Plasmas in space

 

作者: Herbert S. Bridge,  

 

期刊: Physics Today  (AIP Available online 1963)
卷期: Volume 16, issue 3  

页码: 31-37

 

ISSN:0031-9228

 

年代: 1963

 

DOI:10.1063/1.3050802

 

出版商: AIP

 

数据来源: AIP

 

摘要:

About twenty years ago, the so‐called “infall” theory had been thoroughly worked out by Hoyle and by Alfve´n. They reasoned that, since the sun moves through clouds of interstellar hydrogen gas, the neutral hydrogen must fall in toward the sun under the influence of the gravitational field. On its way toward the surface of the sun, the hydrogen encounters a strong flux of ultraviolet radiation and, because of the small rate of recombination, it becomes completely ionized. Thus the inner solar system is filled with a dilute, highly conducting plasma. At about the same time the infall theory was worked out, it became rather generally accepted that the corona of the sun has a temperature of 1 or 2 million degrees. In fact, Hoyle tried to account for the heating of the corona in terms of the energy released by the hydrogen falling into the sun.

 

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