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A study of energetic solar flare X-rays
Solar Physics, 1967A new series of solar flare energetic X-ray events has been detected by an ionization chamber on the OGO-I and OGO-III satellites in free space. These X-rays lie in the range 10–50 keV, and a study has been made of their relationship to 3 and 10 cm radio bursts and with the emission of electrons and protons observed in space.
R. L. Arnoldy +2 more
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Determination of the temperature in a solar X-ray flare
Journal of Atmospheric and Terrestrial Physics, 1973Abstract The equivalent temperature in a solar X-ray flare for λ ≈ 2 A . is deduced from the measurement of the X-ray flux by Explorer 37 and the simultaneous measurement of the ionospheric electron density by VLF and LF records on the Rugby-Turin link. These data yield the value of the effective photoionization cross section in the band 1
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Impulsive X-ray brightenings in solar flares
Advances in Space Research, 1996Abstract An analysis of 40 solar flares observed with the Yohkoh satellite was carried out to investigate the temporal relationship between rapid hard and soft X-ray flaring. Using Bragg Crystal Spectrometer (BCS) and Hard X-ray Telescope (HXT) data it was found that in every event the Neupert effect occurred throughout most of the impulsive phase.
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Solar flare hard X-ray observations
Solar Physics, 1988Recent hard X-ray observations of solar flares are reviewed with emphasis on results obtained with instruments on the Solar Maximum Mission satellite. Flares with three different sets of characteristics, designated as Type A, Type B, and Type C, are discussed and hard X-ray temporal, spatial, spectral, and polarization measurements are reviewed in this
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Investigation of Hemispherical Variations of Soft X-Ray Solar Flares during Solar Cycles 21 to 24
Solar System Research, 2021Sankar Narayan Patra +2 more
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Modeling of the Lower Ionosphere During Solar X‐Ray Flares of Different Classes
Journal of Geophysical Research: Space Physics, 2021Susanna Bekker, Ilya Ryakhovsky
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