Photoelectric observations of the light intensity from the solar crescent before and after totality were made during the eclipses of 7 March, 1970 and 26 February, 1979. Effective wavelengths were determined by interference filters of 20 nm bandwidth. To obtain the limb darkening function, the resul
Airborne total eclipse observation of the extreme solar limb at 400 μm
✍ Scribed by T. Alan Clark; Rita T. Boreiko
- Publisher
- Springer
- Year
- 1982
- Tongue
- English
- Weight
- 714 KB
- Volume
- 76
- Category
- Article
- ISSN
- 0038-0938
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