NASA, SMITHSONIAN ASTROPHYSICAL OBSERVATORY TO SET UP METEORITE NETWORK
Network of astrophysical meteorite observatories
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Network of astrophysical meteorite observatories
Photographic and visual observations made at new mexico state university observatory
Magnetic observatories for use during international quiet sun year /iqsy/
Latitude and longitude of astronomical observatory of Ukraine by zenith observations
Reduction of lunar occultations of stars observed at Kapska observatory
Progressive errors in ocular micrometer screw of vertical circle at astronomical observatory in Ukraine
Launching of second Orbiting Geophysical Observatory satellite by thrust augmented Thor-Agena D rocket
Instrumentation and calibrations of low energy proton and electron experiment for orbiting geophysical observatories
Description of television system for astronomical observatory
Inexpensive balloon solar observatory system functioning in solar and computer modes
Division error correction to degree diameters for meridian circle of Odessa Astronomical Observatory
Data processing plan for eccentric orbiting geophysical observatory
Artificial satellites tracking by Smithsonian Astrophysical Observatory, discussing station locations, instrumentation, operation modes, interface and selection
The vertical scales of turbulence at the Mt. Wilson observatory are inferred from data from the University of California at Berkeley Infrared Spatial Interferometer (ISI), by modeling path length fluctuations observed in the interferometric paths to celestial objects and those in instrumental ground- based paths. The correlations between the stellar and ground-based path length fluctuations and the temporal statistic of those fluctuations are modeled on various time scales to constrain the vertical scales.
In the interest of improving the performance and efficiency of space geodesy a diverse group in the U.S., in collaboration with IGGOS, has begun to establish a unified National Geodetic Observatory (NGO).
This viewgraph presentation reviews the mission and the architecture of NASA's Orbiting Carbon Observatory (OCO). It also discusses the method of making precise measurements of CO2 from space. Due to be launched in September of 2008, the OCO will fly 12 minutes ahead of the EOS Aqua platform in the Earth Observing System (EOS) Afternoon Constellation (A-Train). The OCO's mission is to identify the sources and sinks for atmospheric CO2.
This paper explores the how's and why's of the Spitzer Mission Operations System's (MOS) success, efficiency, and affordability in comparison to other observatory-class missions. MOS exploits today's flight, ground, and operations capabilities, embraces automation, and balances both risk and cost. With operational efficiency as the primary goal, MOS maintains a strong control process by translating lessons learned into efficiency improvements, thereby enabling the MOS processes, teams, and procedures to rapidly evolve from concept (through thorough validation) into in-flight implementation. Operational teaming, planning, and execution are designed to enable re-use. Mission changes, unforeseen events, and continuous improvement have often times forced us to learn to fly anew. Collaborative spacecraft operations and remote science and instrument teams have become well integrated, and worked together to improve and optimize each human, machine, and software-system element.