Geophysical Research Letters · 2018 · 28 citations · 6 references
Natural SciencesEarth SciencesPhysicsAtmospheric RadiationAtmospheric SciencePlasma PhysicsSolar PhysicsSolar RadiationSpace Weather EffectsEuv EmissionIncoming Solar RadiationSolar Physics ObservationsSolar PlasmasSolar Radiation Penetration
Abstract During the 21 August 2017 eclipse two separate DMSP spacecraft passed through the lunar penumbra at local afternoon (F16) and near local sunset (F17) in the topside ionosphere at an altitude of ~850 km. Measurements of the in situ electron temperature by the Langmuir probe on each spacecraft showed regions where the temperature decreased on the order of 500 to 1,000 K in the shadow. The patterns of these decreases were sporadic inside the shadow but generally showed the same overall shape in both passes. Comparing these patterns of temperature reductions with the projection of the gradient of the solar EUV radiation in the ionosphere suggests that these complex patterns are a result of the nonuniform distribution of the solar EUV radiation on the Sun at the time of the eclipse.
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