gnssrefl.sd_libs module
- gnssrefl.sd_libs.RH_ortho_plot(station, H0, year, th_even, spline_whole_time, txtdir, fs, time_rh, rh, gap_min_val)
Makes a plot of the final spline fit to the data. Output time interval controlled by the user.
- Parameters:
station (str) – name of station, 4 ch
H0 (float) – datum correction (orthometric height) to convert RH to MSL data, in meters
year (int) – year of the time series (ultimately should not be needed)
th_even (numpy of floats) – time in fractional days of of year, I think
spline_whole_time (numpy of floats) – RH values (m)
txtdir (str) – location of plot
fs (int) – fontsize
time_rh (numpy of floats) – time of rh values, in fractional doy I believe
rh (numpy of floats) – refl hgt in meters
gap_min_val (float) – minimum length gap allowed, in day of year units
- gnssrefl.sd_libs.find_ortho_height(station, extension)
find orthometric (sea level) height used in plots
- Parameters:
station (str) – 4 ch station name
extension (str) – gnssir analysis, extension mode
- Returns:
Hortho – orthometric height from gnssir json analysis file. calculates it if not in the file
- Return type:
float
- gnssrefl.sd_libs.mirror_plot(tnew, ynew, spl_x, spl_y, txtdir, station, beginT, endT)
Makes a plot of the spline fit to the mirrored RH data Plot is saved to txtdir as station_rhdot1.png
- Parameters:
tnew (numpy of floats) – time in days of year, including the faked data, used for splines
ynew (numpy of floats) – RH in meters
spl_x (numpy of floats) – time in days of year
spl_y (numpy of floats) – smooth RH, meters
txtdir (str) – directory for plot
station (str) – name of station for title
beginT (float) – first time (day of year) real RH measurement
endT (float) – last time (day of year) for first real RH measurement
- gnssrefl.sd_libs.mjd_to_obstimes(mjd)
takes mjd array and converts to datetime for plotting.
- Parameters:
mjd (numpy array of floats) – mod julian date
- Returns:
dt
- Return type:
numpy array of datetime objects
- gnssrefl.sd_libs.numsats_plot(station, tval, nval, Gval, Rval, Eval, Cval, txtdir, fs, hires_figs)
makes the plot that summarizes the number of satellites in each constellation per epoch
- Parameters:
station (str) – name of the station
tval (numpy array) – datetime objects?
nval (numpy array) – number of total satellites at a given epoch
Gval (numpy array) – number of galileo satellites at an epoch
Rval (numpy array) – number of glonass satellites at an epoch
Eval (numpy array) – number of galileo satellites at an epoch
Cval (numpy array) – number of beidou satellites at an epoch
txtdir (str) – where results are stored
fs (int) – fontsize for the plots
hires_figs (bool) – try to plot high resolution
- gnssrefl.sd_libs.print_badpoints(t, outliersize, txtdir, real_residuals)
prints outliers to a file.
- Parameters:
t (numpy array) – lomb scargle result array of “bad points”. Format given below
outliersize (float) – outlier criterion, in meters
txtdir (str) – directory where file is written
real_residuals (numpy array of floats) – assume this is RH residuals in meters
- Return type:
writes to a file called outliers.txt in the Files/station area
- gnssrefl.sd_libs.quickTr(year, doy, frachours)
takes timing from lomb scargle code (year, doy) and UTC hour (fractional) and returns a date string
- Parameters:
year (int) – full year
doy (int) – day of year
frachours (float) – real-valued UTC hour
- Returns:
datestring – date ala YYYY-MM-DD HH-MM-SS
- Return type:
str
- gnssrefl.sd_libs.rh_plots(otimes, tv, station, txtdir, year, d1, d2, percent99)
overview plots for rh_plot
- Parameters:
otimes (numpy array of datetime objects) – observation times
tv (numpy array) – gnssrefl results written into this variable using loadtxt
station (str) – station name, only used for the title
txtdir (str) – directory where the plots will be written to
year (int) – what year is being analyzed
d1 (int) – minimum day of year
d2 (int) – maximum day of year
percent99 (bool) – whether you want only the 1-99 percentile plotted
- gnssrefl.sd_libs.rhdot_plots(th, correction, rhdot_at_th, tvel, yvel, fs, station, txtdir, hires_figs, year)
makes the rhdot correction plots
- Parameters:
th (numpy array) – time of obs, day of year
correction (numpy array) – rhcorrections in meters
rhdot_at_th (numpy array of floats) – spline fit for rhdot in meters
tvel (numpy array of floats) – time for surface velocity in days of year
yvel (numpy array of floats) – surface velocity in m/hr
fs (integer) – fontsize
station (str) – station name
txtdir (str) – file directory for output
hires_figs (bool) – whether you want eps instead of png
year (int) – calendar year
- gnssrefl.sd_libs.stack_two_more(otimes, tv, ii, jj, stats, station, txtdir, sigma, kplt, hires_figs)
makes a plot of the reflector heights before and after minimal editing
- Parameters:
otimes (numpy array of datetime objects) – observation times
tv (numpy array) – variable with the gnssrefl LSP results
ii (numpy array) – indices of good data
jj (numpy array) – indices of bad data
station (str) – station name
txtdir (str) – directory where plots will be written
sigma (float) – what kind of standard deviation is used for outliers (3sigma, 2.5 sigma etc)
kplt (bool) – make extra plot for kristine
- gnssrefl.sd_libs.subdaily_resids_last_stage(station, year, th, biasCor_rh, spline_at_GPS, fs, strsig, hires_figs, txtdir, ii, jj, th_even, spline_whole_time)
Makes the final residual plot for subdaily (after RHdot and IF correction made). Returns the bad points …
- Parameters:
station (str) – 4 character station name
year (int) – calendar year
th (numpy array of ??) – time variable of some kind, fractional day of year ?
biasCor_rh (numpy array of floats) – refl hgts that have been corrected for RHdot and IF
spline_at_GPS (numpy array of floats) – RH derived From the spline fit and calculated at GPS time tags
fs (int) – font size
strsig (str) – sigma string to go on the legend
hires_figs (bool) – whether to save the plots with better resolution
txtdir (str) – directory where the plot will be saved
ii (numpy array) – indices of the outliers?
jj (numpy array) – indices of the values to keep?
th_even (numpy array) – evenly spaced time values, day of year
spline_whole_time (numpy array of flots) – splinefit for ???
- Returns:
badpoints2 – RH residuals
- Return type:
numpy array of floats
- gnssrefl.sd_libs.testing_nvals(Gval, Rval, Eval, Cval)
writing the number of observations per constellation as a test. not currently used
Parameters Gval: numpy array
GPS RH values
- Rvalnumpy array
GLONASS RH values
- Evalnumpy array
Galileo RH values
- Cvalnumpy
Beidou RH values
writes to a file - kristine.txt returns nothing
- gnssrefl.sd_libs.two_stacked_plots(otimes, tv, station, txtdir, year, d1, d2, hires_figs)
This actually makes three stacked plots - not two, LOL It gives an overview for quality control
- Parameters:
otimes (numpy array of datetime objects) – observations times
tv (numpy array) – gnssrefl results written into this variable using loadtxt
station (str) – station name, only used for the title
txtdir (str) – where the plots will be written to
year (int) – what year is being analyzed
d1 (int) – minimum day of year
d2 (int) – maximum day of year
hires_figs (bool) – true for eps instead of png
- gnssrefl.sd_libs.write_spline_output(splineout, iyear, th, spline, delta_out, station, txtdir, Hortho)
Writing the output of the spline fit to the final RH time series. No output other than this text file.
- Parameters:
splineout (bool) – whether file should be created
iyear (int) – full year
th (numpy array) – time values of some kind … maybe fractional day of years?
spline (fit) – needs doc
delta_out (int) – how often you want the splinefit water level written, in seconds
station (str) – station name
txtdir (str) – output directory
Hortho (float) – orthometric height used to convert RH to something more sea level like meters
- gnssrefl.sd_libs.writejsonfile(ntv, station, outfile)
subdaily RH values written out in json format
This does not appear to be used
- Parameters:
ntv (numpy of floats) – LSP results
station (str) – 4 ch station name
outfile (str) – filename for output
- gnssrefl.sd_libs.writeout_spline_outliers(tvd_bad, txtdir, residual, filename)
Write splinefit outliers to a text file.
- Parameters:
tvd_bad (numpy array) – output of the lomb scargle calculations
txtdir (str) – directory for the output, i.e. $REFL_CODE/FiLes/station
residual (numpy array) – RH outliers in units of meters (!)
filename (str) – name of file being written