Observations of EMIC waves in the distant cusp region and in the nearby magnetosheath

0442502 - ÚFA 2015 US eng A - Abstrakt
Grison, Benjamin - Escoubet, C. P. - Santolík, Ondřej - Lavraud, B. - Cornilleau-Wehrlin, N.
Observations of EMIC waves in the distant cusp region and in the nearby magnetosheath.
AGU Fall Meeting. s. l: American Geophysical Union, 2014. SM13F-4220.
[AGU Fall Meeting. 15.12.2014-19.12.2014, San Francisco]
Institucionální podpora: RVO:68378289
https://agu.confex.com/agu/fm14/meetingapp.cgi#Paper/15996

In the early years (2000-2004) of the mission, Cluster crossed the most distant part of the polar cusps. On 05/01/2002, Cluster enters the distant cusp region on the duskside of the southern hemisphere (inbound). The spacecraft are successively crossing the magnetopause between 19:50 UT (SC4) and 20:15 UT (SC3). The interplanetary conditions during the crossing were stable with a dominant negative By. The magnetometer (FGM) data indicates that the entry into the cusp takes place in a region where the magnetic field lines in the magnetosheath are anti-parallel with the field lines in the magnetosphere. Despite this clear picture, the global encounter is rather complex: one can notice partial magnetopause crossings, magnetic null points, and intense monochromatic waves on both sides of the magnetopause. We investigate electromagnetic ion cyclotron (EMIC) waves observed in the cusp and in the nearby magnetosheath, just before the magnetopause crossing by the spacecraft. Left-handed monochromatic waves observed in the cusp display different duration and frequency (below and above the local proton gyrofrequency) on each spacecraft. Both the Poynting flux of these emissions and the simultaneously recorded ion flows propagate in the same direction - toward the Earth. The wavenumber are determined in two ways: considering the Doppler shift and from direct measurements of the refractive index. We analyze these wave parameters and the local plasma conditions to explain the wave generation process on each side of the magnetopause.
Trvalý link: http://hdl.handle.net/11104/0245312