Some statistical features of solar radio SVC in the rising branch of Cycle 22

Details Some statistical features of solar radio SVC in the rising branch of Cycle 22 Some statistical features of solar radio SVC in the rising branch of Cycle 22

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991acaps..11..283z&link_type=abstract

(Acta Astrophysica Sinica, vol. 11, no. 3, 1991, p. 283-286) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 15, Dec.

Astronomy and Astrophysics

Astrophysics

Solar Activity, Solar Flux, Solar Radio Emission, Frequency Distribution, Radio Scattering, Statistical Analysis

Scientific paper

For the rising branch of Cycle 22, 1987 January-1989 November, the daily total flux S is plotted at each of the five wavelengths 2.0, 3.4, 6.0, 10.7, and 21.2 cm against the apparent sunspot area of the dominant sunspot. It is found that, for several large active areas, the locus is located below the average regression line, and the increase in the radio flux is insignificant compared to the increase in the sunspot area.

Affiliated with

Also associated with

No associations

Rating

Some statistical features of solar radio SVC in the rising branch of Cycle 22 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 Some statistical features of solar radio SVC in the rising branch of Cycle 22, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Some statistical features of solar radio SVC in the rising branch of Cycle 22 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1536346