Comparison of solar X-ray line emission with microwave emission during flares.
Solar X ray line emission compared with microwave emission during flares
Neupert, W. M.↗
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Solar x-rays - slow variations and transient events
Oso solar x-ray data from slow variations & flares
SOLAR X-RAY↗
Solar x rays- a comparison with microwave radiation
Comparison of solar x-rays with microwave radiation using orbiting solar observatory /oso/ data
MICROWAVE RADIATION↗
Image and Spectrum of the Sun in the Region 9.5-200 Angstrom
Short wave ultraviolet image and spectrum of sun obtained during course of X-ray flare
IMAGE↗
Comments on high energy x-ray bursts observed by oso i
High energy x-ray bursts observed by orbiting solar observatory i
SOLAR X-RAY↗
Solar x-ray emission - nrl results
X-ray line spectrum, spectroheliograph results, & fan beam scans of solar x-ray emission
SPECTROHELIOGRAPH↗
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
RADIO BURST↗
Some notes on the relations of x-ray, particle, and radio emission of the sun during flares
Relations of x-ray radiation, particle emission, and radio emission during solar flares
SOLAR FLARE↗
Observation of an X-ray flare - Spatial distribution and physical parameters.
Solar flares spectra X ray portion, considering spatial distribution, relation to magnetic fields and time sequence of emitting region
Giacconi, R.↗
On the generation of synchrotron and X-ray emission from electrons with energy below mc super 2 in solar flares.
Synchrotron and X ray emission generation from upper chromosphere electrons during solar flares
Cline, T. L.↗
Solar x-rays - slow variations and transient events.
Slowly varying component of solar x-ray flux below 11 angstroms correlated with 2800 mc solar radiation, sid and h alpha flares
SOLAR X-RAY↗
Comments on high energy x-ray bursts observed by oso-1.
High energy X-ray radiation observations by OSO-I satellite following solar flares
RADIATION MEASUREMENT↗
De-occultation X-ray events of 2 December, 1967
Flare rising from behind solar limb deoccultated by simultaneous recording by OSO III X ray detector and photoheliograph
Hudson, H.↗
X-ray structures of the sun during the importance in flare of 8 June 1968.
Solar X ray structures during june 8, 1968 flare, using data from rocket-borne grazing incidence telescope
Giacconi, R.↗
The limb flare of november 20, 1960 - a coronal phenomenon.
Explosive limb flare of November 20, 1960 shown to coincide with beginning of radio and X-ray emission
CORONA↗
The interpretation of XUV solar radiation.
Discussion of the importance of laboratory and theoretical investigations for the analysis of solar UV and X-ray data by referring to five problems to which space experimenters are currently devoting a great deal of attention: (1) the temperature minimum at the interface between the photosphere and the chromosphere; (2) the temperature and density profiles of the low chromosphere; (3) the transition zone at the chromosphere-corona interface; (4) the corona; and (5) solar flares. Brief comments are made on the special need for laboratory and theoretical data of all kinds to assist in the interpretation of the rapidly accumulating volume of observations in the X-ray region of the solar spectrum.
Goldberg, L.↗
Effect of 2 less lambda less 12 angstrom solar X-rays on the ionosphere between 60 and 100 km
Ionospheric effects caused by 2-12 angstrom solar X ray quiescent flux and flare flux
Sengupta, P. R.↗
Observations of energetic X-rays and solar cosmic rays associated with the 23 May 1967 solar flare event.
Peaks and time intensity profile of energetic X rays and cosmic rays observed by OGO-C ion chamber on May 23, 1967 flare event
Kane, S. R.↗