Results 51 to 60 of about 434,940 (199)
, 1998 This “rapporteur” report discusses the solar photosphere and low chromosphere in the context of chemical composition studies. The highly dynamical nature of the photosphere does not seem to jeopardize precise determination of solar abundances in classical fashion.
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Intensity enhancement of O VI ultraviolet emission lines in solar spectra due to opacity
, 2014 Opacity is a property of many plasmas, and it is normally expected that if an emission line in a plasma becomes optically thick, its intensity ratio to that of another transition that remains optically thin should decrease.
Bowler, L. A. +7 more
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Diagnosis of the solar atmosphere using solar oscillations [PDF]
Symposium - International Astronomical Union, 1988 I present a review of the art of using acoustic and gravity waves as a tool to probe the structure of the solar atmosphere. The principle ideas behind the technique are discussed and a small bouquet of results is presented. The current discrepancies are pointed out, and in the last section a few thoughts are let loose about the inversion of data to ...
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Magneto-seismology of solar atmospheric loops by means of longitudinal oscillations
, 2012 There is increasingly strong observational evidence that slow magnetoacoustic modes arise in the solar atmosphere. Solar magneto-seismology is a novel tool to derive otherwise directly un-measurable properties of the solar atmosphere when ...
Dymova +4 more
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Atmospheric Electrification in the Solar System [PDF]
Surveys in Geophysics, 2006 Atmospheric electrification is not a purely terrestrial phenomenon: all Solar System planetary atmospheres become slightly electrified by cosmic ray ionisation. There is evidence for lightning on Jupiter, Saturn, Uranus and Neptune, and it appears likely to exist on Mars, Venus and Titan.
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Vortex Flows in the Solar Chromosphere -- I. Automatic detection method
, 2017 Solar "magnetic tornadoes" are produced by rotating magnetic field structures that extend from the upper convection zone and the photosphere to the corona of the Sun.
Kato, Yoshiaki, Wedemeyer, Sven
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Oscillations of solar atmosphere neutrinos [PDF]
, 2006 The Sun is a source of high energy neutrinos (E > 10 GeV) produced by cosmic ray interactions in the solar atmosphere. We study the impact of three-flavor oscillations (in vacuum and in matter) on solar atmosphere neutrinos, and calculate their ...
A. Mirizzi +10 more
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Revisiting the Solar Wind Deceleration Upstream of the Martian Bow Shock Based on MAVEN Observations
The Astrophysical JournalThe solar wind deceleration upstream of the Martian bow shock is examined using particle and magnetic field measurements obtained by the Mars Atmosphere and Volatile EvolutioN (MAVEN).
Yuqi Liu +8 more
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Atmospheric attenuation of solar radiation [PDF]
, 1977 The attenuation of solar radiation by the atmosphere between the heliostat and receiver of a Central Receiver solar energy system has been computed for a number of atmospheric conditions and tower-heliostat distances. The most important atmospheric variable is found to be the atmospheric aerosol content.
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Editorial: Connecting solar flows and fields to understand surface magnetism
Frontiers in Astronomy and Space Sciences, 2023 Kiran Jain +2 more
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