Solar radio observations and development of coronal mass ejections
| العنوان: | Solar radio observations and development of coronal mass ejections |
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| المؤلفون: | Ch. Marqué, Dalmiro Maia, Monique Pick |
| المساهمون: | Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Physique solaire, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris |
| المصدر: | Advances in Space Research Advances in Space Research, 2003, 32, pp.467-472. ⟨10.1016/S0273-1177(03)00329-6⟩ |
| بيانات النشر: | Elsevier BV, 2003. |
| سنة النشر: | 2003 |
| مصطلحات موضوعية: | Physics, Atmospheric Science, Astrophysics::High Energy Astrophysical Phenomena, Aerospace Engineering, Astronomy, Astronomy and Astrophysics, Solar radius, Astrophysics, Solar radio, Solar disk, Corona, Imaging data, Geophysics, Space and Planetary Science, Physics::Space Physics, Thermal, Coronal mass ejection, Astrophysics::Solar and Stellar Astrophysics, General Earth and Planetary Sciences, Astrophysics::Earth and Planetary Astrophysics, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Radio imaging |
| الوصف: | We present in this study a synthesis of results on the initiation and development of CMEs using coordinated observations from SOHO and ground-based instruments. The emphasis is placed on radio spectral and imaging data. One important goal of this study is the identification of radio signatures of CMEs providing information below one solar radius above the limb. CMEs can be accompanied by radio emission from thermal or non-thermal origin. Multifrequency radio imaging observations allow us to observe the initial steps of CMEs and to get information on the nature of the triggering mechanisms, on the CME lateral progression above the solar limb as well as above the solar disk. They also reveal the dynamical behavior of CMEs or of the eruptive filament cavity in the low and middle corona and make the link with coronagraphic data. Systematic radio surveys showing the space-time evolution of the emitting sources, like the examples presented in this study, are important tools for synoptic studies. |
| تدمد: | 0273-1177 |
| DOI: | 10.1016/s0273-1177(03)00329-6 |
| DOI: | 10.1016/S0273-1177(03)00329-6⟩ |
| URL الوصول: | https://explore.openaire.eu/search/publication?articleId=doi_dedup___::64737610409187b1b4c3f8d85410f8df https://doi.org/10.1016/s0273-1177(03)00329-6 |
| Rights: | CLOSED |
| رقم الانضمام: | edsair.doi.dedup.....64737610409187b1b4c3f8d85410f8df |
| قاعدة البيانات: | OpenAIRE |
| تدمد: | 02731177 |
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| DOI: | 10.1016/s0273-1177(03)00329-6 |