PMO OpenIR  > 期刊(老文献)
WAVE ENERGY-DISSIPATION IN THE SOLAR ATMOSPHERE
ZHOU, AH
1990
Source PublicationIAU SYMPOSIA
ISSN0074-1809
Issue142Pages:266-267
AbstractThere are two regions of rapid dissipation when alfeven waves propagate from the transition region to the corona. They occur respectively in a range of several hundred kilometers above the base of the transition region and in the corona at about 1-3Ro. The heating of the atmosphere by wave dissipation could be one order of magnitude larger than heat conduction in the coronal part with a lower temperature and density and stronger magnetic field. Wave heating could also become more important when the magnetic field divergence becomes stronger.
Subject Area天文和天体物理
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/8586
Collection期刊(老文献)
Recommended Citation
GB/T 7714
ZHOU, AH. WAVE ENERGY-DISSIPATION IN THE SOLAR ATMOSPHERE[J]. IAU SYMPOSIA,1990(142):266-267.
APA ZHOU, AH.(1990).WAVE ENERGY-DISSIPATION IN THE SOLAR ATMOSPHERE.IAU SYMPOSIA(142),266-267.
MLA ZHOU, AH."WAVE ENERGY-DISSIPATION IN THE SOLAR ATMOSPHERE".IAU SYMPOSIA .142(1990):266-267.
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