FITS format files that contain the NoRH images. See Appendix B for the detailed description for the FITS headers, The unit of intensity in the image is brightness temperature in Kelvin.
File name
Steady mode | |||
ifa YYMMDD_ HHMNSS | Full Sun | 17GHz | (R+L) |
ifs YYMMDD_ HHMNSS | (RL) | ||
ifz YYMMDD_ HHMNSS | 34GHz | (R+L) | |
ipa YYMMDD_ HHMNSS | Partial | 17GHz | (R+L) |
ips YYMMDD_ HHMNSS | (RL) | ||
ipz YYMMDD_ HHMNSS | 34GHz | (R+L) | |
Event mode | |||
ifa YYMMDD_ HHMNSS.LLL | Full Sun | 17GHz | (R+L) |
ifs YYMMDD_ HHMNSS.LLL | (RL) | ||
ifz YYMMDD_ HHMNSS.LLL | 34GHz | (R+L) | |
ipa YYMMDD_ HHMNSS.LLL | Partial | 17GHz | (R+L) |
ips YYMMDD_ HHMNSS.LLL | (RL) | ||
ipz YYMMDD_ HHMNSS.LLL | 34GHz | (R+L) |
Example
ifa981123_020533
Full-Sun, 17GHz, R+L, Steady 1998-11-23 2:5:33 UT
ipz981123_020533.824
Partial, 34GHz, R+L, Event 1998-11-23 2:5:33.824 UT
Directory
Anywhere. We have daily images, 10min-interval images, event images (maximum averaged correlation 1.5%) under images in NoRH archive. The synthesis of a raw data file ( e.g., ss17... ) results in these image files (e.g. ifa... and ifs... ).