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Schumann resonance frequency increase during solar X-ray bursts

✍ Scribed by Roldugin, V. C.


Book ID
119661044
Publisher
American Geophysical Union
Year
2004
Tongue
English
Weight
624 KB
Volume
109
Category
Article
ISSN
0148-0227

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KΞ± line emission during solar X-ray burs
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Kct X-ray line emission from S, Ar, Ca and Fe is calculated for conditions likely to exist in solar flares. We consider both the non-thermal and thermal phases of flares as indicated by X-ray observations. Impulsive non-thermal events seen at the onset of a flare at photon energies > 20 keV generall