Zobrazeno 1 - 10
of 18
pro vyhledávání: '"H. J. McAndrews"'
Autor:
Jared Leisner, Chris S. Arridge, Krishan K. Khurana, Sascha Kempf, Emma J. Bunce, Matthew H. Burger, M. K. Dougherty, P. Schippers, William S. Kurth, Geraint H. Jones, Michelle F. Thomsen, Edward C. Sittler, Kirk C. Hansen, H. J. McAndrews, Hsiang-Wen Hsu, Howard Smith, Robert E. Johnson, Norbert Krupp, Chris Paranicas, Christopher T. Russell, N. André, Elias Roussos
Publikováno v:
Space Science Reviews. 164:1-83
Saturn’s rich magnetospheric environment is unique in the solar system, with a large number of active magnetospheric processes and phenomena. Observations of this environment from the Cassini spacecraft has enabled the study of a magnetospheric sys
Autor:
Anne Wellbrock, M. K. Dougherty, Michelle F. Thomsen, D. T. Young, Hanying Wei, Andrew J. Coates, Christopher T. Russell, Y. J. Ma, H. J. McAndrews, Kirk C. Hansen
Publikováno v:
Advances in Space Research. 48:314-322
Observations of unusually large magnetic fields in the ionosphere indicate periods of maximum stress on Titan’s ionosphere and potentially of the strongest loss rates of ionospheric plasma. During Titan flyby T42, the observed magnetic field attain
Autor:
Nicholas Achilleos, Chris S. Arridge, Andrew J. Coates, Michele K. Dougherty, H. J. McAndrews, Adam Masters, Cesar Bertucci, S. J. Kanani
Publikováno v:
Planetary and Space Science. 57:1769-1778
Crossings of Saturn's magnetopause made by the Cassini spacecraft on 12, 13 and 17 March 2006 are analysed. During this period Cassini's trajectory was approximately parallel to the magnetopause boundary given by a model of the surface. Magnetic fiel
Autor:
Glyn Collinson, Andrew J. Coates, D. T. Young, Chris S. Arridge, L. K. Gilbert, Gethyn R. Lewis, Anne Wellbrock, Colin Forsyth, Caitriona M. Jackman, Michele K. Dougherty, Edward C. Sittler, Christopher T. Russell, Andrew Walsh, H. J. McAndrews
Publikováno v:
Planetary and Space Science. 57:2032-2047
In this paper Saturn's nightside and pre-dawn electron (0.5 eV–28 keV) plasma sheet is studied using Cassini plasma electron and magnetic field data from 2006. Case studies are presented which exemplify the typical and atypical states of the plasma
Autor:
Michelle F. Thomsen, H. J. McAndrews, R. J. Wilson, R. L. Tokar, Andrew J. Coates, Krishan K. Khurana, Michael G. Henderson, E. C. Sittler, Chris S. Arridge, Michele K. Dougherty, Caitriona M. Jackman
Publikováno v:
Planetary and Space Science. 57:1714-1722
We present a bulk ion flow map from the nightside, equatorial region of Saturn's magnetosphere derived from the Cassini CAPS ion mass spectrometer data. The map clearly demonstrates the dominance of corotation flow over radial flow and suggests that
Autor:
Michelle F. Thomsen, Krishan K. Khurana, Michael G. Henderson, R. J. Wilson, R. L. Tokar, Chris S. Arridge, Andrew J. Coates, Michele K. Dougherty, Edward C. Sittler, Caitriona M. Jackman, H. J. McAndrews
Publikováno v:
Planetary and Space Science. 97:86-87
The authors regret that Figure 4 of McAndrews et al. (2009) has been found to contain three errors: first, the horizontal scale is slightly mislabeled; second, the vertical scale in the bottom panel (the Alfven travel time) is wrong by a factor of 10
Autor:
Nick Sergis, Stamatios M. Krimigis, H. J. McAndrews, Norbert Krupp, S. J. Kanani, Michele K. Dougherty, Geraint H. Jones, Andrew Fazakerley, Andrew J. Coates, D. T. Young, Chris S. Arridge, Kirk C. Hansen
Publikováno v:
Journal of Geophysical Research: Space Physics. 115
The shape and location of a planetary magnetopause can be determined by balancing the solar wind dynamic pressure with the magnetic and thermal pressures found inside the boundary. Previous studies have found the kronian magnetosphere to show rigidit
Publikováno v:
Geophysical Research Letters, 36, Article L16101. (2009)
We present results from an investigation of Cassini encounters with Saturn's magnetotail current sheet, using magnetic field and plasma data. In the first of two intervals shown, small periodic changes in the north-south component of the magnetic fie
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d848506220d034de6a8fc3a04aca3ac8
https://discovery.ucl.ac.uk/id/eprint/647080/1/2009GL039149.pdf
https://discovery.ucl.ac.uk/id/eprint/647080/1/2009GL039149.pdf
Autor:
Andrew J. Coates, L. Billingham, H. J. McAndrews, John T. Steinberg, Adam Masters, George Hospodarsky, Steven J. Schwartz, Chris S. Arridge, Nick Sergis, Michelle F. Thomsen, Michele K. Dougherty
Publikováno v:
Journal of Geophysical Research: Space Physics. 114
[1] We present evidence for the occurrence of hot flow anomalies (HFAs) at Saturn’s bow shock. A survey of Cassini magnetic field and electron data taken upstream of the dawn flank bow shock is carried out in order to identify Kronian HFAs. Sevente
Autor:
Nicholas Achilleos, Andrew J. Coates, Chris S. Arridge, Michele K. Dougherty, Emma J. Bunce, Geraint H. Jones, Norbert Krupp, D. G. Mitchell, Caitriona M. Jackman, H. J. McAndrews, Christopher T. Russell
Publikováno v:
Journal of Geophysical Research: Space Physics. 113
Three instances of tail reconnection events at Saturn involving the ejection of plasmoids downtail have been reported by Jackman et al. (2007) using data from Cassini’s magnetometer (MAG). Here we show two newly discovered events, as identified in