Тип публикации: статья из журнала

Год издания: 2017

Идентификатор DOI: 10.1002/2017JA023992

Ключевые слова: solar wind, spherical hybrid model, kinetic hybrid simulation

Аннотация: We present the results of a 1-D global kinetic simulation of the solar wind in spherical coordinates without a magnetic field in the region from the Sun to the Earth's orbit. Protons are considered as particles while electrons are considered as a massless

Журнал: JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS

Выпуск журнала: Vol. 122, Is. 8

Номера страниц: 7854-7864

ISSN журнала: 21699380

Место издания: WASHINGTON

Издатель: AMER GEOPHYSICAL UNION

• Dyadechkin S. (Aalto Univ, Sch Elect Engn, Espoo, Finland; Austrian Acad Sci, Space Res Inst, Graz, Austria)
• Semenov V.S. (St Petersburg State Univ, Earth Phys Dept, St Petersburg, Russia)
• Kallio E. (Aalto Univ, Sch Elect Engn, Espoo, Finland)
• Erkaev N.V. (Russian Acad Sci, Inst Computat Modelling, Siberian Branch, Krasnoyarsk, Russia; Siberian Fed Univ, Dept Appl Mech, Polytech Inst, Krasnoyarsk, Russia)
• Alho M. (Aalto Univ, Sch Elect Engn, Espoo, Finland)
• Lammer H. (Austrian Acad Sci, Space Res Inst, Graz, Austria)

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