| Solar X-rays in the last 24 hours: |
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| Geomagnetic activity: |
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![]() A 3 day plot of 5-minute solar X-ray flux values measured on the GOES 8 and 10 satellites. |
![]() ACE Real-Time Solar Wind 2-hour 6-hour 24-hour 3-day and 7-day ACE RTSW Plots. |
![]() CELIAS/MTOF Proton Monitor on the SoHO Spacecraft. |
![]() Other magnetograms (Europe) (North America) |
GOES magnetogram |
![]() This plot shows the current extent and position of the auroral oval in the northern hemisphere, extrapolated from measurements taken during the most recent polar pass of the NOAA POES satellite. The red arrow in the plot, that looks like a clock hand, points toward the noon meridian. |
![]() A real-time view of the auroral oval as inferred from the CARISMA magnetometer array. |
![]() This plot estimates the visibility of aurora from any northern hemisphere locations assuming optimal observing condition. It is updated every 5 minutes. The color of the plot represents the intensity of the aurora, with increasing trend green-brown-red. The locations at the outskirts of the oval are most likely to see auroral activity. The plot is accurate, but one should bear in mind that some locations might see more than others due to auroral substorming. |
![]() Current Geo-Magnetic Storm Level Based on ACE Real Time Solar Wind Data. Dst values are extrapolated using most recent solar wind and magnetic field data when data gaps are present. Low: Dst > -20 nT Medium: -20 nT > Dst > -50 nT High: -50 nT > Dst > -100 nT Extreme: Dst < -100 nT |
![]() Predicted Geomagnetic Activity Index using Wing Kp Model The current 1-hour and 4-hour Kp predictions are shown to the right of the white dashed line, which marks the current time. Courtesy of NOAA / Space Weather Prediction Center |
![]() The current Kp-index. A red bar indicates extremely high auroral activity and values over 6 make aurora sightings from middle to low latitudes possible. |
Hourly Dst data (University of Kyoto) Extreme values of Dst < -100 nT make aurora sighting from mid-latitudes possible. |