Results 161 to 170 of about 107,783 (198)
IMAP's Role in Understanding Particle Injection and Energization Throughout the Heliosphere. [PDF]
Cohen CMS +30 more
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Day-to-Day Boundary Fluctuations in Coronal Holes: Causes and Consequences. [PDF]
Ugarte-Urra I +3 more
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Polarity-resolved far-side magnetograms based on helioseismic measurements. [PDF]
Hamada A +4 more
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An Efficient Method for Magnetic Field Extrapolation Based on a Family of Analytical Three-Dimensional Magnetohydrostatic Equilibria. [PDF]
Nadol L, Neukirch T.
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Flux equipartition in astrophysical plasma turbulence. [PDF]
Marino R, Xie JH.
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Fluorinated Polymers for Hydrovoltaic Energy Harvesting: Mechanisms and Multifunctional Integration. [PDF]
Lee S, Nam C.
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Measuring the magnetic fields in the chromospheres of low-mass stars
Cang T +13 more
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2003
The solar corona is an extremely hot (106 K or about 0.1 keV), almost fully ionised plasma which extends from a few thousand km above the Sun’s visible surface or photosphere (6000 K) to where it freely expands into the solar system as the solar wind.
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The solar corona is an extremely hot (106 K or about 0.1 keV), almost fully ionised plasma which extends from a few thousand km above the Sun’s visible surface or photosphere (6000 K) to where it freely expands into the solar system as the solar wind.
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Nature, 1966
Physics of the Solar Corona By I. S. Shklovskii. Second edition. Translated by L. A. Fenn. Translation edited by A. Beer. Additional material translated and edited by A. J. Meadows. (International Series of Monographs on Natural Philosophy, Vol. 6.) Pp. x + 475. (London and New York: Pergamon Press, Ltd., 1965.) 120s. net.
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Physics of the Solar Corona By I. S. Shklovskii. Second edition. Translated by L. A. Fenn. Translation edited by A. Beer. Additional material translated and edited by A. J. Meadows. (International Series of Monographs on Natural Philosophy, Vol. 6.) Pp. x + 475. (London and New York: Pergamon Press, Ltd., 1965.) 120s. net.
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