The dynamic spectrum, a three dimensional record of the radio intensity as a function both of time and frequency, has long been used as a probe of plasma processes in the solar corona. Beginning with the work of Wild and McCready (1950) dynamic spectroscopy has beeI1 used to distinguish between the
โฆ LIBER โฆ
A stellar wind dynamic model for S 106
โ Scribed by Jiang Dong-rong; Fu Cheng-qi
- Publisher
- Elsevier Science
- Year
- 1991
- Tongue
- English
- Weight
- 655 KB
- Volume
- 15
- Category
- Article
- ISSN
- 0275-1062
No coin nor oath required. For personal study only.
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