EUMETSAT Monitoring Weather and Climate from Space
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Report of the Commission on the Scientific Case for Human Space Exploration
1 ROYAL ASTRONOMICAL SOCIETY Burlington House, Piccadilly London W1J 0BQ, UK T: 020 7734 4582/ 3307 F: 020 7494 0166 [email protected] www.ras.org.uk Registered Charity 226545 Report of the Commission on the Scientific Case for Human Space Exploration Professor Frank Close, OBE Dr John Dudeney, OBE Professor Ken Pounds, CBE FRS 2 Contents (A) Executive Summary 3 (B) The Formation and Membership of the Commission 6 (C) The Terms of Reference 7 (D) Summary of the activities/meetings of the Commission 8 (E) The need for a wider context 8 (E1) The Wider Science Context (E2) Public inspiration, outreach and educational Context (E3) The Commercial/Industrial context (E4) The Political and International context. (F) Planetary Science on the Moon & Mars 13 (G) Astronomy from the Moon 15 (H) Human or Robotic Explorers 15 (I) Costs and Funding issues 19 (J) The Technological Challenge 20 (J1) Launcher Capabilities (J2) Radiation (K) Summary 23 (L) Acknowledgements 23 (M) Appendices: Appendix 1 Expert witnesses consulted & contributions received 24 Appendix 2 Poll of UK Astronomers 25 Appendix 3 Poll of Public Attitudes 26 Appendix 4 Selected Web Sites 27 3 (A) Executive Summary 1. Scientific missions to the Moon and Mars will address questions of profound interest to the human race. These include: the origins and history of the solar system; whether life is unique to Earth; and how life on Earth began. If our close neighbour, Mars, is found to be devoid of life, important lessons may be learned regarding the future of our own planet. 2. While the exploration of the Moon and Mars can and is being addressed by unmanned missions we have concluded that the capabilities of robotic spacecraft will fall well short of those of human explorers for the foreseeable future. -
Forthcoming Changes in the Global Satellite Observing Systems Mitch Goldberg, NOAA Outline
Forthcoming changes in the Global Satellite Observing Systems Mitch Goldberg, NOAA Outline Overview of CGMS and CEOS. Overview of the key satellite observations for NWP Discuss satellite agencies plans for these key observations Short overview emerging observations or technology which we need to pay attention to. Summary Members: CMA CNES CNSA ESA EUMETSAT IMD IOC/UNESCO JAXA JMA KMA NASA ROSCOSMOS ROSHYRDOMET WMO Observers: CSA EC ISRO KARI KORDI SOA Strategy for addressing key satellite data Begin with WIGOS 5th Workshop of the Impact of Various Observing Systems on NWP (Sedona Report). UKMO impact report: Impact of Metop and other satellite data within the Met Office global NWP system using a forecast adjoint-based sensitivity method- Feb 2012, tech repot #562 and MWR October 2013 paper Recall key observation types for NWP Compare with what space agencies are planning to provide continuity and enhancements to these observing types. Make use of the WMO OSCAR database Time scale between now and 2030. Sedona Report Observations contributing to the largest reduction of forecast errors are those observations with vertical information (temperature, water vapor). The single instrument with the largest impact is hyperspectral IR Microwave dominates because of the number of satellites and ability to view thru low water content clouds. However, there is now no single, dominating satellite sensor. GPSRO shows good impact, and largest impact per observation Atmospheric Motion Vector Winds and Scatterometers are single level data and have modest impacts Concerns about the declining number of observations into the future – mostly due to the replacement of 2 year life satellites with 7 years (e.g. -
Meteosat Third Generation (MTG) Lightning Imager (LI) Calibration and 0-1B Data Processing
Meteosat Third Generation (MTG) Lightning Imager (LI) calibration and 0-1b data processing Marcel Dobber EUMETSAT EUMETSAT-Allee 1, 64295 Darmstadt, Germany; +49-6151-807 7209 [email protected] Stephan Kox EUMETSAT EUMETSAT-Allee 1, 64295 Darmstadt, Germany; +49-6151-807 7248 [email protected] ABSTRACT The European Meteosat Third Generation (MTG) Lightning Imager (LI) is an instrument on the geostationary MTG Imager satellite series, for which the first satellite is scheduled for launch in 2021. The MTG series consists of six satellites in total: Four imager satellites, equipped with the Flexible Combined Imager (FCI) and Lightning Imager (LI) instruments, and two sounding satellites, with the Infrared Sounder (IRS) and Sentinel-4 UVN instruments. EUMETSAT will operate the satellites, instruments and ground facilities for MTG, including LI. The Lightning Imager will continuously provide lightning group and flashes information for almost the complete visible Earth disc from a geostationary orbit around zero degrees longitude in the time period 2021 to 2041. The instrument will measure day and night and will provide detected transient data from lightning optical pulses in the near-infrared at a spatial resolution that corresponds to 4.5 km x 4.5 km at the subsatellite point. The instrument also measures and provides background radiance images every 30 seconds. In this paper the Lightning Imager mission objectives and basic instrument detection principles will be described. In addition, the calibration (on ground and in orbit) and 0-1b data processing will be presented and discussed. at sub-satellite longitude of about 0 degrees, for a 1. SUMMARY geographical coverage area that covers almost the complete visible Earth disc. -
Fred Mistichelli NESDIS Spectrum Manager Rich Kelley Alion Science
WRC-19 Fred Mistichelli Geneva NESDIS Spectrum Manager 28 October to 22 November 2019 Rich Kelley Alion Science for NESDIS 29 Nov – 5 Dec 2017 o discusses spectrum concerns faced by ITSC membership between now and 2019. o covers WRC- 19 agenda items of concern in passive bands and one major new active downlink o describes rfi detection and suppression methods Satellites and agencies possibly affected by WRC-19 decisions Satellite agency Satellite agency Aqua NASA Meteor-M N2 RosHydroMet Coriolis DoD Meteor-M N2-1 RosHydroMet DWSS-1 DoD Meteor-M N2-2 RosHydroMet DWSS-2 DoD Meteor-M N2-3 RosHydroMet FY-3B CMA Meteor-M N2-4 RosHydroMet FY-3C CMA Meteor-M N2-5 RosHydroMet FY-3D CMA Meteor-MP N1 RosHydroMet FY-3E CMA Meteor-MP N2 RosHydroMet FY-3F CMA Metop-A EUMETSAT FY-3G CMA Metop-B EUMETSAT FY-3H CMA Metop-C EUMETSAT FY-3RM-1 CMA Metop-SG-A1 EUMETSAT FY-3RM-2 CMA Metop-SG-A2 EUMETSAT GCOM-W1 JAXA Metop-SG-A3 EUMETSAT GPM Core Observatory NASA Metop-SG-B1 EUMETSAT HY-2A NSOAS Metop-SG-B2 EUMETSAT JPSS-1 NOAA Metop-SG-B3 EUMETSAT JPSS-2 NOAA NOAA-15 NOAA JPSS-3 NOAA NOAA-18 NOAA JPSS-4 NOAA NOAA-19 NOAA Megha-Tropiques ISRO SNPP NOAA [1] National Ocean Satellite Application Center (China) Agenda item spectrum addressed 1.5 17.7-19.7 GHz (space-to-Earth) and 27.5-29.5 GHz (Earth-to-space) 1.6 37.5-39.5 GHz (space-to-Earth), 39.5-42.5 GHz (space-to-Earth), 47.2-50.2 GHz (Earth-to-space) and 50.4-51.4 GHz (Earth-to-space) 1.7 spectrum requirements for telemetry, tracking and command in the space operation service for the growing number of non-GSO satellites with short duration missions (small satellites/microsats/picosats) 1.13 24.25-27.5 GHz (data downlink for JPSS/MetOp) 31.8-33.4 GHz 37-40.5 GHz 47.2-50.2 GHz (passive use only) 50.4-52.6 GHz (passive use only) 81-86 GHz 1.14 regulatory actions for high-altitude platform stations (HAPS), within existing fixed-service allocations Issue 9.1.9 51.4-52.4 GHz n.b.The WMO position paper on WRC 19 agenda items is at (http://wis.wmo.int/file=3379). -
FAME-C: Cloud Property Retrieval Using Synergistic AATSR and MERIS Observations
Atmos. Meas. Tech., 7, 3873–3890, 2014 www.atmos-meas-tech.net/7/3873/2014/ doi:10.5194/amt-7-3873-2014 © Author(s) 2014. CC Attribution 3.0 License. FAME-C: cloud property retrieval using synergistic AATSR and MERIS observations C. K. Carbajal Henken, R. Lindstrot, R. Preusker, and J. Fischer Institute for Space Sciences, Freie Universität Berlin (FUB), Berlin, Germany Correspondence to: C. K. Carbajal Henken ([email protected]) Received: 29 April 2014 – Published in Atmos. Meas. Tech. Discuss.: 19 May 2014 Revised: 17 September 2014 – Accepted: 11 October 2014 – Published: 25 November 2014 Abstract. A newly developed daytime cloud property re- trievals. Biases are generally smallest for marine stratocu- trieval algorithm, FAME-C (Freie Universität Berlin AATSR mulus clouds: −0.28, 0.41 µm and −0.18 g m−2 for cloud MERIS Cloud), is presented. Synergistic observations from optical thickness, effective radius and cloud water path, re- the Advanced Along-Track Scanning Radiometer (AATSR) spectively. This is also true for the root-mean-square devia- and the Medium Resolution Imaging Spectrometer (MERIS), tion. Furthermore, both cloud top height products are com- both mounted on the polar-orbiting Environmental Satellite pared to cloud top heights derived from ground-based cloud (Envisat), are used for cloud screening. For cloudy pixels radars located at several Atmospheric Radiation Measure- two main steps are carried out in a sequential form. First, ment (ARM) sites. FAME-C mostly shows an underestima- a cloud optical and microphysical property retrieval is per- tion of cloud top heights when compared to radar observa- formed using an AATSR near-infrared and visible channel. -
The Meteosat System
THE METEOSAT SYSTEM EUM TD 05 Published by: EUMETSAT (European Organisation for the Exploitation of Meteorological Satellites) ©1998 EUMETSAT Design: Grigat und Neu THE METEOSAT SYSTEM December 1998 TABLE OF CONTENTS PREFACE .............................................................................. 5 Performance monitoring..............................................21-22 Telecommunications ...........................................................22 System frequencies ..........................................................23 1 OVERVIEW.................................................................. 6 User frequencies ...............................................................23 Introduction .............................................................................. 6 Objectives............................................................................ 7 4 THE GROUND SEGMENT................................. 24 Meteorological satellites ................................................... 7 Future programmes ............................................................ 7 Ground segment facilities ................................................24 Meteosat history ...............................................................11 Primary Ground Station ..................................................... 25 The programmes .............................................................12 Overview ........................................................................... 26 Meteosat services ..............................................................12 -
Meteosat SEVIRI Fire Radiative Power (FRP)
1 Meteosat SEVIRI Fire Radiative Power (FRP) Products from the 2 Land Surface Analysis Satellite Applications Facility (LSA 3 SAF): Part 1 - Algorithms, Product Contents & Analysis 4 5 Wooster, M.J. 1,2 , Roberts, G. 3, Freeborn, P. H. 1,4 , Xu, W. 1, Govaerts, Y. 5, Beeby, R. 1, 6 He, J. 1, A. Lattanzio 6, Fisher, D. 1,2 , and Mullen, R 1. 7 8 9 1 King’s College London, Environmental Monitoring and Modelling Research Group, 10 Department of Geography , Strand, London, WC2R 2LS, UK. 11 2 NERC National Centre for Earth Observation (NCEO), UK. 12 3 Geography and Environment, University of Southampton, Highfield, Southampton 13 SO17 1BJ, UK . 14 4 Fire Sciences Laboratory, Rocky Mountain Research Station, U.S. Forest Service, 15 Missoula, Montana, USA. 16 5 Rayference, Brussels, Belgium. 17 6 MakaluMedia, Darmstadt, Germany 18 19 20 Abstract 21 Characterising changes in landscape fire activity at better than hourly temporal 22 resolution is achievable using thermal observations of actively burning fires made 23 from geostationary Earth observation (EO) satellites. Over the last decade or more, a 24 series of research and/or operational 'active fire' products have been developed from 25 geostationary EO data, often with the aim of supporting biomass burning fuel 26 consumption and trace gas and aerosol emission calculations. Such "Fire Radiative 27 Power" (FRP) products are generated operationally from Meteosat by the Land 28 Surface Analysis Satellite Applications Facility (LSA SAF), and are available freely 29 every 15 minutes in both near real-time and archived form. These products map the 30 location of actively burning fires and characterise their rates of thermal radiative 31 energy release (fire radiative power; FRP), which is believed proportional to rates of 32 biomass consumption and smoke emission. -
SATELLITE DATA for Weather Forecasting
VOL. 98 NO. 3 MAR 2017 Mars 2020 Mission Earth Science Jobs: Seven Projections Earth & Space Science News Landsat Archive of Greenland Glaciers SATELLITE DATA for Weather Forecasting Earth & Space Science News Contents MARCH 2017 VOLUME 98, ISSUE 3 PROJECT UPDATE 20 Using LANDSAT to Take the Long View on Greenland Glaciers A new web-based data portal gives scientists access to more than 40 years of satellite imagery, providing seasonal to long-term insights into outflows from Greenland’s ice sheet. PROJECT UPDATE 32 Seeking Signs of Life and More: NASA’s Mars 2020 Mission The next Mars rover will be able to land near rugged terrain, giving scientists access to diverse landscapes. It will also cache core samples, a first step in the quest 26 to return samples to Earth. COVER OPINION Transforming Satellite Data Seven Projections 14 for Earth and Space into Weather Forecasts Science Jobs What do recent political changes mean A NASA project spans the gap between research and operations, for the job market? In the short term, not introducing new composites of satellite imagery to weather much. But long term, expect privatization, forecasters. contract employment, and more. Earth & Space Science News Eos.org // 1 Contents DEPARTMENTS Editor in Chief Barbara T. Richman: AGU, Washington, D. C., USA; eos_ [email protected] Editors Christina M. S. Cohen Wendy S. Gordon Carol A. Stein California Institute Ecologia Consulting, Department of Earth and of Technology, Pasadena, Austin, Texas, USA; Environmental Sciences, Calif., USA; wendy@ecologiaconsulting University of Illinois at cohen@srl .caltech.edu .com Chicago, Chicago, Ill., José D. -
Danish Uses of Copernicus
DANISH USES OF COPERNICUS 50 USER STORIES BASED ON EARTH OBSERVATION This joint publication is created in a collaboration between the Danish Agency for Data Supply and Efficiency – under the Danish Ministry of Energy, Utilities and Climate – and the Municipality of Copenhagen. The Danish National Copernicus Committee, which is a sub-committee under the Interministerial Space Committee, has contributed to the coordination of the publication. This publication is supported by the European Union’s Caroline Herschel Framework Partnership Agreement on Copernicus User Uptake under grant agreement No FPA 275/G/ GRO/COPE/17/10042, project FPCUP (Framework Partnership Agreement on Copernicus User Uptake), Action 2018-1-83: Developing best practice catalogue for use of Copernicus in the public sector in Denmark. Editorial Board Martin Nissen (ed.), - Agency for Data Supply and Efficiency Georg Bergeton Larsen - Agency for Data Supply and Efficiency Olav Eggers - Agency for Data Supply and Efficiency Anne Birgitte Klitgaard - National Space Office, Ministry of Higher Education and Science Leif Toudal Pedersen - DTU Space and EOLab.dk Acknowledgment: Emil Møller Rasmussen and Niels Henrik Broge. The European Commission, European Space Agency, EUMETSAT and NEREUS for user story structure and satellite imagery. Layout: Mads Christian Porse - Geological Survey of Denmark and Greenland Proofreading: Lotte Østergaard Printed by: Rosendahls A/S 2nd edition, 2021 Cover: Mapping of submerged aquatic vegetation in Denmark. The map is produced by DHI GRAS under the Velux Foundation funded project ”Mapping aquatic vegetation in Denmark from space” using machine learning and Sentinel-2 data from the Copernicus program. © DHI GRAS A/S. ISBN printed issue 978-87-94056-03-8 ISBN electronic issue (PDF) 978-87-94056-04-5 The Baltic Sea The Baltic Sea is a semi-enclosed sea bordered by eight EU Member States (Denmark, Germany, Poland, Lithuania, Latvia, Estonia, Finland, Sweden) and Russia. -
First Year of Coordinated Science Observations by Mars Express and Exomars 2016 Trace Gas Orbiter
MANUSCRIPT PRE-PRINT Icarus Special Issue “From Mars Express to ExoMars” https://doi.org/10.1016/j.icarus.2020.113707 First year of coordinated science observations by Mars Express and ExoMars 2016 Trace Gas Orbiter A. Cardesín-Moinelo1, B. Geiger1, G. Lacombe2, B. Ristic3, M. Costa1, D. Titov4, H. Svedhem4, J. Marín-Yaseli1, D. Merritt1, P. Martin1, M.A. López-Valverde5, P. Wolkenberg6, B. Gondet7 and Mars Express and ExoMars 2016 Science Ground Segment teams 1 European Space Astronomy Centre, Madrid, Spain 2 Laboratoire Atmosphères, Milieux, Observations Spatiales, Guyancourt, France 3 Royal Belgian Institute for Space Aeronomy, Brussels, Belgium 4 European Space Research and Technology Centre, Noordwijk, The Netherlands 5 Instituto de Astrofísica de Andalucía, Granada, Spain 6 Istituto Nazionale Astrofisica, Roma, Italy 7 Institut d'Astrophysique Spatiale, Orsay, Paris, France Abstract Two spacecraft launched and operated by the European Space Agency are currently performing observations in Mars orbit. For more than 15 years Mars Express has been conducting global surveys of the surface, the atmosphere and the plasma environment of the Red Planet. The Trace Gas Orbiter, the first element of the ExoMars programme, began its science phase in 2018 focusing on investigations of the atmospheric composition with unprecedented sensitivity as well as surface and subsurface studies. The coordination of observation programmes of both spacecraft aims at cross calibration of the instruments and exploitation of new opportunities provided by the presence of two spacecraft whose science operations are performed by two closely collaborating teams at the European Space Astronomy Centre (ESAC). In this paper we describe the first combined observations executed by the Mars Express and Trace Gas Orbiter missions since the start of the TGO operational phase in April 2018 until June 2019. -
10. Satellite Weather and Climate Monitoring
II. INTENSITY: ACTIVITIES AND OUTPUTS IN THE SPACE ECONOMY 10. Satellite weather and climate monitoring Meteorology was the first scientific discipline to use space Figure 1.2). The United States, the European Space Agency capabilities in the 1960s, and today satellites provide obser- and France have established the most joint operations for vations of the state of the atmosphere and ocean surface environmental satellite missions (e.g. NASA is co-operating for the preparation of weather analyses, forecasts, adviso- with Japan’s Aerospace Exploration Agency on the Tropical ries and warnings, for climate monitoring and environ- Rainfall Measuring Mission (TRMM); ESA and NASA cooper- mental activities. Three quarters of the data used in ate on the Solar and Heliospheric Observatory (SOHO), numerical weather prediction models depend on satellite while the French CNES is co-operating with India on the measurements (e.g. in France, satellites provide 93% of data Megha-Tropiques mission to study the water cycle). Para- used in Météo-France’s Arpège model). Three main types of doxically, although there have never been so many weather satellites provide data: two families of weather satellites and environmental satellites in orbit, funding issues in and selected environmental satellites. several OECD countries threaten the sustainability of the Weather satellites are operated by agencies in China, provision of essential long-term data series on climate. France, India, Japan, Korea, the Russian Federation, the United States and Eumetsat for Europe, with international co-ordination by the World Meteorological Organisation Methodological notes (WMO). Some 18 geostationary weather satellites are posi- Based on data from the World Meteorological Orga- tioned above the earth’s equator, forming a ring located at nisation’s database Observing Systems Capability Analy- around 36 000 km (Table 10.1). -
Meteosat Second Generation
BR-153 November 1999 Meteosat Second Generation The Satellite Development Contact: ESA Publications Division c/o ESTEC, PO Box 299, 2200 AG Noordwijk, The Netherlands Tel. (31) 71 565 3400 - Fax (31) 71 565 5433 BR-153 November 1999 Meteosat Second Generation The Satellite Development i ESA BR-153 ISBN 92-9092-634-1 Technical Coordinators: Bernard Weymiens & Rob Oremus MSG Project, ESA/ESTEC Published by: ESA Publications Division ESTEC, P.O. Box 299 2200 AG Noordwijk The Netherlands Editor: Bruce Battrick Layout: Isabel Kenny Cover: Carel Haakman Copyright: © European Space Agency 1999 Price: 50 DFl / 20 Euros i CONTENTS Foreword 1 1 Introduction 3 1.1 Programme Outline 3 1.2 History of the MSG Satellite Concept 4 1.3 Mission Objectives 6 2 Programmatics 11 2.1 Organisation 11 2.2 Overall Schedule 12 3 Satellite Development 13 3.1 Design & Development of the MSG Satellite 13 3.2 AIT Programme 16 3.3 Product Assurance 18 3.4 Image-Quality Ground Support Equipment 20 4 Payload 4.1 The Spinning Enhanced Visible and Infra-Red Imager (SEVIRI) 23 4.2 The Mission Communication Package (MCP) 33 4.3 The Geostationary Earth Radiation Budget Experiment (GERB) 38 4.4 The Search and Rescue (S&R) Mission 40 5 Satellite Subsystems 43 5.1 The Structure 43 5.2 The Unified Propulsion System 45 5.3 The Attitude and Orbit Control System 47 5.4 The Electrical Power System 50 5.5 Data Handling and Onboard Software 52 iii The authors wish to thank those companies and institutes that have provided illustrations and photographs for this Brochure, but for which a specific acknowledgement has not been possible.