Observation of Energetic Particles at Very Low Altitudes near the Geomagnetic Equator
Dieter Hovestadt, B. Häusler, Manfred Scholer
Abstract
Dieter Hovestadt, B. Häusler, Manfred Scholer
Abstract
A considerable flux on the order of 7 particles/${\mathrm{cm}}^{2}$ sec sr (probably protons) in the energy range above 500 keV is observed in the vicinity of the magnetic equator. The particles show a narrow distribution around 90\ifmmode^\circ\else\textdegree\fi{} pitch angle. The low minimum altitudes of the drift paths of the particles in the $L$ region between 1.0 and 1.15 prevent a full drift around Earth. The particles are probably injected at several hundred kilometers altitude by a yet unknown mechanism.
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A considerable flux on the order of 7 particles/${\mathrm{cm}}^{2}$ sec sr (probably protons) in the energy range above 500 keV is observed in the vicinity of the magnetic equator. The particles show a narrow distribution around 90\ifmmode^\circ\else\textdegree\fi{} pitch angle. The low minimum altitudes of the drift paths of the particles in the $L$ region between 1.0 and 1.15 prevent a full drift around Earth. The particles are probably injected at several hundred kilometers altitude by a yet unknown mechanism.
Key concepts: Equator, Earth's magnetic field, Physics, Magnetic dip, Altitude (triangle), Range (aeronautics), Flux (metallurgy), Pitch angle