Physics
Scientific paper
May 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990jgr....95.6247o&link_type=abstract
Journal of Geophysical Research (ISSN 0148-0227), vol. 95, May 1, 1990, p. 6247-6262.
Physics
2
Centimeter Waves, Solar Flux, Solar Radio Emission, Sunspots, Ultrahigh Frequencies, Solar Cycles, Visible Spectrum
Scientific paper
Results are presented on a detailed statistical analysis of F10.7 emission and its relation to such manifestations of optical activity as evidenced by plages and sunspots. Results show that all individual peaks of F10.7 emission found in the selected east-west (EW) scans could be attributed to individual active regions (ARs). The correlation of the height of the F10.7 peaks with the individual spot area was 0.93. The correlation with the plage area was 0.84, and the combination of plage and spot areas gave a 0.96 correlation. No significant center-to-limb variation of the F10.7 emission from ARs was found, indicating that the source of the F10.7 emission can be modeled as an optically thin spherical emitting region.
No associations
LandOfFree
Reconstructing the emission at 10.7 cm from individual active regions in terms of optical data does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Reconstructing the emission at 10.7 cm from individual active regions in terms of optical data, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Reconstructing the emission at 10.7 cm from individual active regions in terms of optical data will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-782379