Some already-calibrated NoRP data are put in the NRO solar archive
(see section A).
You can obtain them by anonymous FTP. Before synthesizing
by yourself, try them first.
They are loaded into the IDL session by using the IDL command
restore.
There are 1-sec resolution data for steady observatin and
0.1-sec resolution data for events.
IDL> file=getenv('NORP_XDR')+'/1999/08/norp19990828_0056.xdr' 
CR
IDL> restore,file CR
IDL> help CR
DAY STRING = '1999-08-28' FI FLOAT = Array[7, 7590] FIAVG FLOAT = Array[7] FREQ FLOAT = Array[7] FV FLOAT = Array[7, 7590] FVAVG FLOAT = Array[7] MVD BYTE = Array[7, 7590] TIM STRUCT = -> ANYTIM2INTS Array[7590] |
freq is observing frequencies in units of GHz
(in this example, 1, 2, 3.75, 9.4, 17, 3, 80 GHz), tim is
observing time, fi,fv are I (R+L), V (R-L)
comonents of flux density and fiavg, fvavg are daily average,
respectively. mvd is an array including the values of unity (1) for
valid data or zero (0) for non-valid data.