Solar activity on the far side

The far-side seismic signature of magnetic activity

The far-side of the Sun that we cannot directly see from Earth. High value regions indicate locations where there is an accumulation of magnetic field.

References

The far-side images are produced by NSO/GONG, see their detailed description

Spaceweather forecasts and nowcasts

Solar magnetic active regions
SDO AIA 171
SOHO solar corona
Predicted solar wind
Kp forecast
Dst forecast
AE AU AL forecast
dB/dt forecast
Local magnetic field

About Swedish space weather center (SRC)

Swedish Institute of Space Physics (Institutet för rymdfysik, IRF) has been active within space weather since the late 1990’s, and provided web sites with space weather information and predictions. Svenskt rymdvädercentrum (SRC) conducts solar and space weather research and provides forecasts, warnings and observations of space weather conditions. SRC hosts Regional Warning Center - Sweden (RWC) since 2000 within the International Space Environment Service (ISES).

Contact

For generic feedback, scientific and content enquires, please contact Peter Wintoft or Magnus Wik

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