Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95429/1/jgra19967.pd
A new form of Saturn’s magnetopause using a dynamic pressure balance model, based on in situ, multi‐...
The location of a planetary magnetopause is principally determined by the balance between solar wind...
We quantify the magnetospheric stress state of Saturn, revealing the nature of the planetary environ...
The shape and location of a planetary magnetopause can be determined by balancing the solar wind dyn...
[1] The location and shape of a planetary magnetopause is principally determined by the dynamic pres...
We use magnetopause crossings of the Cassini spacecraft to study the response of Saturn's magnetosph...
We describe a new method of constructing an equilibrium magnetopause surface based on the pressure b...
This thesis describes how the structure and dynamics of Saturn’s magnetopause can be explored by mod...
Saturn’s magnetic field acts as an obstacle to solar wind flow, deflecting plasma around the planet ...
Saturn’s magnetic field acts as an obstacle to solar wind flow, deflecting plasma around the planet...
The long-term statistical behavior of the large-scale structure of Saturn's magnetosphere has been i...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/94588/1/grl19801.pd
The long-term statistical behavior of the large-scale structure of Saturn’s magnetosphere has been i...
The location of a planetary magnetopause is principally determined by the balance between solar wind...
Plasma rotation plays a large role in determining the size and shape of Saturn's disk-like magnetosp...
A new form of Saturn’s magnetopause using a dynamic pressure balance model, based on in situ, multi‐...
The location of a planetary magnetopause is principally determined by the balance between solar wind...
We quantify the magnetospheric stress state of Saturn, revealing the nature of the planetary environ...
The shape and location of a planetary magnetopause can be determined by balancing the solar wind dyn...
[1] The location and shape of a planetary magnetopause is principally determined by the dynamic pres...
We use magnetopause crossings of the Cassini spacecraft to study the response of Saturn's magnetosph...
We describe a new method of constructing an equilibrium magnetopause surface based on the pressure b...
This thesis describes how the structure and dynamics of Saturn’s magnetopause can be explored by mod...
Saturn’s magnetic field acts as an obstacle to solar wind flow, deflecting plasma around the planet ...
Saturn’s magnetic field acts as an obstacle to solar wind flow, deflecting plasma around the planet...
The long-term statistical behavior of the large-scale structure of Saturn's magnetosphere has been i...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/94588/1/grl19801.pd
The long-term statistical behavior of the large-scale structure of Saturn’s magnetosphere has been i...
The location of a planetary magnetopause is principally determined by the balance between solar wind...
Plasma rotation plays a large role in determining the size and shape of Saturn's disk-like magnetosp...
A new form of Saturn’s magnetopause using a dynamic pressure balance model, based on in situ, multi‐...
The location of a planetary magnetopause is principally determined by the balance between solar wind...
We quantify the magnetospheric stress state of Saturn, revealing the nature of the planetary environ...