A long-lasting Geomagnetic Storm that reached very close to the Strong G3 Level (Kp =6) took place Monday night and early Tuesday morning. Ham Radio operators were able to make numerous contacts via the Aurora on the 6 meter (50mhz) amateur radio band. This storm was
A Minor Geomagnetic Storm (Kp=5) is now in progress at high latitudes. This is due to a south tilting component of the Interplanetary Magnetic Field (IMF) combined with an elevated solar wind speed. An incoming CME shock swept past our planet at 03:25 UTC. A
A incoming CME shock swept past our planet at 03:25 UTC. A geomagnetic sudden impulse of 31 nT was detected by the Boulder, Colorado magnetometer. The ACE Spacecraft did show a solar wind increase to near 400 km/s. Minor geomagnetic activity will be possible at very
A volley of C-class solar flares sent waves of ionization rippling through the atmosphere high over Europe. Dave Gradwell of Birr, Ireland, detected the disturbances using a VLF radio monitoring system:Below is a video by STEREO Ahead COR2 and Lasco C3 showing
Solar activity has been low and Sunspot 1450 is about to rotate onto the western limb. With Sunspot 1452 struggling to remain visible, the Earth facing side of the Sun is at risk of being spotless for the first time in over 230 days. Old Sunspot 1440 rotated onto the
A magnetic filament connected to sunspot AR1450 erupted on April 2nd, hurling a faint CME in the direction of Earth. This CME has a northerly trajectory and is not expected to be geoeffective. However, a weak impact is expected sometime on April 4th as it can be seen
Solar activity is currently at low levels. All sunspots on the Earth facing side of the Sun remain stable. A small new sunspot looks to be forming to the west of 1445 in the southern hemisphere. Old and active Sunspot 1429 will begin to re-emerge off the eastern limb
A spectacular Filament Eruption (Prominence) ripped off the lower southeast quadrant of the Sun today and large Coronal Mass Ejection followed but is not heading for the earth. Video by: Solarwatcher.netFilaments are large regions that contain very dense, cool
The CME that erupted late on March 4 passed ACE around 04:00 UTC March 7 (11:00 p.m. EST March 6). So far we’ve observed G2 (Moderate) levels of storming in association with that event. Conditions are currently decreasing for that event, so subsequent G2 storming is
Interplanetary Magnetic Field (Bz) has been pointing south at times today (Monday) and combined with the solar wind at near 500 km/s, it has generated a minor G1 Geomagnetic Storm at high latitudes. Storm levels reached Kp index of 5. The geomagnetic field is expected
