This daytime IR photo shows the dune area located on the floor of Russell Crater. Photo details: IR instrument. Please see the THEMIS Data Citation Note for details on attributing THEMIS pictures. Keep in mind: this THEMIS aesthetic picture has not been radiometrically neither geometrically adjusted for this initial launch. Completely calibrated and geometrically forecasted pictures will be released with the Planetary Data System based on Project policies at a later time. NASA's Jet Propulsion Laboratory takes care of the 2001 Mars Odyssey mission for NASA's Office of Space Science, Washington, D. C The Thermal Emission Imaging System was established by Arizona State University, Tempe, in partnership with Raytheon Santa Barbara Remote Sensing. The THEMIS investigation is led by Dr. Philip Christensen at Arizona State University. Lockheed Martin Astronautics, Denver, is the prime professional for the Odyssey project, and built the orbiter and established. Mars Odyssey; Mars; Thermal Emission Imaging System. Purpose: This notice is to inform owners of OLs and CPs of occasions that happened at the North Anna nuclear power facility that could be of safety significance at their centers. Description of Circumstances: On June 6, 1983, the North Anna Unit 2 plant was being returned to full power operation following its second refueling outage, during which time the core was refilled with a low neutron leakage fuel arrangement to lower the neutron fluence on the activator pressure vessel. Since the North Anna Unit 1 plant had also been formerly refueled with a low leakage core, the licensee assessed the setups of the Unit 1 IR high flux journey settings. Volcano Watch is an once a week short article and task upgrade written by U.S. Geological Survey Hawaiian Volcano Observatory scientists and affiliates. And while gases airborne and dissolved volatiles in molten lava might not look like they 'd be gauged the same way, we can use the same principles and techniques to measure both and aid us comprehend eruptive task. Ozone in the ambience protects us from some of the sun's harmful ultraviolet radiation by absorbing UV wavelengths very strongly. SO2 absorbs strongly in the UV range; HVO uses UV to measure SO2 emission rates. Once we have the IR source, we require to position the FTIR so the volcanic gas is between the IR source and the FTIR. The concepts are the same, the laboratory FTIR has an IR resource and a radiation detector that measures IR strength at many different wavelengths.
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