[Date Prev][Date Next][Thread Prev][Thread Next][Date Index][Thread Index]
PIMA 2.13 release
Dear colleagues,
New PIMA version was released. Here is the changelog:
2014.09.18 PIMA 2.13
Added a rudimentary interface to atmosphere opacity
and atmosphere brightness temperature computed from the
output of numerical weather models with software SPD
(Slant Path Delay) http://astrogeo.org/spd.
At the moment, PIMA has an ability to plot atmosphere
opacity and sky brightness temperature.
a) Added new task opag (OPAcity Generation).
Requires spd package installed!
Has keyword atmo_dir that requires the value:
name of the directory with the state of the
atmosphere from numerical weather model in
HEB format. It computes the series of atmosphere
opacity and antenna brightness temperatures
for all stations participated in the VLBI experiment
and time epochs within the time range of the session.
PIMA prepares the control file for SPD and launches
that program which makes all the work.
b) Added new task opal (OPAcity Loading). This task
loads into PIMA internal data structure the output
of computation of SPD that was generated by task opag.
c) Extended task tspl (TSys PLot). Now it accepts keyword
data that has one of the following values:
measured, nwm, and opacity.
When value measured is specified, measured system
temperature is displayed.
When value nwm is specified, atmosphere brightness temperature
computed with SPD using the output of numerical weather
models is displayed. It is assumed that brightness temperature
was loaded to PIMA data structures with task opal.
When value opacity is specified, atmosphere opacity
computed with SPD using the output of numerical weather
models is displayed. It is assumed that brightness temperature
was loaded to PIMA data structures with task opal.
d) PIMA has a new dependency: package spd_client. The tar-ball
can be downloaded from http://astrogeo.org/spd
Have nice fringes,
Leonid
2014.09.18_23:41:21
Archive of PIMA project forum
Message 00005