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SOHO/Michelson Doppler Imager (MDI) and Solar Oscillations Investigation (SOI) Data Archive

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MDI is a project of the Stanford-Lockheed Institute for Space Research and is a joint effort of the Solar Oscillations Investigation (SOI) in the W.W. Hansen Experimental Physics Laboratory of Stanford University and the Solar and Astrophysics Laboratory of the Lockheed-Martin Advanced Technology Center. SOI and the MDI Team are part of an international collaboration to study the interior structure and dynamics of the Sun. The MDI team was responsible for the design and fabrication, and now for the operation, of the MDI instrument on board the Solar and Heliospheric Observatory (SOHO) spacecraft. The primary objective of the SOI investigation is to investigate the solar interior using the tools of helioseismology. To fulfill the potential of helioseismology, observations free of the distortions from the Earth's atmosphere and free of diurnal data gaps must be obtained. The primary data set consists of precision measurements of the line-of-sight surface velocity field from which the oscillation modes of the solar interior can be deduced. In addition to the primary objectives, the SOI program includes investigation of several associated science objectives. They are called associated objectives because they involve the study of observable solar phenomena using traditional techniques, though they share the same goal of understanding the structure and variability of the Sun. These investigations are no less important to the understanding of the solar structure and dynamics than the primary objectives. All SOHO/MDI data are available from the public SOHO data archive: http://sohowww.nascom.nasa.gov/data/archive.html Mirror archives are available at: SOHO Archive at Rutherford Appleton Laboratory, UK.: http://trace.solararchive.rl.ac.uk/soho/ SOHO Archive at the Institut d'Astrophysique Spatiale, France: http://idc-medoc.ias.u-psud.fr/ SOHO Archive at Osservatorio Astronomico di Torino, Torino, Italy: http://solar.to.astro.it/
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