SM010
Do Intrinsic Magnetic Fields Shield Planetary Atmospheres From Escaping?
Do Intrinsic Magnetic Fields Shield Planetary Atmospheres From Escaping?
Session ID#: 74054
Session Description:
The idea that an intrinsic planetary magnetic field shields a planet's atmosphere from being lost to space has been recently questioned, and a suggestion made that it would collect energy, channel it down to ionospheres, and thus enhance escape. There is no current consensus on the influence of global magnetic fields on atmospheric escape, and thus whether they are important for retention of significant atmospheres. This question is increasingly important in an era when terrestrial exoplanets are being discovered in the Habitable Zones of stars more active than our Sun. This session will focus on recent research pertaining to the influence of planetary-scale magnetic fields on atmospheric escape processes. We invite contributions from modelers, theoreticians, and observers on topics related to ion outflow from Earth, ion and neutral escape from unmagnetized objects, and the role of magnetic fields in influencing atmospheric escape from exoplanets, giant planets and small bodies.
Index Terms:
2780 Solar wind interactions with unmagnetized bodies [MAGNETOSPHERIC PHYSICS]
2784 Solar wind/magnetosphere interactions [MAGNETOSPHERIC PHYSICS]
5443 Magnetospheres [PLANETARY SCIENCES: SOLID SURFACE PLANETS]
Primary Convener: Dave A Brain, University of Colorado at Boulder, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States
Conveners: Stanislav V Barabash, Swedish Inst Space Physics, Kiruna, Sweden, Thomas Earle Moore, NASA Goddard Space Flight Ctr, Greenbelt, MD, United States and Kanako Seki, The University of Tokyo, Tokyo, Japan
Primary Liaison: Dave A Brain, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States
See more of: SPA-Magnetospheric Physics
