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The Solar Dynamo

THE SUN 

Why We Study the Sun 
The Big Questions 
Magnetism - The Key 

SOLAR STRUCTURE 

The Interior 
The Photosphere 
The Chromosphere 
The Transition Region 
The Corona 
The Solar Wind 
The Heliosphere 

SOLAR FEATURES 

Photospheric Features 
Chromospheric Features 
Coronal Features 
Solar Wind Features 

THE SUN IN ACTION 

The Sunspot Cycle 
Solar Flares 
Post Flare Loops 
Coronal Mass Ejections 
Surface and Interior Flows 
Waves and Helioseismology 

RESEARCH AREAS 

Flare Mechanisms 
3D Magnetic Fields 
The Solar Dynamo 
Sunspot Cycle Predictions 
Coronal Heating 
Solar Wind Dynamics 

PREVIOUS PROJECTS 

The Skylab Mission 
The Solar Maximum Mission 
The SpaceLab 2 Mission 
MSSTA 

CURRENT PROJECTS 

MSFC TVM  
MSFC EXVM  
The Yohkoh Mission 
The Ulysses Mission 
The SOHO Mission 
The GONG Project 
The Sun in Time (EPO) 

FUTURE PROJECTS 

The Solar B Mission 
The GOES SXI Instruments 
Interstellar Probe  

This page temporarily trashed. To be repaired shortly from backed-up files.

Web Links

Interface Dynamo Homepage - NCAR/High Altitude Observatory solar dynamo research

 

Author: David H. Hathaway, david.hathaway@msfc.nasa.gov, (256) 544-7610
Mail Code SD50, NASA/Marshall Space Flight Center, Huntsville, AL 35812

 

Responsible Official: John M. Davis, john.m.davis@msfc.nasa.gov, (256) 544-7600
Mail Code SD50, NASA/Marshall Space Flight Center, Huntsville, AL 35812

 

Last revised 2000 January 07 - D. H. Hathaway