SH030
Toward understanding the nature and structure of our Heliospheric shield
Toward understanding the nature and structure of our Heliospheric shield
Session ID#: 158239
Session Description:
The heliosphere is an immense shield that protects the solar system from harsh, galactic radiation. The radiation that enters the heliosphere affects life on Earth as well as human space exploration. Galactic cosmic rays are the dominant source of radiation and principal hazard affecting space missions within our solar system. To understand the heliosphere’s shielding properties, we need to understand its structure and large-scale dynamics. Although a fortunate confluence of missions such as Voyager, IBEX, and Casini has provided the scientific community with a treasury of heliospheric data, fundamental features remain unknown. Knowledge gaps include the basic shape of the heliosphere, the extent of its tail, the flow pattern and the width of the heliosheath, and the filtration of galactic cosmic rays in the heliosheath. In this session, we solicit observational and modeling studies that advance our understanding of the global nature and shape of the heliosphere, pickup ion evolution from the termination shock to the heliotail, turbulence in the heliosheath, and the modulation and filtration of galactic cosmic rays through the heliosphere.
Co-Organized:
- SA - SPA-Aeronomy
- SM - SPA-Magnetospheric Physics
Index Terms:
7514 Energetic particles [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7524 Magnetic fields [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7536 Solar activity cycle [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7599 General or miscellaneous [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
Primary Convener: Romina Nikoukar, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States
Conveners: Marc Zachary Kornbleuth, Boston University, Boston, MA, United States, Kostas Dialynas, Office for Space Research and Technology, Academy of Athens, Athens, Greece and Matina Gkioulidou, JHU/APL, Laurel, MD, United States
See more of: SPA-Solar and Heliospheric Physics
