Potential of next-generation imaging spectrometers to detect and quantify methane point sources from space
Daniel Jacob1, Daniel Cusworth1,2, Daniel J Varon1, Christopher Chan Miller3, Xiong Liu4, Kelly Chance3, Andrew K Thorpe5, Riley M Duren5, Charles E Miller6, David R Thompson5, Christian Frankenberg7, Luis Guanter8 and Cynthia A Randles9, (1)Harvard University, Cambridge, MA, United States, (2)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (3)Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States, (4)Harvard-Smithsonian CFA, Cambridge, MA, United States, (5)Jet Propulsion Laboratory, Pasadena, CA, United States, (6)Jet Propulsion Lab, Pasadena, CA, United States, (7)California Institute of Technology, Pasadena, CA, United States, (8)Helmholtz Centre Potsdam GFZ German Research Centre for Geosciences, Potsdam, Germany, (9)ExxonMobil Research and Engineering Company, Annandale, NJ, United States