Time-correlated bursts from widely separated solar active regions at 91.6 centimeter wavelength

Details Time-correlated bursts from widely separated solar active regions at 91.6 centimeter wavelength Time-correlated bursts from widely separated solar active regions at 91.6 centimeter wavelength

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...344l..77l&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 344, Sept. 15, 1989, p. L77-L80.

Other

13

Centimeter Waves, Solar Activity, Solar Magnetic Field, Solar Radio Bursts, Coronal Loops, Solar Flares, Solar X-Rays, Very Large Array (Vla)

Scientific paper

VLA synthesis maps at 20.7 cm wavelength, VLA snapshot maps at 91.6 cm wavelength, and NSO-Kitt Peak photospheric magnetograms indicate that time-correlated radio bursts can occur in active regions on opposite sides of the solar equator. These regions are apparently linked by large-scale, transequatorial magnetic loops that are at least 2.6 x 10 to the 5th km long. Energetic electrons accelerated during a radio burst in one active region probably move along this magnetic conduit at velocities of about one-third the velocity of light, thereby triggering radio bursts in the other active region.

Affiliated with

Also associated with

No associations

Rating

Time-correlated bursts from widely separated solar active regions at 91.6 centimeter wavelength 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 Time-correlated bursts from widely separated solar active regions at 91.6 centimeter wavelength, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Time-correlated bursts from widely separated solar active regions at 91.6 centimeter wavelength will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-761873