Zobrazeno 1 - 10
of 127
pro vyhledávání: '"G. R. Wilson"'
Autor:
N. C. Maynard, W. J. Burke, Y. Ebihara, D. M. Ober, G. R. Wilson, K. D. Siebert, J. D. Winningham, L. J. Lanzerotti, C. J. Farrugia, M. Ejiri, H. Rème, A. Balogh, A. Fazakerley
Publikováno v:
Annales Geophysicae, Vol 24, Pp 3071-3098 (2006)
We combine in situ measurements from Cluster with high-resolution 557.7 nm all-sky images from South Pole to investigate the spatial and temporal evolution of merging on the dayside magnetopause. Variations of 557.7 nm emissions were observed at a
Externí odkaz:
https://doaj.org/article/0bb2ccaf2566405b86320ab41753083a
Publikováno v:
Journal of Geophysical Research: Space Physics. 127
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e9e99a3983687052486150b0bae55156
https://doi.org/10.1029/2022ja030345
https://doi.org/10.1029/2022ja030345
Publikováno v:
Astrobiology. 7:545-577
The Mars Program Plan includes an integrated and coordinated set of future candidate missions and investigations that meet fundamental science objectives of NASA and the Mars Exploration Program (MEP). At the time this paper was written, these possib
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3f3d8fdd519930cde9df8a3692347b2e
https://doi.org/10.1089/ast.2007.0153
https://doi.org/10.1089/ast.2007.0153
Publikováno v:
Environmental Modelling & Software. 19:205-215
TEAM (Texas Tech Erosion Analysis Model) is a process-based mathematical model that predicts detachment, movement, and deposition of soil particles associated with wind processes. TEAM also simulates the suspension and movement of dust above and down
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ecccfc932880ad9979199ed547c24a73
https://doi.org/10.1016/s1364-8152(03)00124-5
https://doi.org/10.1016/s1364-8152(03)00124-5
Autor:
John W. Keller, M.-C. Fok, T. M. Stephen, J. M. Quinn, B. El Marji, S. A. Fuselier, Scott A. Boardsen, Dennis J. Chornay, Peter Wurz, Michael R. Collier, D. C. Hamilton, Barbara L. Giles, G. R. Wilson, A. G. Ghielmetti, K. W. Ogilvie, B. L. Peko, Thomas E. Moore, James L. Burch, Edmond C. Roelof
Publikováno v:
Scopus-Elsevier
We report observations of neutral atoms from the solar wind in the Earth's vicinity with the low-energy neutral atom (LENA) imager on the Imager for Magnetopause-to-Aurora Global Exploration (IMAGE) spacecraft. This instrument was designed to be capa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d36e620395584bc7af6c574db2399743
https://doi.org/10.1029/2000ja000382
https://doi.org/10.1029/2000ja000382
Publikováno v:
Journal of Geophysical Research: Space Physics. 106:18981-18993
Ionospheric ions are energized to suprathermal energies (10–1000 eV) in the auroral zone. This produces a much larger quantity of escaping O+ ions than would otherwise occur, given typical ionospheric energies. Until recently, only limited work had
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7802d6e2b1f2b60fdf10b65a7e013d02
https://doi.org/10.1029/2000ja000434
https://doi.org/10.1029/2000ja000434
Autor:
John W. Keller, B. L. Peko, K. W. Ogilvie, James L. Burch, Thomas E. Moore, J. M. Quinn, T. M. Stephen, Michael R. Collier, Peter Wurz, Barbara L. Giles, D. C. Hamilton, Dennis J. Chornay, Federico A. Herrero, G. R. Wilson, S. A. Fuselier, A. G. Ghielmetti
Publikováno v:
Geophysical Research Letters. 28:1143-1146
We report observations of low energy neutral atoms (LENA) from the solar wind and the ionosphere, obtained by the LENA Imager on the IMAGE spacecraft. The LENA Imager detects and images LENAs arriving at the spacecraft from within a 90° field of vie
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e188a0552ede51bdfb198dfc6e6502f7
https://doi.org/10.1029/2000gl012500
https://doi.org/10.1029/2000gl012500
Publikováno v:
Planetary and Space Science. 48:1349-1355
Experiments were conducted to determine the flux of dust (particles less than few microns in diameter) under Martian atmospheric conditions for surface of three aerodynamic roughness (z(sub 0)). For smooth surface on Mars (z(sub 0) = 0.00125 cm corre
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::05993f2222667b490ca104d52c22f210
https://doi.org/10.1016/s0032-0633(00)00115-x
https://doi.org/10.1016/s0032-0633(00)00115-x
Publikováno v:
Journal of Atmospheric and Solar-Terrestrial Physics. 62:901-909
Intense (10 6 cm −2 sr −1 s −1 ) fluxes of upflowing ENAs from the polar cap have been observed in the energy range 0.1–13 keV (hydrogen assumed) from the Astrid satellite at 1000 km altitude. If a source altitude of 400 km is assumed, the EN
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3ca2ded75efea7b819b7d6a9c8ba288c
https://doi.org/10.1016/s1364-6826(00)00040-7
https://doi.org/10.1016/s1364-6826(00)00040-7
Publikováno v:
Journal of Geophysical Research: Space Physics. 104:17263-17275
We apply a recently developed dynamic fluid-kinetic (DyFK) model to simulate and investigate the effects of soft auroral electron precipitation and perpendicular ion heating by waves on the plasma outflow along auroral field lines. The DyFK model is
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7ae4455c4b7bd08a2c042dbd611563b5
https://doi.org/10.1029/1999ja900114
https://doi.org/10.1029/1999ja900114