Raid Suleiman
Harvard University
56 Papers
289 Citations
Raid Suleiman is an academic researcher from Harvard University. The author has contributed to research in topics: Solar flare & Corona. The author has an hindex of 18, co-authored 52 publications. Previous affiliations of Raid Suleiman include University of New Hampshire.
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Papers
Tropospheric emissions: Monitoring of pollution (TEMPO)
P. Zoogman,Xiong Liu,Raid Suleiman,W. F. Pennington,David Flittner,Jay Al-Saadi,B.B. Hilton,D. K. Nicks,Michael J. Newchurch,J. L. Carr,Scott J. Janz,M.R. Andraschko,Antti Arola,B. Baker,B. Canova,C. Chan Miller,Ronald C. Cohen,J.E. Davis,M.E. Dussault,David P. Edwards,Jack Fishman,Abduwasit Ghulam,G. Gonzalez Abad,Michel Grutter,Jay R. Herman,J. Houck,Daniel J. Jacob,Joanna Joiner,Brian Kerridge,Jhoon Kim,Nickolay A. Krotkov,Lok N. Lamsal,Can Li,Can Li,Anders V. Lindfors,Randall V. Martin,Randall V. Martin,C. T. McElroy,Chris A. McLinden,Vijay Natraj,Doreen Neil,Caroline R. Nowlan,E.J. O׳Sullivan,Paul I. Palmer,Robert B. Pierce,M.R. Pippin,Alfonso Saiz-Lopez,Robert Spurr,J. Szykman,Omar Torres,J. P. Veefkind,B. Veihelmann,Huiqun Wang,Jun Wang,Kelly Chance +54 more
TL;DR: TEMPO was selected in 2012 by NASA as the first Earth Venture Instrument, for launch between 2018 and 2021, and it will measure atmospheric pollution for greater North America from space using ultraviolet and visible spectroscopy as mentioned in this paper.
The Ozone Monitoring Instrument: overview of 14 years in space
Pieternel F. Levelt,Joanna Joiner,Johanna Tamminen,J. Pepijn Veefkind,Pawan K. Bhartia,Deborah Stein Zweers,Bryan N. Duncan,David G. Streets,Henk Eskes,Ronald van der A,Chris A. McLinden,Vitali Fioletov,Simon Carn,Jos de Laat,Matthew T. DeLand,Sergey Marchenko,Richard D. McPeters,Jerald R. Ziemke,Jerald R. Ziemke,Dejian Fu,Xiong Liu,Kenneth E. Pickering,Arnoud Apituley,G. Gonzalez Abad,Antti Arola,Folkert Boersma,Folkert Boersma,C. Chan Miller,Kelly Chance,Martin de Graaf,Janne Hakkarainen,S. Hassinen,Iolanda Ialongo,Quintus Kleipool,Nickolay A. Krotkov,Can Li,Lok N. Lamsal,Paul A. Newman,Caroline R. Nowlan,Raid Suleiman,L. G. Tilstra,Omar Torres,Huiqun Wang,Krzysztof Wargan +43 more
TL;DR: The Ozone Monitoring Instrument (OMI) on board the Aura satellite spanning a period of nearly 14 years has been used in a wide range of applications and research resulting in many new findings as mentioned in this paper.
An Empirical Model of a Polar Coronal Hole at Solar Minimum
Steven R. Cranmer,J. L. Kohl,Giancarlo Noci,Ester Antonucci,Giuseppe Tondello,M. C. E. Huber,Leonard Strachan,Alexander Panasyuk,L. D. Gardner,Marco Romoli,Silvano Fineschi,D. Dobrzycka,John C. Raymond,Piergiorgio Nicolosi,O. H. W. Siegmund,Daniele Spadaro,Carlo Benna,Angela Ciaravella,S. Giordano,Shadia Rifai Habbal,Margarita Karovska,Xing Li,Randall V. Martin,J. Michels,A. Modigliani,Giampiero Naletto,R. O'Neal,Claudio Pernechele,Giannina Poletto,P. L. Smith,Raid Suleiman +30 more
TL;DR: In this article, the authors present a self-consistent empirical model for several plasma parameters in the extended solar corona above a polar coronal hole, derived from observations with the SOHO Ultraviolet Coronagraph Spectrometer (UVCS/SOHO) during the period between 1996 November and 1997 April.
354
Updated Smithsonian Astrophysical Observatory Ozone Monitoring Instrument (SAO OMI) formaldehyde retrieval
TL;DR: The Smithsonian Astrophysical Observatory (SAO) formaldehyde (H2CO) retrieval algorithm for the Ozone Monitoring Instrument (OMI) is the operational retrieval for NASA OMI H2CO.
204
The first COMPTEL source catalogue
V. Schönfelder,K. Bennett,J. J. Blom,H. Bloemen,Werner Collmar,Alanna Connors,Roland Diehl,W. Hermsen,A. F. Iyudin,R. M. Kippen,Jürgen Knödlseder,L. Kuiper,G. G. Lichti,Mark L. McConnell,D. Morris,R. Much,Uwe Oberlack,James M. Ryan,G. Stacy,Helmut Steinle,Andrew W. Strong,Raid Suleiman,R. van Dijk,M. Varendorff,C. Winkler,O. R. Williams +25 more
TL;DR: The first complete all-sky survey in the energy range 0.75 to 30 MeV was provided by NASA's Compton Gamma-Ray Observatory (COMPTEL) as discussed by the authors, which contains firm and marginal detections of continuum and line emitting sources and presents upper limits for various types of objects.