IAA. 1.9: Aerosol-UA - Satellite remote sensing of aerosols in the Earth atmosphere

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IAA. 1.9: Aerosol-UA - Satellite remote sensing of aerosols in the Earth atmosphere Ya. Yatskiv (1), O. Degtyaryov (3), G. Milinevsky (1,2), I. Syniavskyi (1), A. Bovchaliuk (1), Yu. Ivanov (1), M. Sosonkin (1), E. Udodov (2), A. Delets (1), M. Mishchenko (4), V. Rosenbush (1), A. Makarov (3), V.Masley (3), V. Danylevsky (2), S.Moskalev (3), V. Bovchaliuk (2), D. Hladikov (1,2), D. Ivanov (1), A. Lukenyuk (5), A. Shymkiv (5) (1) Main Astronomical Observatory, NAS of Ukraine (2) Taras Shevchenko National University of Kyiv, Ukraine (3) Yangel Yuzhnoye State Design Office of State Space Agency of Ukraine (4) NASA Goddard Institute for Space Studies, USA (5) Lviv Center of the Institute of Space Research, NAS and State Space Agency of Ukraine genmilinevsky@gmail.com

Forest fire near Kyiv (200 km) from 10km altitude, November 1, 2015

Climate system shift

Atmospheric aerosol, shape and size Saharan dust Smoke cluster Pollen China pollution Typical size 0.001 20 μm Lot of types natural and industrial/ anthropogenic aerosols Volcanic ash Pollen Sea salt Soot

Microphysics of aerosol for climate models Atmospheric aerosols direct climate impact by absorbing and reflecting sunlight producing heating or cooling Aerosols also cause indirect cooling effect by modulating cloud properties: increased numbers of aerosols lead to larger numbers of smaller cloud droplets Climate effects of aerosols remain poorly quantified due to lack data for microphysics (IPCC 2007) 1367 W/m 2 vs 341 W/m 2 (refractive index, type, size )

Why aerosol? Radiative forcing concept Stocker et al. (2013)

Why polarization? Why scanning? Microphysics dependency in polarimetric data Needs in polarization and many scattering angles! (Kokhanovsky et al., Earth-Science Reviews, 2015)

Structure Aerosol-UA project Instruments: ScanPol + MSIP Data processing: GRASP, Mission products Platform: YuzhSat? Validation AERONET, Lidar

Basic strategy: receive max information in the reflected sunlight Aerosol-UA: ScanPol (I, Q, U) + MSIP (image, I, Q, U) Polarization is a relative measurement that can be made accurately. Polarimetric ScanPol measurements can stably calibrated on the orbit. Polarization change with scattering angle and wavelength gives size, refractive index and shape of aerosol. Synergy of scanner and imager will produce new quality of data different from similar aerosol missions.

Orbital platform characteristics needs Orbit Type: sun-synchronous Inclination: ~98 Altitude: ~670 km Platform needs Pointing accuracy: ~0.1 Total mass of scientific payload estimated: ~20 kg Power for payload: 50 W Design life: >3 years ScanPol: Scan: period 1.5 sec, exp. 1ms, along ground track, +50/-60 Spatial resolution: ~6 km at nadir MSIP: Image:+60/-60, 770x770 km Spatial resolution: ~3 km at nadir

Aerosol-UA scanning-imaging geometry ScanPol Lengths IFOV along trajectory MSIP

Field-Of-View MSIP and ScanPol MSIP ScanPol track

ScanPol polarimeter: optical alignment Spectral band: 370-1610 nm, six spectral channels: 370 nm tropospheric aerosol and top of clouds 410 nm aerosol over ocean and surface 555 нм aerosol over ocean and surface, ocean color 865 nm aerosol over ocean and surface 1378 nm separate cirrus clouds, stratosphere aerosol, separation of troposphere and stratosphere aerosol in case of volcanic eruption 1610 nm separation surface signal from aerosol over Earth surface Observable Stokes parameters: I, Q, U (0,90,45,135 ) Photometric accuracy: 4% Polarimetric accuracy: 0.15% On-board calibration: all three Stokes parameters Filter ½ width 20-60 nm

Optic-mechanical unit of ScanPol designed for test from aircraft in 2017 Data acquisition unit Opticmechanical unit Motor Scanning mirrors and calibration

MultiSpectral Imager-Polarimeter (MSIP) MSIP main purposes: aerosol/clouds parameters measurements and aerosol - clouds separation Three spectral polarimetric channels: 410, 555, 865 nm 0, 45, 90, 135 polarization each Two intensity channels: (1) 410, 443, 470, 490; (2) 555, 670, 865, 910 nm FOV: 60 x60, 770x770 km, resolution 3 km Images rate 1.5 s -1 6.0 s -1 (dependent on data rate transmission), exposure <0.5 s Calibration using ScanPol scans, <1% accuracy

MultiSpectral Imager-Polarimeter (MSIP) Polarization 0, 45, 90, 135 410 nm 555 nm 865 nm Overall 20 Sp/Pol channels Intensity 410+443+ 555+670+ +470+490 nm +865+936 nm

MSIP optical channel design, 2016 Input windows of MSIP Five units of MSIP linear design

ScanPol and MSIP polarimeters for space missions Aerosol-UA, August 2016

ScanPol and MSIP polarimeters for space missions Aerosol-UA, September 2016

Characteristics of payload 1. Total mass of scientific payload ~23 kg 2. Power for payload: 50 W approximate estimate 3. Data volume per 24 hours : SkanPol MSIP 0.2 Gbyte 24 Gbyte approximate estimate and will be optimized for the capabilities of the platform The experiment features 1. The need for measurements at each orbit round. 2. The ability to deploy the platform in the direction of the Moon (the Sun) for calibration.

Data processing 1. Data Center concept has been developed 2. Testing the GRASP software for synthetic data processing

Aerosol-UA performance analysis using synthetic observation Angstrom exponent Aerosol optical thickness (AOT) calculations by GRASP for synthetic data and PARASOL data for August, 14, 2010

Ground-based support of Aerosol-UA: data validation in AERONET network Direct simultaneous measurements - Permanent AERONET sites - mobile AERONET sites POLDER/AERONET data comparison

Conclusions and Objectives In comparison to the several aerosol polarimetric missions planned for 2017-2020 where Aerosol-UA instrument concept provides synergy of precision scanner-polarimeter and imager-polarimeter 1. Finalizing ScanPol model calibration spring of 2017 2. Construction of MSIP one channel spring of 2017 3. Data processing algorithm mid 2017 4. On flight ScanPol testing fall 2017 5. Platform choice mid-2017 6. MSIP channel construction end of 2017