Observations of coronal Fe xiv emission lines from the NE quadrant during the 1973 solar eclipse are reported. Temperatures are deduced from a pure thermal broadening model, and, in the region near an observed white-light enhancement, an alternative interpretation ofhalfwidth as being in part due to
The effect of the solar eclipse on the air temperature near the ground
✍ Scribed by Karol Szałowski
- Publisher
- Elsevier Science
- Year
- 2002
- Tongue
- English
- Weight
- 464 KB
- Volume
- 64
- Category
- Article
- ISSN
- 1364-6826
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