Theoretical studies on physical processes of emerging flux in the solar atmosphere

Details Theoretical studies on physical processes of emerging flux in the solar atmosphere Theoretical studies on physical processes of emerging flux in the solar atmosphere

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003asthe..96..474m&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 96, No. 9, p. 474 - 481 (2003)

Astronomy and Astrophysics

Astronomy

1

Solar Atmosphere, Emerging Flux

Scientific paper

We have studied physical processes of emerging flux in the solar atmosphere by using MHD numerical simulations. It is found that: (1) Depending on the initial state of the emerging flux, several characteristic magnetic structures, (e.g., the helical structure as a seed of prominence, and the sigmoid structure observed in soft X-rays) are formed in the corona; (2) Coronal jets are produced by chromospheric evaporation as the result of magnetic reconnection between emerging flux and pre-existing overlying magnetic fields; and (3) Our scaling-law on mass of such coronal jets explains their density very well.

Affiliated with

Also associated with

No associations

Rating

Theoretical studies on physical processes of emerging flux in the solar atmosphere 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 Theoretical studies on physical processes of emerging flux in the solar atmosphere, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Theoretical studies on physical processes of emerging flux in the solar atmosphere will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1151532