✦ LIBER ✦
The emission of solar X-rays in the 0.5–3 Å wavelength range and its relation to the magnetic configuration of active centers
✍ Scribed by G. Chambe
- Publisher
- Springer
- Year
- 1969
- Tongue
- English
- Weight
- 302 KB
- Volume
- 8
- Category
- Article
- ISSN
- 0038-0938
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✦ Synopsis
The slowly varying component of solar X-rays in the 0.5-3 ~ wavelength range has been studied using data obtained by the satellite Explorer 30 (Solrad 8). The intensity of these X-rays is poorly correlated with the centimeter radio flux, contrary to the good correlation found in the spectral bands 1-8, 8-16 and 44-60 &. On the other hand the 0.5-3 & X-ray intensity is often connected to the development of a specific magnetic configuration in the sun spot group which may thus be associated with the X-ray producing active center.