Parker Solar Probe In Situ Observations of Magnetic Reconnection Exhausts during Encounter 1

Magnetic reconnection in current sheets converts magnetic energy into particle energy. The process may play an important role in the acceleration and heating of the solar wind close to the Sun. Observations from Parker Solar Probe (PSP) provide a new opportunity to study this problem, as it measures...

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Veröffentlicht in:	The Astrophysical journal. Supplement series 2020-02, Vol.246 (2), p.34
Hauptverfasser:	Phan, T. D., Bale, S. D., Eastwood, J. P., Lavraud, B., Drake, J. F., Oieroset, M., Shay, M. A., Pulupa, M., Stevens, M., MacDowall, R. J., Case, A. W., Larson, D., Kasper, J., Whittlesey, P., Szabo, A., Korreck, K. E., Bonnell, J. W., de Wit, T. Dudok, Goetz, K., Harvey, P. R., Horbury, T. S., Livi, R., Malaspina, D., Paulson, K., Raouafi, N. E., Velli, M.
Format:	Artikel
Sprache:	eng
Schlagworte:	Acceleration Alfven waves Astrophysics Coronal mass ejection Current sheets Magnetic fields Magnetic reconnection Particle energy Perihelions Physics Plasma astrophysics Sciences of the Universe Shear Solar and Stellar Astrophysics Solar corona Solar magnetic fields Solar magnetic reconnection Solar probes Solar wind Space Physics Space plasmas Velocity
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