Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Theresa Kucera"'
Autor:
S. Hill, J. Gerulskis, C. Chrissotimos, Russell A. Howard, L. Ratta, Antoinette B. Galvin, E. Drobnes, Theresa Kucera, B. Mendez, Janet G. Luhmann, K. Beisser, Laura Peticolas, D. J. Michels, Robert J. MacDowall, K. Marren, N. Craig
Publikováno v:
Space Science Reviews. 136:627-646
The STEREO mission’s Education and Outreach (E/PO) program began early enough its team benefited from many lessons learned as NASA’s E/PO profession matured. Originally made up of discrete programs, by launch the STEREO E/PO program had developed
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c687ec9bb977774b5e04cdc5b0742847
https://doi.org/10.1007/s11214-007-9287-y
https://doi.org/10.1007/s11214-007-9287-y
Autor:
Ed Sittler, Dave McComas, Theresa Kucera, Richard R. Fisher, M. Guhathakurta, Ruth M. Skoug, Sarah Gibson
Publikováno v:
Space Science Reviews. 97:45-50
The large-scale coronal magnetic fields of the Sun are believed to play an important role in organizing the coronal plasma and channeling the high and low speed solar wind along the open magnetic field lines of the polar coronal holes and the rapidly
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1a203ce22a3fa0c99e35d0b6346670f0
https://doi.org/10.1023/a:1011834413147
https://doi.org/10.1023/a:1011834413147
Autor:
Madhullika Guhathakurta, Ed Sittler, Richard Fisher, Theresa Kucera, Sarah Gibson, Dave McComas, Ruth Skoug
Publikováno v:
The 3-D Heliosphere at Solar Maximum ISBN: 9789048157235
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::842c7fff4b07c893441cb24208f3b03c
https://doi.org/10.1007/978-94-017-3230-7_8
https://doi.org/10.1007/978-94-017-3230-7_8
Autor:
Guhathakurta, Madhullika, Sittler, Ed, Fisher, Richard, Kucera, Theresa, Gibson, Sarah, McComas, Dave, Skoug, Ruth
Publikováno v:
Space Science Reviews; May2001, Vol. 97 Issue 1-4, p45-50, 6p
Autor:
R.G. Marsden
Our knowledge of the heliosphere in three dimensions near solar minimum has advanced significantly in the last 10 years, largely as a result of the on-going ESAINASA Ulysses mission. Similar advances in our understanding of the global heliosphere nea