Ground based solar radio observations during solar maximum mission

Details Ground based solar radio observations during solar maximum mission Ground based solar radio observations during solar maximum mission

Mar 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983stin...8320887k&link_type=abstract

Final Report Maryland Univ., College Park. Astronomy Program.

Astronomy and Astrophysics

Astronomy

Bipolarity, Coronal Loops, Mapping, Radio Telescopes, Ring Structures, Solar Flares, Solar Radio Bursts, Electron Radiation, Interferometers, Luminous Intensity, Mathematical Models, Microwaves, Solar Maximum Mission, Spectroheliographs, Very Large Array (Vla), X Rays

Scientific paper

The Very Large Array (VLA) and the Westerbork Synthesis Radio Telescope (WSRT) were used for making aperture synthesis maps of solar active and flaring regions. Observations of the Flare buildup in the form of increased intensity and polarization were made. Ring structure associated with sunspots were interpreted as due to the existence of cool material above the spot. Model computations were performed to explain the total intensity and polarization structures of a continuous set of active region maps.

Affiliated with

Also associated with

No associations

Rating

Ground based solar radio observations during solar maximum mission 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 Ground based solar radio observations during solar maximum mission, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Ground based solar radio observations during solar maximum mission will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1471144