Overview of Megha-Tropiques Mission - ceres

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The Megha-Tropiques mission An equatorial orbit Courtesy M. Capderou & K. Ramage Roca et al., the CERES/GERB/SCARAB Meeting, GFDL Princeton, 23 October 2012
The ScaRaB instrument 22 kg, 52 cm width, 40 watts 4 telescopes (in red) 2 main channels (# 2 & 3, broad band) 2 auxiliary channels (# 1 & 4 narrow band) Cross track scanning (2300 km swath) 40 km resolution at nadir Calibration module Presentations To follow from Nadia Karouche and Alain Rosak ScaRaB goal : To determine the longwave and shortwave outgoing fluxes observations at the TOA. L LW (daytime) =L TOTAL – A’×L SW A’ depends on the spectral response of T and SW channels Roca et al., the CERES/GERB/SCARAB Meeting, GFDL Princeton, 23 October 2012
Page 1 and 2: ScaRaB-3 on the Megha-Tropiques mis
Page 3 and 4: The Megha-Tropiques mission Overvie
Page 5: The Megha-Tropiques mission Scienti
Page 9 and 10: What ‘s up since we met in Paris
Page 15 and 16: The products that are anticipated L
Page 17 and 18: The products that are anticipated P
Page 19 and 20: The products that are anticipated L
Page 21 and 22: Short term plan for the futur Roca

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