Tomographic Imaging of the Velocity and Magnetic Fields in the Sun's Atmosphere
Entry ID: NSF-ANT06-32399

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Summary
Abstract: The ultimate goal of this project is to determine the structure and dynamics of the Sun's atmosphere, assess the role of MHD waves in heating the chromosphere/corona and driving the solar wind, and better understand how the Sun's atmosphere couples to the solar interior. As the solar atmosphere is 'home' to many of the solar phenomena that can have a direct impact on the biosphere, including ... View entire text
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Description: Original data submitted.

Description: NSF Award Abstract #0632399
Geographic Coverage
Spatial coordinates   
  N: -60.0   S: -90.0   E: 180.0   W: -180.0

Temporal Coverage
Start Date: 2006-03-29
Stop Date: 2010-03-31
ISO Topic Category
Data Set Progress
COMPLETE
Data Center
Data Coordination Center, United States Antarctic Program Supplemental Info
Data Center URL: http://www.usap-data.org/
Dataset ID: NSF-ANT06-32399

Data Center Personnel
Name: ROBERT A. ARKO
Email: info at usap-data.org
Contact Address:
Lamont-Doherty Earth Observatory
61 Route 9W
City: Palisades
Province or State: NY
Postal Code: 10964
Country: USA
Personnel
Role: INVESTIGATOR
Phone: 808 875 2389
Fax: 808 875 2387
Email: stuartj at msrc.unm.edu
Contact Address:
Maui Scientific Research Center
590 Lipoa Pkwy, Ste 262
City: Kihei
Province or State: HI
Postal Code: 96753
Country: U.S.A.
Creation and Review Dates
DIF Creation Date: 2010-03-10
Last DIF Revision Date: 2010-03-15
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