Titlebook: Coronal Disturbances; Gordon Newkirk Book 1974 International Astronomical Union 1974 Corona.Planet.Solar flare.Variation.cosmic ray.observ

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Total Quality Management — worldwide effectt potential field) as well as disturbances which appear to be related to changes in these configurations. Thirdly, the role of the field in guiding coronal disturbances is considered. This is evident for bulk motions (sprays, surges, flare loops, green line events, etc.), wave motions (flare associa

Cosmopolitan

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Bulk growth of widegap II–VI single crystalsd for qualitative analysis of energetic particle and white light events. The ultimate good may possibly come from spectral analysis of the minute by minute variation of the burst microwave radiation spectral slope α (above .) in the area between 15 000 and 35 000 MHz. This may be used alone or in re

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II–VI electroluminescent devicesavelength range covered was 0.5–20 Å. The type III radio data was obtained from two sources: The 169 MHz radio-heliograph at Nancay which provided east-west position of the radio burst on the Sun with an accuracy of ~ 1′ and the radio spectra measured by various ground based observatories. The findi

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X-Ray Emission in Absence of Flares Related to Hα Activity and Type III Burst Productionavelength range covered was 0.5–20 Å. The type III radio data was obtained from two sources: The 169 MHz radio-heliograph at Nancay which provided east-west position of the radio burst on the Sun with an accuracy of ~ 1′ and the radio spectra measured by various ground based observatories. The findi