Space Weather

Space Weather Analysis Center

Space Weather Analysis Center SINP MSU

SINP MSU Space Weather Analysis Centre provides information about the current state of near-Earth's space. Information Services (SWX) on the website of the center provide access to current data describing the level of solar activity, geomagnetic and radiation state of the magnetosphere and the heliosphere in the real time. For data analysis, the models of the space environment, working in off-line as well as on-line mode have been implemented. Interactive services allow one to retrieve and analyze data in a given time moment. SWX is a flexible system for the analysis and forecasting of space weather in the near_Earth's space.

Current Near-Earth Space Environment condition (2025-12-22 18:33:06 UT)

Solar X-rays

Kp-index

Protons > 10 MeV

RB Electrons > 0.6 MeV

Magnetosphere today

The Earth's magnetosphere {% translate "is the result of constant and active interaction between the supersonic flow of a magnetized, fully ionized plasma flowing from the solar corona, and its own magnetic field of the Earth. During this interaction, the head shock wave, magnetopause, and magnetospheric current systems are created. Large-scale currents in the Earth's magnetosphere determine the structure of the magnetic field and, therefore, the size and the position of plasma formations in near-earth space, the motion of energetic charged particles. The Earth's magnetosphere and the solar wind are in constant interconnection and represent a single system. Being under the constant influence of the solar wind, the Earth's magnetosphere displays variations in the parameters of the interplanetary medium, connected, both with active, and with cyclic processes on the Sun. The most striking manifestation of such impact explosive processes in the magnetosphere: magnetospheric substorms and magnetic storms, leading to a significant energy release in the inner magnetosphere. Along with this, the effects of the rotation of the Sun, an eleven-year solar cycle activity, are also confidently recorded according to the state of the magnetosphere, according to variations in the magnetospheric magnetic field.

The structure of the magnetic field (figure on the right) gives specialists an idea of the processes, occurring in the Earth's magnetosphere. To obtain a similar structure, numerical models of the magnetospheric magnetic field, Based on the theoretical assumptions, according to measurements, it is possible to construct a magnetic field cathrine in the entire magnetosphere. Together with measurements on space vehicles (spacecraft), this allows for full scientific research  and build forecasts of space weather." %}.

Watch magnetosphere in 3D