard.math.interpolation.interpolated_univariate_spline
Signature: (x: numpy.ndarray, y: numpy.ndarray, **ipargs: Any) -> Callable
One-dimensional interpolating spline for the given points
Uses the scipy.interpolate.InterpolatedUnivariateSpline function behind the scenes.
The original only deals with one-dimensional y arrays, so multiple calls are made for higher dimensional y arrays. The dimensions are handled independently of each other.
Args:
x
: 1-dimensional array with original x-values.y
: Array with original y-values.ipargs
: Keyword arguments passed on to the scipy-interpolator.
Returns:
Interpolating spline function
interpolators()
Full name: midgard.math.interpolation.interpolators
Signature: () -> List[str]
Return a list of available interpolators
Returns:
Names of available interpolators.
lagrange()
Full name: midgard.math.interpolation.lagrange
Signature: (x: numpy.ndarray, y: numpy.ndarray, *, window: int = 10, bounds_error: bool = True, assume_sorted: bool = False) -> Callable
Computes the lagrange polynomial passing through a certain set of points
See https://en.wikipedia.org/wiki/Lagrange_polynomial
Uses window
of the original points to calculate the Lagrange polynomials. The window of points is chosen by
finding the closest original point and essentially picking the window // 2
indices on either side.
Args:
x
: 1-dimensional array with original x-values.y
: Array with original y-values.window
: Number of points used in interpolation.bounds_error
: If True, a ValueError is raised if extrapolation is attempted.assume_sorted
: If True, x must be an array of monotonically increasing values.
Returns:
Lagrange interpolation function.
linear()
Full name: midgard.math.interpolation.linear
Signature: (x: numpy.ndarray, y: numpy.ndarray, **ipargs: Any) -> Callable
Linear interpolation through the given points
Uses the scipy.interpolate.interp1d function with kind='linear' behind the scenes.
Args:
x
: 1-dimensional array with original x-values.y
: Array with original y-values.ipargs
: Keyword arguments passed on to the interp1d-interpolator.
Returns:
Linear interpolation function
register_interpolator()
Full name: midgard.math.interpolation.register_interpolator
Signature: (func: Callable) -> Callable
Register an interpolation function
This function should be used as a @register_interpolator-decorator
Args:
func
: Function that will be registered as an interpolator.
Returns:
Same function.
midgard.math.linear_regression
Midgard library module for linear regression
Description: The 'statsmodels' module is used for the linear regression. Outlier can be rejected beside normal linear regression analysis. Hereby a linear regression analysis is carried out, whereby a linear trend is estimated of the given data. The root-mean square (RMS) of the residuals (observation - linear trend) is used to detect outliers. As default the following outlier limit is defined:
limit = outlier_limit_factor * RMS (with outlier_limit_factor=1.0)
The 'outlier_limit_factor' can be chosen as argument by initialization of a LinearRegression class object. In addition the number of iteration for the outlier detection can be chosen with the argument 'outlier_iteration'.
Example:
Import Midgard LinearRegression class of linear_regression module
from midgard.math.linear_regression import LinearRegression
Generate LinearRegression object
linreg = LinearRegression(x,y)
Get solution
interception = linreg.interception slope = linreg.slope
LinearRegression
Full name: midgard.math.linear_regression.LinearRegression
Signature: (x: Union[numpy.ndarray, list], y: Union[numpy.ndarray, list], reject_outlier: bool = False, outlier_limit_factor: float = 1.0, outlier_iteration: int = 1) -> None
Linear regression class
Following arguments can be chosen by initialization of LinearRegression class objects:
| Arguments | Type | Description |
|:----------------------| :----------| :---------------------------------------------------------------------|
| outlier_limit_factor | float | RMS of residuals are used for detecting outliers, whereby |
| | | 'outlier_limit_factor' * 'RMS' is used as limit. As default is |
| | | 'outlier_limit_factor' = 1.0 chosen. |
| outlier_iteration | int | Number of iteration used to detect and reject outliers. Default is 1. |
| reject_outlier | bool | Determine if outliers should be detected and rejected. Default is |
| | | 'False', which means that no outliers are rejected. |
| x | np.ndarray | X training data |
| y | np.ndarray | Y target data |
midgard.math.nputil
Utility wrapper for numpy functions
Makes sure numpy functions can be called in a similar fashion for different use cases + both 1- and 2-dimensional input + both single values and arrays
HashArray
Full name: midgard.math.nputil.HashArray
Signature: (val)
col()
Full name: midgard.math.nputil.col
Signature: (vector)
hashable()
Full name: midgard.math.nputil.hashable
Signature: (func)
Decorator for functions with numpy arrays as input arguments that will benefit from caching
Example:
from midgard.math import nputil from functools import lru_cache
@nputil.hashable @lru_cache() def test_func(a: np.ndarray, b: np.ndarray = None) do_something return something
norm()
Full name: midgard.math.nputil.norm
Signature: (vector)
row()
Full name: midgard.math.nputil.row
Signature: (vector)
take()
Full name: midgard.math.nputil.take
Signature: (vector, item)
unit_vector()
Full name: midgard.math.nputil.unit_vector
Signature: (vector)
midgard.math.planetary_motion
Midgard library for planetary motion
Example:
from migard.math import planetary_motion
findsun()
Full name: midgard.math.planetary_motion.findsun
Signature: (time: 'Time') -> numpy.ndarray
Obtains the position vector of the Sun in relation to Earth (in ECEF).
This routine is a reimplementation of routine findSun() in model.c of gLAB 3.0.0 software. The gLAB 3.0.0 software core excecutables are distributed under the Apache License version 2.0 related to following copyright and license:
COPYRIGHT 2009 - 2016 GAGE/UPC & ESA
LICENSED UNDER THE APACHE LICENSE, VERSION 2.0 (THE "LICENSE"); YOU MAY NOT USE THIS ROUTINE EXCEPT IN COMPLIANCE WITH THE LICENSE.  SEE THE LICENSE FOR THE SPECIFIC LANGUAGE GOVERNING PERMISSIONS AND LIMITATIONS UNDER THE LICENSE.
Args:
time
: Time object
Returns:
Sun position vector given in ECEF [m]
gsdtime_sun()
Full name: midgard.math.planetary_motion.gsdtime_sun
Signature: (time: 'Time') -> Tuple[numpy.ndarray]
Get position of the sun (low-precision)
This routine is a reimplementation of routine GSDtime_sun() in model.c of gLAB 3.0.0 software. The gLAB 3.0.0 software core excecutables are distributed under the Apache License version 2.0 related to following copyright and license:
COPYRIGHT 2009 - 2016 GAGE/UPC & ESA
LICENSED UNDER THE APACHE LICENSE, VERSION 2.0 (THE "LICENSE"); YOU MAY NOT USE THIS ROUTINE EXCEPT IN COMPLIANCE WITH THE LICENSE.  SEE THE LICENSE FOR THE SPECIFIC LANGUAGE GOVERNING PERMISSIONS AND LIMITATIONS UNDER THE LICENSE.
Args:
time
: Time object
Returns:
Tuple with following entries:
| Elements | Description |
|---|---|
| gstr | GMST0 (to go from ECEF to inertial) [deg] |
| slong | Sun longitude [deg] |
| sra | Sun right Ascension [deg] |
| sdec | Sun declination in [deg] |
midgard.math.plate_motion
Midgard library module for handling tectonic plate motion
Description:
Example:
import numpy as np from midgard.math.plate_motion import PlateMotion
pm = PlateMotion(plate="eura") pos = np.array([2102928.189605,<PHONE_NUMBER>78, 5958196.398820]) # in meter vel = pm.get_velocity(pos) # in mm/yr
PlateMotion
Full name: midgard.math.plate_motion.PlateMotion
Signature: (plate: str, model: str = 'itrf2014') -> None
A class for handling of tectonic plate motion
midgard.math.rotation
Library for basic rotation matrices
Description:
Creates rotation matrices for rotation around the axes of a right handed Cartesian coordinate system and their derivatives.
For instance, for an XYZ-system, R1 returns a rotation matrix around the x-axis and for an ENU-system, R1 returns a rotation matrix around the east-axis. dR1 returns the derivative of the R1 matrix with respect to the rotation angle. All functions are vectorized, so that one rotation matrix is returned per input angle.
Example:
from where.lib import rotation rotation.R1([0, 1]) array([[[ 1. , 0. , 0. ], [ 0. , 1. , 0. ], [ 0. , -0. , 1. ]],
[[ 1. , 0. , 0. ],
[ 0. , 0.54030231, 0.84147098],
[ 0. , -0.84147098, 0.54030231]]])
R1()
Full name: midgard.math.rotation.R1
Signature: (angle: ~np_float) -> numpy.ndarray
Rotation matrix around the first axis
Args:
angle
: Scalar, list or numpy array of angles in radians.
Returns:
Numpy array: Rotation matrix or array of rotation matrices.
R2()
Full name: midgard.math.rotation.R2
Signature: (angle: ~np_float) -> numpy.ndarray
Rotation matrix around the second axis
Args:
angle
: Scalar, list or numpy array of angles in radians.
Returns:
Numpy array: Rotation matrix or array of rotation matrices.
R3()
Full name: midgard.math.rotation.R3
Signature: (angle: ~np_float) -> numpy.ndarray
Rotation matrix around the third axis
Args:
angle
: Scalar, list or numpy array of angles in radians.
Returns:
Numpy array: Rotation matrix or array of rotation matrices.
dR1()
Full name: midgard.math.rotation.dR1
Signature: (angle: ~np_float) -> numpy.ndarray
Derivative of a rotation matrix around the first axis with respect to the rotation angle.
Args:
angle
: Scalar, list or numpy array of angles in radians.
Returns:
Numpy array: Rotation matrix or array of rotation matrices.
dR2()
Full name: midgard.math.rotation.dR2
Signature: (angle: ~np_float) -> numpy.ndarray
Derivative of a rotation matrix around the second axis with respect to the rotation angle
Args:
angle
: Scalar, list or numpy array of angles in radians.
Returns:
Numpy array: Rotation matrix or array of rotation matrices.
dR3()
Full name: midgard.math.rotation.dR3
Signature: (angle: ~np_float) -> numpy.ndarray
Derivative of a rotation matrix around the third axis with respect to the rotation angle
Args:
angle
: Scalar, list or numpy array of angles in radians.
Returns:
Numpy array: Rotation matrix or array of rotation matrices.
enu2trs()
Full name: midgard.math.rotation.enu2trs
Signature: (lat: ~np_float, lon: ~np_float) -> numpy.ndarray
Rotation matrix for rotating an ENU coordinate system to an earth oriented one
See for instance http://www.navipedia.net/index.php/Transformations_between_ECEF_and_ENU_coordinates This is equal to doing::
R3(-(np.pi/2 + lon)) @ R1(-(np.pi/2 - lat))
Args:
lat (Float or Array): Latitude of origin of ENU coordinate system. lon (Float or Array): Longitude of origin of ENU coordinate system.
Returns:
Numpy array: Rotation matrix or array of rotation matrices.
np_float (TypeVar)
np_float = ~np_float
trs2enu()
Full name: midgard.math.rotation.trs2enu
Signature: (lat: ~np_float, lon: ~np_float) -> numpy.ndarray
Rotation matrix for rotating an earth oriented coordinate system to an ENU one
See for instance http://www.navipedia.net/index.php/Transformations_between_ECEF_and_ENU_coordinates This is equal to doing::
R1(np.pi/2 - lat) @ R3(np.pi/2 + lon)
Args:
lat (Float or Array): Latitude of origin of ENU coordinate system. lon (Float or Array): Longitude of origin of ENU coordinate system.
Returns:
Numpy array: Rotation matrix or array of rotation matrices.
midgard.math.spatial_interpolation
Methods for spatial interpolation in numpy arrays
Description:
Example:
TODO
interpolate_for_position()
Full name: midgard.math.spatial_interpolation.interpolate_for_position
Signature: (grid_x: numpy.ndarray, grid_y: numpy.ndarray, values: numpy.ndarray, x: float, y: float, method: str = 'linear') -> float
Interpolation in grid with size (n, m) for a given position
Interpolation is based on scipy.interpolate.griddata module. More information about this module can be found under: https://docs.scipy.org/doc/scipy/reference/generated/scipy.interpolate.griddata.html
Args:
grid_x
: (n,m) Array with x-positions for each grid pointgrid_y
: (n,m) Array with y-positions for each grid pointvalues
: (n,m) Array with data values for each grid pointx
: x-positiony
: y-positionmethod
: Method of interpolation: linear: tessellate the input point set to N-D simplices, and interpolate linearly on each simplex nearest: value of data point closest to the point of interpolation cubic: value determined from a piecewise cubic
Returns:
Interpolated value in data grid for a given position
midgard.math.transformation
Midgard library module for handling of geodetic conversions
Description:
delta_acr2trs_posvel()
Full name: midgard.math.transformation.delta_acr2trs_posvel
Signature: (acr: 'AcrPosVelDelta') -> 'TrsPosVelDelta'
Convert position deltas from ACR to TRS
delta_enu2trs()
Full name: midgard.math.transformation.delta_enu2trs
Signature: (enu: 'EnuPositionDelta') -> 'TrsPositionDelta'
Convert position deltas from ENU to TRS
delta_enu2trs_posvel()
Full name: midgard.math.transformation.delta_enu2trs_posvel
Signature: (enu: 'EnuPosVelDelta') -> 'TrsPosVelDelta'
Convert position deltas from ENU to TRS
delta_trs2acr_posvel()
Full name: midgard.math.transformation.delta_trs2acr_posvel
Signature: (trs: 'TrsPosVelDelta') -> 'AcrPosVelDelta'
Convert position deltas from TRS to ACR
delta_trs2enu()
Full name: midgard.math.transformation.delta_trs2enu
Signature: (trs: 'TrsPositionDelta') -> 'EnuPositionDelta'
Convert position deltas from TRS to ENU
delta_trs2enu_posvel()
Full name: midgard.math.transformation.delta_trs2enu_posvel
Signature: (trs: 'TrsPosVelDelta') -> 'EnuPosVelDelta'
Convert position deltas from TRS to ENU
kepler2trs()
Full name: midgard.math.transformation.kepler2trs
Signature: (kepler: 'KeplerPosVel') -> 'TrsPosVel'
Compute orbit position and velocity vector in geocentric equatorial coordinate system based on Keplerian elements for elliptic orbits.
The implementation is based on Section 2.2.3 in :cite:montenbruck2012
.
llh2trs()
Full name: midgard.math.transformation.llh2trs
Signature: (llh: numpy.ndarray, ellipsoid: midgard.math.ellipsoid.Ellipsoid = None) -> numpy.ndarray
Convert geodetic latitude-, longitude-, height-coordinates to geocentric xyz-coordinates
Reimplementation of GD2GCE.for from the IUA SOFA software collection.
trs2kepler()
Full name: midgard.math.transformation.trs2kepler
Signature: (trs: 'TrsPosVel') -> 'KeplerPosVel'
Compute Keplerian elements for elliptic orbit based on orbit position and velocity vector given in ITRS.
The used equations are described in Section 2.2.4 in Montenbruck :cite:montenbruck2012
.
The position and velocity vector in ITRS and GM must be given in consistent units, which are [m], [m/s] and [m^3/s^2]. The resulting unit of the semimajor axis is implied by the unity of the position vector, i.e. [m].
.. note:: The function cannot be used with position/velocity vectors describing a circular or non-inclined orbit.
Returns:
tuple with numpy.ndarray types: Tuple with following Keplerian elements:
=============== ====== ================================================================================== Keys Unit Description =============== ====== ================================================================================== a m Semimajor axis e Eccentricity of the orbit i rad Inclination Omega rad Right ascension of the ascending node omega rad Argument of perigee E rad Eccentric anomaly =============== ====== ==================================================================================
trs2llh()
Full name: midgard.math.transformation.trs2llh
Signature: (trs: numpy.ndarray, ellipsoid: midgard.math.ellipsoid.Ellipsoid = None) -> numpy.ndarray
Convert geocentric xyz-coordinates to geodetic latitude-, longitude-, height-coordinates
Reimplementation of GC2GDE.for from the IUA SOFA software collection.
midgard.math.unit
Midgard library module for handling of SI-unit conversions
Description:
This module provides unit conversion constants and functions. The heavy lifting is done by the pint
package. The
basic usage is as follows:
>>> from midgard.math.unit import Unit
>>> seconds_in_two_weeks = 2 * Unit.week2secs
>>> seconds_in_two_weeks
1209600.0
In general Unit.spam2ham
will give the multiplicative conversion scale between the units spam
and ham
. Through
the pint
package we support a lot of units. See Unit.list()
or
https://github.com/hgrecco/pint/blob/master/pint/default_en.txt
. Another notation is also available, and might be
necessary for some more complicated conversions:
>>> seconds_in_two_weeks = 2 * Unit('week', 'seconds')
>>> miles_per_hour_in_meters_per_second = Unit('mph', 'meters / sec')
Do note that we support most normal aliases as well as singular and plural forms of the units. For instance can
second
be represented as s
, sec
, secs
and seconds
. Prefixes are also handled:
>>> nanoseconds_in_an_hour = Unit.hour2nanosecs
>>> inches_in_a_kilometer = Unit.km2inches
For more complicated conversions (for instance from Celsius to Fahrenheit) one can create custom conversion functions
using convert
:
>>> c2f = Unit.function('celsius', 'fahrenheit')
>>> absolute_zero_in_fahrenheit = c2f(-273.15)
For convenience, this can also be written using the attribute notation as Unit.spam_to_ham(spam_value)
. Then the
previous example simply becomes:
>>> absolute_zero_in_fahrenheit = Unit.celsius_to_fahrenheit(-273.15)
(or even easier Unit.kelvin_to_fahrenheit(0)
).
Finally, we can access the unit/quantity system of pint
by using the name of a unit by itself, e.g. Unit.spam
. For
instance:
>>> distance = 42 * Unit.km
>>> time = 31 * Unit('minutes')
>>> speed = distance / time
>>> speed.to(Unit.mph)
<Quantity(50.511464659292955, 'mph')>
>>> speed.to_base_units()
<Quantity(22.580645161290324, 'meter / second')>
However, using the full unit system adds some overhead so we should be careful in using it in heavy calculations.
Note that pint
has a system for defining new units and constants if necessary,
http://pint.readthedocs.io/en/latest/defining.html
. To use this system, add units to the unit.txt
file in the
current (midgard/math) directory.
Unit
Full name: midgard.math.unit.Unit
Signature: (from_unit: str, to_unit: Optional[str] = None) -> Any
Unit converter
The implementation of the unit conversion is done in the _convert_units
-metaclass.
np_float (TypeVar)
np_float = ~np_float


threejs
- WebGL - Multiple Render Targets
Renders geometry into a G-Buffer.
Visualized here is the color and normal data from the G-Buffer.
Created by
@mattdesl
.
Your browser does not support
WEBGL_draw_buffers
.
This demo will not work.


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Video: Jon Gruden’s NSFW Message To Referee Is Going Viral
by Andrew HolleranJon Gruden is not a happy man today. The Oakland Raiders are currently getting shellacked by the New York Jets. It’s Jets 34, Raiders 3 in the fourth quarter.
Yikes.
Gruden hasn’t been happy all day, it appears.
The Raiders’ head coach had a NSFW message for an official when the game was tied, 3-3, early in the second quarter.
WARNING: The language is graphic.
It’s not very hard to read his lips there…
Gruden had a reason to be upset, though. This was called roughing the passer:
That might be one of the worst calls of the season. Bad call or not, though, the Raiders have not played well enough to win.
Oakland had been playing better as of late, but the Raiders will suffer a bad loss against the Jets today. Gruden’s team will drop to 6-5 with the loss. New York, meanwhile, will improve to 4-7.


You can read public gists and create them for anonymous users without a token. To read or write gists on a user's behalf, you need the gist OAuth scope and a token.


The phrase you entered was:
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{%else%}"{{ words[l] }}" was not found in the top {{ depth }} results
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Examples: Production Applications¶
Table of Contents¶
Commodities¶
Glucosinolates
ChEFS
Metabolomics¶
Chemical Entities with Medical Applications, Therapeutic Indications and Consequences (ChEMATIC)
Reference Library¶
Based on USDA National Agricultural Library Thesaurus (NALT)


Real Name: Terenzio Joseph Estrella
Alias(es): "Captain," "Jack Sparrow," "Handsome Jack," and "McDowell"
Height: 5'5"
Weight: 165 lbs.
First Appearance: BIRTH OF SUPER-AWESOME GUY #1 Jul. 1986
Quite possibly the most awesome individual to ever grace this planet known as Earth-- TJ Estrella is a man who knows of no bounds!  Growing up as a very awesome kid, T.J. would go on to do many great things in life. A US Marine from the East Coast, this Devil Dog currently works as a site surveyor and designer for a solar and roofing company.
Feel free to contact me on any of these social media platforms!


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- ${certificate_id_number}
- ${certificate_date_issued_title}
- ${certificate_date_issued}


#include <SBWatchpoint.h>
Detailed Description
Definition at line 17 of file SBWatchpoint.h.
Constructor & Destructor Documentation
| lldb::SBWatchpoint::SBWatchpoint |
( |
| ) |
|
| lldb::SBWatchpoint::SBWatchpoint |
( |
const lldb::WatchpointSP & |
wp_sp | ) |
|
| lldb::SBWatchpoint::~SBWatchpoint |
( |
| ) |
|
Member Function Documentation
| void lldb::SBWatchpoint::Clear |
( |
| ) |
|
| static bool lldb::SBWatchpoint::EventIsWatchpointEvent |
( |
const lldb::SBEvent & |
event | ) |
|
|
static |
| const char* lldb::SBWatchpoint::GetCondition |
( |
| ) |
|
| bool lldb::SBWatchpoint::GetDescription |
( |
lldb::SBStream & |
description, |
|
|
DescriptionLevel |
level |
|
) |
| |
| SBError lldb::SBWatchpoint::GetError |
( |
| ) |
|
| int32_t lldb::SBWatchpoint::GetHardwareIndex |
( |
| ) |
|
With -1 representing an invalid hardware index.
| uint32_t lldb::SBWatchpoint::GetHitCount |
( |
| ) |
|
| watch_id_t lldb::SBWatchpoint::GetID |
( |
| ) |
|
| uint32_t lldb::SBWatchpoint::GetIgnoreCount |
( |
| ) |
|
| lldb::WatchpointSP lldb::SBWatchpoint::GetSP |
( |
| ) |
const |
| lldb::addr_t lldb::SBWatchpoint::GetWatchAddress |
( |
| ) |
|
| static lldb::WatchpointEventType lldb::SBWatchpoint::GetWatchpointEventTypeFromEvent |
( |
const lldb::SBEvent & |
event | ) |
|
|
static |
| size_t lldb::SBWatchpoint::GetWatchSize |
( |
| ) |
|
| bool lldb::SBWatchpoint::IsEnabled |
( |
| ) |
|
| bool lldb::SBWatchpoint::IsValid |
( |
| ) |
const |
| void lldb::SBWatchpoint::SetCondition |
( |
const char * |
condition | ) |
|
| void lldb::SBWatchpoint::SetEnabled |
( |
bool |
enabled | ) |
|
| void lldb::SBWatchpoint::SetIgnoreCount |
( |
uint32_t |
n | ) |
|
| void lldb::SBWatchpoint::SetSP |
( |
const lldb::WatchpointSP & |
sp | ) |
|
Friends And Related Function Documentation
The documentation for this class was generated from the following file:


Webstation is a web application that displays information to a dispatcher via browser in different forms (tabular, schematic, diagrams, reports, etc.) and provides sending commands. Reports are generated in commonly used HTML and Microsoft Excel formats.
Figure 1. Webstation application. Scheme view
Figure 2. Webstation application. Table view
User is able to choose a view (table or scheme) and a date to access archive data. To show a diagram of an input channel, click an item icon in a table or an appropriate element in a scheme.
Webstation is available from any computer or tablet connected to an organization network without any software installation. Access is managed by a system administrator who defines user rights.
The functionality of Webstation can be extended by additional plugins. For example, Chart Pro Plugin extends the capabilities of Rapid SCADA charts: adds scaling, displaying of multiple charts, export to PNG and PDF. Elastic Report Plugin allows to generate reports according to a custom configuration. Using this plugin, you can build almost any desired report. Developers can download Rapid SCADA source code and the documentation to learn how to implement plugins.


We're bringing together high quality tools and resources from the field to build a comprehensive toolkit for districts redesigning their professional development systems.
Partner with us to digitize your tools and expand your reach.
Use our toolkit with your district partners to plan and implement system change with teachers at the center.
Create communities of practice among the districts in your network to share solutions.


dvitomp - convert a TeX DVI file to a MetaPost MPXFILE
dvitomp
dvifile [ \fB.dvi\fP ]
mpost --dvitomp dvifile [ \fB.dvi\fP ]
dvitomp translates the given dvifile to a MetaPost MPXFILE. The default mpxfile is the basename of dvifile extended with .mpx .
write usage summary and exit.
output version information and exit.
Email bug reports to metapost@tug.org.


Money Play. How should red play 43?
pips Red=153 White=135
(CorrectAnswer= 0/0, ErrorScore= 0)
Backgammon is not just a race so while 22/15* might seem attractive with its triplication of 3’s Red should not give up his only real asset while his opponent has the stronger home board.
8/4*, 6/3 is very clear here.22/15* is a blunder although at DMP the two plays are equal.
8/4*, 6/3 is very clear here.22/15* is a blunder although at DMP the two plays are equal.
1. Cubeful 2-ply 8/4* 6/3 Eq.: -0.415 0.385 0.095 0.003 - 0.615 0.133 0.005 2. Cubeful 2-ply 22/15* Eq.: -0.499 (-0.083) 0.390 0.084 0.002 - 0.610 0.231 0.011 3. Cubeful 2-ply 6/3 6/2 Eq.: -0.602 (-0.187) 0.324 0.059 0.001 - 0.676 0.094 0.003 4. Cubeful 2-ply 13/9 6/3 Eq.: -0.619 (-0.204) 0.328 0.064 0.002 - 0.672 0.114 0.004 5. Cubeful 0-ply 13/6 Eq.: -0.607 (-0.192) 0.315 0.054 0.001 - 0.685 0.093 0.003


--- layout: post status: publish published: true title: Episode 5.22 - Interview with Cubs Prospect, Albert Almora author: display_name: Corey Fineran login: Corey email<EMAIL_ADDRESS>url: '' author_login: Corey author_email<EMAIL_ADDRESS>wordpress_id: 8553 wordpress_url: http://ivyenvy.com/?p=8553 date: '2013-07-31 09:06:24 +0000' date_gmt: '2013-07-31 14:06:24 +0000' categories: - Minor Leagues - Prospects tags: - Albert Almora - Kane County Cougars comments: [] ---
On this episode, you will hear an interview that I did with Albert Almora. Almora was the Cubs first pick, and the sixth overall in the 2012 draft. Almora is currently playing with the Cubs Single A Midwest League affiliate, the kane county cougars. After starting this season on the disabled list, the 19-year old has lived up to his hype by playing excellent defense and at the time of this recording, in 57 games, he is batting .328 and he's struck out in just 12% of his at-bats.
Almora is currently ranked the #2 prospect in the entire Cubs minor league system. In the most recent rankings, Baseball America has Almora listed as the 16th best prospect in all of baseball. So here is my interview with Cubs prospect, Albert Almora.
We have interviewed other Cubs prospects and you can hear them by clicking on these links:
Dan Vogelbach interview
Javier Baez interview
Matt Szczur interview


Pakistan's ailing ex-PM Sharif flown by air ambulance to London
LAHORE: Pakistan's ailing ex-prime minister Nawaz Sharif left by air ambulance on Tuesday (Nov 19) for London, where he is due to receive medical treatment after battling the government for permission to travel, his doctor and close aides said.
Sharif, 69, is suffering from an autoimmune blood disorder, has high blood pressure, and his kidney functions are deteriorating, according to aides. His doctor has said he is "fighting for his life".
He had been in prison serving a sentence for corruption, but was bailed last month to receive treatment. Since then his party and family have been fighting to get his name removed from a travel stop list to allow him to go overseas for treatment.
READ: Ailing Pakistan ex-PM Sharif seeks permission to travel abroad
The government of Sharif's rival Imran Khan had said it would not stand in the way, but last week demanded he pay a bond of seven billion Pakistani rupees (US$45 million) as a condition of his travel - which Sharif's party, the Pakistan Muslim League-Nawaz (PML-N), immediately rejected.
After days of political deadlock the condition was finally lifted and Sharif was flown to London via Doha on a Qatar Airways air ambulance.
Party workers showered rose petals on his car as it left his house on the outskirts of the eastern city of Lahore.
Senior PML-N member Pervaiz Rasheed confirmed to reporters that Sharif was en route to London.
Sharif's aides have said the unexplained cause and uncertain diagnosis of his illness require advanced investigations and specialised care.
The courts have granted him four weeks to receive treatment, though that can be extended pending medical advice.
Known as the "Lion of Punjab", Sharif is a political survivor who has repeatedly roared back to the country's top office. He served three terms - but did not complete a single one.
His first, beginning in 1990, ended in 1993 when he was sacked for corruption. The second lasted from 1997 to 1999, when he was deposed by the powerful military.
Sharif blamed the security establishment for again targeting him in 2017 when the Supreme Court disqualified him from politics for life over graft allegations, which he denies.


named-checkzone checks the syntax and integrity of a zone file. It performs the same checks as named does when loading a zone. This makes named-checkzone useful for checking zone files before configuring them into a name server.
Enable debugging.
Quiet mode - exit code only.
Print the version of the named-checkzone program and exit.
When loading the zone file read the journal if it exists.
Specify the class of the zone. If not specified "IN" is assumed.
The domain name of the zone being checked.
The name of the zone file.


Thanks to Phil Kast for writing the original bookmarklet for submitting
links to Hacker News, the excellent (*read* useless echochamber 99% of the time, with priceles anecdotes from experienced Google, Facebook, "that-place-that-built-what-you're using" ex-employees 1% of the time) computer science site. This fork is for DataTau, the fledgling (*read* ghost town doomed to be continuously superseded by random Twitter comments from @agibsonccc, @fchollet, "that-person-that-wrote-the-deep-learning-framework-you're-using", [can't forget @hardmaru]) data science site. When you click on the bookmarklet, it will submit the page you're on.
To install, drag this link to your browser toolbar:


Players compete for influence over the city of Megapolis . They gain influence by upgrading and expanding their own restaurant empire, at first each player starts with one restaurant but can start taking over other food joints once they have the necessary upgrades.
Real time
The game is played in real time. Players gain resources over time whch they use to upgrade their restaurant and hire workers. Each upgrade takes a certain amount of time which increases as the restaurant progresses. Players can hire workers to interfere with their neighbor business.
Ending
The server stops accepting new players after a certain amount of time/players thus allowing a domination victory.


Data to Show
FLU
POLLEN
City Map
One Day
Two Days
Three Days
One Week
One Month
CROWDSOURCE DATA
We are getting data from everyone so people can visualize places which have a lot of the flu so you know when to stay safe stay clean from those germs.


This is the 17th Century Page!
Click through below to find rebellions, revolutions, riots, and more in 17th century Tsarist Russia. I hope you enjoy and learn something new!
Uprising of Bolotnikov
- Date: 1606-1607
- Location: Southern & Central Russia
- Groups Uprising: Peasants, Cossacks, Nobles
- Number of People: Up to 25-30,000
- Leaders: Ivan Bolotnikov
- Reason(s): Rise of serfdom, political instability, famine
- Result: Supression
Moscow Uprising of 1648 (Salt Riot)
- Date: June 1648
- Location: Moscow, Russia (sparked some smaller riots across Russia)
- Groups Uprising: Moscovites, Strelsy
- Number of People: Unknown
- Leaders: Unknown
- Reason(s): Installation of a universal salt tax, which drove up its prices, poorer boyars wanted to reclaim escaped serfs, widespread (local) corruption
- Result: Death of Leontii Pleshcheyev (head of Moscow police), creation of the Assembly of the Land, through which the legal code used for centuries was formed (which, among other things, made it practically impossible for serfs to escape their boyars)
Copper Coin Riot
- Date: (N.S.) August 4th, 1662
- Location: Moscow, Russia
- Groups Uprising: Mainly Moscovites
- Number of People: Up to 10,000
- Leaders: Unknown (or N/A)
- Reason(s): Financial Crisis (deteriation of Moscow's economy due to the Livonian war, rise in taxes, inflation due to the issuing and then devaluation of copper coins, and the production of counterfeit money)
- Result: Merciless suppression, fear among officials
Bashkir Rebellion of 1662-1664
- Date: Summer 1662 - Autumn 1664
- Location: (Mostly) Bashkortostan (Bashkiria), Russia
- Groups Uprising: Bashkir Rebels
- Number of People: Unknown
- Leaders: Gaura Akbulatov, Ulekeya Krivoy, Ishmukhammed, Konkas Davletbaev, Uraslanbek Bakkin
- Reason(s): Fear of losing rights to land, increased taxes, abuse by officials
- Result: Officials removed for mistreatement, promised end to abuse by tax collectors, patrimonial right to land officially confirmed
Stepan (Or Stenka) Razin Rebellion
- Date: 1670-1671
- Location: Don and Volga regions of Russia; Kazan, Russia
- Groups Uprising: Rebel Cossacks
- Number of People: 500-20,000 (Varies between different periods)
- Leaders: Stepan Razin, Vasily Us, Alena Arzamasskaia
- Reason(s): Protect independence of the Cossacks, protest centralized government (and give more power to the people)
- Result: Brutal suppression and the execution of Razin (among others), increased government control and increased fear among the upper class and tsar of rebellion
Bashkir Rebellion of 1676 and 1681-1684
- Date: 1676, 1681-1684
- Location: Volga and Ural regions (Western Bashkortostan/Bashkiria)
- Groups Uprising: Bashkir Rebels, Tatars
- Number of People: Unknown
- Leaders: Seit Saafer (Sadiir), Ish-Mukhammed Devletbaev, other Bashkir nobles
- Reason(s): Russian governmant tried to impose Christianity on the Muslim Bashkir (and on the Muslim Tatars)
- Result: Promise to end forceful Christinization
Moscow Uprising of 1682
- Date: May 1682
- Location: Moscow, Russia
- Groups Uprising: Moscow Strelsy Regiments (firearm infantry)
- Number of People: Unknown
- Leaders: Sophia Alekseyevna, Prince Ivan Andreyevich Khovansky (Tararui)
- Reason(s): Death of Tsar Feodar III (and ensuing succession "crisis"), discontent of Moscow regiments
- Result: Deaths/Murders of multiple Naryshkin supporters (including Peter I's uncles), top commanders, and boyars, installation of Ivan V and Peter I as the "first" and "second" tsar (respectively), with Ivan's sister and Peter's half-sister, Sophia, as regent
Strelsy Uprising of 1698
- Date: June 6th-18th, 1698
- Location: West of Moscow, Russia
- Groups Uprising: Four Strelsy Regiments sent to Velikiye Luki
- Number of People: 2,300
- Leaders: Chosen Strelsy electives
- Reason(s): Not entirely agreed upon (rebellion due to Peter the Great's reforms or due to oppression of serfs and military hardships and mistreatment), discontentment among the Strelsy
- Result: Major investigations leading to the execution, torture, and exile of many Strelsy, disbanding of the Moscow regiments and the removal of them and their families from Moscow


Watch: Megan Thee Stallion Dating Rumors Heat Up, Tory Lanez Drops New Video, French Montana Gets Medical Treatment
by Jonny FastlaneThe rap news cycle never slows down. Today, online personality Jonny Fastlane focuses on Megan Thee Stallion dating rumors, Tory Lanez dropping visual heat, French Montana experiencing a medical scare and more. Let’s talk hip-hop!


Made with
by Brandon & Raphael
Windows
Shell Access
File Access
OS X
Shell Access
File Access
Linux (Ubuntu)
Shell Access
File Access


To view this video please enable JavaScript, and consider upgrading to a web browser that supports HTML5 video


JavaScript methods are the actions that can be performed on objects.
A JavaScript method is a property containing a function definition.
You create an object method with the following syntax:
methodName : function() { code lines }
You access an object method with the following syntax:
objectName.methodName()
You will typically describe fullName() as a method of the person object, and fullName as a property.
The fullName property will execute (as a function) when it is invoked with ().
This example uses the toUpperCase() method of the String object, to convert a text to uppercase:
var message = "Hello world!";
var x = message.toUpperCase();
The value of x, after execution of the code above will be:
Defining methods to an object is done inside the constructor function:
function person(firstName, lastName, age, eyeColor) {
this.firstName = firstName;
this.lastName = lastName;
this.age = age;
this.eyeColor = eyeColor;
this.changeName = function (name) {
this.lastName = name;
};
}
The changeName() function assigns the value of name to the person's lastName property.


Protest against ‘Muslim’ faculty continues in BHU
Appointment as per norm, clarification not needed: varsity
by Special CorrespondentProtests against the appointment of a “Muslim” assistant professor in the Sanskrit Faculty of Banaras Hindu University continued on Tuesday, 12 days after it began.
The university, however, reiterated that the appointment was made as per norms and there was no need for further clarification.
The students opposed to the appointment of Assistant Professor Firoz Khan in the Sahitya (Literature) Department of the Sanskrit Vidya Dharm Vigyan of the central university staged a sit-in and recited the Hanuman Chalisa.
They argued that Mr. Khan may be eligible to teach the Sanskrit ‘language’ but not the Sanskrit ‘vidya dharma’, primarily due to his religious identity.
The students have been demanding that Mr. Khan be transferred to another faculty.
‘Dharma yudh’
“The dharma yudh (holy war) goes on,” posted Shubham Tiwary, one of the students leading the protest, on Facebook.
While he was not reachable on phone, in another Facebook post Mr. Tiwary, a Ph.D scholar, said: “Everyone has rights over a language, but not over religion”.
Umakant Chaturvedi, the head of department, said the deadlock was still on and classes were not being held in the department.
Amid speculation that the administration held another meeting to convince the students to drop the protests and resume classes, BHU spokesperson Rajesh Singh clarified there was no such discussion by the Vice-Chancellor on Tuesday.
“Once appointment is made as per rules, we have taken a stand, [there is] no use to reiterate it,” the spokesperson said.
However, asked about Mr. Khan not being able to discharge his duties as a teacher, Mr. Singh said: “He has officially joined and is getting his salary.”
Mr. Khan did not respond to phone calls.


External Funding Manager
Aly is a Finance and Supply Chain Management student graduating in May 2017. She has worked with GE Aviation in Cincinnati in their Financial Management Program internship and will be returning to intern with GE in June 2016. Aly is an avid traveler who has visited Singapore, Malaysia and the United Arab Emirates through programs offered through UIUC's College of Business, in addition to spending a semester studying in Vienna, Austria. Outside of MakerGirl, Aly is involved with the business fraternity Delta Sigma Pi and the Business Student Ambassador Program.


Before we’d start, I’d like to clear up a few questions you might have about Vita homebrewing. If you’re confused about how or why people enable homebrew on their Vitas, make sure to read this next bit.
What is homebrew?
Homebrew are games and other software which are not officially approved. For example, VitaDoom is a port of the classic game DOOM and mGBA lets you play Game Boy Advance ROMs. You can find more examples of Vita homebrew here.
What is HENkaku?
HENkaku is the first ever homebrew enabler for PS Vita and PSTV. Running homebrew on your Vita is 100% free using HENkaku. No cost, no ads, and no “donations”. As long as you’re on version 3.60 or below, you’re good to go! If you paid for this software, you should ask for your money back.
What can I do with HENkaku?
HENkaku allows much more freedom than ever before possible with the PS Vita. It allows you to break free from the restrictions Sony set down such as:
- Playing older games with emulators
- Backing up your physical games and installing them to your memory card to play any time
- Using a microSD card instead of Sony’s expensive propriety memory cards
- Installing homebrew titles and having them appear on your home menu
What do I need to know before starting?
- Using this kind of software does come with a risk. There’s always be a chance that your Vita may become permanently unusable
- Make sure to keep your device is charged before starting to avoid data loss or damage from an unexpected power-off
- If you are using a Vita 1000, you must have a memory card
- This guide will not work on versions 3.61 and above
- There is no exploit for 3.61 and above available
- Do not trust anyone who says they do


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Reports invalid node names. Node names should match
[a-zA-Z0-9,._+@-]+
and should only include at most one
@
.


This document contains instructions for building the Cmajor compiler, tools and libraries from sources.
Select the LLVM-12.0.0-win64.exe link.
This is a direct link: LLVM-12.0.0-win64.exe
Installation
- After installation add C:\Program Files\LLVM\bin directory to PATH.
5. CMake
Version
3.24.3
Default location:
C:\Program Files\CMake
Download
From the Download page select cmake-3.24.3-windows-x86_64.msi link.
This is a direct link: cmake-3.24.3-windows-x86_64.msi
Installation
-
Installation using these settings:
6. Python
Version
3.11.0
Default location
C:\Program Files\Python311
Download
From the Python Releases for Windows page select Download Windows installer (64-bit).
Installation
Installation using these settings:
7. LLVM sources
Version
12.0.0
Default location:
C:\llvm-12.0.0.src
Download
- From the Download page select the 12.0.0/download link.
- LLVM 12.0.0 page select llvm-12.0.0.src.tar.xz link.
This is a direct link: llvm-12.0.0.src.tar.xz
Extract package to C:\llvm-12.0.0.src.tar.xz folder.
Compilation
-
Open x64 Native Tools Command Prompt for VS 2022.
-
Change to C:\llvm-12.0.0.src directory.
-
Make directory build:
C:\llvm-12.0.0.src>mkdir build
-
Change to build directory:
C:\llvm-12.0.0.src>cd build
-
Run CMake:
C:\llvm-12.0.0.src\build> cmake -G "Visual Studio 17 2022" -Thost=x64 -DLLVM_TARGETS_TO_BUILD="X86" -DLLVM_ENABLE_EH=On -DLLVM_ENABLE_RTTI=On ..
-
Open C:\llvm-12.0.0.src\build\LLVM.sln solution in Visual Studio 2022.
-
Build solution using Debug/x64 configuration.
-
Build solution using Release/x64 configuration
8. Git for Windows
Version
2.28.0
Download
Git for Windows
.
9. Cmajor compiler and C++ runtime
Default location
C:\work\cmajorm
Download
From https://github.com/slaakko/cmajorm page select Code | https://github.com/slaakko/cmajorm.git
-
Start Git Bash.
-
Change to C:\work directory.
-
Clone cmajorm repository:
git clone https://github.com/slaakko/cmajorm.git
-
Clones repository to cmajorm directory.
Configuration
MS Visual C++ configuration
Open the C:\work\cmajorm\cmajor\config\build.props file with a text editor and set the value of the following Visual Studio user macros:
- BOOST_INCLUDE_DIR. The default value is C:\boost\include\boost-1_80.
- BOOST_LIB_DIR. The default value is C:\boost\lib.
- LLVM_SRC_INCLUDE_DIR. The default value is C:\llvm-12.0.0.src\include.
- LLVM_BUILD_INCLUDE_DIR. The default value is C:\llvm-12.0.0.src\build\include.
- LLVM_RELEASE_LIB_DIR. The default value is C:\llvm-12.0.0.src\build\Release\lib.
- LLVM_DEBUG_LIB_DIR. The default value is C:\llvm-12.0.0.src\build\Debug\lib.
Mingw-w64 configuration
Open the C:\work\cmajorm\cmajor\rts\build\gcc\Makefile.common file with a text editor and set the following paths:
- BOOST_INCLUDE_DIR. The default value is C:/mingw-boost/include/boost-1_80.
- BOOST_LIB_DIR. The default value is C:/mingw-boost/lib.
- BOOST_DEBUG_FILESYSTEM_LIB. The default value is boost_filesystem-mgw12-mt-d-x64-1_80.
- BOOST_DEBUG_IOSTREAMS_LIB. The default value is boost_iostreams-mgw12-mt-d-x64-1_80.
- BOOST_DEBUG_SYSTEM_LIB. The default value is boost_system-mgw12-mt-d-x64-1_80.
- BOOST_RELEASE_FILESYSTEM_LIB. The default value is boost_filesystem-mgw12-mt-x64-1_80.
- BOOST_RELEASE_IOSTREAMS_LIB. The default value is boost_iostreams-mgw12-mt-x64-1_80.
- BOOST_RELEASE_SYSTEM_LIB. The default value is boost_system-mgw12-mt-x64-1_80.
Static Boost library gcc tool chain configuration
Optional.
Open the C:\work\cmajorm\cmajor\config\tool-chains.json file with a text editor and set Boost library version numbers in the following
lines:
- line 302. The default libraries are boost_filesystem-mgw12-mt-d-x64-1_80,
boost_iostreams-mgw12-mt-d-x64-1_80 and boost_system-mgw12-mt-d-x64-1_80.
- line 323. The default libraries are boost_filesystem-mgw12-mt-x64-1_80,
boost_iostreams-mgw12-mt-x64-1_80 and boost_system-mgw12-mt-x64-1_80.
Compilation
There's a makefile that builds the system using nmake (Option 1), but it may not always succeed due to file sharing issues (bugs in the compiler).
If the nmake does not succeed (after a couple of retries), it's possible to build the system the elaborate way (Option 2 and 10. onward) in stages.
Option 1: with makefile
- Add environment variable CMAJOR_ROOT with value C:\work\cmajorm\cmajor.
- Create directory C:\work\cmajorm\cmajor\bin.
- Add C:\work\cmajorm\cmajor\bin directory to PATH.
- Open x64 Native Tools Command Prompt for VS 2022
- Change to C:\work\cmajorm\cmajor\bat directory
- Run nmake
Option 2: elaborate way
- Add environment variable CMAJOR_ROOT with value C:\work\cmajorm\cmajor.
- Make subdirectory C:\work\cmajorm\cmajor\lib
- Make subdirectory C:\work\cmajorm\cmajor\lib\gcc
- Make subdirectory C:\work\cmajorm\cmajor\lib\vs
- Make subdirectory C:\work\cmajorm\cmajor\bin
- Make subdirectory C:\work\cmajorm\cmajor\rts\build\gcc\lib
- Make subdirectory C:\work\cmajorm\cmajor\rts\build\gcc\bin
- Add C:\work\cmajorm\cmajor\bin directory to PATH.
- Open x64 Native Tools Command Prompt for VS 2019
- Change to C:\work\cmajorm\cmajor\system\ext\pdcurs36\build directory.
- Run build.bat.
- Change to C:\work\cmajorm\cmajor\system\ext\zlib-1.2.11\contrib\masmx64 directory
- Run bld_ml64.bat
- Open C:\work\cmajorm\cmajor\cmajor.sln in Visual Studio 2019.
- Select Debug/x64 configuration.
- Build solution.
- Select Release/x64 configuration.
- Build solution.
- Open Windows Terminal to C:\work\cmajorm\cmajor\bat directory.
- Run inst.bat. Does not find all the files, but does not matter for now.
- Open Windows Terminal to C:\work\cmajorm\cmajor\rts\build\gcc directory.
- Run mingw32-make (assumed that can be found from PATH):
C:\work\cmajorm\cmajor\rts\build\gcc> mingw32-make
- Run mingw32-make install:
C:\work\cmajorm\cmajor\rts\build\gcc> mingw32-make install
10. Unicode
Not required if 9. Option 1 succeeded.
Download
Download Unicode 12.1 Character Database: ucd.all.flat.zip
and extract it to C:\work\cmajorm\cmajor\unicode directory.
Installation
- Open Windows Terminal to C:\work\cmajorm\cmajor\unicode directory.
- Run makecmajorucd. Makes cmajor_ucd.bin Unicode database for Cmajor:
C:\work\cmajorm\cmajor\unicode> makecmajorucd
11. Cmajor system libraries
Not required if 9. Option 1 succeeded.
Installation
- Open Windows Terminal to C:\work\cmajorm\cmajor\system\platform\windows directory.
- Build System library using the debug configuration (LLVM):
C:\work\cmajorm\cmajor\system\platform\windows> cmc -u -v System.cms
- Build System library using the release configuration (LLVM):
C:\work\cmajorm\cmajor\system\platform\windows> cmc -u -v -c=release System.cms
- Build System library using the debug configuration (C++):
C:\work\cmajorm\cmajor\system\platform\windows> cppcmc -st -u -v System.cms
- Build System library using the releaseconfiguration (C++):
C:\work\cmajorm\cmajor\system\platform\windows> cppcmc -st -u -v -c=release System.cms
12. Cmajor Visual Studio extension
Optional.
- Open C:\work\cmajorm\cmajor\task\task.sln in Visual Studio 2019
- Select Debug|Any CPU -konfiguraaatio
- Build solution
- Select Release|Any CPU -konfiguraaatio
- Build solution
- Open Windows Terminal to C:\work\cmajorm\cmajor\bat directory.
- Run install_vstask.bat: copies C:\work\cmajorm\cmajor\task\bin\Release\CmajorTasks.dll to bin directory.
- Change to C:\work\cmajorm\cmajor\vs\2019 directory.
- Run CreateCmajorCPS.exe:
C:\work\cmajorm\cmajor\vs\2019>CreateCmajorCPS
- Close Windows Terminal
- Right click C:\work\cmajorm\cmajor\vs\2019\cmajor.vsix and select install.
13. Cmajor tools
Optional and not required if 9. Option 1 succeeded.
- Open Windows Terminal to C:\work\cmajorm\cmajor\projects\cm directory.
- Compile Cm.cms solution using debug config:
C:\work\cmajorm\cmajor\projects\cm>cmc -u -v Cm.cms
- Compile Cm.cms solution using release config:
C:\work\cmajorm\cmajor\projects\cm>cmc -u -v -c=release Cm.cms
- Change to C:\work\cmajorm\cmajor\projects\tools\soulcm\scmlg directory.
- Compile scmlg.cmp project using debug config:
cmc -u -v scmlg.cmp
- Compile scmlg.cmp project using release config:
cmc -u -v -c=release scmlg.cmp
- Change to C:\work\cmajorm\cmajor\projects\tools\soulcm\scmpg directory.
- Compile scmpg.cmp project using debug config:
cmc -u -v scmpg.cmp
- Compile scmpg.cmp project using release config:
cmc -u -v -c=release scmpg.cmp
- Change to C:\work\cmajorm\cmajor\projects\tools\soulcm\scm2html directory.
- Compile scm2html.cmp project using debug config:
cmc -u -v scm2html.cmp
- Compile scm2html.cmp project using release config:
cmc -u -v -c=release scm2html.cmp
- Change to C:\work\cmajorm\cmajor\projects\tools\spring directory.
- Compile spring.cmp project using debug config:
cmc -u -v spring.cmp
- Compile spring.cmp project using release config:
cmc -u -v -c=release spring.cmp
- Change to C:\work\cmajorm\cmajor\projects\tools\supd directory.
- Compile supd.cmp project using debug config:
cmc -u -v supd.cmp
- Compile supd.cmp project using release config:
cmc -u -v -c=release supd.cmp
14. Cmajor examples
Optional and not required if 9. Option 1 succeeded.
- Open Windows Terminal to C:\work\cmajorm\cmajor\projects\examples directory.
- Compile examples.cms solution using debug config:
C:\work\cmajorm\cmajor\projects\examples>cmc -u -v examples.cms
- Compile examples.cms solution using release config:
C:\work\cmajorm\cmajor\projects\examples>cmc -u -v -c=release examples.cms
15. System X
Optional.
- Open Windows Terminal to C:\work\cmajorm\cmajor\projects\cmsx directory.
- Compile cmsx.cms solution using debug config:
C:\work\cmajorm\cmajor\projects\cmsx> cmc -u -v cmsx.cms
- Compile cmsx.cms solution using release config:
C:\work\cmajorm\cmajor\projects\cmsx> cmc -u -v -c=release cmsx.cms
16. Installation
- Open Windows Terminal to C:\work\cmajorm\cmajor\bat directory.
- Run inst.bat.
Changed files are copied to C:\work\cmajorm\cmajor\bin and C:\work\cmajorm\cmajor\lib directories.


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“Sometimes, with their bony limbs flung forth in gnarled unnatural gestures, they remind me of frantic skeletons suddenly petrified in their dance of death. They are frenzied, and unutterably tragic. They seem to move; yet they are so dead. And I imagine their denuded tortured arms reaching toward unanswering Heaven in an agony of protest against the fate that has gripped all nature.” — Katherine Shortall, Where The Sabots Clatter Again


SkyDateRangeCalculatorId values specify calculator objects that return two Date objects to represent date ranges. The SkyDateRangeCalculatorId values are used to populate the options in the date range picker's dropdown.
SKY UX uses the SkyDateRangeService to create calculators and configures each one with a validate function to confirm that the dates users select are compatible. For example, validate functions ensure that start dates are before end dates. SKY UX also configures calculators to call a getValue function after the validate function and return a range of two Date objects.
Enables users to select a start date with no end date.
Selects no dates and considers all dates within the date range. This is the default selection.
Enables users to select an end date with no starting date.
Sets the start date to the first day of the year before the current year and the end date to the last day of that year.
Sets the start date to the first day of the fiscal year before the current fiscal year and the end date to the last day of that fiscal year. The fiscal year is Oct. 1 to Sept. 30.
Sets the start date to the first day of the month before the current month and the end date to the final day of that month.
Sets the start date to the first day of the quarter before the current quarter and the end date to the last day of that quarter. Quarters are January to March, April to June, July to September, and October to December.
Sets the start date to Sunday of the week before the current week and the end date to Saturday of that week.
Sets the start date to the first day of the year after the current year and the end date to the last day of that year.
Sets the start date to the first day of the fiscal year after the current fiscal year and the end date to the last day of that fiscal year. The fiscal year is Oct. 1 to Sept. 30.
Sets the start date to the first day of the month after the current month and the end date to the last day of that month.
Sets the start date to the first day of the quarter after the current quarter and the end date to the last day of that quarter. Quarters are January to March, April to June, July to September, and October to December.
Sets the start date to Sunday of the week after the current week and the end date to Saturday of that week.
Enables users to select specific start and end dates.
Sets the start date to the first day of the current year and the end date to the last day of the year.
Sets the start date to the first day of the current fiscal year and the end date to the last day of the fiscal year. The fiscal year is Oct. 1 to Sept. 30.
Sets the start date to the first day of the current month and the end date to the last day of the month.
Sets the start date to the first day of the current quarter and the end date to the last day of the quarter. Quarters are January to March, April to June, July to September, and October to December.
Sets the start date to Sunday of the current week and the end date to Saturday.
Sets the start and end dates to the current day.
Sets the start and end dates to the day after the current day.
Sets the start and end dates to the day before the current day.


What Planet Are You From? * * * (out of * * * * )
Directed by Mike Nichols. Cast: Garry Shandling, Annette Bening, John Goodman, Greg Kinnear, Ben Kingsley, Linda Fiorentino, Judy Greer, Caroline Aaron, Nora Dunn, Camryn Manheim, Ann Cusack, Janeane Garofalo. 2000 - 107 minutes Rated R (for profanity, sex, nudity, and much sex-related humor). Reviewed by Dustin Putman, March 4, 2000.
The premise of "What Planet Are You From?" is one of great convolution and foolishness, the type that, more often than not, would simply be written off as a dimwitted movie without any value or merit. Who could possibly take a film seriously in which an alien (Garry Shandling) from a planet "way the hell out there" is sent to Earth for one mission, and one mission only: to mate with a woman and have a child? Sounds like the usual low-rent junk that is released in theaters in the spring, or sent direct-to-video, eh? Certainly not, if it aims directly for laughs, and is in the hands of acclaimed director Mike Nichols (1983's "Silkwood," 1988's "Working Girl," 1998's "Primary Colors"), and stars, among others, Garry Shandling (TV's "The Larry Sanders Show"), Annette Bening (1999's "American Beauty"), and John Goodman (TV's "Roseanne").
Following a prologue on the distant planet, where the human-looking aliens (who otherwise exhibit no ability to have feelings or emotions) are misdirected in their teachings on how to treat the opposite sex, one such alien, who is given the name Harold, is chosen to make his way down to Earth. Locating himself in Seattle, Washington, he gets himself a job at a bank and makes friends with his womanizing, married coworker, Perry (Greg Kinnear), who begins to help him in his quest to meet a woman.
One evening, Perry takes Harold to an AA meeting (a prime place, Perry believes, to pick up conflicted and vulnerable females), where Harold is instantly smitten with Susan Hart (Annette Bening), a recovering alcoholic/real estate agent whose biological clock is ticking very loudly, but who has sworn to herself she will only sleep with someone again when she has married. After just one date, in which Harold and Susan hit it off, Harold proposes marriage to Susan, and in a moment of haste, she accepts. Their relationship soon grows problematic, however, when Harold becomes very distant and unloving towards Susan after she has gotten pregnant. What she doesn't know is that he isn't purposefully being emotionally cold to her: he just doesn't know how to love.
Meanwhile, following a mysterious blast on an airplane that allegedly was Harold's entrance to Earth, a Federal Aviation Administration agent (John Goodman) begins to investigate the strange occurrence, and gradually catches on to the true identity of Harold, causing stress on his own marriage to a fed-up housewife (Caroline Aaron) who believes he is having an affair.
"What Planet Are You From?" may very well be the trickiest motion picture of the year, thus far, because its admittedly ludicrous nature only adds to the delicate balancing act that must constantly be obtained by director Nichols and screenwriters Garry Shandling, Michael Leeson, Ed Solomon, and Peter Tolan. One prominent misstep, and the whole film would be in danger of crumbling to the ground, making the movie be a complete embarrassment for all involved.
It's a stroke of luck (and an obvious boatload of comedic talent), then, that the film is, overall, the most laugh-out-loud funny comedy in ages. For the first hour, it is genuinely perfect, a masterwork in which literally almost every attempt at a laugh works, so much so that I often was still laughing at one part, when the next would arise and make me laugh even more. Suffice to say, I wasn't able to inhale much oxygen during that sixty-minute time span. Everything, even right down to the use of a particular musical chord that echoes the raising of a character's eyebrows, is an example of comic brilliance, the way all comedies should work.  It may be silly, and it may sometimes be even graphic in its sexual innuendo, but it is also an undeniable riot.
The second hour of "What Planet Are You From?" shifts tones, and while still effective, much of its comedy is put on the back burner for a more somber, poignant look at love relationships that may involve an alien in this case, but stands for a great deal of marriages, in general. Changing from something that is so highly entertaining and relatively breezy to something that delves a little deeper into the characters and story comes as a marginal disappointment on the outset, but in another way, the latter half is vital to what the whole picture has been setting itself up for. By getting more serious, but never totally abandoning its comedy, director Nichols wants us to invest our feelings into the fate of Harold and Susan's relationship, and we are surprised to realize that, while the opening had been wavering along the lines of even being considered a spoof, a 'la "The Naked Gun," we have, indeed, grown to care about them.
Only the climax, which briefly takes us back to Harold's planet for a rather saccharine speech on the importance of compassion and human emotions, does the film stumble for more than a fleeting moment, but, fortunately, it recoups itself by the finale.
Garry Shandling, in his first starring film role, is outstanding as Harold, the very important and flawless comedic center of the film. While being unable to feel things inside, Shandling, nonetheless, is able to gain our sympathies, and the eccentric romance that blossoms between he and Susan is sweet-natured and involving. Susan, as played with energy and appropriate pinnache by Annette Bening, is Harold's total match because, although she gradually becomes dissatisfied with his uncaring ways, makes it clear that she had meaningless sex with so many men in her life that she has forgotten herself how to love, or what it even is. Only after meeting the one-of-a-kind Harold does she start to rebuild her life and understand what it means to feel love, even when it isn't outwardly being returned to her.
As the slimy Perry, this is Greg Kinnear's most memorable role to date. Usually an extremely bland actor, Kinnear jumps off the screen here and makes his, albeit unlikable, character come alive. Judy Greer (1999's "Jawbreaker"), as a flight attendant turned off by Harold's advances until she meets him at the AA meeting, is entertaining and gets a great big laugh in the last second of her final scene due to the aforementioned musical chord that strikes at just the right time. And although just an unbilled cameo, Janeane Garofalo brings her usual sparkling presence to the role of a nervous flier whom Harold hits on, even in her horrified state. Meanwhile, Linda Fiorentino (1997's "Men in Black") is severely wasted as Perry's wife, who Harold considers having an affair with after he is married.
Whatever you do, do not be turned off by the premise, or the title itself, of "What Planet Are You From?" Rated R, and rightfully so, this film will delight adult viewers who are in the mood for a feel-good comedy that turns out to not only be about the punchline of jokes, but also, within the context, takes its characters and their situations seriously. In fact, perhaps the most gratifying thing of all is that director Mike Nichols and his cast of high-profile actors took a big risk on making this offbeat movie, and do not embarrass themselves. Not one little bit.
- Copyright 2000 by Dustin Putman Http://www.young-hollywood.com Http://www.atnzone.com
The review above was posted to the
rec.arts.movies.reviews newsgroup (de.rec.film.kritiken for German reviews).
The Internet Movie Database accepts no responsibility for the contents of the
review and has no editorial control. Unless stated otherwise, the copyright
belongs to the author.
Please direct comments/criticisms of the review to relevant newsgroups.
Broken URLs inthe reviews are the responsibility of the author.
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Related links: index of all rec.arts.movies.reviews reviews


The footballer has denied that he has married longtime girlfriend Georgina Rodriguez, following reports they tied the knot in Morocco.
Italian gossip magazine Novella 2000 reported that the couple may have married back in May, with an insider adding that Ronaldo, 34, had changed his will to protect Georgina, 25.
However, a rep for Ronaldo told TMZ Sports: ‘He has not got married’ – with another rep saying the report was ‘fake news’.
Former shop assistant Georgina admitted in February she would love to become the Portuguese star’s wife but shut down speculation they were already engaged.
She told glossy Spanish magazine Hola! he had yet to ask for her hand in marriage, but she admitted: ‘Every couple wants to get married and I would love to personally.
Advertisement Advertisement
‘Right how we have priorities and a lot of responsibilities, although in the future it would be marvellous to become Cristiano’s wife.’
Cristiano forged his relationship with Georgina in 2016 during lock-ins at the upmarket clothes store in Madrid where she used to work.
She soon became his first serious girlfriend since he broke up with Russian beauty Irina Shayk at the start of 2015.
He moved her into his luxury home on a gated estate on the outskirts of the Spanish capital before setting up home with her in Turin, and they welcomed their first child together, Alana, in 2017.
Ronaldo is also dad to Cristiano Jr, nine, and two-year-old twins Eva Maria and Mateo, who he welcomed via surrogate.
Last year the footballer’s mum said of Georgina during a magazine interview about her son’s love life: ‘She is the mother of my grand-daughter. She is a future daughter-in-law. She’s not my daughter-in-law yet. She’s a future daughter-in-law. She’s a very calm person.’
So perhaps a wedding isn’t too far off.
Got a showbiz story?
If you've got a story, video or pictures get in touch with the Metro.co.uk Entertainment team by emailing us<EMAIL_ADDRESS>calling 020 3615 2145 or by visiting our Submit Stuff page - we'd love to hear from you.


Download socklog into any directory and run ./configure
# cd socklog-2.2.0 # ./configure # make # make install
Compile and install the socklog programs
# package/installIf you want to make the man pages available in the /usr/local/man/ hierarchy, do:
# package/install-manTo report success:
# mail<EMAIL_ADDRESS><compile/sysdepsIf you use socklog regularly, please contribute to the project.
Refer to Configuration for configuring and setting up socklog services.


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There are so many different recipes that contains Blueberries. There is no way I can forget to mention the Brain Power Salad that is so famous. Very simple to make and enjoy for lunch. Naked juice are the true pioneers in making maintaing the natural taste of berries. Even though the famous blue machine is mixed with different berries, it remains a power drink
PLEASE CLICK ON THE LINK - The Most Delicious Super Fruit Drink
PLEASE CLICK ON THE LINK - Delicious Blueberry Pie Recipe
PLEASE CLICK ON THE LINK - Amazing Blueberry Salad
Enjoy the journey towards better health. There are many other recipes on how to prepare Blueberries, but these are truly my favorite. Enjoy and now go find some purple gems.


{{item.title}}
{% extends "base.html"%} {% load staticfiles %} {%block head_title%} Libraries {%endblock%} {% block content%}
On this page you will find libraries and APIs that I have contributed to. Useful, streamlined and decoupled APIs allow developers to produce work without reinventing the wheel first, for me this runs in the same vein as tool development, I can help to make other people's jobs easier by sharing robust libraries that I have worked on. I greatly appreciate any feedback or suggestions.


D&D Dice Demos
This page contains demos of the D&D dice web components.
Check out the source of this page to see how they work.
For detailed information see the
github project.
D&D Dice Result
Standard D&D Dice
Pressed:
Preset D&D Dice
(This preset is associated with the first dice result)
Pressed:
(This preset shows a 1x2 grid)
D&D Dice Panel


--- layout: home ---
I am software engineer and consultant freelancer working remotely, for now. I actively share what I learn over on my blog. I graduated - in May 2021 - with a MSci in Computing Science from The University Of Glasgow where I had the opporuntity to research uncertainty calibration methods for Deep Neural Networks in Inverse Reinforcement Learning and build various applications for a range of clients. Whilst studying I co-founded TÓCE, worked part time as a full stack software engineer and tutored students in computing science. If you have a project you think I could help with, or just want to chat, don't hesistate to get in touch!


{% load l10n finance %}
| within norms | 25% to 40% |
| outside norms | less than 25% or more than 40% |
Employee-related costs are typically the largest portion of operating expenditure, but they should not grow so large that they threaten the sustainability of the operating budget.
The normal range for this indicator is between 25% - 40% of total operating expenditure. Municipalities must guard against spending too much on staff while also making sure they have the people they need to deliver services effectively.
| within norms | up to 5% |
| outside norms | more than 5% |
Private contractors are sometimes needed for certain work, but they are usually more expensive than municipal staff. This should be kept to a minimum and efforts should be made to provide services in-house, where possible.
This measure is normally between 2 percent and 5 percent of total operating expenditure.


---
sort_order: 65
tei_id: rdx_b5h9g.p.idp11371328
annotation_count: 0
images:
small-thumbnail: https://readux.library.emory.edu/books/emory:b5h9g/pages/emory:pckf0/mini-thumbnail/
json: https://readux.library.emory.edu/books/emory:b5h9g/pages/emory:pckf0/info/
full: https://readux.library.emory.edu/books/emory:b5h9g/pages/emory:pckf0/fs/
page: https://readux.library.emory.edu/books/emory:b5h9g/pages/emory:pckf0/single-page/
thumbnail: https://readux.library.emory.edu/books/emory:b5h9g/pages/emory:pckf0/thumbnail/
title: Page 65
number: 65
---
{% raw %}JACOB HODGES.{% endraw %}
{% raw %}57{% endraw %}
{% raw %}great sinner, and he appeared to me as a{% endraw %}
{% raw %}deliverer from sin. 0! the mercy."{% endraw %}
{% raw %}" How could he be a deliverer?"{% endraw %}
{% raw %}" It is because he was the Son of God{% endraw %}
{% raw %}that came into the world to seek and save{% endraw %}
{% raw %}that which was lost."{% endraw %}
{% raw %}Here he drew near to me and rested his{% endraw %}
{% raw %}arm upon my knee.{% endraw %}
{% raw %}" Do you ever have any affecting views{% endraw %}
{% raw %}of his character?"{% endraw %}
{% raw %}" Very often, very often. And it is my{% endraw %}
{% raw %}daily desire and striving to know more{% endraw %}
{% raw %}and more and more of his character."{% endraw %}
{% raw %}" What are the views you have of him ?"{% endraw %}
{% raw %}"He appears to me daily as the Saviour{% endraw %}
{% raw %}of the world, able and willing to save all{% endraw %}
{% raw %}who come to God by him."{% endraw %}
{% raw %}" How do others appear to you in com¬{% endraw %}
{% raw %}parison with him ?"{% endraw %}
{% raw %}" Nothing but chaff before the wind, and{% endraw %}
{% raw %}the things of the earth appear as dust com¬{% endraw %}
{% raw %}pared with the glory of the Son of God."{% endraw %}
{% raw %}" How car. he bear to be seen by such{% endraw %}
{% raw %}a sinner as you and I ?"{% endraw %}
{% raw %}" Because he bears with us a long t;me{% endraw %}


Civil Money Claims - Alpha
Defendant responding
- Letter
- Start page
- Enter claim number and security code
- View claim
- Create account
- Verify your email address instructions (click on<EMAIL_ADDRESS>- Email with link to verify account
- Sign in page
Task list
Check before you start
Respond to claim
Full admission
- When will you pay
- Full amount by set date
- Full amount after 28 days (shown if date is after 28 days)
- Instalments
Statement of means
Shown when claimant makes payment offer via installments or in full after 28 days
- Statement of means explanation
- Where are you living
- Do any children live with you?
- Children aged 16 to 19 living with you(show if value is entered in 16 - 19 input)
- Do you or your partner pay maintenance for any children?
- Do you support anyone else financially?
- Are you currently working?
- Who employs you?(show if employed is selected)
- What are you self-employed as?(show if self-employed is selected)
- Are you unemployed or retired?(show if not working is selected)
- List your bank and saving accounts
- List your monthly income
- List your monthly expenses
- Do you have any debts?
- Has a court ordered you to pay anyone else?
Part admission
A: The claim amount is too much
- How much money do you believe you owe?
- Timeline of events
- Add evidence
- Affected you
- When will you pay
- Free mediation
B: I've paid what I believe I owe


"COVID-19 pandemic, also known as the coronavirus pandemic is an ongoing of coronavirus disease 2019(COVID-19) caused by severe acute respiratory syndrome coronavirus 2 (SARS-CoV-2). First identified in Wuhan, China. (Wikipedia)


Constructor
new EventListener(channel, fn, scope, once)
Event Listener constructor
Parameters:
| Name | Type | Description |
|---|---|---|
channel |
string | The channel on witch the events will be broadcast |
fn |
function | The listener callback function |
scope |
function | The listener scope |
once |
boolean | If it's a one time listener |
- Source:
Members
channel
- Source:
fn
- Source:
once
- Source:
scope
- Source:
Methods
emit(event)
Emit the event to the listener function
Parameters:
| Name | Type | Description |
|---|---|---|
event |
BusEvent |
- Source:
is(listener) → {boolean}
Check if the given callback is the same as the listener ones
Parameters:
| Name | Type | Description |
|---|---|---|
listener |
function |
- Source:
Returns:
- Type
- boolean


From August 2018:
Please refer to Engineers.sg/events for the
list of upcoming open developer, design and maker events in Singapore!
webuild.sg, data.webuild.sg, live.webuild.sg and notes.webuild.sg are now available as archived sites.
Refer to this discussion thread for more details.
The journey towards a vibrant developer, designer and maker community continues...
🤗 🚀 🔌 🔩 📱 💻 ✏ 🚤 🔨 💡 ⛄ 🎈 📡 🎤 👫 👭 👬


Welcome to our Fur Family. We are excited to see you have taken your pet ownership serious. Please utilize our tools to give your pup the unconditional love it deserves.


| Interface | Description |
|---|---|
| Entry<T,S extends Geometry> | |
| EntryFactory<T,S extends Geometry> | |
| Factory<T,S extends Geometry> | |
| Leaf<T,S extends Geometry> | |
| LeafFactory<T,S extends Geometry> | |
| NearestEntry<T,S extends Geometry,D> | |
| Node<T,S extends Geometry> | |
| NonLeaf<T,S extends Geometry> | |
| NonLeafFactory<T,S extends Geometry> | |
| Selector |
The heuristic used on insert to select which node to add an Entry to.
|
| Splitter | |
| Visitor<T,S extends Geometry> |
| Class | Description |
|---|---|
| Candidate<R,D> | |
| Context<T,S extends Geometry> |
Configures an RTree prior to instantiation of an
RTree . |
| DistanceBrowsing |
Implements k-nearest neighbor search over a multi-dimensional R-tree.
|
| Iterables | |
| Iterables.FilterIterable<T> | |
| Iterables.FilterIterator<T> | |
| MultiMetricSimilaritySearch |
Implements the method for top-k similarity search against the an index holding (embedded) multi-dimensional points using various distances.
|
| NodePosition<T,S extends Geometry> | |
| RectangleDepth | |
| RTree<T,S extends Geometry> |
Immutable in-memory 2D R-Tree with configurable splitter heuristic.
|
| RTree.Builder |
RTree Builder.
|
| RTree.Builder.MidComparator | |
| Search | |
| Search.SearchIterable<T,S extends Geometry> | |
| Search.SearchIterator<T,S extends Geometry> | |
| SelectorMinimalOverlapVolume | |
| SelectorMinimalVolumeIncrease |
Uses minimal volume increase to select a node from a list.
|
| SelectorRStar |
Uses minimal overlap volume selector for leaf nodes and minimal volume increase
selector for non-leaf nodes.
|
| SplitterQuadratic | |
| SplitterRStar |
| Enum | Description |
|---|---|
| Precision |


{% extends "articles/articles-base.html" %} {% block main %}
You've created the article successfully.


Panomic Cancer Analyzer
Introducing the first Big-Data-driven cancer diagnosis framework for twelve most widespread cacner types.
Based on the genome profiles from 3,316 cancer patients participated in NIH The Cancer Genome Atlas project, we created a framework for precise diagnosis and treatment strategy planning.


100 years of ineptitude
Walking around like some dude with nothing to do, unaware of the current inner workings of my own mind.
All the people around don’t know anything, they’re so dumb.
Parachuting molly in Washington Sq.
“That’s the thing about the moon,” Audrey says, “if I wanted to, nothing could stop me from going there.”

Feeling not high enough, me and Audrey go back home to insufflate more MDMA where she asks about my first memory.
“A picnic,” I say, “with my mom and someone else, I don’t remember.”
“Stupid,” she says.
I display a disconcerted facial expression.
“Stupid memories,” she says to herself, “they don’t mean anything to anyone.”
On our way to the reading, I’m thinking about puddles and other bodies of water when a man punches me in the back of the head.
“Excuse me,” I say before laughing and walking away.
“Where do you think you’re going, motherfucker?”  Audrey yells as the whole future feels like it’s opening up right in front of me.
“That was cool,” I observe.
“It was cool and kind of funny,” Audrey responds in the immediate aftermath.
We finally make it to the reading where Sarah pleads with me, “Theo, stop patting my back when we hug, just hug me for real!”
We’re all conversing within a group when Rachel jokingly says, “Where did my parents go wrong?”
“That’s a good tweet,” I say.
“That is a good tweet!” she rehashes.
After a mercifully short list of readers, me and Audrey go to the roof to smoke weed.
“It’s beautiful up here.”
“Roofs don’t really do anything for me,” she says.
“In the summertime, I’ll go on my roof everyday.”
“I’m not saying they’re bad, they’re just nothing special. I guess I enjoy the perspective, but-“
“I wasn’t trying to argue,” I say.

Waiting in line for the bathroom, Henry notes that not only are the current occupants probably doing drugs, but we also plan to do the same.
“It’s always so nice seeing you,” I tell him after sharing a laugh.

Showing off to Audrey, I hop down the last three steps of the stoop and shout, “I give tonight a 7/10!”
Discussing the recent meaningful interactions on our way home, I think about how how this time last year I was in San Francisco.
The hills toppled around like sedated seagulls, there was a lot of yellow and pink, even nicer things probably.
It’s weird how I always feel like the same person until I think about stuff for a little while.
“You never pay any attention to me,” Audrey says as it starts to rain.
I sincerely apologize to her.
“Rain, rain,” she says a few times until her voice quiets to a low murmur, “this is a secret to everyone asleep.”
The next day, I wake up and it feels distinctly like a fade-in, or maybe a very long dissolve, through waking, pooping, showering whilst singing, dressing too long, coffee-ing, smoking, eating, smoking, talking too loudly, whispering unnecessarily, wondering hopefully, sleeping maybe.
Ugh, I don’t want to get out of bed, there’s nothing to do and it’s all so hard.

“Bastards,” I whisper dramatically and laugh.
I visualize laughter as something akin to magnetic waves that intensifies in proximity to domesticated animals.
“Holy shit,” I realize, “I can apply meaning to anything.”
I stare out the window at a spot on the neighboring building, a group of bricks midway between two third floor windows, and think to myself, “This must be it, this must be meaning.”


Installation¶
TensorLayer has some prerequisites that need to be installed first, including TensorFlow, numpy and matplotlib. For GPU support CUDA and cuDNN are required.
If you run into any trouble, please check the TensorFlow installation instructions which cover installing the TensorFlow for a range of operating systems including Mac OX and Linux, or ask for help on<EMAIL_ADDRESS>Prerequisites¶
Python + pip¶
TensorLayer is build on the top of Python-version TensorFlow. Please install Python first.
Note
We highly recommend python3 instead of python2 for the sake of future.
Python includes pip
command for installing additional modules is recommended.
Besides, a virtual environment
via virtualenv
can help you to manage your python packages.
Take Python3 for example, to install Python includes pip
, run the following commands:
sudo apt-get install python3
sudo apt-get install python3-pip
sudo pip3 install virtualenv
To build a virtual environment and install matplotlib and numpy into it, run the following commands:
virtualenv env
env/bin/pip install matplotlib
env/bin/pip install numpy
Check the installed packages, run the following command:
env/bin/pip list
TensorFlow¶
The installation instructions of TensorFlow are written to be very detailed on TensorFlow website. However, there are something need to be considered.
TensorFlow release¶
TensorFlow only officially supports GPU acceleration for Linux at present. If you want to use GPU with Mac OX, you need to compile TensorFlow from source.
Warning
For ARM processor architecture, you also need to install TensorFlow from source.
TensorLayer¶
Hao Dong highly recommend you to install TensorLayer as follow.
cd to the root of the git tree
pip3 install . -e
This command will run the setup.py
to install TensorLayer. The -e
allows
you to edit the scripts in tensorlayer folder, this help you to extend and modify
TensorLayer easily.
GPU support¶
Thanks to NVIDIA supports, training a fully connected network on a GPU, which may be 10 to 20 times faster than training them on a CPU. For convolutional network, may have 50 times faster. This requires an NVIDIA GPU with CUDA and cuDNN support.
CUDA¶
The TensorFlow website also teach how to install the CUDA and cuDNN, please click: TensorFlow: CUDA install.
Install the latest CUDA and cuDNN available from NVIDIA:
After installation, make sure /usr/local/cuda/bin
is in your PATH
(use echo #PATH
to check), and
nvcc --version
works. Also ensure /usr/local/cuda/lib64
is in your
LD_LIBRARY_PATH
, so the CUDA libraries can be found.
TensorFlow¶
If CUDA is set up correctly, the following command should print some GPU information on the terminal:
python -c "import tensorflow"
cuDNN¶
NVIDIA provides a library for common neural network operations that especially speeds up Convolutional Neural Networks (CNNs). Again, it can be obtained from NVIDIA after registering as a developer (it take a while): cuDNN install
To install it, copy the *.h
files to /usr/local/cuda/include
and the
lib*
files to /usr/local/cuda/lib64
.


Part sandal, part running tight and introduced in a bumblebee color scheme, the Nike Sock Racer wasn't your average shoe. It was inspired by Bill Bowerman’s mandate to strip away all unnecessary elements of a running shoe and honed to act as an extension of the foot.
Still, no one expected this ultralight racing flat to make the impact it did, but it became an instant favourite of marathon runners and triathletes. Transcending sports and genders, the Sock Racer also inspired cult favorites like the Air Sock, Air Flow, Air Current and Aqua Sock — and made a fashion statement, due to its avant-garde styling.
Debuting in 1996, the Nike Air Rift wasn't heavily advertised — but word of mouth and a fascination with its statement looks helped it move quickly. A stretch fit, Velcro fastening and, most of all, unique split-toe design made the Air Rift instantly recognizable.
Developed with insight from Tinker Hatfield, its design was inspired by the running style of Kenyan barefoot athletes. Named after Kenya’s Rift Valley Province and debuting in the colors of the country's flag, the Air Rift would also attract an audience who simply wanted to wear something this strange and beautiful on their feet.
The Nike Air Presto was created as a kind of T-shirt for the foot, with a unique XXXS-XXXL sizing structure that referred to its apparel inspiration. It also conveyed the sock-like snugness of the elastic upper's fit, which drew upon the technical advances of the 1993 Air Huarache Light. Additionally, an injection-moulded ‘finger cage’ provided extra support around the mid-foot and heel, while eyelets located at the tips of the ‘fingers’ were laced across the V-notch of the mesh upper.
Once laced, the shoe’s flexibility meant it could be pulled on and off like a slip-on, using the heel clip. This commitment to minimalism won it fans from the start, when the Air Presto arrived the same year as the equally experimental Air Woven, in a spectrum of bright colorways derived from the ‘fruit flavours’ of the original Apple iMac computer. Reworked as an HTM (Hiroshi Fujiwara, Tinker Hatfield, Mark Parker) release, given an early NIKEiD option and spawning an entire series of its own, the Presto design was a favorite of runners and collectors alike.
Pitched halfway between a bare foot and a regular running shoe, the Nike Free 5.0 was so revolutionary that it spawned countless imitators and came with a warning attached.
Due to its flexible design and the natural motion philosophy, the Free 5.0 struck a chord with athletes everywhere. But the seamless upper and responsive cushioning—elements that had been designed purely for performance—began to resonate with a discerning audience seeking progressive design for everyday wear, too.
Back in 2011, urban running clubs were gaining in popularity and the traditional running shoe was growing stale. Nike designed the Free Run+ 2 to flex and move naturally with the foot, and it offered a more sock-like fit, distinctive asymmetrical lacing and decidedly non-traditional design lines.
A great ride supported its good looks, and the shoe quickly transcended the performance running world to become an icon of modern sport style. Later, the City Pack dropped, featuring color schemes for New York, London, Tokyo, Shanghai and Rio, cementing the shoe as a global classic and helping to redefine what a running shoe could be.
This is the epitome of natural performance, wrapped in Flyknit and cushioned with a hex outsole. The new flexible hex design evolves from the classic square-cut Nike Free to bring better multi-directional movement to a runner’s natural stride.
Allowing the foot to move like it’s meant to, the Free 3.0 helps to ensure ultimate natural motion for a better, stronger run. Up top, flexibility meets the ultralight support and contoured fit of Flyknit, creating the most adaptive, natural fit to ever hit the road.
Marking the 10th anniversary of Nike Free, 2014’s Nike Free 5.0 brings everyday flexibility to the people. More supportive and cushioned than the 3.0 or 4.0, the versatile 5.0 shares their new hexagonal outsole—an evolution of the iconic square-cut Nike Free design, bringing better multi-directional movement to a runner’s natural stride.
Up top, an ultra-breathable Flywire-reinforced upper delivers a secure, lightweight and highly adaptive fit. Engineered to move as you’re meant to, the Free 5.0 is the perfect fit for every foot.
press the play button to spin up the zoetrope. scroll to zoom and
click and drag to rotate the camera.


By setting up multiple registration types, you can charge different amounts and ask different questions depending on the type of registration. You can drag and drop these registrant types into the order that people registering will see them.
If blank, full cost will be required at time of registration.
Registrants must login in order to accept multiple payments. Require a login under the Registrant Options tab.
You must accept a payment method in order to set a minimum payment. Setup payment methods under the Payment Options tab.


The professional Sanika staff operating on our sites
are experienced and have undergone comprehensive
training in all waterproofing application methods.
They have full security and medical clearance by
Impala Platinum Refineries, Anglo Platinum Refineries
and many more. Our dedicated and loyal teams apply
their extensive knowledge and skill to each project
and are backed by their site supervisors.
All Sanika staff are covered by Workman’s
Compensation insurance. Consequential damage and
public liability insurance cover on all projects.
Our registered systems and application methods
have already been utilised and approved by senior
Impala Platinum, Anglo American, Investec Property
Services, Spar Group, JHI, Johnson Matthey,
Growthpoint Property Services and Broll Engineering
Management and many more.
STAFF PROFILE
SYSTEMS