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Spacelab 2 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.

Spacelab 2, launched on the Space Shuttle Challenger on July 29, 1985, carried several solar instruments including the Solar Optical Universal Polarimeter (SOUP), the Coronal Helium Abundance Spacelab Experiment (CHASE), the High Resolution Telescope and Spectrograph (HRTS) , and the Solar Ultraviolet Spectral Irradiance Monitor (SUSIM).

The SOUP instrument was designed to observe the strength, structure, and evolution of magnetic fields in the photosphere and to determine the relationship between these magnetic elements and other solar features. It obtained a superb sequence of images showing the structure and evolution of the solar granulation.

The goal of the CHASE experiment was to accurately determine the helium abundance and to derive the temperature, density, and composition of the coronal gas from measurements of ultraviolet emissions.

The HRTS experiment studied features in the chromosphere, corona, and transition region using a telescope and spectrograph to observe emissions in the ultraviolet region of the solar spectrum.

SUSIM was used to determine both the long-term and the short-term variations in the total ultraviolet flux emitted by the Sun.

Web Links

STS 51-F - Spacelab 2 Shuttle Mission

NRL HRTS Instrument - Naval Research Laboratory High Resolution Telescope and Spectrograph

NRL SUSIM Instrument - Naval Research Laboratory Solar Ultraviolet Spectral Irradiance Monitor


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