Minor solar wind stream could spark auroras tonight

Minor solar wind stream could spark auroras tonight

 Earth is entering a minor solar wind stream that could spark auroras around the Arctic Circle. High-latitude sky watchers should be alert for Northern Lights tonight.

Solar wind
speed: 452.2 km/sec
density: 1.5 protons/cm3


The Radio Sun
10.7 cm flux: 140 sfu


Planetary K-index
Now: Kp= 2 quiet
24-hr max: Kp= 2 quiet


Interplanetary Mag. Field
Btotal5.0 nT
Bz2.9 nT south 


A very large solar filament channel that measures longer than 300,000 miles, is currently visible across the entire northeast quadrant. Click on the image below to view.


Joint USAF/NOAA Report of Solar and Geophysical Activity (11 Dec 2011)

Solar activity was at very low levels with only B-class activity observed. Two filament eruptions were observed during the period. A 40 degree long filament, centered near N25E25, was first observed erupting at about 11/0600Z. Shortly after, a 10 degree long filament, centered near N30W17, was first observed lifting off at about 11/0900Z. Stereo-A COR2 imagery observed a pair of CMEs off the NE limb at 11/0754Z and 11/1024Z as a result of the filament activity. At this time, neither of these CMEs are expected to be geoeffective. Solar activity is expected to be at low levels with a slight chance for M-class activity all three days of the period (12 - 14 December).

The geomagnetic field was at quiet to unsettled levels. Solar wind velocities generally varied between 450 to 500 km/s while the Bz component of the interplanetary magnetic field did not vary much beyond +/- 5 nT. The geomagnetic field is expected to be at mostly quiet levels all three days of the period (12 - 14 December).

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Tags: cme, solar wind

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