The effects of scattering and refraction on radio waves in the solar corona are considered for several different coronal models. By considering a source near the plasma level in a spherically symmetric corona and in a streamer enhancement superimposed on a spherically symmetric corona we obtain resu
Radio emission from quasi-parallel shock waves in the corona
โ Scribed by G. Mann
- Publisher
- Springer Netherlands
- Year
- 1994
- Tongue
- English
- Weight
- 473 KB
- Volume
- 68
- Category
- Article
- ISSN
- 0038-6308
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