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The solar oscillations investigation: Michelson Doppler imagerThe Solar Oscillations Investigation (SOI) developed the Michelson Doppler Imager (MDI) to investigate the properties of the solar interior using the tools of helioseismology and of the photosphere and corona using more conventional techniques. The fundamental goal is to understand the Sun by determining its structure and observing its dynamics. The basic observables, velocity, intensity, and magnetic field, are computed on board from up to twenty 1024 by 1024 filtergrams made each minute. Subsequent analysis will extend the region to be explored downward into the solar interior and upward into the corona. While the instrument is dedicated to producing an uninterrupted series of helioseismology data, several magnetograms will be made each day and special eight hour campaigns are being developed to address specific scientific questions, some in coordination with other SOHO (Solar and Heliospheric Observatory) instruments.
Document ID
19930022156
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Hoeksema, J. Todd
(Stanford Univ. CA, United States)
Scherrer, P. H.
(Stanford Univ. CA, United States)
Bush, R. I.
(Stanford Univ. CA, United States)
Title, A.
(Lockheed Aircraft Corp. Palo Alto, CA., United States)
Tarbell, T.
(Lockheed Aircraft Corp. Palo Alto, CA., United States)
Date Acquired
September 6, 2013
Publication Date
November 1, 1992
Publication Information
Publication: ESA, Proceedings of the First SOHO Workshop: Coronal Streamers, Coronal Loops, and Coronal and Solar Wind Composition
Subject Category
Solar Physics
Accession Number
93N31345
Funding Number(s)
CONTRACT_GRANT: NAS5-30386
Distribution Limits
Public
Copyright
Other
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