Plasmaspheric Plumes and EMIC Rising Tone Emissions

0501792 - ÚFA 2019 RIV US eng J - Článek v odborném periodiku
Grison, Benjamin - Hanzelka, Miroslav - Breuillard, H. - Darrouzet, F. - Santolík, Ondřej - Cornilleau-Wehrlin, N. - Dandouras, I.
Plasmaspheric Plumes and EMIC Rising Tone Emissions.
Journal of Geophysical Research-Space Physics. Roč. 123, č. 11 (2018), s. 9443-9452. ISSN 2169-9380. E-ISSN 2169-9402
Grant CEP: GA ČR(CZ) GA18-05285S
Grant ostatní: AV ČR(CZ) AP1401; AV ČR(CZ) JSPS-17-14
Program: Akademická prémie - Praemium Academiae; Bilaterální spolupráce
Institucionální podpora: RVO:68378289
Klíčová slova: statistical - analysis * cluster * waves * magnetosphere * plasma * field
Obor OECD: Fluids and plasma physics (including surface physics)
Impakt faktor: 2.821, rok: 2018
https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2018JA025796

Due to its polar orbit Cluster spacecraft crossed plasmaspheric plumes out of the magnetic equatorial plane. We study the occurrence of broadband, narrowband, and rising tone emissions in the plume vicinity, below the local proton gyrofrequency. Based on a database of 935 Cluster plumes crossings, reduced to 189 unique plumes, we find that broadband activity is the most common case. We confirm result from a previous study showing that plume vicinity is not a preferred place for observing narrowband emissions. Rising tones are the less frequently observed of these three kinds of emissions. Nevertheless, ElectroMagnetic Ion Cyclotron (EMIC) rising tone occurrence rate is high compared to the narrowband one: Tones are seen in six of 30 plume events (20%) when narrowband emissions are observed. Rising tones are observed at absolute magnetic latitudes larger than 17 degrees and up to 35 degrees. We detail the 16 August 2005 plume crossing when a rising tone is observed. Results of a ray tracing analysis agree with a tone triggering process taking place above 15 degrees of magnetic latitude.
Trvalý link: http://hdl.handle.net/11104/0293781