Zobrazeno 1 - 10
of 222
pro vyhledávání: '"Mario H. Acuña"'
Autor:
Jean-Jacques Berthelier, Douglas E. Rowland, Jeffrey Klenzing, Henry Freudenreich, S. Martin, Matthew D. McCarthy, R. F. Pfaff, Mario H. Acuña, J. Houser, Abram R. Jacobson, R. Kramer, P. Uribe, C. Liebrecht, Robert H. Holzworth, R. Fourre, Guan Le, C. Steigies, William M. Farrell, J. Kujawski, Kenneth R. Bromund, F. Hunsaker, N. C. Maynard
Publikováno v:
Space Science Reviews
Space Science Reviews, Springer Verlag, 2021, 217, pp.85. ⟨10.1007/s11214-021-00859-y⟩
Space Science Reviews, Springer Verlag, 2021, 217, pp.85. ⟨10.1007/s11214-021-00859-y⟩
The Vector Electric Field Investigation (VEFI) on the C/NOFS satellite comprises a suite of sensors controlled by one central electronics box. The primary measurement consists of a vector DC and AC electric field detector which extends spherical sens
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b8d345d200d1ea429a93ac6835ed6889
https://hal-insu.archives-ouvertes.fr/insu-03502515/document
https://hal-insu.archives-ouvertes.fr/insu-03502515/document
Autor:
Konrad Schwingenschuh, Karl-Heinz Fornacon, G. Musmann, T. Oddy, M. W. Dunlop, Patrick Brown, A. Balogh, Chris Carr, J. Harris, Karl-Heinz Glassmeier, T. Beek, Mario H. Acuña, E. Georgescu
Publikováno v:
Annales Geophysicae, Vol 19, Pp 1207-1217 (2001)
Annales Geophysicae, Vol 19, Iss 10/12, Pp 1207-1217 (0000)
Annales Geophysicae, Vol 19, Iss 10/12, Pp 1207-1217 (0000)
The accurate measurement of the magnetic field along the orbits of the four Cluster spacecraft is a primary objective of the mission. The magnetic field is a key constituent of the plasma in and around the magnetosphere, and it plays an active role i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::78e542d734eed2d47e2e3e53daa88345
https://www.ann-geophys.net/19/1207/2001/
https://www.ann-geophys.net/19/1207/2001/
Autor:
Mario H. Acuña, Chris Piker, D. Bodet, John E. P. Connerney, Robert J. MacDowall, J. Odom, J. R. Phillips, Scott R. Bounds, S. L. Remington, B. T. Mokrzycki, Douglas E. Rowland, D. Mark, R. T. Dvorsky, Craig Kletzing, D. Crawford, Ondrej Santolik, Roy B. Torbert, R. A. Johnson, Charles W. Smith, R. Schnurr, Vania K. Jordanova, J. Howard, T. F. Averkamp, G. Needell, D. Sheppard, George Hospodarsky, Richard M. Thorne, J. Tyler, M. Chutter, J. S. Dolan, William S. Kurth, R. F. Pfaff, D. L. Kirchner
Publikováno v:
Space Science Reviews. 179:127-181
The Electric and Magnetic Field Instrument and Integrated Science (EMFISIS) investigation on the NASA Radiation Belt Storm Probes (now named the Van Allen Probes) mission provides key wave and very low frequency magnetic field measurements to underst
Autor:
Erin Simpson, Robert P. Lin, Marit Øieroset, Mario H. Acuña, Tai Phan, Jasper Halekas, David L. Mitchell, David Brain
Publikováno v:
Icarus. 206:189-198
More than 490 elliptical aerobraking and science phasing orbits made by Mars Global Surveyor (MGS) in 1997 and 1998 provide unprecedented coverage of the solar wind in the vicinity of the orbits of the martian moons Phobos and Deimos. We have perform
Autor:
David Brain, Jeffrey J. Plaut, Janet G. Luhmann, Mario H. Acuña, J. David Winningham, David Morgan, R. A. Frahm, Jared Espley, D. L. Kirchner, Erling Nielsen, David L. Mitchell, Donald A. Gurnett
Publikováno v:
Icarus. 206:95-103
Mars Advanced Radar for Subsurface and Ionospheric Sounding (MARSIS) is a subsurface and topside ionosphere radar sounder aboard the European Space Agency spacecraft Mars Express, in orbit at Mars since 25 December 2003, and in operation since 17 Jun
Autor:
Sean C. Solomon, Thomas H. Zurbuchen, Ralph L. McNutt, H. Uno, George Gloeckler, Brian J. Anderson, James A. Slavin, Catherine L. Johnson, Michael E. Purucker, Mario H. Acuña, Jim M. Raines, Haje Korth
Publikováno v:
Space Science Reviews. 152:307-339
The magnetic field strength of Mercury at the planet’s surface is approximately 1% that of Earth’s surface field. This comparatively low field strength presents a number of challenges, both theoretically to understand how it is generated and obse
Autor:
James A. Slavin, Robert E. Gold, George C. Ho, Thomas H. Zurbuchen, Menelaos Sarantos, Ralph L. McNutt, Brian J. Anderson, George Gloeckler, David Schriver, Haje Korth, Mehdi Benna, Mario H. Acuña, Stamatios M. Krimigis, Sean C. Solomon, Daniel N. Baker, Scott A. Boardsen, Jim M. Raines, Pavel M. Trávníček
Publikováno v:
Science. 324:606-610
MESSENGER from Mercury The spacecraft MESSENGER passed by Mercury in October 2008, in what was the second of three fly-bys before it settles into the planet's orbit in 2011. Another spacecraft visited Mercury in the mid-1970s, which mapped 45% of the
Autor:
Peter J. Wasilewski, Mario H. Acuña, Robert Lillis, John E. P. Connerney, Norman F. Ness, Gunther Kletetschka
Publikováno v:
Meteoritics & Planetary Science. 44:131-140
Intense magnetic anomalies over Martian surface suggest preservation of large volumes of very old crust (>3 Gyr) that formed in the presence of a global magnetic field. The global distribution of the magnetic intensities observed above the Martian cr
Autor:
Jean-André Sauvaud, P. Schroeder, Janet G. Luhmann, Stuart D. Bale, Ying Liu, Mario H. Acuña, Robert P. Lin, Yuan Li, Reinhold Müller-Mellin, Linghua Wang
Publikováno v:
The Astrophysical Journal. 689:563-571
The biggest halo coronal mass ejection (CME) since the Halloween storm in 2003, which occurred on 2006 December 13, is studied in terms of its solar source and heliospheric consequences. The CME is accompanied by an X3.4 flare, EUV dimmings and coron
Autor:
Rosemary M. Killen, Haje Korth, Pavel Trávníček, George Gloeckler, Ralph L. McNutt, Larry R. Nittler, Sean C. Solomon, George C. Ho, Jim M. Raines, Mehdi Benna, Daniel N. Baker, Stamatios M. Krimigis, James A. Slavin, R. D. Starr, Mario H. Acuña, David Schriver, Thomas H. Zurbuchen, Robert E. Gold, Brian J. Anderson
Publikováno v:
Science. 321:85-89
Observations by MESSENGER show that Mercury's magnetosphere is immersed in a comet-like cloud of planetary ions. The most abundant, Na + , is broadly distributed but exhibits flux maxima in the magnetosheath, where the local plasma flow speed is high