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TRICE 2 Observations of Low‐Energy Magnetospheric Ions Within the Cusp
Author(s) -
Sawyer R. P.,
Fuselier S. A.,
Kletzing C. A.,
Bonnell J. W.,
Roglans R.,
Bounds S. R.,
Kim M. J.,
Vines S. K.,
Cairns I. H.,
Moser C.,
LaBelle J.,
Moen J. I.,
Trattner K. J.,
Petrinec S. M.,
Burch J. L.,
Giles B. L.,
George D.
Publication year - 2021
Publication title -
journal of geophysical research: space physics
Language(s) - English
Resource type - Journals
eISSN - 2169-9402
pISSN - 2169-9380
DOI - 10.1029/2021ja029382
Subject(s) - magnetosheath , magnetosphere , physics , magnetopause , cusp (singularity) , pitch angle , geophysics , population , ion , field line , ionosphere , sounding rocket , solar wind , computational physics , plasma , astronomy , geometry , quantum mechanics , demography , sociology , mathematics
On December 08, 2018 the Twin Rocket Investigation of Cusp Electrodynamics 2 (TRICE 2) mission was successfully launched. The mission consisted of two sounding rockets, each carrying a payload capable of measuring electron and ion distributions, electric and magnetic fields, and plasma waves occurring in the northern magnetospheric cusp. This study highlights the ion and wave observations obtained by TRICE 2 in the cusp and observations from the magnetospheric multiscale (MMS) spacecraft at the low‐latitude magnetopause two hours prior to the TRICE 2 traversal of the cusp. Within the cusp, typical ion cusp features were observed, that is, energy‐latitude dispersion of injected magnetosheath plasma. However, a lower energy population was also measured near the equatorward edge of the cusp on open field lines. Pitch‐angle distributions of the low‐energy ions suggest that this population was magnetospheric in origin, and not from ionospheric upflows. Data from MMS show that counterstreaming ions were present in the outer magnetosphere and low‐latitude boundary layer at similar energies to those observed by TRICE 2 in the cusp. Correlations between the low‐energy ions within the cusp and broadband extremely low frequency waves suggest that the low‐energy magnetospheric ions that filled the flux tube may have undergone wave‐particle interactions. These interactions may cause pitch‐angle scattering of low‐energy magnetospheric ions closer to the loss cone, thereby allowing them to precipitate into the cusp and be measured by the TRICE 2 sounding rockets.