Electron heat flux in the magnetosheath is shaped by magnetic field draping, increases with field strength, and is limited by whistler instability thresholds.
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eROSITA data from solar minimum enables isolation and removal of solar wind charge exchange foreground emission, yielding a less contaminated diffuse soft X-ray sky and demonstrating X-ray mapping of interstellar matter flow.
Geomagnetic storms during Forbush decreases bias neutron monitor spectra at rigidities as low as 1 GV, and AMS space data can be used to remove these localized anomalies while preserving the main FD signal.
citing papers explorer
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Electron Heat Flux and Whistler Instability in the Earth's Magnetosheath
Electron heat flux in the magnetosheath is shaped by magnetic field draping, increases with field strength, and is limited by whistler instability thresholds.
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Determination of the Solar System contribution to the soft X-ray sky
eROSITA data from solar minimum enables isolation and removal of solar wind charge exchange foreground emission, yielding a less contaminated diffuse soft X-ray sky and demonstrating X-ray mapping of interstellar matter flow.
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Effects of Geomagnetic Cutoff Rigidity Variations during Forbush Decreases
Geomagnetic storms during Forbush decreases bias neutron monitor spectra at rigidities as low as 1 GV, and AMS space data can be used to remove these localized anomalies while preserving the main FD signal.