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Nonlinear magneto-acoustic waves in the solar atmosphere

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UNSPECIFIED (2001) Nonlinear magneto-acoustic waves in the solar atmosphere. In: 3rd Conference on Mixing in Geophysical and Astrophysical Flows, UNIV SHEFFIELD, SHEFFIELD, ENGLAND, APR 12-14, 2000. Published in: DYNAMICS OF ATMOSPHERES AND OCEANS, 34 (2-4). pp. 399-409. ISSN 0377-0265.

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Abstract

The weakly nonlinear evolution of quasi-isentropic magnetoacoustic waves in the solar atmosphere is analyzed. The plasma is assumed to be initially homogeneous, in thermal equilibrium and with a straight and homogeneous magnetic field frozen in. Additionally, the plasma is assumed to be cooled by the standard cooling function in the range of 10(4) K < T < 10(7) K and heated by a mechanism which is proportional to the density and temperature. The range of temperature where the plasma is isentropically unstable, the e-folding time for thermal instability and the corresponding time and length-scale for wave breaking are found. (C) 2001 Elsevier Science B.V. All rights reserved.

Item Type: Conference Item (UNSPECIFIED)
Subjects: Q Science > QE Geology
Q Science > QC Physics
G Geography. Anthropology. Recreation > GC Oceanography
Journal or Publication Title: DYNAMICS OF ATMOSPHERES AND OCEANS
Publisher: ELSEVIER SCIENCE BV
ISSN: 0377-0265
Official Date: October 2001
Dates:
DateEvent
October 2001UNSPECIFIED
Volume: 34
Number: 2-4
Number of Pages: 11
Page Range: pp. 399-409
Publication Status: Published
Title of Event: 3rd Conference on Mixing in Geophysical and Astrophysical Flows
Location of Event: UNIV SHEFFIELD, SHEFFIELD, ENGLAND
Date(s) of Event: APR 12-14, 2000

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