A numerical study of the thermal stability of solar loops

Details A numerical study of the thermal stability of solar loops A numerical study of the thermal stability of solar loops

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987nascp2483..113k&link_type=abstract

In NASA-Goddard Space Flight Center, Theoretical Problems in High Resolution Solar Physics, 2 p 113-116 (SEE N88-11609 02-92)

Physics

Coronal Loops, Solar Activity, Solar Wind, Thermal Stability, Chromosphere, Computerized Simulation, Magnetic Flux, Stellar Temperature

Scientific paper

An important property of all loops is their thermal stability. If low lying hot loops were thermally unstable, for example, a great majority of the low loops on the Sun might be expected to be cool. How small perturbations evolve in low lying, linearly unstable hot loops was determined and how high lying, linearly stable hot loops respond to large amplitude disturbances such as might be expected on the Sun were examined. Only general descriptions and results are given.

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