Zobrazeno 1 - 4
of 4
pro vyhledávání: '"S. E. Lasley"'
Autor:
W. I. Axford, E. Marsch, J. Geiss, K. C. Hsieh, Eberhard Möbius, Berndt Klecker, Peter Wurz, J. A. Paquette, M. A. Lee, Peter Bochsler, B. Wilken, S. E. Lasley, Marcia Neugebauer, Hans Balsiger, Reinald Kallenbach, K.-U. Reiche, A. Bürgi, M. I. Verigin, G. G. Managadze, H. Grünwaldt, D. Hovestadt, F. M. Ipavich, Michael A. Coplan, Antoinette B. Galvin, George Gloeckler, Manfred Scholer, Fritz Gliem, Martin Hilchenbach, S. Hefti
Publikováno v:
Journal of Geophysical Research: Space Physics. 103:17205-17213
The proton monitor, a small subsensor in the Charge, Element, and Isotope Analysis System/Mass Time-of-Flight (CELIAS/MTOF) experiment on the SOHO spacecraft, was designed to assist in the interpretation of measurements from the high mass resolution
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2e525cf5e3e124137377be7aab75b5cd
https://doi.org/10.1029/97ja02770
https://doi.org/10.1029/97ja02770
Publikováno v:
AIP Conference Proceedings.
The MTOF sensor uses time of flight measurements in a harmonic potential region to identify elements and isotopes in the solar wind with excellent mass resolution. The combination of MTOF’s large bandwidth electrostatic deflection system and the 3-
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::03958a966e707bd73ef3e4f1ba71caa5
https://doi.org/10.1063/1.1433989
https://doi.org/10.1063/1.1433989
Publikováno v:
AIP Conference Proceedings.
Chromium and iron are two heavy elements in the solar wind with similar masses. The MTOF (Mass Time Of Flight) sensor of the CELIAS investigation on the SOHO spacecraft easily allows these two elements to be resolved from one another. Taking the rati
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::049c06300433770a99681217f4af1778
https://doi.org/10.1063/1.1433985
https://doi.org/10.1063/1.1433985
Publikováno v:
SPIE Proceedings.
In the proposed Mercury-Messenger mission, a satellite will approach the Sun to a distance of around 0.3 AU. A plasma instrument to be flown on this satellite provides a unique possibility to probe the inner heliosphere in a distance range which has
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::587fe93d0b27c1e239a5b37529cf5c0f
https://doi.org/10.1117/12.330260
https://doi.org/10.1117/12.330260