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- Publications
- Influence
Modeling the size and shape of Saturn's magnetopause with variable dynamic pressure
- C. Arridge, N. Achilleos, M. Dougherty, K. Khurana, C. Russell
- Physics
- 1 November 2006
[1] The location and shape of a planetary magnetopause is principally determined by the dynamic pressure, Dp, of the solar wind, the orientation of the planet's magnetic dipole with respect to the… Expand
Saturn's magnetodisc current sheet
- C. Arridge, C. Russell, +5 authors D. Southwood
- Physics, Computer Science
- 1 April 2008
TLDR
An empirical model of Saturn's bow shock: Cassini observations of shock location and shape
- A. Masters, N. Achilleos, +4 authors A. Coates
- Physics, Geology
- 1 October 2008
We present a new empirical model of Saturn's bow shock that utilizes observations from the Cassini spacecraft. Shock crossings are identified in magnetic field and plasma observations made by Cassini… Expand
Sources of rotational signals in Saturn's magnetosphere
- K. Khurana, D. Mitchell, +5 authors A. Coates
- Physics, Geology
- 1 February 2009
[1] Saturn's internal magnetic field is exceptionally symmetric about its rotation axis. Yet local and remotely sensed observations of field and plasma in Saturn's magnetosphere display periodicities… Expand
Cassini observations of the variation of Saturn's ring current parameters with system size
- E. Bunce, S. Cowley, +4 authors C. Russell
- Physics, Computer Science
- 1 October 2007
TLDR
Cassini Magnetometer Observations During Saturn Orbit Insertion
- M. Dougherty, N. Achilleos, +15 authors B. Tsurutani
- Physics, Medicine
- Science
- 25 February 2005
Cassini's successful orbit insertion has provided the first examination of Saturn's magnetosphere in 23 years, revealing a dynamic plasma and magnetic environment on short and long time scales. There… Expand
Titan's Magnetic Field Signature During the First Cassini Encounter
- H. Backes, F. M. Neubauer, +8 authors A. Wennmacher
- Physics, Medicine
- Science
- 13 May 2005
The magnetic field signature obtained by Cassini during its first close encounter with Titan on 26 October 2004 is presented and explained in terms of an advanced model. Titan was inside the… Expand
Ionospheric electrons in Titan's tail: Plasma structure during the Cassini T9 encounter
- A. Coates, F. Crary, +6 authors T. W. Hill
- Physics
- 1 December 2007
[1] We present results from the CAPS electron spectrometer obtained during the downstream flyby of Titan on 26 December 2005, which occurred during a period of enhanced plasma pressure inside the… Expand
A new form of Saturn's magnetopause using a dynamic pressure balance model, based on in situ, multi-instrument Cassini measurements
- S. Kanani, C. Arridge, +9 authors N. Krupp
- Physics, Geology
- 1 June 2010
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… Expand
Magnetic field structure of Saturn's dayside magnetosphere and its mapping to the ionosphere: Results from ring current modeling
- E. Bunce, C. Arridge, S. Cowley, M. Dougherty
- Physics
- 1 February 2008
TLDR