Presentation + Paper
30 September 2022 Optical design of the Carbon Plume Mapper (CPM) imaging spectrometer
Author Affiliations +
Abstract
The Carbon Plume Mapper (CPM) instrument is a high-fidelity imaging spectrometer developed to pinpoint, quantify, and track methane (CH4) and carbon dioxide (CO2) point source emissions to help enable reduction of greenhouse gases in the Earth’s atmosphere. CPM will operate over the spectral range of 400 – 2500 nm with a spectral sampling of 5.0 nm. CPM will be integrated into an industry partner spacecraft bus and launched into low-Earth orbit (LEO). The optical design comprises a three-mirror anastigmat (TMA) telescope and Dyson form spectrometer which reduces volume and mass for a fast (F/1.8) optical system. An overview of the CPM optical design, development, and current status is discussed.
Conference Presentation
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Sander R. Zandbergen, Riley Duren, Paul Giuliano, Robert O. Green, Justin M Haag, Lori B. Moore, Lucas Shaw, and Pantazis Mouroulis "Optical design of the Carbon Plume Mapper (CPM) imaging spectrometer", Proc. SPIE 12235, Imaging Spectrometry XXV: Applications, Sensors, and Processing, 1223505 (30 September 2022); https://doi.org/10.1117/12.2633767
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KEYWORDS
Spectroscopy

Telescopes

Carbon

Methane

Optical design

Mirrors

Staring arrays

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