The solar irradiance modulation due to active regions during 1980 has been investigated in detail. Specifically, we estimate the uncertainties caused by ground-based data used as input in the modeling effort, and by our currently incomplete knowledge of the proper parameters that describe the angula
Ephemeral active regions during solar minimum
β Scribed by Sara F. Martin; Karen L. Harvey
- Publisher
- Springer
- Year
- 1979
- Tongue
- English
- Weight
- 848 KB
- Volume
- 64
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
## Formations'' I n the present paper we are trying to demonstrate the importance of detailed observations for the theory of solar local magnetic field generation. Mutual relations of solar background magnetic fields and new active region formations are described. The influence of various factors,
## Abstract Irradiance records of the Nimbusβ7 and SMM satellites indicate a systematic downward trend of the solar constant of the order of a few hundredths of a percent and a slow variation of the solar constant on a time scale from days to weeks. The reason for the downward trend is not known as