Zobrazeno 1 - 10
of 256
pro vyhledávání: '"Norman F. Ness"'
Autor:
L. F. Burlaga, Lan Jian, Norman F. Ness, William S. Kurth, D. A. Gurnett, D. B. Berdichevsky, J. Park, Adam Szabo
Publikováno v:
The Astrophysical Journal. 911:61
Voyager 1 has been moving through the very local interstellar medium (VLISM) from the time that it crossed the heliopause on 2012/DOY 238 to 2020/DOY 292. Three notable objects in the magnetic field of the VLISM have been observed: two shocks and one
Autor:
D. B. Berdichevsky, Adam Szabo, Norman F. Ness, L. F. Burlaga, John D. Richardson, J. Park, Lan Jian, A. Koval
Publikováno v:
The Astrophysical Journal. 906:119
We present observations of the magnetic field in the outermost region of the heliosheath made by Voyager 2 (V2) from 2016 to 2018.6, just before V2 entered the magnetic barrier inside of the heliopause. The average magnetic field strength (B) during
Autor:
L. F. Burlaga, R. B. Decker, Bryant C. Heikkila, Norman F. Ness, Stamatios M. Krimigis, A. C. Cummings, William S. Kurth, D. A. Gurnett, Nand Lal, E. C. Stone
Publikováno v:
The Astronomical Journal. 161:11
The Voyager 1 (V1) and Voyager 2 (V2) spacecraft were launched in 1977 on a mission to explore the outer planets and reach the heliopause, the boundary between the hot solar plasma and the relatively cool interstellar plasma. V1 reached the heliopaus
Publikováno v:
The Astrophysical Journal Letters. 901:L2
Voyager 1 (V1) observed q-Gaussian distributions of 1 hr increments of the components the magnetic field ${\boldsymbol{B}}$ throughout the very local interstellar medium (VLISM) on scales on the order of 1 year, from 2013 through 2019, excluding the
Publikováno v:
The Astronomical Journal. 160:40
J.P. was supported by the NASA Voyager Project to the NASA/GSFC Magnetometer Team under internal NASA funding. N.F.N. was supported by the NASA Voyager Project under a cooperative agreement to the University of Maryland, Baltimore County. L.F.B. was
Autor:
Norman F. Ness
Publikováno v:
Space Science Reviews. 152:5-22
This chapter gives a brief overview of the major observational advances in our quantitative knowledge of the intrinsic magnetic fields of the 8 planets, except Earth, from Mercury to Neptune, since “The Space Age” began on 4 October 1957 with 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:
Norman F. Ness, Robert B. Decker, Stamatios M. Krimigis, A. C. Cummings, Donald A. Gurnett, L. F. Burlaga, William S. Kurth, E. C. Stone
On or about 2012 August 25, the Voyager 1 spacecraft crossed the heliopause into the nearby interstellar plasma. In the nearly three years that the spacecraft has been in interstellar space, three notable particle and field disturbances have been obs
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2d85bcff892d7ddabb3661442393bf8d
https://resolver.caltech.edu/CaltechAUTHORS:20151020-083336736
https://resolver.caltech.edu/CaltechAUTHORS:20151020-083336736
Autor:
Norman F. Ness, Peter J. Wasilewski, Mario H. Acuña, Tomas Kohout, Michael D Fuller, Emilio Herrero-Bervera, Gunther Kletetschka
Publikováno v:
Physics of the Earth and Planetary Interiors. 154:290-298
Thermally acquired remanent magnetization is important for the estimation of the past magnetic field present at the time of cooling. Rocks that cool slowly commonly contain magnetic grains of millimeter scale. This study investigated 1-mm-sized magne
Autor:
R. P. Lin, John E. P. Connerney, Mario H. Acuña, Norman F. Ness, David L. Mitchell, H. Rème, Gunther Kletetschka
Publikováno v:
Proceedings of the National Academy of Sciences. 102:14970-14975
Mars currently has no global magnetic field of internal origin but must have had one in the past, when the crust acquired intense magnetization, presumably by cooling in the presence of an Earth-like magnetic field (thermoremanent magnetization). A n