Shuttle Ionospheric Modification with Pulsed Localized Exhaust Experiments (SIMPLEX) - 10.21.14

Overview | Description | Applications | Operations | Results | Publications | Imagery
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Science Objectives for Everyone
The Shuttle Ionospheric Modification with Pulsed Localized Exhaust Experiments (SIMPLEX) investigates plasma turbulence driven by rocket exhaust in the ionosphere using ground-based radars.

Science Results for Everyone
Information Pending



The following content was provided by Paul A. Bernhardt, Ph.D., and is maintained in a database by the ISS Program Science Office.

Experiment Details

OpNom

Principal Investigator(s)

  • Paul A. Bernhardt, Ph.D., Naval Research Laboratory, Washington, DC, United States

  • Co-Investigator(s)/Collaborator(s)
    Information Pending
    Developer(s)
    United States Department of Defense Space Test Program, Johnson Space Center, Houston, TX, United States

    Sponsoring Space Agency
    National Aeronautics and Space Administration (NASA)

    Sponsoring Organization
    National Laboratory - Department of Defense (NL-DoD)

    Research Benefits
    Information Pending

    ISS Expedition Duration
    October 2008 - September 2011

    Expeditions Assigned
    18,19/20,21/22,23/24,25/26,27/28

    Previous ISS Missions
    SIMPLEX will be operated on Space Shuttle missions 17A and 2JA during Expedition 19/20.

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    Experiment Description

    Research Overview

    • SIMPLEX investigates plasma turbulence driven by rocket exhaust in the ionosphere using ground based radars by providing direct measurements of exhaust flow sources and developing quantitative models of plasma turbulence that degrades tracking and imaging radars.


    • This is a payload of opportunity on every shuttle flight based on available Orbital Maneuvering System (OMS) fuel, crew time, and overflight of ground sites.

    Description
    The Orbital Maneuver Subsystem (OMS) engines produce exhaust at 3 kilometers per second (km/s) relative to the Space Shuttle. In addition, the Space Shuttle is moving at 7.7 km/s so a ram burn produces exhaust at 10.7 km/s. The constituents of the OMS exhaust are carbon dioxide, water, carbon monoxide, hydrogen, and nitrogen. Each of these species can charge exchange in the ionospheric to give high speed ions with energies over 12 electron Volts.

    High speed ions moving at over 10 km/s through the ionosphere leave a trail of turbulence in the plasma. Radar waves scattering off this trail provide details on the plasma irregularities and on the processes that create the irregularities. Previous flights have produced radar scatter spectra that have yet to be understood. Shuttle Ionospheric Modification with Pulsed Localized Exhaust Experiments (SIMPLEX) observations will employ OMS burns at different times of day and at different latitudes to clarify the source mechanisms for the plasma turbulence.

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    Applications

    Space Applications
    Artificially created plasma turbulence can affect military navigation and communications using radio systems. The plasma turbulence can also be used to promote communications by opening radio channels at abnormally high frequencies. The processes by which chemical releases can produce plasma waves is fundamental to many applications. These processes are quantified with the SIMPLEX measurements.

    Earth Applications
    Results will help in the interpretation of spacecraft engine plumes when they are observed from Earth.

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    Operations

    Operational Requirements
    Astronauts initiate a 10-second dual OMS engine burn at a point where the far field exhaust plume will intersect beam of ground radars. NASA provides orbit updates for coordination with the SIMPLEX diagnostic radars. Knowledge of Shuttle orbit is needed prior to an OMS burn with 10 km accuracy and 1 second resolution. After Shuttle burn is performed the actual ignition point is needed with 1 km accuracy and engine attitude to 5 degrees accuracy. The groud radar will initially make measurements at a fixed azimuth and elevation. After the Space Shuttle has moved well past the radar, some spatial scanning by the radar may occur.

    Operational Protocols
    Commander and Pilot perform OMS engine burns with the Space Shuttle when the shuttle is over one of the follwing ground radar sites for observation: Millstone Hill, Massachusetts; Arecibo, Puerto Rico; Kwajalein, Marshall Islands; Jicamarca, Peru.

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    Results/More Information

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    Results Publications

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    Ground Based Results Publications

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    ISS Patents

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    Related Publications

      Lemoine FG, Smith DE, Zuber MT, Neumann GA, Rowlands DD.  A 70th degree lunar gravity model (GLGM-2) from Clementine and other tracking data. Journal of Geophysical Research. 1997; 102: 16,339-16,359.

      Bernhardt PA, Ganguli G, Kelley MC, Swartz WE.  Enhanced radar backscatter from space shuttle exhaust in the ionsphere. Journal of Geophysical Research. 1995; 100: 23811-23818.

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    Related Websites
    Jicamarca Radio Observatory (JRO)
    NRL Plasma Physics Division
    Millstone Hill Radar at the Haystack Observatory
    Arecibo Ionospheric Observatory

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    Imagery

    image Ground radar data collection during OMS burn of the Space Shuttle. The radar scatter provides data on the ionospheric interactions of the high speed OMS exhaust. (SIMPLEX concept image provided by Dr. Paul A. Bernhardt, Plasma Physics Division, Naval Research Laboratory, Washington, DC 20375)
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    image NASA Image: STS00718778 - This image shows the Glow experiment documentation of OMS/RCS pods and vertical stabilizer from STS-007.
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