Viewing archive of Tuesday, 8 April 2003
Solar wind (Speed, Density), Interplanetary Magnetic Field (IMF) (Bt, Bz)
Solar wind
Interplanetary Magnetic Field (IMF)
Courtesy of NASA and the ACE Science Center (SWEPAM, MAG instruments teams) and/or NASA/NOAA DSCOVR (PlasMag instrument team)
All times in UTC
Current data suggests there is a slight possibility for aurora to appear at the following high latitude regions in the near future
Iqaluit, NUNuuk
Rovaniemi, Sodankylä, Utsjoki
Reykjavik
Tromsø
Kiruna
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X2.0 solar flare from sunspot region 4001
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Coronal hole faces Earth, Minor G1 geomagnetic storm watch
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Saturday, 15 March 2025
13:48 UTC - Hemispheric Power Index
The OVATION model predicts the Hemispheric Power Index to reach 52GW at 14:31 UTC
Space weather facts
| Last X-flare | 2025/02/23 | X2.0 |
| Last M-flare | 2025/03/14 | M1.1 |
| Last geomagnetic storm | 2025/03/14 | Kp6- (G2) |
| Spotless days | |
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| Monthly mean Sunspot Number | |
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| February 2025 | 154.6 +17.6 |
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| Last 30 days | 136.5 -20.3 |