LANL* V1.0: a radiation belt drift shell model suitable for real-time and reanalysis applications
We describe here a new method for calculating the magnetic drift invariant, <i>L*</i>, that is used for modeling radiation belt dynamics and for other space weather applications. <i>L*</i> (pronounced L-star) is directly proportional to the int...
| Main Authors: | , , |
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| Format: | Article |
| Language: | English |
| Published: |
Copernicus Publications
2009-07-01
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| Series: | Geoscientific Model Development |
| Online Access: | http://www.geosci-model-dev.net/2/113/2009/gmd-2-113-2009.pdf |