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-1. Reflected sunlight is comparable to the instrument noise level. For the south polar region, spectral radiance corresponding to that expected for solar reflectance by a Lambertian surface at the pole with albedo of 0.5 was subtracted from the TES observation before converting to brightness temperatures.
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27
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note
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2 band corresponding to a weighting function peaked near 3 mbars.
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note
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We wish to thank the entire TES engineering team at the Hughes Santa Barbara Research Center, led by S. Silverman and M. Greenfield, and at Arizona State University (ASU), led by G. Mehall. We thank N. Gorelick, K. Bender, S. Anwar, M. Weiss-Malik, J. Bandfield, V. Hamilton, M. Lane, S. Ruff, and K. Qazi at ASU. We thank B. Allen II, L. Fenton, A. Gordon, L. Mazzuca, W. McMillan, S. Mason Jr., K. Walker, and W. Maguire. We thank the Goddard Software Development Team, headed by S. Dason and E. Greene, including J. Guerber, K. Horrocks, M. Kaelberer, C. Martin, R. Thompson, E. Winter. We thank T. Titus and K. Mullins at the U.S. Geological Survey in Flagstaff. Finally, we thank the entire spacecraft and mission operations teams at Jet Propulsion Laboratory and Lockheed Martin.
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