Zobrazeno 1 - 10
of 72
pro vyhledávání: '"Vytenis M. Vasyliunas"'
Autor:
Rumi Nakamura, Alessandro Retinò, Michael Hesse, Tai Phan, Larry Kepko, Lei Li, Lei Dai, Y. C. Zhang, Yuri V. Khotyaintsev, Rongsheng Wang, Elena Grigorenko, Daniel B. Graham, Chi Wang, Shiyong Huang, Zhiming Cai, Linggao Kong, Huishan Fu, Jianshen He, Vassilis Angelopoulos, Andrei Runov, Kyoung-Joo Hwang, Quanming Lu, Meng Zhou, Walter D. Gonzalez, Vytenis M. Vasyliunas, Lev Zelenyi, Malcolm Dunlop, Philippe Escoubet
Publikováno v:
Frontiers in Physics
Frontiers in Physics, Frontiers, 2020, 8, ⟨10.3389/fphy.2020.00089⟩
Frontiers in Physics, Vol 8 (2020)
Frontiers in Physics, Frontiers, 2020, 8, ⟨10.3389/fphy.2020.00089⟩
Frontiers in Physics, Vol 8 (2020)
A major subset of solar–terrestrial relations, responsible, in particular, for the driver of space weather phenomena, is the interaction between the Earth's magnetosphere and the solar wind. As one of the most important modes of the solar–wind–
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5e09946cf66c9845289730ab74f4a384
http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-412334
http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-412334
Autor:
Donald V. Reames, V. J. Pizzo, Jean-Louis Bougeret, Mario H. Acuña, Dusan Odstrcil, David J. McComas, Pete Riley, Andrew Davis, Davin Larson, K. W. Ogilvie, R. Mueller-Mellin, A. C. Cummings, G. M. Mason, H. Kunow, Robert P. Lin, Tamas I. Gombosi, C. Aoustin, D. W. Curtis, A. Korth, T. T. von Rosenvinge, T. R. Sanderson, Vytenis M. Vasyliunas, Jon A. Linker, Volker Bothmer, Darren L. DeZeeuw, Mark E. Wiedenbeck, Philippe Louarn, Christopher T. Russell, P. Schroeder, C. K. Ng, Karoly Kecskemety, Richard G. Marsden, J. Dandouras, R. A. Mewaldt, E. C. Stone, Janet G. Luhmann, A. Sauvaud, J. T. Gosling
Publikováno v:
Advances in Space Research. 36:1534-1543
The in situ measurements of particles and CME transients (IMPACT) investigation on the twin STEREO spacecraft focuses on the solar energetic particle, solar wind and suprathermal electron, and magnetic field measurements needed to address STEREO’s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9d2341f71108ef40f473d7e108dde78b
https://doi.org/10.1016/j.asr.2005.03.033
https://doi.org/10.1016/j.asr.2005.03.033
Autor:
Dennis L. Gallagher, Bodo W. Reinisch, Gary S. Sales, Shing Fung, Paul Song, James L. Green, Vytenis M. Vasyliunas, Xueqin Huang
Publikováno v:
Geophysical Research Letters. 28:4521-4524
A new technique is introduced that remotely measures the plasma density profile in the plasmasphere. Radio plasma imager (RPI) echo observations provide echo delay time as function of frequency, from which the plasma density as function of position a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9b5ca70cf1f3e6ac92ad712e05cb427c
https://doi.org/10.1029/2001gl013684
https://doi.org/10.1029/2001gl013684
Autor:
Bruce T. Tsurutani, T.J. Hughes, J. K. Arballo, Gordon Rostoker, X.-Y. Zhou, Walter D. Gonzalez, Tohru Araki, Vytenis M. Vasyliunas, D. B. Berdichevsky, Gurbax S. Lakhina, H. Yang, R. P. Lepping, Jolene S. Pickett
Publikováno v:
Journal of Atmospheric and Solar-Terrestrial Physics. 63:513-522
Significant charged-particle precipitation occurs in the dayside auroral zone during and after interplanetary shock impingements on the Earth's magnetosphere. The precipitation intensities and spatial and temporal evolution are discussed. Although th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d43bf8d7e59b45abb672860bc30fba33
https://doi.org/10.1016/s1364-6826(00)00161-9
https://doi.org/10.1016/s1364-6826(00)00161-9
Autor:
G.S. Lakhina, Bruce T. Tsurutani, X.-Y. Zhou, G. Haerendel, J. K. Arballo, Vytenis M. Vasyliunas
Publikováno v:
Surveys in Geophysics. 22:101-130
Dayside near-polar auroral brightenings occur when interplanetary shocks impinge upon the Earth's magnetosphere. The aurora first brightens near local noon and then propagates toward dawn and dusk along the auroral oval. The propagation speed of this
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::01ce18b83cd794fbce992900abcf0398
https://doi.org/10.1023/a:1012952414384
https://doi.org/10.1023/a:1012952414384
Autor:
A. S. Sharma, Manuel Grande, Howard J. Singer, Ioannis A. Daglis, Gordon Rostoker, Wolfgang Baumjohann, Bruce T. Tsurutani, John L. Phillips, Walter D. Gonzalez, E. G. D. Reeves, J. A. Joselyn, Yohsuke Kamide, Vytenis M. Vasyliunas, Robert L. McPherron
Publikováno v:
Journal of Geophysical Research: Space Physics. 103:17705-17728
This paper attempts to summarize the current understanding of the storm/substorm relationship by clearing up a considerable amount of controversy and by addressing the question of how solar wind energy is deposited into and is dissipated in the const
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7b378b41f5a96917814c7798c6c14ba4
https://doi.org/10.1029/98ja01426
https://doi.org/10.1029/98ja01426
Autor:
Manfred Scholer, Kalevi Mursula, Zuyin Pu, A. Korth, Wing-Huen Ip, Daniel N. Baker, P. Tanskanen, Manuel Grande, D. Hall, P. W. Daly, Ioannis A. Daglis, J. B. Blake, Joachim Woch, Larry R. Lyons, Vytenis M. Vasyliunas, W. Güttler, W. I. Axford, F. Sørass, S. McKenna-Lawlor, I. Sandahl, Michael Schulz, B. Wilken, J. F. Fennell, S. Ullaland, Richard D. Belian, R. Rathje, Stefano Livi, K. Kecsueméty, G. Kremser, Fritz Gliem, E. T. Sarris, Theodore A. Fritz, H. Borg
Publikováno v:
Space Science Reviews. 79:399-473
The RAPID spectrometer (Research with Adaptive Particle Imaging Detectors) for the Cluster mission is an advanced particle detector for the analysis of suprathermal plasma distributions in the energy range from 20–400 keV for electrons, 40 keV–15
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2902fa51378ebdf5adeb7c47608fa0a0
https://doi.org/10.1023/a:1004994202296
https://doi.org/10.1023/a:1004994202296
Autor:
Norman F. Ness, John D. Richardson, Vytenis M. Vasyliunas, Charles W. Smith, John W. Belcher, R. P. Lepping, Ming Zhang
Publikováno v:
Geophysical Research Letters. 18:1071-1074
Plasma and magnetic field observations from the Voyager 2 spacecraft when it was outbound from Neptune reveal low-frequency waves in the solar wind which are clearly associated with the planet. The waves have frequencies below the proton cyclotron fr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7262a44db2fccc618e66ac251c87837d
https://doi.org/10.1029/91gl01050
https://doi.org/10.1029/91gl01050
Autor:
Thomas H. Zurbuchen, Karoly Kecskemety, M. J. Reiner, Charlie J. Farrugia, Jon A. Linker, Antoinette B. Galvin, A. Llebaria, Noé Lugaz, J. W. Cook, Dusan Odstrcil, Sami K. Solanki, Rainer Schwenn, David M. Alexander, Martin A. Lee, Manfred Scholer, Victor J. Pizzo, József Kóta, Markus J. Aschwanden, Ilia I. Roussev, Vytenis M. Vasyliunas, L. F. Burlaga, Robert F. Wimmer-Schweingruber, Bernd Inhester, Anne Sandman, Ward B. Manchester, Thomas Wiegelmann, Donald V. Reames, Peter Bochsler, Peter A. Robinson, Pete Riley, Milan Maksimovic, M. L. Kaiser, C. K. Ng, Janet G. Luhmann, Z. Mikic, Volker Bothmer, Russell A. Howard, Tamas I. Gombosi, L. M. Blush, P. C. Liewer, Iver H. Cairns
Publikováno v:
Space Science Reviews
Space Science Reviews, 2008, 136 (136, 1-4), pp.565-604. ⟨10.1007/s11214-006-9027-8⟩
Space Science Reviews, 2008, 136 (136, 1-4), pp.565-604. ⟨10.1007/s11214-006-9027-8⟩
International audience; We summarize the theory and modeling efforts for the STEREO mission, which will be used to interpret the data of both the remote-sensing (SECCHI, SWAVES) and in-situ instruments (IMPACT, PLASTIC). The modeling includes the cor
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::11c19eed9edea7e2858c960d40a29b08
https://hal.science/hal-03742804
https://hal.science/hal-03742804
Publikováno v:
Geophysical Research Letters. 17:2285-2288
Voyager's post-encounter trajectory at Neptune allows the directions of the magnetic field in the magnetosheath produced by the draping of the typical interplanetary field and by alignment with the magnetotail to be distinguished. Changes of the fiel
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::87ac395a83e949ae60ebdc70f9b6e970
https://doi.org/10.1029/gl017i013p02285
https://doi.org/10.1029/gl017i013p02285