Physics – Plasma Physics
Scientific paper
Jan 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...241..197s&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 241, no. 1, Jan. 1991, p. 197-202. Research supported by ASI, Ministero dell'U
Physics
Plasma Physics
113
Scale Effect, Solar Flares, Stellar Flares, Chemical Composition, Plasma Density, Plasma Physics, Pressure Effects, Solar Corona, Stellar Models, Stellar Structure, Temperature Effects
Scientific paper
A simple analytical approximate solution for the hydrodynamic equations describing the decay of a flaring loop is derived. It is found that, independent of chemical composition of the plasma, the entropy per particle at the top of the loop undergoes an initial phase of linear decay, with a slope related to the initial loop conditions. The characteristic decay time is shorter than conductive or radiative times for typical solar flare conditions. The analytical solution is compared with numerical solutions of the full set of hydrodynamic equations for loop flares, and it is shown that its validity extends over a large fraction of the decay. Also the decay times of temperature, density and pressure are related to the entropy decay time.
Jakimiec Jerzy
Reale Fabio
Serio Salvatore
Sylwester Barbara
Sylwester Janusz
No associations
LandOfFree
Dynamics of flaring loops. I - Thermodynamic decay scaling laws 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 Dynamics of flaring loops. I - Thermodynamic decay scaling laws, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dynamics of flaring loops. I - Thermodynamic decay scaling laws will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1894582