Open AccessTHEMIS observations of duskside compressional Pc5 waves
Author(s) -
Constantinescu O. D.,
Glassmeier K.H.,
Plaschke F.,
Auster U.,
Angelopoulos V.,
Baumjohann W.,
Fornaçon K.H.,
Georgescu E.,
Larson D.,
Magnes W.,
McFadden J. P.,
Nakamura R.,
Narita Y.
Publication year - 2009
Publication title -
journal of geophysical research: space physics
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.67
H-Index - 298
eISSN - 2156-2202
pISSN - 0148-0227
DOI - 10.1029/2008ja013519
Subject(s) - magnetosphere , physics , geophysics , magnetic field , spacecraft , instability , ionosphere , computational physics , mechanics , astronomy , quantum mechanics
The five Time History of Events and Macroscale Interactions during Substorms (THEMIS) spacecraft offer new possibilities to analyze ULF waves in the magnetosphere by means of multipoint measurements. During the coast phase, THEMIS observed many compressional oscillations with periods in the Pc5 range and longer. The observed events occur inside a well‐defined spatial domain in the outer equatorial duskside magnetosphere. We analyze these waves using the unique string‐of‐pearls configuration of the THEMIS constellation to evaluate their phase speed and propagation direction. We find that the waves are propagating sunward (westward) and radially outward, orthogonal to the mean magnetic field, with phase speeds around 30 km/s and higher in the spacecraft frame. In the plasma frame the propagation direction is still sunward, with lower speeds (up to 30 km/s for most events). The oscillations exhibit a strong anticorrelation between the magnetic field and the plasma density. On the basis of this, as well as their low propagation speed, orthogonal to the mean magnetic field propagation direction and almost parallel to the magnetic field maximum variance direction, we conclude that the most likely source of these waves is the drift mirror instability.