NASA Scientific and Technical Aerospace Reports
NASA Scientific and Technical Aerospace Reports
NASA Scientific and Technical Aerospace Reports
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20040121082 Ball <strong>Aerospace</strong> <strong>and</strong> Technologies Corp., Boulder, CO, USA<br />
Final Results of the Ball AMSD Beryllium Mirror<br />
Chaney, David M.; [2004]; 1 pp.; In English; Technology Days in the Government, 17-19 Aug. 2004, Huntsville, AL, USA;<br />
No Copyright; Avail: Other Sources; Abstract Only<br />
The 1.4-meter semi-rigid, beryllium Advanced Mirror System Demonstrator (AMSD) mirror completed initial cryogenic<br />
testing at Marshall’s X-ray Calibration Facility (XRCF) in August of 2003. Results of this testing show the mirror to have very<br />
low cryogenic surface deformation <strong>and</strong> possess exceptional figure stability. Subsequent to this cryogenic testing beryllium was<br />
selected as the material of choice for the James Webb Space Telescope (JWST) multi-segment primary mirror. Therefore, the<br />
AMSD mirror was sent back to SSG-Tinsley for additional ambient polishing to JWST requirements. The mirror was<br />
successfully polished to less than 22nm rms of low frequency error. Those additional results are presented with comparisons<br />
to the JWST requirements.<br />
Author<br />
Beryllium; Cryogenics; Segmented Mirrors; James Webb Space Telescope<br />
20040121099 South Dakota State Univ., Brookings, SD, USA<br />
Development of a Hydrazine/Nitrogen Dioxide Fiber Optic Sensor<br />
Andrawis, Alfred S.; Santiago, Josephine; 2003 Research <strong>Reports</strong>: <strong>NASA</strong>/ASEE Fellowship Program; December 15, 2003,<br />
pp. A-1 - A-12; In English; See also 20040121096; No Copyright; Avail: CASI; A03, Hardcopy<br />
Bromothymol Blue (BT)/Bromocresol Green (BG) mixture (1/1) in hydrogel (l/l), produces a blue-green indicator for HZ<br />
<strong>and</strong>/or NO2. The stability over a two months period of this BT/BG (1/1) indicator solution was tested <strong>and</strong> no evidence of<br />
performance deterioration was detected. A dual HZ/NO2 prototype sensor utilizing an acid-base indicator was previously<br />
constructed. A monitor <strong>and</strong> control circuit are also designed, built d tested during the course of this project. The circuit is<br />
controlled with Motorola MC68HC II microcontroller evaluation board to monitor the voltage level out of the photodetector.<br />
Low-pass filter <strong>and</strong> amplifier are used to interface the sensor’s small voltage with the microcontroller’s AD input. The sensor,<br />
interface circuit <strong>and</strong> the microcontroller board are then all placed in one unit <strong>and</strong> powered with a single power supply. The<br />
unit is then tested several times <strong>and</strong> the response was consistent <strong>and</strong> proved the feasibility of dual ‘J@ leak detection. Other<br />
sensor types, suitable for silica glass fiber, smaller in size, more rugged <strong>and</strong> suitable for use on board of the Space Shuttle <strong>and</strong><br />
missile canisters, are then proposed.<br />
Author<br />
Detection; Fiber Optics; Gas Detectors; Glass Fibers; Nitrogen Dioxide; Hydrazines<br />
20040121106 Oklahoma Baptist Univ., Shawnee, OK, USA<br />
Development of Charge to Mass Ratio Microdetector for Future Mars Mission<br />
Chen, Yuan-Lian Albert; 2003 Research <strong>Reports</strong>: <strong>NASA</strong>/ASEE Fellowship Program; December 15, 2003, pp. B-1 - B-9; In<br />
English; See also 20040121096; No Copyright; Avail: CASI; A02, Hardcopy<br />
The Mars environment comprises a dry, cold <strong>and</strong> low air pressure atmosphere with low gravity (0.38g) <strong>and</strong> high resistivity<br />
soil. The global dust storms that cover a large portion of Mars are observed often from Earth. This environment provides an<br />
ideal condition for turboelectric charging. The extremely dry conditions on the Martian surface have raised concerns that<br />
electrostatic charge buildup will not be dissipated easily. If turboelectrically generated charge cannot be dissipated or avoided,<br />
then dust will accumulate on charged surfaces <strong>and</strong> electrostatic discharge may cause hazards for future exploration missions.<br />
The low surface on Mars helps to prolong the charge decay on the dust particles <strong>and</strong> soil. To better underst<strong>and</strong>ing the physics<br />
of Martian charged dust particles is essential to future Mars missions. We research <strong>and</strong> design two sensors, velocity/charge<br />
sensor <strong>and</strong> PZT momentum sensors, to measure the velocity distribution, charge distribution <strong>and</strong> mass distribution of Martian<br />
wed dust particles. These sensors are fabricated at <strong>NASA</strong> Kenney Space Center, Electrostatic <strong>and</strong> Surface Physics Laboratory.<br />
The sensors are calibrated. The momentum sensor is capable to measure 45 pan size particles. The designed detector is very<br />
simple, robust, without moving parts, <strong>and</strong> does not require a high voltage power supply. Two sensors are combined to form<br />
the Dust Microdetector - CHAL.<br />
Author<br />
Charge Distribution; Charged Particles; Electrical Resistivity; Electrostatics; Fabrication; Dust Storms; Sensors<br />
20040121125 <strong>NASA</strong> Langley Research Center, Hampton, VA, USA<br />
Single-element Electron-transfer Optical Detector System<br />
Jordan, Jeffrey D., Inventor; June 15, 2004; 12 pp.; In English; Original contains black <strong>and</strong> white illustrations<br />
Patent Info.: Filed 13 Mar. 2002; US-Patent-6,750,438; US-Patent-Appl-SN-097702; US-Patent-Appl-SN-276568;<br />
<strong>NASA</strong>-Case-LAR-16279-1; No Copyright; Avail: CASI; A03, Hardcopy<br />
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