𝔖 Bobbio Scriptorium
✦   LIBER   ✦

Modeling the size and shape of Saturn's magnetopause with variable dynamic pressure

✍ Scribed by Arridge, C. S.; Achilleos, N.; Dougherty, M. K.; Khurana, K. K.; Russell, C. T.


Book ID
119667611
Publisher
American Geophysical Union
Year
2006
Tongue
English
Weight
485 KB
Volume
111
Category
Article
ISSN
0148-0227

No coin nor oath required. For personal study only.


πŸ“œ SIMILAR VOLUMES


Empirical models of pressure and density
✍ Ravit Helled; Gerald Schubert; John D. Anderson πŸ“‚ Article πŸ“… 2009 πŸ› Elsevier Science 🌐 English βš– 326 KB

We present 'empirical' models (pressure vs. density) of Saturn's interior constrained by the gravitational coefficients J 2 , J 4 , and J 6 for different assumed rotation rates of the planet. The empirical pressuredensity profile is interpreted in terms of a hydrogen and helium physical equation of