The transfer of the solar angular momentum to the interplanetary field by means of the coronal expansion

Details The transfer of the solar angular momentum to the interplanetary field by means of the coronal expansion The transfer of the solar angular momentum to the interplanetary field by means of the coronal expansion

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992chjss..12...89l&link_type=abstract

Chinese Journal of Space Science (ISSN 0254-6124), vol. 12, no. 2, p. 89-94.

Computer Science

Angular Momentum, Interplanetary Magnetic Fields, Momentum Transfer, Solar Corona, Solar Rotation, Comet Tails, Stochastic Processes

Scientific paper

In this paper, the feature of angular momentum in the coronal expansion is discussed. According to the calculation of data on the Type-I cometary tails, the tangential component of coronal expansion is verified; not only does it have a stochastic change, but also it has a confirmed value (9.8 km/s). Since the solar evolution reached to the main sequence stage, the sun lost the 80 pct of its angular momentum, thus the angular velocity of its rotation is reducing by the power index law.

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