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NASA Scientific and Technical Aerospace Reports

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approximately the same values, i.e. few cm. These conditions are expected to be observed in the ionosphere at the altitude of<br />

approximately 700 km <strong>and</strong> therefore our model may be directly applied for the interpretation of the current measurements on<br />

the board the DEMETER satellite.<br />

Author<br />

Electrostatic Probes; Plasma Probes; Thermal Plasmas; Space Plasmas; Measuring Instruments; Electric Current<br />

20040111102 Centre National de la Recherche Scientifique, Toulouse, France<br />

In-Flight Anomalies Attributed to ESD’s. Recent Cases <strong>and</strong> Trends<br />

Catani, Jean-Pierre; 8th Spacecraft Charging Technology Conference; March 2004; 8 pp.; In English; See also 20040111031;<br />

No Copyright; Avail: CASI; A02, Hardcopy<br />

The general problem of charging is usually shared out four domains of physics or technology: astrophysics for the<br />

knowledge of environment, materials technology for underst<strong>and</strong>ing <strong>and</strong> prediction of charge build-up, plasma physics for<br />

predicting thermal or electromagnetic effects of discharges, <strong>and</strong> space engineering for assessing effects of transients on the<br />

space system. The environment monitoring at the geosynchronous altitude has been carried out for years beginning with the<br />

first launches of NOAA GOES satellites. Their drawback is they provide only local data. The development of Space Weather<br />

activities let foresee the possibility of deriving the charging particles content in the immediate vicinity of the space vehicle<br />

from a limited set of flight-monitored data. Today, anomalies attributed to charging are fortunately infrequent, making<br />

unreliable statistical correlation between environmental data <strong>and</strong> event occurrence. It can be conclusive only in some cases<br />

of surface charging. The underst<strong>and</strong>ing of interaction of materials with a well-representative simulation of environment is a<br />

priority in Europe, especially at CNES, the French Space Agency. In a CNES/ONERA test facility in Toulouse the main<br />

features leading to both surface <strong>and</strong> internal charging are simulated for all altitudes. An aim is the characterization of new<br />

technologies <strong>and</strong> new materials: electrical thrusters, active antennas, conductive coatings. Another aim is the issuing of design<br />

rules in the frame of the European Space St<strong>and</strong>ardization. The plasma discharge is the source of an electromagnetic field<br />

transient. At equipment level an ElectoStatic Discharge (ESD) immunity test has been used for now fifteen years. A system<br />

level test remains to be defined.<br />

Author<br />

Electromagnetic Fields; Spacecraft Charging; Electrostatic Charge; Spacecraft Environments; Spacecraft Instruments;<br />

Electric Discharges<br />

20040111107 European Space Agency, Greenbelt, MD, USA<br />

Space Weather Effects on SOHO <strong>and</strong> its Role as a Space Weather Watchdog<br />

Brekke, P.; Fleck, B.; Haugan, S. V.; vanOverbeek, T.; Schweitzer, H.; Chaloupy, M.; 8th Spacecraft Charging Technology<br />

Conference; March 2004; 13 pp.; In English; See also 20040111031; No Copyright; Avail: CASI; A03, Hardcopy<br />

Since its launch on 2 December 1995, the Solar <strong>and</strong> Heliospheric Observatory (SOHO) has provided an unparalleled<br />

breadth <strong>and</strong> depth of information about the Sun, from its interior, through the hot <strong>and</strong> dynamic atmosphere, <strong>and</strong> out to the solar<br />

wind. In addition SOHO has several times demonstrated its leading role in the early-warning system for space weather. SOHO<br />

is in a halo orbit around L1 Lagrangian point where it views the Sun 24 hours a day. Thus, it is situated outside the Earth’s<br />

protective magnetosphere which shields other satellites from high energy particles <strong>and</strong> the solar wind. We present a summary<br />

of the observed effects on the instruments <strong>and</strong> electronics on SOHO throughout the mission. In particular we focus on a<br />

number of large particle events during the recent years while the Sun was approaching maximum activity, <strong>and</strong> how they<br />

affected both the scientific data as well as hardware components.<br />

Author<br />

Soho Mission; Space Weather; Spacecraft Design; Spacecraft Instruments<br />

20040111311 <strong>NASA</strong> Langley Research Center, Hampton, VA, USA<br />

In-Flight Thermal Performance of the Lidar In-Space Technology Experiment<br />

Roettker, William; [1995]; 9 pp.; In English<br />

Report No.(s): AIAA Paper 95-2016; Copyright; Avail: CASI; A02, Hardcopy<br />

The Lidar In-Space Technology Experiment (LITE) was developed at <strong>NASA</strong> s Langley Research Center to explore the<br />

applications of lidar operated from an orbital platform. As a technology demonstration experiment, LITE was developed to<br />

gain experience designing <strong>and</strong> building future operational orbiting lidar systems. Since LITE was the first lidar system to be<br />

flown in space, an important objective was to validate instrument design principles in such areas as thermal control, laser<br />

performance, instrument alignment <strong>and</strong> control, <strong>and</strong> autonomous operations. Thermal <strong>and</strong> structural analysis models of the<br />

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