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MSFC NSSTC Science@NASA Space Weather Plasmasphere

Sounding of the Cleft Ion Fountain Energization Region (SCIFER)


On 25 January 1995, the NASA rocket for "Sounding of the Cleft Ion Fountain Energization Region" (SCIFER) was launched from the Norwegian Andoya rocket range into the high altitude dayside auroral ionosphere.

The goal was to investigate the causes of a plasma fountain, discovered ten years ago using MSFC's Retarding Ion Mass Spectrometer on the Dynamics Explorer satellite, and known to shoot thousands of miles into space from Earth's dayside ionosphere.

The SCIFER instrument payload flew geographically northward over the heart of the Svalbard Archipelego, attaining an apogee of nearly 1500 km, before reentering the atmosphere and impacting the Earth's north polar ice cap. As the payload travelled upward out of the ionosphere, the plasma density dropped rapidly. Then, as the payload travelled poleward it entered a region of much higher plasma density near apogee, the fountain proper.


The SCIFER flight through the ion fountain energization region allows scientists to "zoom in" on the source of the fountain and to investigate how solar wind energy is converted into plasma flow.


  
Views of the BlackBrant rocket before and during launch.

Two of the seven SCIFER instruments were developed at MSFC. These were the STICS (Scanning Thermal Ion Composition Spectrometer), and the TECHS (Thermal Electron Capped Hemisphere spectrometer). Both were developed through collaboration between Marshall's Space Sciences and Astrionics Laboratories.


View of the STICS instrument during construction.

The STICS measures the 3D thermal distribution functions of Hydrogen, Helium, and Oxygen ions and has flown successfully on three previous sounding rocket flights in the nightside auroral ionosphere, where ion outflows also occur.


Closeup of TECHS instrument and deployment system.

The TECHS represents a new technology for measurement of the 3D ionospheric thermal electron distribution function. From the thermal distribution functions, species density, temperature, and flow may be derived, and non-equilibrium features may be identified and used to diagnose operative plasma energization processes.


The SCIFER rocket payload during integration procedures.

Preliminary indications are that two high-quality and richly-detailed data sets have been obtained with these instruments on SCIFER. These data promise to provide significant insight into the physics of ionospheric plasma fountain formation. Quantitative computer analysis of the telemetered data, amounting to over 1000 MegaBytes, will be required to understand and assimilate the observations that have been obtained.

The SCIFER project has been a scientific collaboration among Cornell University, NASA/MSFC, the Norwegian Space Centre, University of Alabama in Huntsville, University of Alaska, University of New Hampshire, University of Oslo, University of Tromsoe, and University of Texas at Dallas.

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Last Updated: July 11, 2016