pyart.correct#
Description
Radar Corrections (pyart.correct)#
Correct radar fields.
Velocity unfolding#
|
Dealias Doppler velocities using the 4DD algorithm. |
|
Dealias Doppler velocities using multi-dimensional phase unwrapping. |
|
Dealias Doppler velocities using a region based algorithm. |
Attenuation#
calculate_attenuation calculate_attenuation_zphi calculate_attenuation_philinear
Phase processing#
|
Phase process using a LP method [1]. |
|
Phase process using a LP method [1] using Py-ART's Gatefilter. |
|
Public method Alternative determination of the system phase. |
|
correction of the system offset. |
|
correction of the system offset and smoothing using one window |
|
correction of the system offset and smoothing using two window |
Other corrections#
sun_retrieval get_sun_hits get_sun_hits_psr get_sun_hits_ivic correct_vpr correct_vpr_spatialised despeckle_field correct_noise_rhohv correct_bias correct_visibility est_rhohv_rain est_zdr_precip est_zdr_snow selfconsistency_bias selfconsistency_bias2 selfconsistency_kdp_phidp
Helper functions#
|
Find objects (i.e., contiguous gates) in one or more sweeps that match thresholds. |
|
Constructs a mask to mask data placed thickness m below data at min_temp and beyond. |
|
computes the theoretical sun power detected at the antenna [dBm] as it would be without atmospheric attenuation (sun power at top of the atmosphere) for a given solar flux and radar characteristics |
|
Converts the sun power at the top of the atmosphere (in dBm) into solar flux. |
|
Given the observed solar flux at 10.7 cm wavelength, returns the solar flux at the given radar wavelength |
|
Given the antenna beam width and the integration angle, compute the losses due to the fact that the sun is not a point target and the antenna is scanning |
|
smoothes the data using a rolling window. |
|
obtains the sun position in antenna coordinates using the pysolar library. |
|
Calculate the sun position for the given time (dt) at the given position (lat, lon). |
|
Computes the apparent VPR |
|
Computes an idealized vertical profile of reflectivity |
Classes
|
A class for building a boolean arrays for filtering gates based on a set of condition typically based on the values in the radar fields. |
Functions
|
Calculate the attenuation from a polarimetric radar using Z-PHI method. |
|
Calculate the attenuation and the differential attenuation from a polarimetric radar using linear dependece with PhiDP. |
|
Calculate the attenuation and the differential attenuation from a polarimetric radar using Z-PHI method. |
|
Computes the apparent VPR |
|
Computes an idealized vertical profile of reflectivity |
|
Corrects a radar data bias. |
|
Corrects RhoHV for noise according to eq. |
|
correction of the system offset. |
|
Corrects the reflectivity according to visibility. |
|
Correct VPR using the Meteo-France operational algorithm |
|
Correct VPR using a spatialised version of the Meteo-France operational algorithm |
|
Dealias Doppler velocities using the 4DD algorithm. |
|
Dealias Doppler velocities using a region based algorithm. |
|
Dealias Doppler velocities using multi-dimensional phase unwrapping. |
|
Despeckle a radar volume by identifying small objects in each scan and masking them out. |
|
Public method Alternative determination of the system phase. |
|
Estimates the quantiles of RhoHV in rain for each sweep |
|
Filters out all undesired data to be able to estimate ZDR bias, either in moderate rain or from vertically pointing scans |
|
Filters out all undesired data to be able to estimate ZDR bias in snow |
|
Find objects (i.e., contiguous gates) in one or more sweeps that match thresholds. |
|
estimates a gaussian fit of sun hits data |
|
Constructs a mask to mask data placed thickness m below data at min_temp and beyond. |
|
get data from suspected sun hits. |
|
get data from suspected sun hits. |
|
get data from suspected sun hits. |
|
Create a filter which removes undesired gates based on moments. |
|
Phase process using a LP method [1]. |
|
Phase process using a LP method [1] using Py-ART's Gatefilter. |
|
Converts the sun power at the top of the atmosphere (in dBm) into solar flux. |
|
computes the physical parameters of the sun retrieval from the results of a Gaussian fit. |
|
Given the antenna beam width and the integration angle, compute the losses due to the fact that the sun is not a point target and the antenna is scanning |
|
Estimates reflectivity bias at each ray using the self-consistency algorithm by Gourley |
|
Estimates reflectivity bias at each ray using the self-consistency algorithm by Gourley |
|
Estimates KDP and PhiDP in rain from Zh and ZDR using a selfconsistency relation between ZDR, Zh and KDP. |
|
smoothes the data using a rolling window. |
|
correction of the system offset and smoothing using two window |
|
correction of the system offset and smoothing using one window |
|
Given the observed solar flux at 10.7 cm wavelength, returns the solar flux at the given radar wavelength |
|
Calculate the sun position for the given time (dt) at the given position (lat, lon). |
|
obtains the sun position in antenna coordinates using the pysolar library. |
|
computes the theoretical sun power detected at the antenna [dBm] as it would be without atmospheric attenuation (sun power at top of the atmosphere) for a given solar flux and radar characteristics |
|
Estimates sun parameters from sun hits |