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- b6b426a9-4342-4df8-8101-0ff8498daece definition "The Michelson Doppler Imager (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. The MDI is flown on the Solar Heliospheric Observatory (SOHO). The Michelson Doppler Imager is capable of making a wide range of observations within the constraints imposed by the instrument design, by telemetry availability, and by the limits associated with the running observing programs. This page summarizes the instrument observables and the nature of the observing programs. It is intended to provide sufficient background for potential proposers of research investigations involving either special observations or the analysis of standard program observations. For a full description of the instrument capabilities and mission observing plans, see The Solar Oscillations Investigation - Michelson Doppler Imager (Scherrer et al., Solar Physics. in press). For more information, see: http://soi.stanford.edu/ Group: Instrument_Details Entry_ID: MDI Group: Instrument_Identification Instrument_Category: Solar/Space Observing Instruments Instrument_Class: Photon/Optical Detectors Short_Name: MDI Long_Name: Michelson Doppler Imager End_Group Group: Associated_Platforms Short_Name: SOHO End_Group Group: Spectral_Frequency_Information Wavelength_Keyword: Ultraviolet Number_Channels: 1 Spectral_Frequency_Coverage_Range: 676.8 nm Spectral_Frequency_Resolution: 0.01 nm End_Group Online_Resource: http://soi.stanford.edu/ Sample_Image: http://soi.stanford.edu/operations/drawings/optical_layout.gif Group: Instrument_Logistics Data_Rate: 73 kbps Instrument_Start_Date: 2005-12-02 Instrument_Owner: NASA Instrument_Owner: Stanford University End_Group End_Group" @default.
- b6b426a9-4342-4df8-8101-0ff8498daece id "1655374" @default.
- b6b426a9-4342-4df8-8101-0ff8498daece path_id 02c354fd-8e2d-4825-b786-aa4b0782d1d6 @default.
- b6b426a9-4342-4df8-8101-0ff8498daece path_id 386ea533-9d98-4202-bad3-bb630ac39a93 @default.
- b6b426a9-4342-4df8-8101-0ff8498daece path_id b2140059-b3ca-415c-b0a7-3e142783ffe8 @default.
- b6b426a9-4342-4df8-8101-0ff8498daece path_label "Instruments" @default.
- b6b426a9-4342-4df8-8101-0ff8498daece path_label "Photon/Optical Detectors" @default.
- b6b426a9-4342-4df8-8101-0ff8498daece path_label "Solar/Space Observing Instruments" @default.
- b6b426a9-4342-4df8-8101-0ff8498daece prefLabel "MDI" @default.
- b6b426a9-4342-4df8-8101-0ff8498daece reference "" @default.
- b6b426a9-4342-4df8-8101-0ff8498daece tag "Instruments" @default.
%20is%20a%20project%20of%20the%20Stanford-Lockheed%0AInstitute%20for%20Space%20Research%20and%20is%20a%20joint%20effort%20of%20the%20Solar%20Oscillations%0AInvestigation%20(SOI)%20in%20the%20W.W.%20Hansen%20Experimental%20Physics%20Laboratory%20of%0AStanford%20University%20and%20the%20Solar%20and%20Astrophysics%20Laboratory%20of%20the%0ALockheed-Martin%20Advanced%20Technology%20Center.%20The%20MDI%20is%20flown%20on%20the%20Solar%20%0AHeliospheric%20Observatory%20(SOHO).%0A%0AThe%20Michelson%20Doppler%20Imager%20is%20capable%20of%20making%20a%20wide%20range%20of%20observations%0Awithin%20the%20constraints%20imposed%20by%20the%20instrument%20design%2C%20by%20telemetry%0Aavailability%2C%20and%20by%20the%20limits%20associated%20with%20the%20running%20observing%20programs.%0AThis%20page%20summarizes%20the%20instrument%20observables%20and%20the%20nature%20of%20the%20observing%0Aprograms.%20It%20is%20intended%20to%20provide%20sufficient%20background%20for%20potential%0Aproposers%20of%20research%20investigations%20involving%20either%20special%20observations%20or%0Athe%20analysis%20of%20standard%20program%20observations.%20For%20a%20full%20description%20of%20the%0Ainstrument%20capabilities%20and%20mission%20observing%20plans%2C%20see%20The%20Solar%20Oscillations%0AInvestigation%20-%20Michelson%20Doppler%20Imager%20(Scherrer%20et%20al.%2C%20Solar%20Physics.%20in%0Apress).%0A%0AFor%20more%20information%2C%20see%3A%0Ahttp%3A%2F%2Fsoi.stanford.edu%2F%0A%0A%0AGroup%3A%20Instrument_Details%0A%20%20%20Entry_ID%3A%20MDI%0A%20%20%20Group%3A%20Instrument_Identification%0A%20%20%20%20%20%20Instrument_Category%3A%20Solar%2FSpace%20Observing%20Instruments%0A%20%20%20%20%20%20Instrument_Class%3A%20Photon%2FOptical%20Detectors%0A%20%20%20%20%20%20Short_Name%3A%20MDI%0A%20%20%20%20%20%20Long_Name%3A%20Michelson%20Doppler%20Imager%0A%20%20%20End_Group%0A%20%20%20Group%3A%20Associated_Platforms%0A%20%20%20%20%20%20Short_Name%3A%20SOHO%0A%20%20%20End_Group%0A%20%20%20Group%3A%20Spectral_Frequency_Information%0A%20%20%20%20%20%20Wavelength_Keyword%3A%20Ultraviolet%0A%20%20%20%20%20%20Number_Channels%3A%201%0A%20%20%20%20%20%20Spectral_Frequency_Coverage_Range%3A%20676.8%20nm%0A%20%20%20%20%20%20Spectral_Frequency_Resolution%3A%200.01%20nm%0A%20%20%20End_Group%0A%20%20%20Online_Resource%3A%20http%3A%2F%2Fsoi.stanford.edu%2F%0A%20%20%20Sample_Image%3A%20http%3A%2F%2Fsoi.stanford.edu%2Foperations%2Fdrawings%2Foptical_layout.gif%0A%20%20%20Group%3A%20Instrument_Logistics%0A%20%20%20%20%20%20Data_Rate%3A%2073%20kbps%0A%20%20%20%20%20%20Instrument_Start_Date%3A%202005-12-02%0A%20%20%20%20%20%20Instrument_Owner%3A%20NASA%0A%20%20%20%20%20%20Instrument_Owner%3A%20Stanford%20University%0A%20%20%20End_Group%0AEnd_Group%22){kind=link}