The method of has been used with a variety of spectral lines to study oscillating longitudinal gas velocities inside solar magnetic elements. Oscillations have been found inside all elements observed, the amplitudes increasing with height from typically +0.27kms -I in Fe 15166 ~ (a line of low orig
Motions in solar magnetic tubes
โ Scribed by R. G. Giovanelli; C. Slaughter
- Publisher
- Springer
- Year
- 1978
- Tongue
- English
- Weight
- 444 KB
- Volume
- 57
- Category
- Article
- ISSN
- 0038-0938
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