The operational deployment of MSG-1 at the beginning of 2004, the first of a series of four Meteosat Second Generation (MSG) satellites, marks the start of a new era in Europe for the meteorological observations from the geostationary orbit. This new system shall be the backbone of the European operational meteorological services up to at least 2015. The time required for the definition and the development of new space systems as well as the approval process of such complex programs implies to plan well ahead for the future missions. EUMETSAT have initiated in 2001, with ESA support, a User Consultation Process aiming at preparing for a future operational geostationary meteorological satellite system in the post-MSG era, named Meteosat Third Generation (MTG). The first phase of the User Consultation Process was devoted to the definition and consolidation of end user requirements and priorities in the field of Nowcasting and Very Short Term Weather Forecasting (NWC), Medium/Short Range global and regional Numerical Weather Prediction (NWP), Climate and Air Composition Monitoring and to the definition of the relevant observation techniques.
After an initial post-MSG mission study (2003-2004) where preliminary instrument concepts were investigated allowing in the same time to consolidate the technical requirements for the overall system study, a MTG pre-phase A study has been performed for the overall system concept, architecture and programmatic aspects during 2004-2005 time frame.
This paper provides an overview of the outcome of the MTG sensor concept studies conducted in the frame of the pre-phase A. It namely focuses onto the Imaging and Sounding Missions, highlights the resulting instrument concepts, establishes the critical technologies and introduces the study steps towards the implementation of the MTG development programme.
EUMETSAT and ESA initiated in 2000 joint preparatory activities for the formulation and definition of the
Meteosat Third Generation (MTG) geostationary system, to ensure continuity and improvement of current
Meteosat Second Generation (MSG) services. MTG will become the backbone of the European operational
meteorological applications taking the relay from MSG by 2017, and warranting the continuation of the earth
imagery mission supported by the Spin Enhanced Visible and Infrared Imager (SEVIRI).
The early program definition phases were devoted to the discussion and consolidation of end user
requirements and their priorities in meteorology fields as Nowcasting and Very Short Term Weather
Forecasting (NWC), Medium/Short Range global and regional Numerical Weather Prediction (NWP),
Climate and Air Composition Monitoring and the identification of the relevant observation techniques. In the
system conceptualization process, the following missions have been analyzed:
• Full Disc High Spectral resolution Imagery (FDHSI)
• High Resolution and Fast Imagery (HRFI)
• Lightning detection Mission (LI)
• IR Sounding Mission (IRS)
• UV-VIS-NIR Sounding Mission as a payload complement (UVN).
After pre-phase A mission studies (2003-2006), where preliminary instrument concepts were investigated
allowing the consolidation of the most critical and demanding technical requirements, phase A studies were
launched at the beginning of February (2007-2008) addressing both the space segment system feasibility and
ground and operations programmatic aspects.
The space segment, phase A level, studies covered the entire suite of optical instruments identified in the
preliminary assessments including: 1) a flexible combined imager for both FDHSI and HRFI missions; 2) a
Fourier Transform Spectrometer for IRS observations; and 3) a lightning detector sensor. The study of
concepts and implementation of the UVN mission are covered by the efforts of ESA and the European Union
(EU) in the framework of the Global Monitoring for Environment and Security (GMES) Sentinel 4 program.
This paper provides an overview of the outcome of the MTG System analyses at the end of phase A
confirming its technical feasibility, the key characteristics of the intended missions, and the progress
accomplished in the definition of the satellite optical payloads.
ESA and EUMETSAT have initiated joint preparatory activities for the formulation and definition of
the Meteosat Third Generation (MTG) geostationary system to ensure the continuity and improvement
of the Meteosat Second Generation (MSG) system. The MTG will become the new system to be the
backbone of the European operational meteorological services from 2015, in particular, will ensure the
continuation of the imagery missions. The first phases were devoted to the definition and consolidation
of end user requirements and priorities in the field of Nowcasting and Very Short Term Weather
Forecasting (NWC), Medium/Short Range global and regional Numerical Weather Prediction (NWP),
Climate and Air Composition Monitoring and to the definition of the relevant observation techniques.
The following missions have been analysed and preliminary concepts studied:
The Flexible Combined Imager, an improvement of the actual MSG-SEVIRI Imager
Lightning Imagery Mission
IR Sounding Mission
UV-VIS-NIR Sounding Mission as a payload complement from GMES.
After pre-phase A mission studies (2003-2006), where preliminary instrument concepts were
investigated allowing in the same time to consolidate the technical requirements for the overall system
study, a phase A study on MTG has been launched at the beginning of February 2007 for the space
segment system feasibility and programmatic aspects to be accomplished during 2007-2008 time
frame. The space segment phase A study will cover all elements to the level of details allowing to
conclude on the feasibility of the system and to produce cost estimates with a good level of confidence.
This paper provides an overview of the outcome of the MTG space segment at the end of phase A,
addressing the progress accomplished for the various payloads in terms of achievable performances
including Radiometry and Image Navigation and Registration aspects. It namely focuses onto the
Imaging and IR Sounding, Lightning Missions, introduces the UV-VIS-NIR Sounding mission concept
status, establishes the critical technologies and introduces the way forward to the implementation of the
MTG development programme.
ESA and EUMETSAT have initiated joint preparatory activities for the formulation and definition of the Meteosat Third
Generation (MTG) geostationary system to ensure the continuity and improvement of the Meteosat Second Generation
(MSG) system. The MTG will become the new system to be the backbone of the European operational meteorological
services from 2015, in particular, will ensure the continuation of the imagery missions. The first phases were devoted
to the definition and consolidation of end user requirements and priorities in the field of Nowcasting and Very Short
Term Weather Forecasting (NWC), Medium/Short Range global and regional Numerical Weather Prediction (NWP),
Climate and Air Composition Monitoring and to the definition of the relevant observation techniques. The following
missions have been analysed and preliminary concepts studied:
- High Resolution Fast Imagery Mission (successor to MSG SEVIRI HRV mission)
- Full Disk High Spectral Resolution Imagery Mission (successor to the mission of other MSG-SEVIRI channels)
- Lightning Imagery Mission
- IR Sounding Mission
- UV-VIS-NIR Sounding Mission
After pre-phase A mission studies (2003-2006), where preliminary instrument concepts were investigated allowing in the
same time to consolidate the technical requirements for the overall system study, a phase A study on MTG has been
launched at the beginning of February 2007 for the space segment system feasibility and programmatic aspects to be
accomplished during 2007-2008 time frame. The space segment phase A study will cover all elements to the level of
details allowing to conclude on the feasibility of the system and to produce cost estimates with a good level of
confidence.
This paper addresses an overview of the outcome of the MTG space segment progress (spacecraft concept, payload
preliminary design studies) accomplished in the frame of the phase A. It namely focuses onto the Imaging and IR
Sounding Missions, highlights the platform and resulting instrument concepts, establishes the critical technologies and
introduces the study progress towards the implementation of the MTG development programme.
The operational deployment of MSG-1 at the beginning of 2004, the first of a series of four Meteosat Second Generation (MSG) satellites, marks the start of a new era in Europe for the meteorological observations from the geostationary orbit. This new system shall be the backbone of the European operational meteorological services up to at least 2015. The time required for the definition and the development of new space systems as well as the approval process of such complex programs implies anyhow to plan well ahead for the future missions. EUMETSAT have initiated in 2001, with ESA support, a User Consultation Process aiming at preparing for a future operational geostationary meteorological satellite system in the post-MSG era, named Meteosat Third Generation (MTG). The first phase of the User Consultation Process was devoted to the definition and consolidation of end user requirements and priorities in the field of Nowcasting and Very Short Term Weather Forecasting (NWC), Medium/Short Range global and regional Numerical Weather Prediction (NWP), Climate and Air Composition Monitoring and to the definition of the relevant observation techniques. The following missions have been analysed and preliminary concepts studied: High Resolution Fast Imagery Mission (successor to MSG SEVIRI HRV mission); Full Disk High Spectral Resolution Imagery Mission (successor to the mission of other MSG-SEVIRI channels); Lightning Imagery Mission; IR Sounding Mission; UV-VIS-NIR Sounding Mission. After an initial post-MSG mission study (2003-2004) where preliminary instrument concepts were investigated allowing in the same time to consolidate the technical requirements for the overall system study, a pre-phase A study on MTG is on its final way for the overall system concept, architecture and programmatic aspects during 2004-2005 time frame. This paper provides an overview of the outcome of the MTG sensor concept studies conducted in the frame of the pre-phase A. It namely focuses onto the Imaging and Sounding Missions, highlights the resulting instrument concepts, establishes the critical technologies and introduces the study steps towards the implementation of the MTG development programme.
The operational deployment of MSG-1 at the beginning of 2004, the first of a series of four Meteosat Second Generation (MSG) satellites, marks the start of a new era in Europe for the meteorological observations from the geostationary orbit. The new system shall be the backbone of the European operational meteorological services up to at least 2015. The time required for the definition and the development of new space systems as well as the approval process of such complex programs implies anyhow to plan well ahead for the future missions.
EUMETSAT have initiated in 2001, with ESA support, a User Consultation Process aiming at preparing for a future operational geostationary meteorological satellite system in the post-MSG era, named Meteosat Third Generation (MTG). The first phase of the User Consultation Process was devoted to the definition and consolidation of end user requirements and priorities in the field of Nowcasting and Very Short Term Weather Forecasting (NWC), Medium/Short Range global and regional Numerical Weather Prediction (NWP), Climate and Air Composition Monitoring and to the definition of the relevant observation techniques. The intermediate results of this first phase were presented to and discussed with the user community at the first Post-MSG User Consultation Workshop convened by EUMETSAT in November 2001 and further consolidated with the support of ESA in the area of potential observation techniques and sensor concepts via dedicated studies conducted in the 2003/2004 time frame. The following missions have been analysed and preliminary concepts studied:
-High Resolution Fast Imagery Mission (successor to MSG SEVIRI HRV mission)
-Full Disk High Spectral Resolution Imagery Mission (successor to the mission of other MSG-SEVIRI channels)
-Lightning Imagery Mission
-IR Sounding Mission
-UV-VIS-NIR-SWIR Sounding Mission
In March 2003, ESA and EUMETSAT derived technical requirements applicable to the MTG mission study where preliminary instrument concepts were investigated allowing in the same time to consolidate the technical requirements for the overall system study.
This paper provides an overview of the outcome of the MTG observation techniques and sensor concept studies conducted in 2003-2004. It namely focuses onto the Imaging and Sounding Missions, highlights the resulting instrument concepts and introduces the study steps towards the implementation of the MTG development programme.
Following the successful commissioning of the first Meteosat Second Generation (MSG) series, EUMETSAT and the European Space Agency (ESA) are actively preparing the Meteosat Third Generation (MTG) mission to plan for a future operational geostationary meteorological satellite system in the post 2015 time frame.
Early user consultation activities of EUMETSAT and ESA for the MTG mission culminated with a user consultation workshop held in November 2001. The User Consultation Process was devoted to the definition and consolidation of end user requirements and priorities in the field of Medium/Short Range global and regional Numerical Weather Prediction (NWP), Nowcasting and Very Short Term Weather Forecasting (NWC) and to the definition of the relevant observation techniques.
Studies on potential observation techniques and sensor concepts have been initiated, covering three distinct imagery missions dedicated to operational meteorology, with emphasis on nowcasting and very short term forecasting and two sounding missions:
- The high resolution fast imagery mission aiming at 5 minutes revisit time with 0.5 km resolution
- The full disk high spectral resolution imagery mission with a large number of spectral channels and with high radiometric performance
- The lighting imagery mission, capable of detecting very low energy events with high reliability
- The infrared sounding mission supporting NWP through the provision of atmospheric motion vectors and temperature and water vapour profiles
- The UV/VIS/SWIR sounding mission dedicated to atmospheric chemistry
The paper describes the MTG user requirements and the preliminary instruments concept, with emphasis on the observation missions.
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