I have studied the observational relationship between the location of flare sites in active regions and three other observables, viz., Ha line width, hard X-ray burst parameters, and peak microwave fluxes. Results suggest that the strength of the magnetic field plays a role in governing the magnitud
A new microwave/X-ray diagnostic for the thermal phase of solar flares
โ Scribed by E. J. Schmahl; M. R. Kundu; F. T. Erskine
- Publisher
- Springer
- Year
- 1986
- Tongue
- English
- Weight
- 670 KB
- Volume
- 105
- Category
- Article
- ISSN
- 0038-0938
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