Visibility of Type III burst source location as inferred from stereoscopic space observations
We study solar Type III radio bursts simultaneously observed by RPWS/Cassini, URAP/Ulysses and WAVES/Wind experiments. The observations allows us to cover a large frequency bandwidth from 16 MHz down to a few kHz. We consider the onset time of each burst, and estimate the corresponding intensity lev...
| Main Authors: | , , , |
|---|---|
| Format: | Article |
| Language: | deu |
| Published: |
Copernicus Publications
2014-11-01
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| Series: | Advances in Radio Science |
| Online Access: | http://www.adv-radio-sci.net/12/167/2014/ars-12-167-2014.pdf |