Global Planning
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Global Planning

This section describes the current global planning for operational geostationary satellites and Low-Earth Orbit satellites, as developed in consultation among WMO and satellite operators within the Coordination Group for Meteorological Satellites (CGMS)It includes a nominal configuration and a global contingency plan.

Space-based GOS
Schematic overview of the space-based GOS
(click to enlarge)

Observation requirements and related observing capabilities are kept under review as part of the Rolling Review of Requirements (RRR) process and a Gap Analysis of the space-based GOS is regularly performed. Gap analyses are maintained in the on-line database tool OSCAR (Observing System Capabilities Analysis and Review)

WMO has developed its "Vision for the GOS in 2025" that provides a long-term goal to foster the development of the GOS and meet the challsenges of future weather and climate observation. The vision (addressing both surface- and space-based observation) was finalized by the 14th session of the Commission for Basic Systems (CBS-XIV) and endorsed by the Executive Council (EC-LX).

Examples of Low Earth Orbit configurations are provided for illustration purpose.


Global planning for operational geostationary satellites

The nominal constellation of operational geostationary satellites includes 6 spacecraft to ensure full coverage from 50°S to 50°N with a zenith angle lower than 70°.

Nominal geostationary locations agreed among CGMS satellite operators are:

Region Nominal operator Nominal operational locations Footprint on Map
North, Central and South America (GOES-West) USA (NOAA) 135° W Show/hide
East Pacific (GOES-East) USA (NOAA) 75° W Show/hide
Europe & Africa EUMETSAT
Indian Ocean Russian Federation (Roshydromet) 76° E Show/hide
Asia China (CMA) 105° E Show/hide
West Pacific Japan (JMA) 140° E Show/hide

Note that different locations may be used, depending on operational constraints and spacecraft availability.

The following interactive map shows the nominal footprints of these satellites (Assuming a zenith angle of 75°) : Show / Hide all footprints

While space-based observation increasingly involves Low-Earth Orbit satellites (either from operational or from R&D environmental missions) that provide essential input to numerical modelling, the constellation of operational meteorological geostationary satellites remains the backbone of permanent and near-global monitoring of the weather situation. Infrared composite imagery as shown above is produced on an operational basis with data from GOES-West and GOES-East (NOAA, USA), Meteosat and Meteosat/IODC (EUMETSAT) and MTSAT (JMA, Japan). Additional satellites like the FY-2 series (CMA, China) contribute to strengthen the system and ensure its operational continuity.

Global planning for Low Earth Orbit sun-synchronous operational missions

2-satellite baseline for LEO satellites
Illustration 3: Current baseline

The current baseline for the core constellation is described in Chapter 4 of the WMO Manual on the GOS and in Section 5.4 of the CGMS Global Contingency Plan mentioned below.

It foresees four operational LEO sun-synchronous satellites optimally spaced in time, two in morning orbits (a.m), two in afternoon orbits (p.m.), and two other spacecrafts as in-orbit back-up.

A morning orbit (respectively an afternoon orbit) is a sun-synchronous orbit for which the day-time equatorial plan crossing occurs at a Local Solar Time before (respectively after) 12:00. The illustration represents morning and afternoon orbits over the Northern hemisphere.

New baseline in the Vision for the GOS in 2025

The new baseline for the core LEO constellation is to be deployed over three orbital planes around 13:30, 17:30 and 21:30 Equatorial Crossing Time (ECT) in Local Solar Time (LST). This should ensure regular sampling of the atmosphere avoiding too large a temporal gap around dawn and dusk, in order to satisfy as far as possible the observing cycle requirements from NWP and climate monitoring as concerns atmospheric temperature and humidity profiles. In addition, in-orbit redundancy should be available around these orbital planes, to the extent possible.

3-orbit new LEO baseline
Illustration 4: Proposed new baseline with in-orbit redundancy

Global Contingency Planning

The CGMS members have agreed a Global Contingency Plan among satellite operators and they keep this plan under regular review.

Continuity of the geostationary imaging service is essential for meteorological operations in support of severe weather warning, and Numerical Prediction in general. Such continuity is ensured through maintaining additional satellites in stand-by position for in-orbit back-up, and through bilateral contingency agreements among neighbouring geostationary satellite operators. Through such agreements, operators agree that, in case of major satellite failure encountered by an operator, and if another operator has a spare satellite available, the spare satellite could be relocated to replace the failing satellite on a temporary basis until a nominal configuration can be recovered through the launch of a new satellite.

Continuity of low-Earth orbit services is achieved through redundancy on the am and pm orbital missions.

Download the CGMS Global Contingency Plan.


New Vision for the GOS (Summary of the space-based component)

Download the description of the WMO "Vision for the GOS in 2025".

A short summary of the space-based component only is given below.

For the space-based GOS, the new vision calls upon enhancements and additions in comparison with the current baseline. It includes, as operational components:

  • High-resolution multispectral Vis/IR imagery on operational geostationary satellites
  • IR hyperspectral sensors on operational geostationary satellites
  • Lightning detection from operational geostationary satellites
  • High-resolution multispectral Vis/IR imagery on mid-am, pm and early morning orbit
  • MW sounding on mid-am, pm and early morning orbit
  • Hyperspectral IR sounding on mid-am, pm and early morning orbit
  • Operational radio occultation sounding constellation
  • Ocean altimetry missions providing accurate reference measurements and global coverage
  • Ocean surface wind missions with scatterometry and microwave imagery
  • Global precipitation measurement by active (radars) and passive (MW imagers) sensors
  • Earth radiation budget measurements including total solar irradiance
  • Atmospheric composition including UV sounding from geostationary and am/pm LEO
  • Specific imagery for ocean colour and vegetation monitoring
  • Dual-angle view imagery
  • High-resolution IR/VIS land surface imaging
  • Synthetic Aperture Radar observation
  • Space Weather monitoring from geostationary and LEO

In addition, the Vision calls upon Operational pathfinders and technology demonstrators e.g.:

  • Visible/Infrared Imagery in Highly Elliptical Orbit(HEO) for Plar Regions
  • Doppler wind lidar, Low-frequency microwave missions
  • Geostationary microwave
  • Geostationary high-resolution narrow-band imagers
  • Gravimetric sensors

Implementing the Vision also requires:

  • Enhanced data sharing, interoperability and integration
  • Data homogeneity and traceability
  • Enhanced cooperation and coordination on global long-term planning
  • Transition of relevant R&D missions to an operational status to ensure long-term sustained observation of Essential Climate Variables.


Examples of Low Earth Orbit configurations


Non sun-synchronous orbit types

Low-Earth Orbits may have different altitudes and different inclination (angle between the orbital plane and the equatorial plane) depending on the mission for which the satellite is designed.

For instance, tropical monitoring missions will have low inclination, cryosphere monitoringmust have a near-polar inclination.

Such orbits are not necessarily sun-synchronous.


Sun-synchronous orbits enable providing observations with stable solar illumination conditions. The orbital plane maintains a constant angle with the sun's direction throughout the year.

The scene viewed by the spacecraft at a given latitude is at a same local solar time at every orbital revolution. In particular, local solar time upon crossing the equator is constant.
The Equatorial Crossing Time (ECT) characterizes the orbit.
Sun-synchronous orbits have a near-polar retrograde inclination
(around 98 degrees).

Sun-synchronous orbits

For a more detailed description of orbit types, see:



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