Evolutino of Coronal mm-Wave Sources

Details Evolutino of Coronal mm-Wave Sources Evolutino of Coronal mm-Wave Sources

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994kofu.symp..259k&link_type=abstract

In: Proceedings of Kofu Symposium, Kofu, Japan, Sept. 6-10, 1993, p.259-262.

Physics

1

Scientific paper

Coronal mm-wave emission at source heights up to the order 100 000 km above the photosphere are sporadically observed as off-limb sources by radio telescopes of medium angular resolution. Previous work showed that coronal mm-wave sources (CMMS) fall into different categories, e.g., explosive burst emission, post- and interflare radiation, and radiation from prominences. The source heights can be checked in the case of behind-limb sources. Systematic knowledge on the evolution of CMMS is still lacking. The present report discusses some general properties of CMMS and considers new observations from the Metsahovi Radio Research Station at 37 GHz of the year 1992 with respect to the effect of temporal evolution.

Affiliated with

Also associated with

No associations

Rating

Evolutino of Coronal mm-Wave Sources 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 Evolutino of Coronal mm-Wave Sources, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Evolutino of Coronal mm-Wave Sources will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-821390