National Solar Observatory

Global Oscillation Network Group

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What is GONG?
Instrumentation
Observing Sites 		Gallery Science
Data Archives

Global Helioseismology
Local Helioseismology
Merged Mags /
Synoptic Maps
Mag,Velocity,Intensity		 Oscillation modes of the Sun Potential-Field Source-Surface Models Near-Real-Time Data

Magnetograms / Intensity
Synoptic Maps
Magnetic Field Models
Farside
Network Monitor
Venus Transit 2012
Venus Transit 2012
 Farside
Far Side
 H-alpha
H-alpha
       

SOHO 2012 Meeting

GONG 2012 / SOHO 27
LWS/SDO-5
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IRES Program
 

Dave Armet and Ruth A. Kneale |

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National Solar Observatory

National Science Foundation
The National Solar Observatory is operated by the Association of Universities for Research in Astronomy, under a cooperative agreement with the National Science Foundation.
 Association of Universities for Research in Astronomy