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R. G. Gomez

Publications and source records attributed to R. G. Gomez.

2 recordsLinked to original sources

Simultaneous TRACERS and THEMIS Observations of Reversed Cusp Ion Dispersions and Dual-Lobe Reconnection

We present observations from two consecutive TRACERS-2 orbits through the northern low-altitude cusp. During the first crossing, TRACERS-2 observed reversed cusp ion dispersion and sunward convection, consistent with magnetopause reconnection tailward of the cusp during this northward IMF interval. Simultaneous THEMIS-D observations at the equatorial magnetopause show heated magnetosheath plasma captured on closed field lines, with similar particle spectra as in in the low-altitude cusp, indicating that reconnection indeed occurred tailward of the cusp and in both hemispheres. When TRACERS-2 traversed the northern cusp again, 95 minutes later, the IMF was dominated by a negative BX component. Despite the different IMF conditions, TRACERS-2 recorded nearly the same cusp signatures as before, i.e., reversed ion dispersion and sunward convection. The observations indicate that tailward-of-cusp reconnection can occur for both northward and BX-dominated IMF and that these distinct IMF geometries can produce remarkably similar plasma and field signatures in the low-altitude cusp.

physics.space-ph

Atomic and Molecular Nitrogen Ions at the Dayside Magnetopause During the 2024 Mother's Day Storm

Ion measurements made with the Hot Plasma Composition Analyzers of the Magnetospheric Multiscale Mission (MMS-HPCAs) during the Mother's Day Storm (Gannon Storm) of 10-13 May 2024 yield the first observations of atomic and molecular nitrogen ions in the Earth's dayside outer magnetosphere. A population of ions identified as doubly charged nitrogen and oxygen was also measured. These observations were made within a highly compressed magnetosphere at a geocentric distance of ~6 Earth Radii during the early recovery phase of the storm. From the ion composition measurements and accompanying magnetic field data, we determine the reconnection rate at the magnetopause; we compare this result to a model reconnection rate that assumes the presence of only atomic oxygen and hydrogen. The heavy ion-laden-mass density in the magnetosphere was greater than the shocked solar wind mass density in the magnetosheath. Despite these conditions, magnetic reconnection still occurred at the magnetopause.

physics.space-ph