Stokes parameters of the O VI 103.2 NM line as a probe of the matter velocity field vector in the solar wind acceleration region

Autor: Sahal-Bréchot, S., Feautrier, N., Bommier, V., de Kertanguy, Amaury

Publikováno v: ESA Workshop on Solar Physics and Astrophysics at Interferometric Resolution (SIMURIS)
ESA Workshop on Solar Physics and Astrophysics at Interferometric Resolution (SIMURIS), Feb 1992, Paris, France. pp.81-85

International audience; A theoretical method to determine the matter velocity field vector in the solar wind acceleration region is presented. The O VI 103.2 nm line should be observed high in the corona in the solar wind acceleration region. Prelimi

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::a0130c2424352e8d483800ca6375acce
https://hal.archives-ouvertes.fr/hal-02393418