X-ray bright points, coronal heating and the solar cycle

Details X-ray bright points, coronal heating and the solar cycle X-ray bright points, coronal heating and the solar cycle

Apr 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975soph...41..381g&link_type=abstract

Solar Physics, vol. 41, Apr. 1975, p. 381-386.

Physics

3

Astronomical Models, Solar Corona, Solar Cycles, Solar Granulation, Solar Magnetic Field, Solar X-Rays, Magnetic Flux, Plasma Heating, Point Sources, Skylab Program, Solar Flux, Solar Heating, Solar Temperature

Scientific paper

Recent Skylab observations about the bright points in the solar X-ray images seem to confirm an essential prediction of a model proposed by this author for the appearance and the disappearance of the photospheric fields during a solar cycle. The segments of the individually rising strands of the 'fundamental flux-loops' proposed in the model may lead to the X-ray bright points with the observed properties. The emergence of such strands may substantially contribute to the coronal heating at different heights.

Affiliated with

Also associated with

No associations

Rating

X-ray bright points, coronal heating and the solar cycle 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 X-ray bright points, coronal heating and the solar cycle, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and X-ray bright points, coronal heating and the solar cycle will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-949158