Results 31 to 40 of about 174,511 (298)

Light scattering and absorption properties of dust particles retrieved from satellite measurements [PDF]

open access: yes, 2008
We use the radiative transfer model and chemistry transport model to improve our retrievals of dust optical properties from satellite measurements. The optical depth and absorbing optical depth of mineral dust can be obtained from our improved retrieval ...
Hu, R-M., Sokhi, R.S.
core   +1 more source

Aerosol Mineralogical Study Using Laboratory and IASI Measurements: Application to East Asian Deserts

open access: yesRemote Sensing, 2022
East Asia is the second-largest mineral dust source in the world, after the Sahara. When dispersed in the atmosphere, mineral dust can alter the Earth’s radiation budget by changing the atmosphere’s absorption and scattering properties.
Perla Alalam   +4 more
doaj   +1 more source

Dustbuster: a compact impact-ionization time-of-flight mass spectrometer for in situ analysis of cosmic dust [PDF]

open access: yes, 2002
We report on the design and testing of a compact impact-ionization time-of-flight mass spectrometer for analysis of cosmic dust, suitable for use on deep space missions.
Ahrens, Thomas J.   +2 more
core   +1 more source

Long-term (2002–2012) investigation of Saharan dust transport events at Mt. Cimone GAW global station, Italy (2165 m a.s.l.)

open access: yesElementa: Science of the Anthropocene, 2016
Mineral dust transport from North Africa towards the Mediterranean basin and Europe was monitored over an 11-y period (2002–2012) using the continuous observations made at Mt. Cimone WMO/GAW global station (CMN).
Rocco Duchi   +10 more
doaj   +1 more source

Pollution affects Arabian and Saharan dust optical properties in the eastern Mediterranean [PDF]

open access: yesAtmospheric Chemistry and Physics
Uncertainties in the direct radiative effect of mineral dust result from the variability in its optical properties but are also influenced by mixing with anthropogenic aerosols (“pollution”), e.g., black carbon or sulfates.
M. Teri   +16 more
doaj   +1 more source

Changes in dissolved iron deposition to the oceans driven by human activity: a 3-D global modelling study [PDF]

open access: yes, 2015
The global atmospheric iron (Fe) cycle is parameterized in the global 3-D chemical transport model TM4-ECPL to simulate the proton- and the organic ligand-promoted mineral-Fe dissolution as well as the aqueous-phase photochemical reactions between the ...
Baker, Alex   +5 more
core   +2 more sources

Carbon sequestration in the deep Atlantic enhanced by Saharan dust [PDF]

open access: yes, 2017
Enhanced atmospheric input of dust-borne nutrients and minerals to the remote surface ocean can potentially increase carbon uptake and sequestration at depth.
A Baker   +89 more
core   +5 more sources

Understanding Haze: Modeling Size-Resolved Mineral Aerosol from Satellite Remote Sensing

open access: yesRemote Sensing, 2022
Mineral dust aerosols are composed of a complex mixture of silicates, carbonates, oxides, and sulfates. The minerals’ chemical composition and size distribution are vital parameters to evaluate dust environmental impacts.
Nivedita Sanwlani, Reshmi Das
doaj   +1 more source

Saharan dust deposition may affect phytoplankton growth in the mediterranean sea at ecological time scales [PDF]

open access: yes, 2014
The surface waters of the Mediterranean Sea are extremely poor in the nutrients necessary for plankton growth. At the same time, the Mediterranean Sea borders with the largest and most active desert areas in the world and the atmosphere over the basin is
Baldasano Recio, José María   +4 more
core   +1 more source

3+2 + X: what is the most useful depolarization input for retrieving microphysical properties of non-spherical particles from lidar measurements using the spheroid model of Dubovik et al. (2006)? [PDF]

open access: yes, 2019
The typical multiwavelength aerosol lidar data set for inversion of optical to microphysical parameters is composed of three backscatter coefficients (β) at 355, 532, and 1064 nm and two extinction coefficients (α) at 355 and 532 nm.
Burton, Sharon P.   +6 more
core   +3 more sources

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