Solar radio emission at 9.1 CM and sector boundaries

Details Solar radio emission at 9.1 CM and sector boundaries Solar radio emission at 9.1 CM and sector boundaries

Sep 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975soph...44..195g&link_type=abstract

Solar Physics, vol. 44, Sept. 1975, p. 195-204.

Physics

Interplanetary Magnetic Fields, Solar Activity Effects, Solar Corona, Solar Radio Emission, Solar Cycles, Solar Magnetic Field, Statistical Analysis, Sunspots

Scientific paper

A possible connection between solar radio emission from 1.0 to 9.4 GHz and the interplanetary sector boundaries has been previously reported. The present research does not support the previous work as expected. The 9.1-cm activity appears to be organized around sector boundaries only in a very limited sense in that the distribution of very strong active regions peaks near the negative-sector/positive-sector boundaries. However, this phenomenon is only observed during the most active part of the solar cycle. A peculiar asymmetry is found regarding the length of the positive and negative sectors.

Affiliated with

Also associated with

No associations

Rating

Solar radio emission at 9.1 CM and sector boundaries 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 Solar radio emission at 9.1 CM and sector boundaries, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar radio emission at 9.1 CM and sector boundaries will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-912527