๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Explosive hydrogen-burning model of solar flares

โœ Scribed by L. Manihar Singh; L. Randhoni Devi


Publisher
Springer Netherlands
Year
1990
Tongue
English
Weight
112 KB
Volume
172
Category
Article
ISSN
0004-640X

No coin nor oath required. For personal study only.


๐Ÿ“œ SIMILAR VOLUMES


The explosive phase of solar flares
โœ Karen L. Harvey ๐Ÿ“‚ Article ๐Ÿ“… 1971 ๐Ÿ› Springer ๐ŸŒ English โš– 349 KB

The explosive phase of a flare can be defined by a simple photometric measurement of Ha film records of the flare development. Using the quantitative definition, improved correlations are found between the start of the explosive phase and the start of 10.7 cm radio bursts and Sudden Frequency Deviat

Decay studies of importance to explosive
โœ C. Iliadis; R.E. Azuma; J. Chow; J.D. King; A.C. Morton; L. Buchmann; M. Dombsky ๐Ÿ“‚ Article ๐Ÿ“… 1997 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 248 KB

The fl-delayed s-particle decay of a6K has been measured in order to search for natural parity states near the proton threshold in Z~Ar. Such states could correspond to resonances in the reaction 35C1(p,(~)32S and might influence mass flows in explosive hydrogen burning scenarios appreciably. We hav

A model of solar flares and faculae
โœ J. H. Piddington ๐Ÿ“‚ Article ๐Ÿ“… 1973 ๐Ÿ› Springer ๐ŸŒ English โš– 767 KB

Theories of solar flares based on the storage of energy (usually as magnetic energy) in the solar atmosphere are shown to be incompatible with observational data. The sunspot energy deficit and the photospheric faculae both involve energy fluxes comparable with the flare requirement ( ~ 3 โ€ข 1029 er