Concept information
Terme préférentiel
solar wind
Définition
- A mass outflow, consisting of protons, electrons, and other subatomic particles, expelled constantly from the solar corona at about 500 km per second. The solar mass-loss rate in this phenomenon amounts to about 2 x 10⁻¹⁴ solar masses per year, or about 106 tons per second. (An Etymological Dictionary of Astronomy and Astrophysics, by M. Heydari-Malayeri, https://dictionary.obspm.fr/index.php?formSearchTextfield=solar+wind&formSubmit=Search&showAll=1)
Concept générique
Traductions
-
français
URI
http://data.loterre.fr/ark:/67375/MDL-HD0NWS2L-J
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