Resonance and satellite lines of highly ionized iron in the solar spectrum near 1.9 A
Resonance and satellite lines of highly ionized iron in solar spectra, discussing spectrum features during chromospheric flares
Neupert, W. M.↗
Engineering topics
Neupert, W. M.
Publications and source records attributed to Neupert, W. M..
X-ray and extreme ultraviolet /1-400 angstrom units/ spectroscopy of the sun, from OSO-III.
Solar X ray and extreme UV spectra during flares, attributing intense emissions to optical transitions
Gates, W. J.↗
X rays from the sun.
Solar X rays observations, describing instrumentation, radiation characteristics, association with flares, spectrum analysis, etc
Neupert, W. M.↗
Observations of the solar flare soft X-ray spectrum and comparison with centimetric radio bursts.
Solar flare soft X ray and EUV emission spectra data obtained on OSO-3 satellite compared with centimetric radio bursts
Neupert, W. M.↗
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.↗
The solar corona above active regions - A comparison of extreme ultraviolet line emission with radio emission.
Extreme UV line emission observations applied to solar corona above active regions, comparing extreme UV line emission to radio emission
Neupert, W. M.↗
Glancing incidence telescope for far ultraviolet and soft X-rays
Glancing-incidence telescope makes observations of distant celestial radiant bodies at wavelengths in the spectral region between 3 and 500 angstroms. The device can be used as a fore-optics system for a laboratory extreme ultraviolet spectrometer, or for the collection or imaging of thermal neutrons.
Neupert, W. M.↗
The solar corona above active regions - A comparison of extreme ultraviolet line emission with radio emission.
Extreme UV line and radio emission from solar corona above active regions, noting electron density and temperature
Neupert, W. M.↗
Observation of the solar flare X-ray emission line spectrum of iron from 1.3 to 20 angstrom units.
Solar X-ray emission line spectrum from 1.3 to 20 angstroms in solar flares identified as Fe XXVI through Fe XX transitions
SOLAR FLARE↗
The solar corona above active regions - A comparison of extreme ultraviolet line emission with radio emission
Solar corona above active regions - comparison of extreme ultraviolet line emission with radio emission
ULTRAVIOLET RADIATION↗
Multiple element soft x-ray source.
Multiple element soft X-ray source for study of soft X-ray region of electromagnetic spectrum, obtaining absolute photon yield of carbon K and boron K
X-RAY ANALYSIS↗
Intensity variations in the solar extreme ultraviolet spectrum observed by oso-1.
OSO observations of extreme UV radiation with application to identification of emission lines in spectral region 170-1400 angstroms
SOLAR RADIATION↗
Multiple element soft X-ray source produces wide range of radiation
A rotating mount with target elements positioned independently for direct electron bombardment produces soft X ray radiation with a wide range of characteristics. The device may be used to study solar radiation from a satellite.
Caruso, A. J.↗
The effect of a coronal expansion on the computation of an electron temperature from emission-line intensities
Coronal expansion effect on calculation of electron temperature from emission-line intensities
EMISSION SPECTRUM↗
Intensity variations in the solar extreme ultraviolet spectrum observed by OSO-1.
OSO observations of EUV radiation applied to identification of emission lines in spectral region 170-1400 angstroms
OSO↗