feb23
listing file |
fileSize |
#file entries |
Notes |
NAS_arun_listing_nz | 832MB | 8278688 |
|
listing file |
fileSize |
#file entries |
Notes |
atm |
|||
atm.flist -->large file |
61MB |
669,690 |
all file that include ./tnnnn_ .shs files, gio ri files, atmspectra from plasma line processing does not include the hf files. Large file..clicking to display can take a long time. better to right click and download. |
atmshs.flist |
1.4MB |
15133 |
echotek files. all files in
NAS_arun.. ending in .shs (includes /hfxxx files) |
atmgio.flist |
90KB |
1391 |
ri files written via gio. Mostly the ion
line data. (leftout: substorm_21sep2005.nnn.. 14 files) |
atmspc.flist -->large file |
59MB |
653,624 |
the .hdr,.dcd files holding the plasma
line spectra.
Large file..clicking to display can take a long time.
better to right click and download. |
HF |
|||
hf.flist |
8.8MB |
101,662 |
|
Arun used a prefix subdir name for all
data sent to tacc.
The table below lists these names with a link to a file
containing a list of all file names in this group (be careful, some links point to very
large files).
file prefix |
# of files |
Size in MBytes |
AO327 | 85 | 0.004 |
AODATA | 18733 | 0.960 |
AOPULS | 658 | 0.038 |
AOUSRP | 120138 | 5.499 |
CLPSPEC | 283608 | 13.778 |
ECHOTEK | 5162 | 0.232 |
GALFACTS | 1847875 | 101.631 |
GALFAHI | 59225 | 2.673 |
MOCKSPEC0 | 603894 | 29.100 |
MOCKSPEC1 | 1151902 | 55.712 |
P2722 | 560 | 0.036 |
P3218 | 95 | 0.004 |
PALFA | 45552 | 2.683 |
PUPPI | 7182 | 0.414 |
Planetary | 2908759 | 192.271 |
S3043 | 927 | 0.043 |
S3453 | 54262 | 3.662 |
USRP | 294410 | 19.373 |
USRPRAW | 244583 | 12.072 |
VLBI | 130 | 0.004 |
WAPPDATA | 34492 | 1.578 |
ao | 68189 | 6.099 |
arun | 8279 | 0.486 |
clp | 471668 | 20.752 |
p3184 | 509 | 0.023 |
processing: /share/s3453g1/keysha/Arun_files/phil/doit.pro
Fits source |
used for |
mock spectral line fits files |
regular spectral line observing with the
mock spectrometer.
|
mock psrfits files |
pulsar observing with the mock
spectrometer
|
puppi files |
pulsar observing with puppi backend.
puppi uses 8 gpu's. Each processes 100 MHz
bandwidth.
|
wapp spectral line |
spectral line observing with the wapp
backend. (I think the wapp pulsar observing is not a
fits file). |
galfa HI files |
the galfa backend was used for galactic
Hi surveys. It generated its own fits file. |
galfa cubes |
these are data cubes in fits file format
generated offline. I noticed that these have normally
been compressed (so they don't end in .fits.) |
misc fits formats |
radar processing generated fits files
offline to store some of the generated maps. |
fitsType |
# projects |
Notes |
galfa |
24 |
|
galfacube |
1 |
|
puppi (no gpu
in name) |
19 |
|
puppi (with gpu) |
8 |
|
wapp |
183 |
|
mock |
140 |
|
planetary |
684 |
|
processing: /share/s3453g1/keysha/Arun_files/phil/dofits.pro