[Loops] Innovation Session at AGU - Re: AGU Session on Coronal Heating

[Ed DeLuca]

Hi,

  Nicky's session is very relevant to the current science being done by 
the loops community.

  If you have thoughts on the hardware, modeling or infrastructure 
innovations needed to move from 1-d coronal studies to 3-D 
photosphere-solar wind analysis (as an example). Integration of new 
observations (maybe high resolution mirco-calorimeters) with new 
laboratory results (plasma and atomic physics) might be another example.
Please consider sharing those thoughts in the session:

SA011: Solar and Space Physics Science and the Need for Innovation Into 
the Next Decade
"The solar and space physics community has recently completed its 
Decadal Survey to identify the most important scientific questions to be 
addressed during the next decade and beyond. Innovations in 
instrumentation, flight systems, and information technology will be 
required to address these questions. This session focuses on the 
present-day science that informs the innovation process toward this 
goal. Especially encouraged are contributions that show how their 
science results could be enhanced through enabling innovations."

Spann, Clemmons & DeLuca Conveners

Best wishes,
Ed

On 7/30/12 2:56 PM, VIALL-KEPKO, NICHOLEEN M. (GSFC-6710) wrote:
>
> Dear Coronal Loop Enthusiasts,
>
> We are organizing a session at this Fall's AGU: 'Recent Advances in 
> Solar Coronal Heating' and particularly welcome and encourage 
> participation from the loops community. Please consider submitting an 
> abstract to our session!
>
> Details for the meeting can be found at 
> http://fallmeeting.agu.org/2012/. The abstract deadline is approaching 
> fast! They are due 08 August at 23:59 EDT.
>
> Session Description: Solving the solar coronal heating problem is of 
> critical importance for space weather and understanding the Sun-Earth 
> environment. This session emphasizes understanding the underlying 
> physical process that heats the corona through the integration of 
> macro and micro modeling, constrained by observations. Advances in 
> theory and modeling as well as a host of new observational data 
> provide an excellent opportunity for bridging the gap and providing 
> feedback between these different methods. We solicit a broad variety 
> of approaches including global models of the solar corona, kinetic 
> models and theories of the energy dissipation and local heating 
> mechanisms, as well as observations to test and compare with models.
>
> Best Regards,
>
> SH012 Conveners:
>
> N. M. Viall, Nicholeen.M.Viall at nasa.gov
>
> Z. Mikic, mikicz at predsci.com
>
> P. Cassak, Paul.Cassak at mail.wvu.edu
>
> **************
> Nicholeen Viall
> Code 671
> NASA/Goddard Space Flight Center
> Greenbelt, MD 20771
> Email: Nicholeen.M.Viall at nasa.gov 
> <https://mail02.ndc.nasa.gov/owa/UrlBlockedError.aspx>
> Phone: 301-286-4054
>
>
>
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> Loops at solar.physics.montana.edu
> https://mithra.physics.montana.edu/mailman/listinfo/loops


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