International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences, Volume XXXIX-B4, 2012 
XXII ISPRS Congress, 25 August — 01 September 2012, Melbourne, Australia 
Examples of the interfaces, implemented in the listed systems, 
are shown in Fig. 7. Experience of using GEOSMIS in 
development of these systems has shown that technology is 
indeed fairly universal, easy scalable and extendable for 
different tasks. This makes it possible to start using the 
technology also in other projects conducted in the Space 
Research Institute and Kotel'nikov Institute of 
Radioengineering and Electronics. 
5. CONCLUSIONS 
1. User requirements that determine service stack of modern 
EO CUS should include 
e possibilities for permanent data upgrades; 
e support of long-term data storage; 
e functionality of distributed archives and catalogues; 
e functionality implementing automatic stream- 
oriented data collecting, processing, distributing, and 
displaying technologies; 
e tools for dynamic formation of product variety by 
user request; 
e ability to get and analyse wide range of graphic 
object types; 
e ability to get and to incorporate space data from 
different external space data systems. 
2. Proposed and motivated EO CUS architecture provides 
basic service stack functionality. It is worthwhile to 
construct and develop EO CUS as two-layer model: 
1) presentation layer and application layer. Presentation 
layer is based on map and presentation (display) modules 
while application one — on data integration module and 
application APL 
3. EO CUS is implemented as IKI GEOSMIS technology. 
Presentation layer is implemented in GEOSMIS map data 
module (smisMap) and metadata module (smisMeta). 
Application layer is implemented in GEOSMIS as data 
integration module (smiswms) and applied API. 
4. GEOSMIS technology formed basis of various monitoring 
systems based on GEOSMIS: a) FFA ISDM, b) satellite 
service VEGA, c) OSM Rosrybolovstvo, d) Joint catalog 
at SC EOM, e) Joint system of data access of SRC 
“Planeta”. 
ACKNOWLEDGEMENTS 
The work was supported by Russian Foundation for Basic 
Research - grant No. 11-07-12028-ofi-m-2011. 
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