Joint Astrophysical Plasma Experiment (JPEX)
Silver
Engineering, Inc. contributed to the ARGOS program providing electrical,
software, mechanical and manufacturing. The JPEX mission marks a radical
advance in incorporating a spectrometer with an unprecedented combination
of high effective area and high spectral resolving power. The JPEX experiment
payload is launched on
a sounding rocket with the scientific goal to understand the evolutionary paths
which lead
from the diverse central stars of planetary nebulae
to the observed population of white dwarfs.
CCD Camera Interface (CCDC Buffer)
Buffers
image for slower speed transmission to PCM Encoder
80C51 based control with Actel 1280 logic section
SRAM buffer storage
Sounding rocket flight duration
CCDC Power Supply
Interpoint
DC-DC converters for camera and buffer electronics
V, I, and T telemetry points
Launch of JPEX Rocket
The
JPEX sounding rocket was launched February 21, 2001 from White Sands Missle
Range, New Mexico. The flight was highly successful with the acquiring of four
high-resolution spectra (from the four multilayer-coated diffraction gratings)
Silver
Engineering, Inc. designed the JPEX sounding rocket CCD camera interface box
and the BLDC motor controller for the detector door. SEI designed the rocket
interconnect systems and is responsible for electrical interface management.
Silver Engineering, Inc. designed and built the JPEX ground support equipment
that supports integration and test of the rocket during rocket integration and
launch preparations.
Click
on photo to enlarge
Click
on photos to enlarge
of the white dwarf star G191-B2B, which was the sole target of the mission.
The pointing control and aspect camera worked flawlessly, enabling to correct
the spectral images down to the
arc-second level, something that may have never been done before on sounding
rocket flights except when pointing at the sun (a brighter and easier target).
Some quick-look spectra shall be out soon, but the real science questions about
helium in the star's outer atmosphere, complex
and difficult questions (because the spectra are quite complex) shall demand
a full analysis with the highest spectral resolution from the instrument