Dynamical properties of stellar coronas and stellar winds. iii. the dynamics of coronal streamers
Filamentary structure of solar corona and effect on dynamics of solar wind
CORONA↗
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Radiation of soft x-rays by the solar corona <ob izluchenii solnechnoy korony v myakov rentgenovskoy oblasti<
Radiation of soft x-rays by solar corona
CORONA↗
Radiation of the solar corona in the spectral region with lambda less than 10 angstroms <izlucheniye solnechoy korony v oblasti spektra koroche 10 angstroms<
Radiation of solar corona in spectra region with lambda less than 10 angstroms
CORONA↗
On the Intensity and Polarization of Solar Corona's Forbidden Lines
Intensity and polarization of forbidden bands of solar corona spectrum
INTENSITY↗
Observations of the solar corona from the limb of the sun to the zodiacal light, july 20, 1963
Observing solar corona from limb of sun to zodiacal light
ZODIACAL LIGHT↗
Type ii bursts and the magnetic field in the corona
Type ii solar radio bursts and magnetic field in corona
CORONA↗
Methods of observation of the solar corona during non-eclipse time <les methodes d'observation de la couronne solaire en dehors des eclipses<
Solar corona observation during noneclipse time
CORONA↗
The velocity of corpuscular streams in the solar corona based on observations of solar radio emission <o skorosti potokov chastits v solnechnoy korone po nablyudeniyam radioizlucheniya solntsa<
Velocity measurement of corpuscular streams in solar corona by solar radio emission
RADIO EMISSION↗
Dynamical properties of stellar coronas and stellar winds. i - integration of the momentum equation.
Stationary hydrodynamic expansion of spherical stellar corona, studied from integrated hydrodynamic momentum and mass conservation equations
CORONA↗
Observations of the white light corona from a rocket
White light solar corona observations by rocketborne photographic and photoelectric coronagraphs
CORONAGRAPH↗
Conductive heating of the solar wind, ii- the inner corona
Coupling between solar wind and exosphere - conductive heating of solar wind and inner corona
EXOSPHERE↗
The uv lines of fexiv in the solar corona
Ultraviolet radiation lines of iron XIV in solar corona
IRON↗
The uv lines of fe xiv in the solar corona.
Relative line strengths of UV lines of Fe XIV CALCULATED for solar corona
CORONA↗
The emission of the quiet corona at meter wavelengths.
Quiet corona emission at meter wavelengths calculated on new radiative transfer basis, obtaining new results on radiative temperature and limb brightening
SOLAR RADIO WAVE↗
Dynamical properties of stellar coronas and stellar winds. iv - the separate existence of subsonic and supersonic solutions.
Stationary stellar corona energy supplied by thermal conduction from base surrounded by cold vacuum
STELLAR STRUCTURE↗
Observations of the white-light corona by rocket.
White-light corona of Sun photographed with rocket mounted Lyot coronagraph equipped with external occulter, noting agreement of rocket with eclipse data
SOLAR ECLIPSE↗
Profiles of lyman-alpha scattered by free electrons in the solar corona.
Half-intensity profile width of Lyman-alpha radiation Doppler-scattered by free electrons in solar corona considered as measure of coronal temperature
FREE ELECTRON↗
Use of the Moon to Distinguish the F from the K Corona Using a Rocket Coronagraph During an Eclipse
F and K corona observations by rocket coronagraph during solar eclipse
K CORONA↗