On spicules and the stability analysis of the minimum flux corona theory

Details On spicules and the stability analysis of the minimum flux corona theory On spicules and the stability analysis of the minimum flux corona theory

Dec 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979soph...64..229v&link_type=abstract

Solar Physics, vol. 64, Dec. 1979, p. 229-236. Research supported by the Nederlandse Organisatie voor Zuiver-Wetenschappelijk On

Physics

6

Atmospheric Heating, Chromosphere, Dynamic Stability, Solar Corona, Atmospheric Models, Energy Dissipation, Heat Balance, Radiative Heat Transfer

Scientific paper

It is shown that the stability analysis of coronae envisaged by Hearn (1975, 1979) does not lead to a unique stable configuration. The chromosphere-corona transition region is inevitably nonsteady. Spicules are a manifestation of this. It is suggested that a point to point analysis of energy losses and gains, rather than a stability analysis, can determine the coronal parameters.

Affiliated with

Also associated with

No associations

Rating

On spicules and the stability analysis of the minimum flux corona theory 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 On spicules and the stability analysis of the minimum flux corona theory, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On spicules and the stability analysis of the minimum flux corona theory will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1450267