The GHGSat-D imaging spectrometer
2021
D. Jervis | J. McKeever | B. O. A. Durak | J. J. Sloan | D. Gains | D. J. Varon | D. J. Varon | A. Ramier | M. Strupler | E. Tarrant
<p>The demonstration satellite GHGSat-D, or “Claire”, launched on 21 June 2016, is the first in a planned constellation of small satellites designed and operated by GHGSat, Inc. to measure greenhouse gas emissions at the facility scale from space. Its instrument measures methane concentrations by collecting and spectrally decomposing solar backscattered radiation in the shortwave infrared using a compact fixed-cavity Fabry–Pérot imaging spectrometer. The effective spatial resolution of <span class="inline-formula">50×50</span> <span class="inline-formula">m<sup>2</sup></span> over targeted <span class="inline-formula">12×12</span> <span class="inline-formula">km<sup>2</sup></span> scenes is unprecedented for a space-based gas-sensing spectrometer. Here we report on the instrument design and forward model and retrieval procedure, and we present several examples of retrieved methane emissions observed over industrial facilities. We discuss the sources of error limiting the performance of GHGSat-D and identify improvements for our follow-on satellites. Claire's mission has proven that small satellites can be used to identify and quantify methane emissions from industrial facilities, enabling operators to take prompt corrective action.</p>
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