A survey of the interpretations of radio and x-ray bursts
Generation mechanisms of radio and x-ray bursts from solar flares - bremsstrahlung from solar plasma, gyro and synchrotron radiation from electrons, and plasma radiation
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Generation mechanisms of radio and x-ray bursts from solar flares - bremsstrahlung from solar plasma, gyro and synchrotron radiation from electrons, and plasma radiation
High energy x-ray bursts observed by orbiting solar observatory i
Correlation of variations of explorer vi count rates with simultaneous visual auroras and high- altitude x-ray bursts
Solar X-ray bursts in 20 to 100 keV range observed by OSO- I
Observations of Van Allen radiation regions by Explorer VI satellite - visual auroras, high altitude X-ray bursts, and simultaneous satellite observations during magnetic storms
High energy X-ray radiation observations by OSO-I satellite following solar flares
Microwave and hard X ray bursts from solar flares
Solar X ray bursts observed by proportional counter on IMP-F satellite to correlate optical H alpha flares and radio bursts
Solar flares microwave and hard X ray bursts, discussing gyrosynchroton plasma, nonthermal electron bremsstrahlung and electron relaxation
Solar X ray detector aboard OGO 5 satellite observing two components in energetic solar X ray bursts, attributing impulsive component to bremsstrahlung
Solar soft X rays observed from OSO-3, correlating to solar flares and radio bursts
Solar flare observations with Mariner 5, and Explorer 33 and 35 satellites
A diffuse atmospheric fluorescence pulse having the proper signatures of an excitation caused by a fast burst of X-ray photons incident from the general direction of the recent supernova in NGC 5253, was recorded on May 3, 1972, at 20 hr 48 min 51 sec UT. Due to excessive background pulses of terrestrial origin, it is concluded that the evidence should at best be regarded as suggestive. It is recommended that the data of satellite-borne X-ray detectors be examined for anomalies at the indicated time.
Solar flare soft X ray and EUV emission spectra data obtained on OSO-3 satellite compared with centimetric radio bursts
Supernova 1987A (February 23, 1987) in the Large Magellanic Cloud is the brightest supernova to be observed since SN 1604 AD (Kepler). Detection of a burst of neutrinos indicates that a neutron star was formed. Radioactive decay of about 0.07 solar mass of Co-56 is responsible for the observed optical light as well as hard X-rays and gamma-ray lines. Ultraviolet, optical, and infrared 'light echoes' and soft X-rays provide information on the distribution of circumstellar matter and the evolution of the progenitor star.
Impulsive solar X ray bursts observed by xenon methane filled proportional counter on IMP-F satellite
Solar flare X ray bursts detected by OGO spacecraft correlated with radio emission and solar flare electron and proton events