STATUS OF CURRENT AND FUTURE RUSSIAN SATELLITE SYSTEMS by Roscosmos / Roshydromet. Presented to CGMS-45 plenary session

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STATUS OF CURRENT AND FUTURE RUSSIAN SATELLITE SYSTEMS by Roscosmos / Roshydromet Presented to CGMS-45 plenary session 2017

Objectives: Hydrometeorological Satellite Observation System HYDROMETEOROLOGY AND GEOPHYSICAL MONITORING - atmosphere and ocean monitoring and forecasting; - ice monitoring for navigation in Arctic and Antarctic regions; - heliogeophysical information service; - ground-based observation data collection and retransmission via satellite. DISASTER MONITORING - disaster features detection; - disaster impact /damage assessment; - risk areas examination, including an assessment of probability and scale of disaster. CLIMATE MONITORING - climate, ocean and landscape studies based on radiation balance, cloud cover, ozone layer, cryosphere, sea surface temperature and ocean color, vegetation cover data, etc. ENVIRONMENTAL POLLUTION MONITORING - environmental pollution mapping for atmosphere, land surface and ocean; - assessment of risk areas for spreading contamination, including radioactive contamination. Slide: 2

Ground Segment of Earth Observation Satellite System Core Centers of the Integrated Geographically Distributed Information System of Earth Remote Sensing (IGDIS ERS) Satellite Data Receiving Centers: European (SRC Planeta, Moscow - Obninsk - Dolgoprudny) Moscow Novosibirsk Khabarovsk Siberian (SRC Planeta, Novosibirsk) Far-Eastern (SRC Planeta, Khabarovsk) - more than 70 local points Daily State Research Center "Planeta": receives more than 1,3 TB satellite data; produces more than 430 types of satellite-based products; provides data for more than 540 federal and regional users. Slide: 3

Slide: 4 Coordination Group for Meteorological Satellites - CGMS Russian Meteorological Satellite Systems (Federal Space Program for 2016-2025) 2009 2010 2011 2012 2013 2014 2015 2016 2017 2018 2019 2020 2021 2022 2023 2024 2025 ELECTRO-L N 1 (76 E) launched on January 20, 2010 GEO ELECTRO-L N 2 (77.8 E) launched on December 11, 2015 ELECTRO-L N 3 (TBD) ELECTRO-L N 4 (TBD) ELECTRO-L N 5 (TBD) ARCTICA-M N 1 HEO ARCTICA-M N 2 ARCTICA-M N 3 ARCTICA-M N 4 ARCTICA-M N 5 METEOR-М N 1 launched on September 17, 2009 LEO METEOR-M N 2 - launched on July 8, 2014 METEOR-М N 2-1 METEOR-М N 2-2 METEOR -М N 2-3 METEOR-М N 2-4

CAL/VAL System for Satellite Data and Products

Status of Current GEO Satellite Systems Slide: 6

ELECTRO-L General Design Three-axis high-precision stabilization In-orbit mass 1500 kg Payload mass 370 kg Lifetime 10 years Longitude 76 E, 14.5 E, 165.8 E Data dissemination format HRIT/LRIT Image repeat cycle 30/15 min Russian geoary satellite Electro-L N2 on 11 December 2015 Mission objectives Operational observation of the atmosphere and the Earth surface Heliogeophysical measurements Maintaining Data Collection System and COSPAS/SARSAT Service Slide: 7

MSU-GS Basic Characteristics Number of channels VIS IR Spectral channels (µm) Parameter Value 10 3 7 0.5-0.65; 0.65-0.80; 0.8-0.9; 3.5-4.0; 5.7-7.0; 7.5-8.5; 8.2-9.2; 9.2-10.2; 10.2-11.2; 11.2-12.5 Image frame (deg x deg) 20 ± 0.5 x 20 ± 0.5 HRIT spatial resolution at sub-satellite point (km) 1.0 (VIS); 4.0 (IR) S/N ratio for VIS channels 200 NE T at 300K (K) in the band 3.5-4.0 µm in the band 5.7-7.0 µm in the band 7.5-12.5 µm Power (W) 150 0.2 0.1 0.1 Mass (kg) 88 Lifetime of basic and reserve units (years) 10 Slide: 8

Status of Electro-L N2 MSU-MR is functional with limitations (12 mkm channel is out-of-order). Absolute calibration work is currently ongoing; DCS is functional; COSPAS-SARSAT system is functional; GGAK instrument is functional; HRIT/LRIT data is being distributed via the land channels, including Internet channels. Slide: 9

Core Ground Segment for Electro-L Electro-L N2 Data collection platforms (800 DCPs) APPI-M (80 DCPs) APPI-G (3 DCPs) DCP network SKS 8/7 Receiving, transmitting and preprocessing SRC Planeta, Moscow SKS 8/7 Transmitting SPDP-E Receiving SPOI-E Receiving SRC Planeta, Dolgoprudny European Center APPI-M Control SKS 8/7 Receiving, transmitting and preprocessing SPDP-E Receiving SPOI-E Receiving SRC Planeta, Novosibirsk APPI-M Control SKS 8/7 Receiving and transmitting SPOI-E Receiving APPI-M Control SRC Planeta, Khabarovsk Siberian Center Far Eastern Center Central data processing, archiving and dissemination node SRC Planeta, Moscow Users Slide: 10

Russian Data Collection System based on geoary satellites Electro-L (76 E) Luch-5B (95 E) DCS comprises of the network of DCPs at Roshydromet observation sites, relay transponders at Russian geoary satellites of Electro and Luch series, and ground reception s at SRC Planeta centers. The system will be further complemented with the launch of high-elliptical orbit satellites of Arctica series. Data is currently being collected from over 600 Roshydromet observation network, including difficult to access s (114), and hydrological sites (over 20). 11

Status of Current LEO Satellite Systems Slide: 12

METEOR-M General Design In-orbit mass 2700 kg Payload mass 1200 kg Lifetime 5 years Russian meteorological satellite Meteor-М N2 was launched on July 8, 2014 Orbit Sun-synchronous Altitude 820 km Data dissemination format HRPT/LRPT Slide: 13

Meteor-M N 2 Basic Instruments Specifications Instrument Application Spectral band Swathwidth (km) Resolution (km) MSU-MR Low-resolution multi-channel scanning radiometer Global and regional cloud cover mapping, ice and snow cover observation, forest fire monitoring 0,5 12,5µm (6 channels) 2900 1 x 1 KMSS Visible spectrum scanning imager Earth surface monitoring for various applications (floods, soil and vegetation cover, ice cover) 0,4-0,9 µm (3+3 channels) 450/900 0,05/0,1 MTVZA-GY Imager-sounder (module for temperature and humidity sounding of the atmosphere) Atmospheric temperature and humidity profiles, SST, sea level wind, etc. 10,6-183,3 GHz (26 channels) 1500 16 90 IRFS-2 Advanced IR sounder (infrared Fourierspectrometer) Atmospheric temperature and humidity profiles 5-15 µm 2000 35 Severjanin-M X-band synthetic aperture radar GGAK-M Heliogeophysical measurements suite BRK SSPD Data collection system (DCS) All-weather Ice coverage monitoring 9500-9700 MHz 600 0,5/1 Heliogeophysical data Data retransmission from DCPs Slide: 14

Advanced IR Sounder IRFS-2 Spectral range: wavelength wave number Parameter Units Value µm cm -1 5-15 2000-665 Reference channel wavelength µm 1.06 Maximum optical path difference (OPD) mm 17 Angular size of FOV mrad 40 x 40 Spatial resolution (at sub-satellite point) km 35 Swath width and spatial sampling km 2500, 110 2000, 100 Duration of the interferogram measurement s 0.5 Mass kg 45-50 Power W 50 Spectral range Absorption band Application 665 to 780 cm -1 CO 2 Temperature profile 790 to 980 cm -1 Atmospheric window Surface parameters (T s, ε ν ), cloud properties 1000 to 1070 cm -1 O 3 Ozone sounding 1080 to 1150 cm -1 Atmospheric window T s, ε ν,; cloud properties 1210 to 1650 cm -1 H 2 O, N 2 O, CH 4 Moisture profile, CH 4, N 2 O, column amounts Slide: 15

Status of Meteor-M N2 Spacecraft MSU-MR instrument is fully functional; MTVZA-GY instrument is fully functional; KMSS instrument is fully functional; IKFS-2 instrument is fully functional; Severjanin instrument is functional with limitations (due to low signal/noise ratio); DCS is functional; LRPT transmission is functional; GGAK-M is functional. Slide: 16

1. Direct broadcast Coordination Group for Meteorological Satellites - CGMS Meteor-M N2 Data Dissemination MSU-MR and MTVZA-GY data are currently being disseminated at 1.7 GHz band in direct broadcast mode (HRPT-like). Data format description is available at SRC Planeta WEB-site http://planet.iitp.ru/english/spacecraft/meteor_m_n2_structure_eng.htm 2. Global data access MTVZA instrument data, declared as Essential according to Roshydromet- EUMETSAT bilateral Agreement, is available in HDF format to EUMETSAT third party service in near-real time via FTP channel, free to be redistributed to all interested parties. Test distribution of preprocessed IRFS-2 data has been started. 3. L2 products access Some L2 products are regularly generated by SRC Planeta and can be accessed via SRC Planeta WEB-site. Slide: 17

Core Ground Segment for Meteor-M N 2 Meteor-M N 2 transmitting radio terminals DCP Dolgoprudny, Kursk, Obninsk, Valday, Ryazan LRPT s network PK-9 Receiving PK-3,5 Receiving SPOI-2L Receiving KPI-4,8 Receiving PRI-PM Receiving PRI-PM Receiving SPOI-2L Receiving KPI-4,8 Receiving KPI-4,8 Receiving PK-9 Receiving SPOI-2L Receiving Operational archive and data transfer system SRC Planeta, Dolgoprudny European Center Operational archive and data transfer system SRC Planeta, Obninsk Central data processing, archiving and dissemination node Data processing, archiving and dissemination system SRC Planeta, Novosibirsk Siberian Center Users Data processing, archiving and dissemination system SRC Planeta, Khabarovsk Far Eastern Center SRC Planeta, Moscow Slide: 18

Status of Future GEO Satellite Systems Slide: 19

The launch dates for: Electro-L N3 2018; Electro-L N4 2020; Electro-L N5 2022. The Electro-L N 3,4,5 payload is similar to the Electro-L N 2, but with improved instrument performance. Orbital positions: for Electro-L N3, 4, 5 TBD. Slide: 20

Electro-M (3-rd generation) Parameter Electro-M N 1 longitude Electro-M N 2 longitude Electro-M N 3 longitude Value 14,5º E 76º E 165,8º E MSU-GS-M channels 20 MSU-GSM spatial resolution at sub-satellite point, km - VIS and NIR - IR 0,5 2 Mission objectives Operational observation of the atmosphere and the Earth surface (MSU-GSM, IRFS-GS, ERBR, LM, GGAK-E/M) Heliogeophysical measurements Maintaining Data Collection System and COSPAS/SARSAT Service MSU-GSM scan period, min - regular mode (full Earth disk) - frequent mode (fragments of the Earth disk) 15 5 Mass, kg 1870 Expected lifetime, years 10 Slide: 21

Electro-M Basic Payload MSU-GSM (Multichannel scanning unit Geoary-M) instrument, providing full Earth disk measurements in 20 channels (VIS, NIR, IR) with 10 min period between scanning sessions and spatial resolution about 0,5 km for VIS and 2,0 km for IR channels at sub-satellite point; IKFS-GS (Infrared Fourier-transform Spectrometer - Geoary) instrument providing measurements in 3.7-6 µm and 8.3-15.4 µm spectral bands with 4 km spatial resolution (at sub-satellite point). The spectral resolution is about 0,625 cm -1. Repeat cycle is 1 hour. ERBR (Earth Radiation Budget Radiometer) instrument, providing measurements in 0.32 4.0 and 0.32 30.0 µm spectral bands with spatial resolution 50 km every 5 min. LM (Lightning Mapper) instrument, providing continuous detection at 777,4 µm. GGAK-E/M (Geliogeophysical instrument suite) modernized GGAK-E. BRTK-M on-board radio-retransmitting suite, providing data downlink in UHF and SHF bands. Slide: 22

Status of Future LEO Satellite Systems Slide: 23

Future LEO Satellite Orbit Orbit Satellite Operator Time, ETC Height Launch data Instrument SSO SSO METEOR-M N2-1 METEOR-M N2-2 ROSH 15.09 816,4 km 2017 MSU-MR, MTVZA, IRFS-2, KMSS, DCS, ROSH COSPAS-SARSAR 09.00 815,2 km 2018 Dissemination: HRPT, LRPT SSO SSO METEOR-M N2-3 METEOR-M N2-4 ROSH 15.09 820,7 km 2020 ROSH 09.00 820,7 km 2021 MSU-MR, MTVZA, IRFS-2, KMSS, DCS, COSPAS-SARSAR, METEOSAR, GGAK-M2 Dissemination: HRPT, LRPT Slide: 24

Meteor-MP (4-th generation) Spacecraft mass: 3300 kg, deployed size: 21,5 3,2 4,4 m Slide: 25

METEOR-MP Basic Payload (Meteorological) Low-resolution multi-channel scanning radiometer; Visible spectrum scanning imager (moderate resolution multispectral imaging system); Infra-red Fourier-transform spectrometer; Atmospheric composition spectrometer; Microwave imager-sounder (module for temperature and humidity sounding of the atmosphere); Side-looking radar system; Radio-occultation instrument; Data collection system; Heliogeophysical instruments suite; 137MHz data downlink system; 1.7GHz data downlink system; X-band data downlink system. Slide: 26

Status of Future HEO Satellite Systems Slide: 27

Arctica-M Parameter Value Orbit: Apogee, km Perigee, km Inclination, deg Period, h 40000 1000 63,4 12 Full number of MSU-A spectral channel 10 Spectral range, µm from 0,5 to 12,5 Resolution (at nadir): - VIS-channel, km 1 - IR-channel, km 4 Frequency of full Earth disk observation, min: - regular mode 30 - frequent mode 15 Spacecraft mass, kg 2000 Slide: 28

Advantages of the High-Elliptic Orbits (HEO) over Geoary Orbits for Arctic Observations End of the operational part of HEO Beginning of the operational part of HEO 1. Providing the quasi-continuous observations for Arctic region (areas at latitude higher than 60 о N). 2. The quasi- continuous observations need no more than 2 satellites Available area for monitoring from HEO 70 - limiting angle of available observation Available area for monitoring from geoary orbit Slide: 29

Space System Ballistic Configuration Spacecraft N 2 Spacecraft N 1 Parameter of the spacecraft orbits: - apogee altitude (α) ~ 40000 km; - perigee altitude (π) ~ 1000 km; - inclination (i) ~ 63 о ; - orbital period - 12 hours Positional relationship of the spacecraft orbits: coincidence of ascending node (Ω) of the spacecraft N1 orbit and descending node ( ) of the spacecraft N2 orbit Ω Location of the orbit operational parts: - beginning of the operational part of each spacecraft is 3.2 hours before the apogee passing; - end of the operational part is 3.2 hours after the apogee passing; - relative drift of the orbit operational parts of spacecraft N1 and spacecraft N2 equals 6 hours; - provides continuous observation of the arctic territories, located at the latitude, higher than 60 о N; - provides continuous radio visibility of the spacecrafts orbit operational parts at the ground s in Moscow, Novosibirsk, Khabarovsk Slide: 30

Arctica-M Basic Payload The multichannel scanning unit MSU-A, 10 spectral channels (3 VIS and 7 IR channels). The heliogeophysical instruments suite GGAK-A, providing the heliogeophysical measurements at the Molnia orbit. The on-board radio-retransmitting complex BRTK-A, providing data downlink in UHF and SHF bands. The launch of the first satellite of Arctica series is scheduled for 2019. Slide: 31

Thanks for attention! Slide: 32