Survey of current situation in radiation belt modeling.
The study of Earth's radiation belts is one of the oldest subjects in space physics. Despite the tremendous progress made in the last four decades, we still lack a complete understanding of the radiation belts in terms of their configurations, dynamics, and detailed physical accounts of their sources and sinks. The static nature of early empirical trapped radiation models, for examples, the NASA AP-8 and AE-8 models, renders those models inappropriate for predicting short-term radiation belt behaviors associated with geomagnetic storms and substorms. Due to incomplete data coverage, these models are also inaccurate at low altitudes (e.g., <1000 km) where many robotic and human space flights occur. The availability of radiation data from modern space missions and advancement in physical modeling and data management techniques have now allowed the development of new empirical and physical radiation belt models. In this paper, we will review the status of modern radiation belt modeling.
Fung
Shing F
SF
Space Physics Data Facility, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA. shing.fung@gsfc.nasa.gov
D001272:Atmosphere; D002138:Calibration; D003359:Cosmic Radiation; D005118:Extraterrestrial Environment; D008280:Magnetics; D008962:Models, Theoretical; D011522:Protons; D011829:Radiation Dosage; D011834:Radiation Monitoring; D011874:Radiometry
D011522:Protons