Forecast of solar wind parameters according to STOP magnetograph observations
| Autor: | V. S. Peshcherov, A. Tlatov, M. L. Demidov, D. I. Ponyavin, M. P. Pashchenko, P. M. Svidskii |
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| Rok vydání: | 2016 |
| Předmět: |
Physics
010504 meteorology & atmospheric sciences Meteorology Astrophysics::High Energy Astrophysical Phenomena Interplanetary medium 01 natural sciences law.invention Magnetic field Telescope Solar wind Geophysics Space and Planetary Science law Physics::Space Physics 0103 physical sciences Astrophysics::Solar and Stellar Astrophysics Satellite Astrophysics::Earth and Planetary Astrophysics 010303 astronomy & astrophysics Physics::Atmospheric and Oceanic Physics 0105 earth and related environmental sciences Remote sensing |
| Zdroj: | Geomagnetism and Aeronomy. 56:1095-1103 |
| ISSN: | 1555-645X 0016-7932 |
| DOI: | 10.1134/s0016793216080223 |
| Popis: | The paper discusses the results of the forecast of solar wind parameters at a distance of 1 AU made according to observations made by the STOP telescope magnetograph during 2014–2015. The Wang–Sheeley–Arge (WSA) empirical model is used to reconstruct the magnetic field topology in the solar corona and estimate the solar wind speed in the interplanetary medium. The proposed model is adapted to STOP magnetograph observations. The results of the calculation of solar wind parameters are compared with ACE satellite measurements. It is shown that the use of STOP observations provides a significant correlation of predicted solar wind speed values with the observed ones. |
| Databáze: | OpenAIRE |
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