Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Jesse Coburn"'
Autor:
Chuanpeng Hou, Alexis P. Rouillard, Jiansen He, Bahaeddine Gannouni, Victor Réville, Philippe Louarn, Andrey Fedorov, Lubomír Přech, Christopher J. Owen, Daniel Verscharen, Raffaella D’Amicis, Luca Sorriso-Valvo, Naïs Fargette, Jesse Coburn, Vincent Génot, Jim M. Raines, Roberto Bruno, Stefano Livi, Benoit Lavraud, Nicolas André, Gabriel Fruit, Rungployphan Kieokaew, Illya Plotnikov, Emmanuel Penou, Alain Barthe, Dhiren Kataria, Matthieu Berthomier, Frederic Allegrini, Vito Fortunato, Gennaro Mele, Timothy Horbury
Publikováno v:
The Astrophysical Journal Letters, Vol 968, Iss 2, p L28 (2024)
The Parker Solar Probe's discovery that magnetic switchbacks and velocity spikes in the young solar wind are abundant has prompted intensive research into their origin(s) and formation mechanism(s) in the solar atmosphere. Recent studies, based on in
Externí odkaz:
https://doaj.org/article/7a836c2f50414a569db6b8ee8759f7ee
Autor:
Daniel Verscharen, Christopher Owen, Georgios Nicolaou, Jesse Coburn, Alfredo Micera, Maria Elena Innocenti
The electrons in the solar wind exhibit non-thermal velocity distribution functions. Observed non-thermal features of the electron distribution in the inner heliosphere include the field-aligned strahl, the suprathermal halo, the sunward deficit, and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::378237d3eaed5c3cd8c17161740d53c1
https://doi.org/10.5194/egusphere-egu23-15283
https://doi.org/10.5194/egusphere-egu23-15283
Autor:
Jesse Coburn, Daniel Verscharen, Christopher Owen, Timothy Horbury, Milan Maksimovic, Christopher Chen, Fan Guo, Xiangrong Fu
Non-Maxwellian features of the coronal electron population are important for some models of solar wind acceleration processes. Remnants of these features are detectable in spacecraft observations, in particular in the form of field-aligned beams (str
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4a451449242d7ffcabc609600be109b8
https://doi.org/10.5194/egusphere-egu23-9803
https://doi.org/10.5194/egusphere-egu23-9803
An ambipolar electric field is expected to develop in the solar wind, to maintain quasineutrality between the ions and electrons, which, due to their smaller mass, have a higher mobility than ions (Pierrard and Lemaire, 1996; Maksimovic et al., 2001)
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a748ea4767fa808b45ebfb47c7983410
https://doi.org/10.5194/egusphere-egu23-11785
https://doi.org/10.5194/egusphere-egu23-11785
Autor:
Carrie Wells, Jesse Coburn
Publikováno v:
Washington Post, The. 06/09/2016.