Using solar wind velocity data obtained by Mariner-2 and IMP-1 spacecrafts, an attempt has been made to study its correlation with 25303 coronal intensity. It is shown that the long-lasting regions of enhanced 25303 intensity in the solar corona are well correlated with recurrent streams of solar wi
Solar cycle variation and N-S asymmetry of λ 5303 coronal intensity
✍ Scribed by P. N. Pathak
- Publisher
- Springer
- Year
- 1972
- Tongue
- English
- Weight
- 195 KB
- Volume
- 25
- Category
- Article
- ISSN
- 0038-0938
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