Presentation is loading. Please wait.

Presentation is loading. Please wait.

28-29 October 2004ESF Workshop, Cagliari 1 Future Programmes on Earth Observation World Radiocommunication Conference 2007 Agenda Item 1.20 on unwanted.

Similar presentations


Presentation on theme: "28-29 October 2004ESF Workshop, Cagliari 1 Future Programmes on Earth Observation World Radiocommunication Conference 2007 Agenda Item 1.20 on unwanted."— Presentation transcript:

1 28-29 October 2004ESF Workshop, Cagliari 1 Future Programmes on Earth Observation World Radiocommunication Conference 2007 Agenda Item 1.20 on unwanted emissions - protection of the EESS (passive) - Björn Rommen

2 28-29 October 2004ESF Workshop, Cagliari 2 Future Programmes on Earth Observation * Introduction * * The use of the EESS (passive) * * Scope of agenda item 1.20 * * Regulatory measures * * Summary * Content

3 28-29 October 2004ESF Workshop, Cagliari 3 Future Programmes on Earth Observation Within WRC-07 Agenda Item 1.20 covered by Resolution 738, a total of five EESS (passive) bands (5.340) need to be addressed, i.e. } 1400 – 1427 MHz 23.6 – 24.0 GHz 31.3 – 31.5 GHz 50.2 – 50.4 GHz 52.6 – 54.25 GHz Operational radiometers such as AMSU-A, SSM/I, CMIS  Pre-operational: SMOS, HYDROS, AQUARIUS Introduction “to consider the results of studies, and proposals for regulatory measures, if appropriate, regarding the protection of the Earth exploration-satellite service (passive) from unwanted emissions of active services in accordance with Resolution 738 (WRC 03)”

4 28-29 October 2004ESF Workshop, Cagliari 4 Future Programmes on Earth Observation Use of EESS (passive) important tool widely used for meteorological, climatological, and environmental monitoring and survey (operational and scientific applications) frequency and the strength of natural emissions characterize the type and the status of a number of important geophysical atmospheric and surface parameters (land, sea, and ice caps), which describe the status of the Earth/atmosphere/oceans system, and its mechanisms:  Earth surface parameters such as soil moisture, sea surface temperature, ocean wind stress, ice extension and age, snow cover, rainfall over land, etc;  Three-dimensional atmospheric parameters such as temperature profiles, humidity profiles, total water vapour content and concentration profiles of radiatively and chemically important trace gases (for instance ozone and chlorine monoxide) all-weather capability  60% of the Earth is overcast with clouds

5 28-29 October 2004ESF Workshop, Cagliari 5 Future Programmes on Earth Observation 1400 – 1427 MHz ESA’s SMOS mission (launch 2007) Soil Moisture and Ocean Salinity  new measuring technique: SMOS will carry the first-ever polar-orbiting satellite-borne 2-D interferometric radiometer  Pre-operational: feasibility of measuring soil moisture (key variable in the hydrologic cycle) and ocean salinity (thermohaline circulation, variations in salinity influence the near surface dynamics of tropical oceans)  Protection of this passive band is essential: no capability to measure soil moisture and sea surface salinity directly on a global basis  Airborne campaigns in Europe and US have already identified occasional strong levels of unwanted emissions in this band

6 28-29 October 2004ESF Workshop, Cagliari 6 Future Programmes on Earth Observation 23.6 – 24.0 GHz covers the flank of the water vapour spectral line (located at 22.235 GHz) measurements made at 24 GHz directly lead to the total column water vapour content in the atmosphere potential loss of these data that are assimilated in Numerical Weather Prediction (NWP) models will severely affect the quality of weather forecasting also used for correcting temperature measurements (made between 50-60 GHz) for attenuation due to water vapour:  Without correct measurements at 24 GHz, temperature measurements at 50- 60 GHz cannot be corrected for attenuation due to water vapour content in the atmosphere and thus have severely increased errors that feed back in the NWP models and potentially result in wrong interpretation and in degraded weather forecasts

7 28-29 October 2004ESF Workshop, Cagliari 7 Future Programmes on Earth Observation 31.3 – 31.5 GHz above 26 GHz the opacity of the atmosphere due to water vapour declines to a minimum close to 30 GHz, before slowly rising again sensitivity to cloud liquid water continues to rise such that at 30 GHz sensitivity to cloud is greater than sensitivity to water vapour this channel is therefore used as a window channel to correct at other frequencies for cloud liquid water as well as surface contributions also used for carrying out polarimetric sea surface observations to derive wind speed and direction:  these wind observations are extremely vulnerable to contamination due to their very low signal intensity

8 28-29 October 2004ESF Workshop, Cagliari 8 Future Programmes on Earth Observation 50.2 – 50.4 & 52.6 – 54.25 GHz used for temperature profile observation using the O 2 absorption spectrum in the vicinity of 60 GHz:  volume-mixing ratio of oxygen in the atmosphere up to approximately 90 km stays constant while the atmosphere pressure becomes larger towards the Earth surface according to a known exponential law  by making use of these two effects, the atmospheric temperature can be calculated proven very large positive impact on NWP equating to 1-2 days in forecast period channels further away from the oxygen absorption spectrum (e.g. 52.6 – 54.25 GHz) are sensitive to lower altitudes than those channels closer to 60 GHz

9 28-29 October 2004ESF Workshop, Cagliari 9 Future Programmes on Earth Observation Weighting function for MSU at nadir  Weighting function has a peak at specific altitude  Each channel had different sensitivity to altitudes  by measuring at several channels within the flank of the O 2 absorption spectrum and correcting for several factors (for which information is obtainable in the 31 GHz and 24 GHz frequency bands), an accurate temperature profile of the atmosphere results

10 28-29 October 2004ESF Workshop, Cagliari 10 Future Programmes on Earth Observation Compatibility analyses/ Resolution 738 (1) EESS (passive) bandActive service bandActive service 1 400-1 427 MHz1 350-1 400 MHzFixed service (FS) Mobile service (MS) Radiolocation 1 400-1 427 MHz1 427-1 429 MHzFS, MS and space operation service (Earth-to-space) 1 400-1 427 MHz1 429-1 452 MHzFS and MS 23.6-24 GHz22.55-23.55 GHzInter-satellite service 31.3-31.5 GHz30-31 GHzFSS (Earth-to-space) 50.2-50.4 GHz50.4-51.4 GHzFSS (Earth-to-space) 50.2-50.4 GHz47.2-50.2 GHz (Region 2+3) 49.44-50.2 GHz (Region 1) FSS

11 28-29 October 2004ESF Workshop, Cagliari 11 Future Programmes on Earth Observation f)that according to Recommendation ITU ‑ R SM.1633, the EESS (passive) in the band 31.3-31.5 GHz can be protected if the unwanted emissions of fixed-service systems (except high-altitude platform stations (HAPS)) operating in the band 31.0- 31.3 GHz do not exceed –38 dBW in a 100 MHz reference bandwidth in the band 31.3- 31.5 GHz; g)that according to Recommendation ITU ‑ R SM.1633, the EESS (passive) in the band 52.6-54.25 GHz can be protected if the unwanted emissions of fixed-service systems operating in the band 51.4-52.6 GHz do not exceed –33 dBW in a 100 MHz reference bandwidth in the band 52.6-54.25 GHz; 2to invite ITU ‑ R to further study the impact of implementing the values provided in considering f) and g) for unwanted emissions of fixed-service systems operating in Regions 2 and 3, taking into account that the impact on fixed-service systems in Region 1 has already been investigated; considering f + g: resolves 2: Compatibility analyses/ Resolution 738 (2)

12 28-29 October 2004ESF Workshop, Cagliari 12 Future Programmes on Earth Observation Regulatory measures to be based on numerical limits on unwanted emissions:  limits need to be technology-neutral on the long-term benificial for both active and passive systems:  better use of the spectrum to be applied to systems deployed after a certain date in the future so as to enable a smooth transition of systems to the changed regulatory environment (e.g. beyond 2010) worldwide applicability so as to avoid different regional regulations that could lead to:  unfair competition between different operators or manufacturers  interference to EESS (passive) in some parts of the world

13 28-29 October 2004ESF Workshop, Cagliari 13 Future Programmes on Earth Observation Summary 4 out of 5 bands are used for operational meteorology and are channels on a single radiometer instrument:  signal strength on a given frequency may depend on several variables, making the use of several frequencies at the same time necessary to match the multiple unknowns  interference in one of these bands will lead to misinterpretation or deletion of data unique global coverage needed for climatology and NWP regulations needed to ensure these products in the future  worldwide applicability


Download ppt "28-29 October 2004ESF Workshop, Cagliari 1 Future Programmes on Earth Observation World Radiocommunication Conference 2007 Agenda Item 1.20 on unwanted."

Similar presentations


Ads by Google