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The Ulysses Mission

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 

The MSFC Solar Group 

The People
Their Papers 

RESEARCH AREAS 

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

PREVIOUS PROJECTS 

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

CURRENT PROJECTS 

MSFC Tower Magnetograph 
MSFC Dome Magnetograph 
The Yohkoh Mission 
The Ulysses Mission 
The GONG Project 
The SOHO Mission 
The TRACE Mission 
The Sun in Time (EPO) 

FUTURE PROJECTS 

The HESSI Mission 
The Solar B Mission 
The GOES SXI Instruments 
The STEREO Mission  
Solar Probe  
Interstellar Probe  

Click on image for larger version.

The Ulysses Mission was originally proposed as a dual spacecraft mission to simultaneously explore the regions over the Sun's north and south poles. Funding problems reduced the mission to a single spacecraft set for launch in 1986. The Challenger disaster then pushed the actual launch by four years. The Ulysses spacecraft was launched from the Space Shuttle Discovery on October 6, 1990 on its mission over the Sun's south and north poles.

This ESA/NASA mission is designed to sample the solar wind and the heliosphere at latitudes unexplored by any other spacecraft. The Ulysses spacecraft carried a suite of instruments out to Jupiter where that planet's gravity pulled the spacecraft into a trajectory that carried it over the Sun's south pole in the fall of 1994 and its north pole in the summer of 1995. It will make its next pass over the Sun's south pole in the fall of 2000 and the north pole in the fall of 2001. These two orbital passes provide views of the solar wind at times near the minimum of solar activity and the maximum of solar activity.

Instruments onboard Ulysses measure particles, magnetic fields, and electro-magnetic radiation from radio wavelengths to gamma-rays. MSFC Solar Physics Branch member Steven Suess is a co-investigator on one of the solar wind experiments.

 

Web Links

Ulysses - The European Space Agency's Ulysses Mission webpage

Mission Details - The Jet Propulsion Laboratory's Ulysses Mission webpage


Author: Dr. David H. Hathaway, david.hathaway@msfc.nasa.gov, (256) 961-7610
Mail Code SD50, NASA/Marshall Space Flight Center, Huntsville, AL 35812
 
 
Responsible Official: Dr. John M. Davis, john.m.davis@msfc.nasa.gov, (256) 961-7600
Mail Code SD50, NASA/Marshall Space Flight Center, Huntsville, AL 35812
 
Last revised 2002 April 09 - D. H. Hathaway