An approximation of the height of the O+ - H+ transition level for use in IRI
- 1 January 1984
- journal article
- Published by Elsevier in Advances In Space Research
- Vol. 4 (1) , 119-121
- https://doi.org/10.1016/0273-1177(84)90483-6
Abstract
No abstract availableKeywords
This publication has 2 references indexed in Scilit:
- The behavior of the O+‐H+ transition level at solar maximumJournal of Geophysical Research, 1980
- Flapping motions of the tail plasma sheet induced by the interplanetary magnetic field variationsPlanetary and Space Science, 1976