Zobrazeno 1 - 10
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pro vyhledávání: '"SOLAR-WIND"'
The continuous stream of particles flowing outward from the Sun is called the solar wind. It mostly consists of electrons and protons with energies usually between 1.5 and 10 keV. The stream of particles varies in temperature and speed over time. The
Autor:
Fejer, Bela G.1 bela.fejer@usu.edu, Navarro, Luis A.2, Chakrabarty, Dibyendu3, Truhlik, Vladimir4, Yong-Qiang Hao5
Publikováno v:
Frontiers in Astronomy & Space Sciences. 2024, p01-14. 14p.
In addition to sunshine, the Sun emits about one trillion tons of ionized hydrogen per second into the interplanetary space, a phenomenon known as solar wind. This book systematizes the knowledge of the solar wind acceleration region, which is, figur
Autor:
Sorriso-Valvo, Luca, Malara, Francesco francesco.malara@fis.unical.it
Publikováno v:
Science. 8/30/2024, Vol. 385 Issue 6712, p928-930. 3p. 2 Color Photographs.
Autor:
Rivera, Yeimy J. yeimy.rivera@cfa.harvard.edu, Badman, Samuel T., Stevens, Michael L., Verniero, Jaye L., Stawarz, Julia E., Shi, Chen, Raines, Jim M., Paulson, Kristoff W., Owen, Christopher J., Niembro, Tatiana, Louarn, Philippe, Livi, Stefano A., Lepri, Susan T., Kasper, Justin C., Horbury, Timothy S., Halekas, Jasper S., Dewey, Ryan M., Marco, Rossana De, Bale, Stuart D.
Publikováno v:
Science. 8/30/2024, Vol. 385 Issue 6712, p962-966. 5p. 2 Diagrams, 2 Graphs.