๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

The inter-relationship of hard X-ray and EUV bursts during solar flares

โœ Scribed by A. Gordon Emslie; John C. Brown; Richard F. Donnelly


Publisher
Springer
Year
1978
Tongue
English
Weight
708 KB
Volume
57
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.


๐Ÿ“œ SIMILAR VOLUMES


Hard X-ray bursts from flares behind the
โœ David L. Mckenzie ๐Ÿ“‚ Article ๐Ÿ“… 1975 ๐Ÿ› Springer ๐ŸŒ English โš– 459 KB

The determination of the location of the region of origin of hard X-rays is important in evaluating the importance of 10-100 keV electrons in solar flares arm in understanding flare particle acceleration. At present only limb-occulted events are available to give some information on the height of X-

Great Microwave Bursts and hard X-rays f
โœ Herbert J. Wiehl; David A. Batchelor; Carol Jo Crannell; Brian R. Dennis; Philli ๐Ÿ“‚ Article ๐Ÿ“… 1985 ๐Ÿ› Springer ๐ŸŒ English โš– 908 KB

The microwave and hard X-ray characteristics of 13 solar flares that produced microwave fluxes greater than 500 solar flux units have been analyzed. These Great Microwave Bursts were observed in the frequency range from 3 to 35 GHz at Bern, and simultaneous hard X-ray observations were made in the e

Correlation of hard X-ray and type III b
โœ Vahรฉ Petrosian; John Leach ๐Ÿ“‚ Article ๐Ÿ“… 1983 ๐Ÿ› Springer ๐ŸŒ English โš– 578 KB

The observed correlations between X-ray and type III radio emissions from solar bursts are described by means of a bivariate distribution function. Procedures for determining the form of this distribution are described using a sample of data analyzed by Kane (1981). With the help of this distributio

Observations of fine time structure in s
โœ K. Hurly; M. Niel; R. Talon; I. V. Estulin; V. Ch. Dolidze ๐Ÿ“‚ Article ๐Ÿ“… 1983 ๐Ÿ› Springer ๐ŸŒ English โš– 335 KB

Hard X-ray (ZI00 keY) time histories of solar flares which occurred on 1978 December 4 an@ 1979 February 18 are presented. The first flare was observed by 3 identical instruments from near-earth orbit (Prognoz 7) and interplanetary space (Venera Ii and 12). Fine time structure is present down to t

The solar albedo of hard X-ray flares
โœ N. Santangelo; H. Horstman; E. Horstman-Moretti ๐Ÿ“‚ Article ๐Ÿ“… 1973 ๐Ÿ› Springer ๐ŸŒ English โš– 240 KB