A comparison of type III solar radio burst theories using satellite radio observations and particle measurements |
| |
| Authors: | Larry G Evans Joseph Fainberg R G Stone |
| |
| Institution: | (1) Radio Astronomy Branch, Laboratory for Extraterrestrial Physics, NASA-Goddard Space Flight Center, Greenbelt, Md., U.S.A. |
| |
| Abstract: | The required electron density to excite a type III solar burst can be predicted from different theories, using the low frequency radio observations of the RAE-1 satellite. Electron flux measurements by satellite in the vicinity of 1 AU then give an independent means of comparing these predicted exciter electron densities to the measured density. On this basis, one theory predicts the electron density in closest agreement with the measured values.NAS/NRC Postdoctoral Resident Research Associate. |
| |
| Keywords: | |
| 本文献已被 SpringerLink 等数据库收录！ |
|
