Dear Colleagues,

We would like to bring to your attention our session “Exploring the Slow Solar Wind from the Photosphere to the Heliosphere” at the fall 2012 AGU meeting in San Francisco.

The abstract deadline is *08 August 2012* at 23:59 EDT. More details on the meeting can be found at
http://fallmeeting.agu.org/2012/

Session Description:

Successful theories of the origin, evolution and governing processes of solar and stellar winds must be able to address all physical states. The goal of this session is to discuss the current status of observations, theories and models of the low-speed wind. Specific topics include: 1) The generation and release of the slow solar wind from the corona including the role of high speed outflows from solar active regions 2) Identifying the role of magnetic topology in the origin of the slow wind 3) The processes that impart energy to the wind 4) In situ observations and 5) Spatial distribution of the slow solar wind and its evolution during the solar cycle.

Best wishes,

The Session Conveners:

S. Lepri, slepri -at- umich.edu
H. Warren, harry.warren -at- nrl.navy.mil
J. Edmondson, jkedmond -at- umich.edu
D. Baker, db2 -at- mssl.ucl.ac.uk