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Contribución de congreso (ConferenceOutput). 2020

Multi-wavelengths in-situ scattering and absorption measurements of Saharan dust particles during FRAGMENT

DIGITAL.CSIC. Repositorio Institucional del CSIC
  • Yus-Díez, Jesús
  • Pérez García-Pando, Carlos
  • Alastuey, Andrés
  • Ivančič, M.
  • González-Florez, C.
  • Gonzalez-Romero, A.
  • Klose, M.
  • Querol, Xavier
  • Pandolfi, Marco
Multi-wavelength in-situ surface scattering and
absorption properties of PM2.5 and PM10 Saharan dust
particles were measured during a dust emission field
campaign performed in L’Bour (M’Hamid, Morocco) in
September 2019 (Figure 1) within the FRAGMENT
project (FRontiers in dust minerAloGical coMposition
and its Effects upoN climaTe). The main goal of
FRAGMENT is to understand and constrain the global
mineralogical composition of dust along with its effects
upon climate. Among other issues, the field campaigns
are devoted to understanding the size distribution and
mineralogy of emitted dust and its relationship with the
parent soil properties. A wide variety of instruments for
dust characterization were deployed including a
radiometer, a fully equipped meteorological tower,
cascade impactors, saltation sensors, OPC aerosol
spectrometers, a polar nephelometer and an
aethalometer, among others., FRAGMENT has received funding from the European
Research Council (ERC) under the European Union’s
Horizon 2020 research and innovation programme
(grant agreement No. 773051). Carlos Pérez García-
Pando also acknowledges support by the AXA Research
Fund, and the Spanish Ministry of Science, Innovation
and Universities (RYC-2015-18690 and CGL2017-88911-
R), Peer reviewed
Proyecto: EC/H2020/773051




Contribución de congreso (ConferenceOutput). 2024

Performance and early results from the Earth Surface Mineral Dust Source Investigation (EMIT) Imaging Spectroscopy Mission

UPCommons. Portal del coneixement obert de la UPC
  • Green, Robert O.
  • Mahowald, Natalie
  • Thompson, David R.
  • Ung, Charlene
  • Brodrick, Philip G
  • Pollock, Randy
  • Bennett, Matthew
  • Lundeen, Sara
  • Joyce, Michael
  • Olson-Duvall, Winston
  • Oaida, Bogdan
  • Bradley, Christine
  • Pérez García-Pando, Carlos|||0000-0002-4456-0697
  • Obiso, Vincenzo
  • Gonçalves Ageitos, María|||0000-0003-3857-6403
The Earth Surface Mineral Dust Source Investigation (EMIT) acquires new observations of the Earth from a state-ofthe-art, optically fast F/1.8 visible to short wavelength infrared imaging spectrometer with high signal-to-noise ratio and excellent spectroscopic uniformity. EMIT was launched to the International Space Station from Cape Canaveral, Florida, on July 14, 2022 local time. The EMIT instrument is the latest in a series of more than 30 imaging spectrometers and testbeds developed at the Jet Propulsion Laboratory, beginning with the Airborne Imaging Spectrometer that first flew in 1982. EMIT’s science objectives use the spectral signatures of minerals observed across the Earth’s arid and semi-arid lands containing dust sources to update the soil composition of advanced Earth System Models (ESMs) to better understand and reduce uncertainties in mineral dust aerosol radiative forcing at the local, regional, and global scale, now and in the future. EMIT has begun to collect and deliver high-quality mineral composition determinations for the arid land regions of our planet. Over 1 billion high-quality mineral determinations are expected over the course of the one-year nominal science mission. Currently, detailed knowledge of the composition of the Earth’s mineral dust source regions is uncertain and traced to less than 5,000 surface sample mineralogical analyses. The development of the EMIT imaging spectrometer instrumentation was completed successfully, despite the severe impacts of the COVID-19 pandemic. The EMIT Science Data System is complete and running with the full set of algorithms required. These tested algorithms are open source and will be made available to the broader community. These include calibration to measured radiance, atmospheric correction to surface reflectance, mineral composition determination, aggregation to ESM resolution, and ESM runs to address the science objectives. In this paper, the instrument characteristics, ground calibration, in-orbit performance, and early science results are reported., The authors gratefully acknowledge all the elements of the National Aeronautics and Space Administration, our partners, and the science community who have contributed to the development of the EMIT mission. EMIT is supported by the National Aeronautics and Space Administration Earth Venture Instrument Program under the Earth Science Division of the Science Mission Directorate. This research was performed at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration., Objectius de Desenvolupament Sostenible::13 - Acció per al Clima




Contribución de congreso (ConferenceOutput). 2023

Performance and early results from the Earth Surface Mineral Dust Source Investigation (EMIT) Imaging Spectroscopy Mission

Recercat. Dipósit de la Recerca de Catalunya
  • Green, Robert O.
  • Mahowald, Natalie
  • Thompson, David R.
  • Ung, Charlene
  • Brodrick, Philip G
  • Pollock, Randy
  • Bennett, Matthew
  • Lundeen, Sara
  • Joyce, Michael
  • Olson-Duvall, Winston
  • Oaida, Bogdan
  • Bradley, Christine
  • Pérez García-Pando, Carlos
  • Obiso, Vincenzo
  • Gonçalves Ageitos, María
The Earth Surface Mineral Dust Source Investigation (EMIT) acquires new observations of the Earth from a state-ofthe-art, optically fast F/1.8 visible to short wavelength infrared imaging spectrometer with high signal-to-noise ratio and excellent spectroscopic uniformity. EMIT was launched to the International Space Station from Cape Canaveral, Florida, on July 14, 2022 local time. The EMIT instrument is the latest in a series of more than 30 imaging spectrometers and testbeds developed at the Jet Propulsion Laboratory, beginning with the Airborne Imaging Spectrometer that first flew in 1982. EMIT’s science objectives use the spectral signatures of minerals observed across the Earth’s arid and semi-arid lands containing dust sources to update the soil composition of advanced Earth System Models (ESMs) to better understand and reduce uncertainties in mineral dust aerosol radiative forcing at the local, regional, and global scale, now and in the future. EMIT has begun to collect and deliver high-quality mineral composition determinations for the arid land regions of our planet. Over 1 billion high-quality mineral determinations are expected over the course of the one-year nominal science mission. Currently, detailed knowledge of the composition of the Earth’s mineral dust source regions is uncertain and traced to less than 5,000 surface sample mineralogical analyses. The development of the EMIT imaging spectrometer instrumentation was completed successfully, despite the severe impacts of the COVID-19 pandemic. The EMIT Science Data System is complete and running with the full set of algorithms required. These tested algorithms are open source and will be made available to the broader community. These include calibration to measured radiance, atmospheric correction to surface reflectance, mineral composition determination, aggregation to ESM resolution, and ESM runs to address the science objectives. In this paper, the instrument characteristics, ground calibration, in-orbit performance, and early science results are reported., The authors gratefully acknowledge all the elements of the National Aeronautics and Space Administration, our partners, and the science community who have contributed to the development of the EMIT mission. EMIT is supported by the National Aeronautics and Space Administration Earth Venture Instrument Program under the Earth Science Division of the Science Mission Directorate. This research was performed at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration., Objectius de Desenvolupament Sostenible::13 - Acció per al Clima, Postprint (published version)
Proyecto: EC/H2020/773051