Physics
Scientific paper
Jan 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985nascp2358..125h&link_type=abstract
In NASA. Goddard Space Flight Center The Origin of Nonradiative Heating/Momentum in Hot Stars p 125-129 (SEE N85-17755 08-88)
Physics
Plasma Temperature, Stellar Coronas, Stellar Temperature, Chromosphere, Heat Balance, Stellar Models, Stellar Winds
Scientific paper
The physics of compact, hydrostatic coronal shells formed from the collapse of overheated coronae is addressed. A large number of hydrostatic shells was computed for the usual exponential heating law with constant damping length. The boundary conditions were that on both sides of a shell the conductive flux at chromospheric temperatures is small. The boundary value problem was solved with a shooting technique. The main goal of the calculations was to determine the dependence of the shells on coronal heating flux (FMo) and damping length (L); and in particular, to localize the boundary line in the parameter space (FMo, L) that separates normal extended coronae from coronal shells.
No associations
LandOfFree
Overheated open coronal regions 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 Overheated open coronal regions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Overheated open coronal regions will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-927317