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GCOS Implementation Plan - WMO

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<strong>Implementation</strong> <strong>Plan</strong> for the Global Observing System for Climate in Support of the UNFCCC<br />

(2010 Update)<br />

ECV – Earth Radiation Budget<br />

The Earth Radiation Budget (ERB) measures the overall balance between the incoming energy from<br />

the sun and the outgoing thermal (longwave) and reflected (shortwave) energy from the Earth. It can<br />

only be measured from space, and continuity of observations is an essential issue. The radiation<br />

balance at the top of the atmosphere is the basic radiative forcing of the climate system. Measuring its<br />

variability in space and time over the globe provides insight into the overall response of the system to<br />

this forcing. The satellite measurements include solar irradiance observations as well as the<br />

broadband directional measurements of reflected solar and outgoing longwave radiation. At least one<br />

dedicated satellite ERB mission should be operating at any one time. Satellite observations should be<br />

continued without interruption, and operational plans should provide for overlap so that accuracy and<br />

resolution issues are resolved to meet climate requirements. This should be a continuing priority for<br />

CEOS and CGMS in their planning process. The requirement for this overlap is demonstrated in<br />

Figure 6 below.<br />

Action A25 [IP-04 A24]<br />

Action: Ensure continuation of Earth Radiation Budget observations, with at least one dedicated<br />

satellite mission operating at any one time.<br />

Who: Space agencies.<br />

Time-Frame: Ongoing.<br />

Performance Indicator: Long-term data availability at archives.<br />

Annual Cost Implications: 30-100M US$ (Mainly by Annex-I Parties).<br />

Figure 6: Observations of total solar irradiance (TSI) from a series of different instruments on satellites<br />

as indicated, along with monthly sunspot number. The vertical bar in the upper right corner shows a<br />

relative variation of 0.1% in TSI. Absolute values are uncertain and differ in the past by as much as 9<br />

Wm -2 , and more recently systematically by around 4 Wm -2 so that continuous time series are only made<br />

possible by overlapping measurements from different satellites. (Source:<br />

http://spot.colorado.edu/~koppg/TSI accessed 24 September 2009).<br />

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