Development of a Sensor to Measure
Directly the Ionospheric
Thermal Electron Distribution, 15-9111
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Principal Investigators
Craig J. Pollock
Susan E. Pope
Scott E. Weidner
Inclusive Dates: 01/01/99 - Current
Background - This project was undertaken to
fill a significant gap that exists in space plasma measurement capability. Electron
distribution function measurements are typically conducted from energies upward of a few
eV, with few measurements being made at energies below a few eV. Yet the ionospheric
electron temperature is typically less than one eV, when expressed in energy units. That
is, the kinetic energy of a typical ionospheric electron is less than one eV. Important
electric currents are believed to be carried by ionospheric thermal electrons, and these
electrons may drive high-latitude ion outflows by setting up ambipolar electric fields.
This research project addresses this issue by developing a sensor specifically geared to
measuring electrons in Earths ionosphere at low energy.
Approach - Although the research team is
investigating several aspects, the teams approach is centered on the concept of
miniaturization. Miniaturization is necessary, because the low-energy electrons gyrate
about the geomagnetic field in small circles, and desirable for effective use of
spacecraft resources. Electrons gyrate in the geomagnetic field, making their measurement
difficult using curved parallel plate electrostatic analyzers. Transmission is cut off if
the radius of gyration is not much larger than the radius of analyzer curvature.
Therefore, SwRI emphasized development of a very small analyzer, with a six-millimeter
central radius of curvature. Therefore, the effort involves electrostatic ray tracing of
particle trajectories through such an analyzer in the presence of a background magnetic
field. In the past, the team has observed cutoff in particle count rates in space with
small analyzers near 0.5 eV. The investigators are studying 1) electron transmission using
ray tracing to determine if this cutoff is due to the geomagnetic field and 2) the
manufacturability of small electrostatic analyzers, from the point of view of maintaining
the tight mechanical tolerances required for uniform transmission characteristics
throughout the analyzer. Finally, the team is studying techniques to image the particle
arrivals at the exit aperture of small electrostatic analyzers, using microchannel plate
detectors and a delay line anode.
Accomplishments - To date the team has
conducted ray tracing studies of a numeric model of a small electrostatic analyzer in the
presence of a background magnetic field. This model simulates an instrument flown in the
Earths ionosphere in January 1995 that displayed cutoff in transmitted electrons at
an energy near 0.5 eV. Preliminary results of this ray tracing indicate that the cutoff
was not magnetic, as cutoff was not found in the ray tracing until the electron energy
dropped below 0.1 eV. The ray tracing also revealed an electrostatic analyzer design flaw
that significantly reduces electron transmission at all energies. This flaw will be
corrected when a test model is built as part of this effort. The team has fabricated a
prototype delay line detector and operated it in a vacuum chamber under ultraviolet
illumination, with encouraging results. The measured time delay is in fact a monotonic
function of the position at which a photon strikes the detector. This result will be
directly applicable to electrons when this detector is incorporated into an electron
sensor.
Space Sciences Program
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