Simulating the Earth's Outer Radiation Belt Electron Fluxes and Their Upper Limit: A Unified Physics‐Based Model Driven by the AL Index
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Measurement of relative emission rates of auroral systems
The importance of some of the features observed among the nighttime equatorial data of Explorer 31 is discussed with respect to the nighttime thermal structure of the topside ionosphere. The very short-lived photoelectrons being absent, the nighttime measurements represent the background flux due to magnetospheric particles.
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Many features of Herbig-Haro objects can be reproduced using a kinematical bow shock model.
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