Zobrazeno 1 - 10
of 162
pro vyhledávání: '"John W. Belcher"'
Publikováno v:
Physics Today.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::dbbab902b0f90580272a1dd3c6f19a30
https://doi.org/10.1063/pt.5.10004
https://doi.org/10.1063/pt.5.10004
Autor:
Bravo, Sílvia
Publikováno v:
Revista de física; Volum 4 : núm. 9 : any 2012; p. 31-32
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______613::b5bbc672fea4098003b3c04cc6cd5fd0
http://www.raco.cat/index.php/RevistaFisica/article/view/276071
http://www.raco.cat/index.php/RevistaFisica/article/view/276071
Autor:
John W. Belcher
Publikováno v:
Edutec, Iss 47 (2014)
Tratamos la naturaleza del espacio de aprendizaje utilizado en las clases de introducción a la física del MIT. Estos espacios educativos se han diseñado para la interacción, tanto en términos de experimentos de escritorio, planteamiento y resolu
Externí odkaz:
https://doaj.org/article/013aa415c41f4260974266674812278d
Autor:
Bennett A. Maruca, Timothy S. Horbury, Phyllis Whittlesey, Matthieu Berthomier, Philippe Louarn, Milan Maksimovic, Ruth M. Skoug, John T. Steinberg, Ralph L. McNutt, Roberto Livi, Jasper Halekas, N.-E. Raouafi, David J. McComas, Marco Velli, Nikolai V. Pogorelov, Nathan A. Schwadron, S. P. Gary, K. H. Wright, Robert J. MacDowall, John W. Belcher, Qiang Hu, Dennis L. Gallagher, Gary P. Zank, Davin Larson, Leon Golub, Adam Szabo, Benoit Lavraud, Anthony W. Case, Georges Ho, John D. Richardson, Mihailo M. Martinović, D. McGinnis, Stuart D. Bale, Marc Pulupa, D. W. Curtis, Michael L. Stevens, Katja Klein, Jia Huang, Benjamin D. G. Chandran, Kelly E. Korreck, Justin C. Kasper
Publikováno v:
Nature
Nature, Nature Publishing Group, 2019, 576 (7786), pp.228-231. ⟨10.1038/s41586-019-1813-z⟩
Nature, Nature Publishing Group, 2019, 576 (7786), pp.228-231. ⟨10.1038/s41586-019-1813-z⟩
The prediction of a supersonic solar wind1 was first confirmed by spacecraft near Earth2,3 and later by spacecraft at heliocentric distances as small as 62 solar radii4. These missions showed that plasma accelerates as it emerges from the corona, aid
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c02daeba4bb210e805076b350a90eea0
http://hdl.handle.net/10044/1/75867
http://hdl.handle.net/10044/1/75867
Autor:
L. F. Burlaga, Robert B. Decker, John D. Richardson, A. C. Cummings, John W. Belcher, Merav Opher, E. C. Stone
Publikováno v:
Journal of Physics: Conference Series. 1620:012016
This paper discusses plasma characteristics in the heliosheath region before the heliopause (HP), at the HP, and in the very local interstellar medium (VLISM). The Voyager 2 (V2) HP was a sharp boundary where the radial plasma currents went to backgr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b1fd7124f50258914fbc9dbf9df8de49
https://doi.org/10.1088/1742-6596/1620/1/012016
https://doi.org/10.1088/1742-6596/1620/1/012016
This paper provides the latest data from Voyager 2 on plasma characteristics in the heliosheath including the observations of pressure waves in the plasma and particle data. Models and observations show that solar transients drive pressure waves thro
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2b987edbfca18c36c07fdb396b91defb
https://resolver.caltech.edu/CaltechAUTHORS:20181025-112020309
https://resolver.caltech.edu/CaltechAUTHORS:20181025-112020309
The mixture/interaction of anti-sunward-propagating Alfvenic fluctuations (AFs) and sunward-propagating Alfvenic fluctuations (SAFs) is believed to result in the decrease of the Alfvenicity of solar wind fluctuations with increasing heliocentric dist
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6b8919c64665ad68e7e2338b1c001d94
http://arxiv.org/abs/1606.03308
http://arxiv.org/abs/1606.03308
Publikováno v:
arXiv
We present a new algorithm for computing th e electromagnetic fields of currents inside and outside of finite current sources, for arbitrary time variations in the currents. Unexpectedly, we find that our solutions for these fields are free of the co
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ce672d6f4cb04b5b4708b1be86fb6777
https://doi.org/10.1119/1.3682326
https://doi.org/10.1119/1.3682326
Publikováno v:
The Astrophysical Journal. 864:L41
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b8fe59e44d56d5ac6de5bd619aebad9c
https://doi.org/10.3847/2041-8213/aadcfb
https://doi.org/10.3847/2041-8213/aadcfb
Publikováno v:
Nature. 454:63-66
The solar wind blows outward from the Sun and forms a bubble of solar material in the interstellar medium. The termination shock occurs where the solar wind changes from being supersonic (with respect to the surrounding interstellar medium) to being
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::658d5bb3b82f92ade389129540a2a808
https://doi.org/10.1038/nature07024
https://doi.org/10.1038/nature07024