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Solar-B

ISAS | PPARC | NASA

 

SOLAR-B 

Solar-B Fact Sheet 
Solar-B Brochure 
Solar-B Status 
Sci. Definition Team Report 

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  

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Solar-B is a Japanese Institute of Space and Astronautical Science (ISAS) mission proposed as a follow-on to the highly successful Japan/US/UK Yohkoh (Solar-A) collaboration. The mission consists of a coordinated set of optical, EUV and X-ray instruments that will investigate the interaction between the Sun's magnetic field and its corona. The result will be an improved understanding of the mechanisms which give rise to solar magnetic variability and how this variability modulates the total solar output and creates the driving force behind space weather.

 

ISAS will provide the spacecraft, the launch vehicle (ISAS MV), and major elements of each of the scientific instruments. The spacecraft is being developed by Mitsubishi Electric Corporation (MELCO) and will accommodate three major instruments: a 0.5m solar optical telescope (SOT), an X-ray telescope (XRT), and an EUV Imaging Spectrometer (EIS).

 

The Particle Physics and Astronomy Research Council (PPARC) of the U.K. has responsibility for the EIS instrument. Professor Leonard Culhane (Mullard Space Sciences Laboratory, University College of London, U.K.) is the principal investigator. The EIS links the photosphere to the hot corona. PPARC invited NASA to provide a U.S. science investigation with some hardware responsibility for this instrument.

 

NASA will provide the Focal Plane Package (FPP) for the optical telescope as well as components of the X-ray telescope and Extreme Ultraviolet Imaging Spectrometer. NASA has selected three U.S. teams to participate in the development of these science instruments.

The Solar-B spacecraft is scheduled for launch in the fall of 2005. It will be placed in a sun-synchronous orbit about the Earth. This will keep the instruments in nearly continuous sunlight, with no day/night cycling for nine months each year.

 

An overview of the scientific goals of the Solar-B Mission can be found in the Solar-B Brochure. More scientific details can be found in the Solar-B Science Definition Team Report. Management and technical details are on the Solar-B fact sheet. Updates on the status of the Solar-B mission are on the Solar-B Status Page.

 

Web Links
ISAS The Japanese Institute of Space and Aeronautical Science
PPARC The United Kingdom Particle Physics and Astronomy Research Council
Return to Solar Physics Home

Authors: David H. Hathaway, david.hathaway@msfc.nasa.gov, (256) 961-7610
Mitzi Adams, mitzi.adams@msfc.nasa.gov, (256) 961-7626
Mail Code SD50, NASA/Marshall Space Flight Center, Huntsville, AL 35812

 

Responsible Official: 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 2001 June 12 - M. Adams