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Marcel Dobber

Researcher at Royal Netherlands Meteorological Institute

Publications -  39
Citations -  2601

Marcel Dobber is an academic researcher from Royal Netherlands Meteorological Institute. The author has contributed to research in topics: Ozone Monitoring Instrument & SCIAMACHY. The author has an hindex of 13, co-authored 38 publications receiving 2323 citations. Previous affiliations of Marcel Dobber include University of Amsterdam.

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The ozone monitoring instrument

TL;DR: The Ozone Monitoring Instrument is a ultraviolet/visible nadir solar backscatter spectrometer, which provides nearly global coverage in one day with a spatial resolution of 13 km/spl times/24 km and will enable detection of air pollution on urban scale resolution.
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Earth surface reflectance climatology from 3 years of OMI data

TL;DR: In this paper, a global map of the Earth's surface Lambertian equivalent reflectance (LER) is constructed using 3 years of Ozone Monitoring Instrument (OMI) measurements obtained between October 2004 and October 2007 at 23 wavelengths between 328 and 500 nm.
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Ozone monitoring instrument calibration

TL;DR: The OMI instrument is an ultraviolet-visible imaging spectrograph that uses two-dimensional charge-coupled device detectors to register both the spectrum and the swath perpendicular to the flight direction with a 115/spl deg/ wide swath, which enables global daily ground coverage with high spatial resolution.
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Validation of Ozone Monitoring Instrument level 1b data products

TL;DR: In this article, the spectral and spatial stray light corrections from collection 2 data to collection 3 data are presented and discussed, and the viewing angle dependence of the radiance and the irradiance goniometry are discussed.
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The high-resolution solar reference spectrum between 250 and 550 nm and its application to measurements with the ozone monitoring instrument

TL;DR: In this article, a new high-resolution solar reference spectrum in the spec- tral range between 250 and 550 nm was constructed based on available low and high resolution spectra and discussed the main sources of uncertainty.