Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/94588/1/grl19801.pd
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95313/1/jgra21189.pd
Plasma rotation plays a large role in determining the size and shape of Saturn's disk-like magnetosp...
Swept forward field is the term given to configurations of magnetic field wherein the field lines de...
We have developed global magnetohydrodynamic (MHD) models of the magnetospheres of Jupiter and Satur...
Probability distributions for the location of the Saturnian bow shock and magnetopause have been der...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95429/1/jgra19967.pd
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95292/1/jgra21912.pd
When the Cassini spacecraft flew by Titan on 13 June 2007, at 13.6 Saturn local time, Titan was dire...
Swept forward field is the term given to configurations of magnetic field wherein the field lines de...
We use magnetopause crossings of the Cassini spacecraft to study the response of Saturn's magnetosph...
The long-term statistical behavior of the large-scale structure of Saturn’s magnetosphere has been i...
For over 10 years, the Cassini spacecraft has patrolled Saturn's magnetosphere and observed its magn...
We quantify the magnetospheric stress state of Saturn, revealing the nature of the planetary environ...
The long-term statistical behavior of the large-scale structure of Saturn's magnetosphere has been i...
The interaction between the solar wind and a magnetosphere is central to the dynamics of a planetary...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95313/1/jgra21189.pd
Plasma rotation plays a large role in determining the size and shape of Saturn's disk-like magnetosp...
Swept forward field is the term given to configurations of magnetic field wherein the field lines de...
We have developed global magnetohydrodynamic (MHD) models of the magnetospheres of Jupiter and Satur...
Probability distributions for the location of the Saturnian bow shock and magnetopause have been der...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95429/1/jgra19967.pd
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95292/1/jgra21912.pd
When the Cassini spacecraft flew by Titan on 13 June 2007, at 13.6 Saturn local time, Titan was dire...
Swept forward field is the term given to configurations of magnetic field wherein the field lines de...
We use magnetopause crossings of the Cassini spacecraft to study the response of Saturn's magnetosph...
The long-term statistical behavior of the large-scale structure of Saturn’s magnetosphere has been i...
For over 10 years, the Cassini spacecraft has patrolled Saturn's magnetosphere and observed its magn...
We quantify the magnetospheric stress state of Saturn, revealing the nature of the planetary environ...
The long-term statistical behavior of the large-scale structure of Saturn's magnetosphere has been i...
The interaction between the solar wind and a magnetosphere is central to the dynamics of a planetary...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95313/1/jgra21189.pd
Plasma rotation plays a large role in determining the size and shape of Saturn's disk-like magnetosp...
Swept forward field is the term given to configurations of magnetic field wherein the field lines de...
DOI
Add to ORKG