Аннотация:Paraboloid model of the Earth's magnetosphere has been developed at Moscow State University to represent correctly the electrodynamics processes in the near-Earth's space [1]. This model is intended to calculate the magnetic field generated from a variety of current systems located on the boundaries and within the boundaries of the Earth's magnetosphere under a wide range of environmental conditions, quiet and disturbed, affected by Solar-Terrestrial interactions simulated by Solar activity such as Solar Flares and related phenomena which induce terrestrial magnetic disturbances such as Magnetic Storms. The model depends on a small set of physical input parameters, characterizing the large-scale magnetospheric current systems intensity and location, such as geomagnetic dipole tilt angle, distance to the subsolar point of the magnetosphere etc. The input parameters depend on real-time, or near-real-time Empirical Data that include solar wind and IMF data as well as geomagnetic indices. The generalized model was implemented to represent the magnetospheres of magnetized planets Saturn [2], Jupiter [3], Mercury [4]. Specific features of the magnetospheres and the interactive models of the Earth's, Kronian and Mercury's magnetospheres has been realized at Space Monitoring Data Center of SINP MSU [5]. Real-time model of the Earth's magnetosphere is working at SINP MSU Space Weather Web-site [6]. Under FP7 IMPEX project data from different sources (satellite measurements, simulation data bases and online services) have been accumulated inside the digital framework. Paraboloid model of the magnetospheres (PMM) is part of this infrastructure. Web-services allowing the access to PMM calculations and data post-processing under SOAP protocol have been created. They will be implemented for easy data exchange within IMPEX infrastructure.