Magnetic reconnection as a mechanism for heating the persistent coronal loops

Details Magnetic reconnection as a mechanism for heating the persistent coronal loops Magnetic reconnection as a mechanism for heating the persistent coronal loops

Feb 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983pazh....9...48s&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 9, Jan. 1983, p. 48-52) Soviet Astronomy Letters (ISSN 0360-0327), vol. 9, Jan.-Feb. 19

Physics

4

Coronal Loops, Current Sheets, Solar Magnetic Field, Stellar Models, Electrical Resistivity, Solar Physics, Solar Wind, Thermal Conductivity

Scientific paper

A simplified self-consistent model is applied to determine the parameters describing a steady, high-temperature turbulent current sheet subject to a small transverse magnetic field component as well as anomalous electrical and thermal conductivity. Magnetic reconnection in such a sheet might serve as the energy source and drive the plasma flows observed in slow coronal transients, the long-lived loops that persist in the solar corona for tens of hours.

Affiliated with

Also associated with

No associations

Rating

Magnetic reconnection as a mechanism for heating the persistent coronal loops 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 Magnetic reconnection as a mechanism for heating the persistent coronal loops, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Magnetic reconnection as a mechanism for heating the persistent coronal loops will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1307449