Algorithm theoretical basis for Version 3 TEMPO Level 0-1 processor

Heesung Chong(Center for Astrophysics Harvard & Smithsonian), Laurel Carpenter(Center for Astrophysics Harvard & Smithsonian), J. Lasnik(BAE Systems (Sweden)), D. K. Nicks(National Oceanic and Atmospheric Administration), Caroline R. Nowlan(Center for Astrophysics Harvard & Smithsonian), John E. Davis, James L. Carr(University of Manchester), D. E. Flittner(University of Arizona), K. Chance(Center for Astrophysics Harvard & Smithsonian), Christopher Chan Miller(Center for Astrophysics Harvard & Smithsonian), HUIQUN WANG(Center for Astrophysics Harvard & Smithsonian), Juseon Bak(Center for Astrophysics Harvard & Smithsonian), Xiong Liu(Center for Astrophysics Harvard & Smithsonian), J. C. Houck(Center for Astrophysics Harvard & Smithsonian), R. Suleiman(Harvard University Press), Weizhen Hou(Center for Astrophysics Harvard & Smithsonian), Brian Baker(The Aerospace Corporation), Jean Fitzmaurice(Smithsonian Astrophysical Observatory), Junsung Park(Center for Astrophysics Harvard & Smithsonian), Gonzalo González Abad(Center for Astrophysics Harvard & Smithsonian)
Cited by 2


Related Papers

The Sloan Digital Sky Survey: Technical Summary
|The Astronomical Journal|2000|10.5k
The HITRAN2016 molecular spectroscopic database
|Journal of Quantitative Spectroscopy and Radiative Transfer|2017|7.9k
The HITRAN 2008 molecular spectroscopic database
|Journal of Quantitative Spectroscopy and Radiative Transfer|2009|3.6k
The HITRAN2012 molecular spectroscopic database
|Journal of Quantitative Spectroscopy and Radiative Transfer|2013|3.3k
The HITRAN2020 molecular spectroscopic database
|Journal of Quantitative Spectroscopy and Radiative Transfer|2021|2.3k