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 | |||
| ifaYYMMDD_HHMNSS | Full Sun | 17GHz | (R+L) |
| ifsYYMMDD_HHMNSS | (R L) |
||
| ifzYYMMDD_HHMNSS | 34GHz | (R+L) | |
| ipaYYMMDD_HHMNSS | Partial | 17GHz | (R+L) |
| ipsYYMMDD_HHMNSS | (RL) |
||
| ipzYYMMDD_HHMNSS | 34GHz | (R+L) | |
| Event mode | |||
| ifaYYMMDD_HHMNSS.LLL | Full Sun | 17GHz | (R+L) |
| ifsYYMMDD_HHMNSS.LLL | (RL) |
||
| ifzYYMMDD_HHMNSS.LLL | 34GHz | (R+L) | |
| ipaYYMMDD_HHMNSS.LLL | Partial | 17GHz | (R+L) |
| ipsYYMMDD_HHMNSS.LLL | (RL) |
||
| ipzYYMMDD_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... ).