Results 161 to 170 of about 107,783 (198)

IMAP's Role in Understanding Particle Injection and Energization Throughout the Heliosphere. [PDF]

open access: yesSpace Sci Rev
Cohen CMS   +30 more
europepmc   +1 more source

Polarity-resolved far-side magnetograms based on helioseismic measurements. [PDF]

open access: yesSci Rep
Hamada A   +4 more
europepmc   +1 more source

Measuring the magnetic fields in the chromospheres of low-mass stars

open access: yes
Cang T   +13 more
europepmc   +1 more source

The Solar Corona

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.
openaire   +1 more source

The Solar Corona

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.
openaire   +1 more source

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