Standard
Local time asymmetries in Saturn’s magnetosphere. / Carbary, J. F.; Mitchell, D. G.; Rymer, A. M. et al.
Dawn‐Dusk Asymmetries in Planetary Plasma Environments. ed. / Stein Haaland; Andrei Runov; Colin Forsyth. American Geophysical Union, 2017. p. 323-336 (Geophysical Monograph Series).
Research output: Contribution in Book/Report/Proceedings - With ISBN/ISSN › Chapter
Harvard
Carbary, JF, Mitchell, DG, Rymer, AM, Krupp, N, Hamilton, D, Krimigis, SM
& Badman, SV 2017,
Local time asymmetries in Saturn’s magnetosphere. in S Haaland, A Runov & C Forsyth (eds),
Dawn‐Dusk Asymmetries in Planetary Plasma Environments. Geophysical Monograph Series, American Geophysical Union, pp. 323-336.
https://doi.org/10.1002/9781119216346.ch25APA
Carbary, J. F., Mitchell, D. G., Rymer, A. M., Krupp, N., Hamilton, D., Krimigis, S. M.
, & Badman, S. V. (2017).
Local time asymmetries in Saturn’s magnetosphere. In S. Haaland, A. Runov, & C. Forsyth (Eds.),
Dawn‐Dusk Asymmetries in Planetary Plasma Environments (pp. 323-336). (Geophysical Monograph Series). American Geophysical Union.
https://doi.org/10.1002/9781119216346.ch25Vancouver
Carbary JF, Mitchell DG, Rymer AM, Krupp N, Hamilton D, Krimigis SM et al.
Local time asymmetries in Saturn’s magnetosphere. In Haaland S, Runov A, Forsyth C, editors, Dawn‐Dusk Asymmetries in Planetary Plasma Environments. American Geophysical Union. 2017. p. 323-336. (Geophysical Monograph Series). doi: 10.1002/9781119216346.ch25
Author
Carbary, J. F. ; Mitchell, D. G. ; Rymer, A. M. et al. /
Local time asymmetries in Saturn’s magnetosphere. Dawn‐Dusk Asymmetries in Planetary Plasma Environments. editor / Stein Haaland ; Andrei Runov ; Colin Forsyth. American Geophysical Union, 2017. pp. 323-336 (Geophysical Monograph Series).
Bibtex
@inbook{8c4dbadd474845f19ff30b13c0258ebb,
title = "Local time asymmetries in Saturn{\textquoteright}s magnetosphere",
abstract = "The Cassini orbiter has observed the magnetosphere of Saturn in situ from July 2004 to the present. The spacecraft has visited nearly all local times and a large range of latitudes, including both northern and southern hemispheres, for a large fraction of a Saturn year (=29 Earth years). Local time asymmetries have been observed in the thermal plasma, the energetic particles, energetic neutral atoms, magnetic fields and aurora. Some of these are dawn-to-dusk asymmetries and have Earth-like analogies. Unlike Earth{\textquoteright}s magnetosphere, however, Saturn{\textquoteright}s magnetosphere is rotationally dominated, has no observable tilt relative to the spin axis, and has a major internal plasma and neutrals source in the icy moon Enceladus. These factors contribute to a number of local time asymmetries that are not dawn-to-dusk. This paper reviews Saturn{\textquoteright}s local time asymmetries in charged particles, magnetic fields, and energetic neutral atoms, showing how some are Earth-like and some are not.",
author = "Carbary, {J. F.} and D. G. Mitchell and Rymer, {A. M.} and N. Krupp and D. Hamilton and Krimigis, {S. M.} and Badman, {Sarah Victoria}",
year = "2017",
month = oct,
doi = "10.1002/9781119216346.ch25",
language = "English",
isbn = "9781119216322",
series = "Geophysical Monograph Series",
publisher = "American Geophysical Union",
pages = "323--336",
editor = "Stein Haaland and Andrei Runov and Colin Forsyth",
booktitle = "Dawn‐Dusk Asymmetries in Planetary Plasma Environments",
address = "United States",
}
RIS
TY - CHAP
T1 - Local time asymmetries in Saturn’s magnetosphere
AU - Carbary, J. F.
AU - Mitchell, D. G.
AU - Rymer, A. M.
AU - Krupp, N.
AU - Hamilton, D.
AU - Krimigis, S. M.
AU - Badman, Sarah Victoria
PY - 2017/10
Y1 - 2017/10
N2 - The Cassini orbiter has observed the magnetosphere of Saturn in situ from July 2004 to the present. The spacecraft has visited nearly all local times and a large range of latitudes, including both northern and southern hemispheres, for a large fraction of a Saturn year (=29 Earth years). Local time asymmetries have been observed in the thermal plasma, the energetic particles, energetic neutral atoms, magnetic fields and aurora. Some of these are dawn-to-dusk asymmetries and have Earth-like analogies. Unlike Earth’s magnetosphere, however, Saturn’s magnetosphere is rotationally dominated, has no observable tilt relative to the spin axis, and has a major internal plasma and neutrals source in the icy moon Enceladus. These factors contribute to a number of local time asymmetries that are not dawn-to-dusk. This paper reviews Saturn’s local time asymmetries in charged particles, magnetic fields, and energetic neutral atoms, showing how some are Earth-like and some are not.
AB - The Cassini orbiter has observed the magnetosphere of Saturn in situ from July 2004 to the present. The spacecraft has visited nearly all local times and a large range of latitudes, including both northern and southern hemispheres, for a large fraction of a Saturn year (=29 Earth years). Local time asymmetries have been observed in the thermal plasma, the energetic particles, energetic neutral atoms, magnetic fields and aurora. Some of these are dawn-to-dusk asymmetries and have Earth-like analogies. Unlike Earth’s magnetosphere, however, Saturn’s magnetosphere is rotationally dominated, has no observable tilt relative to the spin axis, and has a major internal plasma and neutrals source in the icy moon Enceladus. These factors contribute to a number of local time asymmetries that are not dawn-to-dusk. This paper reviews Saturn’s local time asymmetries in charged particles, magnetic fields, and energetic neutral atoms, showing how some are Earth-like and some are not.
U2 - 10.1002/9781119216346.ch25
DO - 10.1002/9781119216346.ch25
M3 - Chapter
SN - 9781119216322
T3 - Geophysical Monograph Series
SP - 323
EP - 336
BT - Dawn‐Dusk Asymmetries in Planetary Plasma Environments
A2 - Haaland, Stein
A2 - Runov, Andrei
A2 - Forsyth, Colin
PB - American Geophysical Union
ER -
