𝔖 Bobbio Scriptorium
✦   LIBER   ✦

The intensity decrease of microwave bursts

✍ Scribed by E. Fürst


Publisher
Springer
Year
1973
Tongue
English
Weight
398 KB
Volume
28
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.

✦ Synopsis


A typical microwave burst on 1968 January 11, 1700 UT is used to demonstrate that the radiation spectrum at maximum phase can be described by gyromagnetic absorption. A model for the source is derived from the observed spectrum. With the aid of this model, we try to explain the decreasing phase of the burst intensity. Satisfactory agreement with observation is obtained, when one assumes that the cooling of the burst plasma is caused by heat conduction parallel to the magnetic field lines.


📜 SIMILAR VOLUMES


Forecasting the intensity of solar proto
✍ David L. Croom 📂 Article 📅 1971 🏛 Springer 🌐 English ⚖ 712 KB

A survey of the main characteristics of solar microwave bursts in relation to their usefulness for indicating the intensity of associated solar proton emissions suggests that time parameters give much better results than intensity or spectrum parameters. In particular, best results are obtained by u

The secondary spectral component of sola
✍ M. Stähli; D. E. Gary; G. J. Hurford 📂 Article 📅 1990 🏛 Springer 🌐 English ⚖ 800 KB

Microwave observations in the range 1 to 18 GHz with high spectral resolution (40 frequencies) have shown that many events display a complex microwave spectrum. From a set of 14 events with two or more spectral components, we find that two different classes of complex events can be distinguished. Th

High-resolution microwave spectra of sol
✍ M. Stähli; D. E. Gary; G. J. Hurford 📂 Article 📅 1989 🏛 Springer 🌐 English ⚖ 932 KB

Microwave observations with exceptionally high spectral resolution are described for a set of 49 solar flares observed between May and October 1981. Total power data were obtained at 40 frequencies between 1 and 18 GHz by the Owens Valley frequency-agile interferometer with 10 s time resolution. Sta