The apparent height of radio sources above the photosphere was determined for the period of 1968-1971, by a method which makes use of the displacement in latitude of the centroid of the radio emission relative to the associated optical feature. The apparent height fell progressively in time by amou
Latitude and solar-cycle dependence of radial IMF intensity
β Scribed by Y. -M. Wang
- Publisher
- Springer Netherlands
- Year
- 1995
- Tongue
- English
- Weight
- 220 KB
- Volume
- 72
- Category
- Article
- ISSN
- 0038-6308
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