Aurora Watch 2012 Forecasts, analysis and sightings for the year.
#26
Posted 25 January 2012 - 00:01
Another good side effect of these storms is that they inspire you to go hunting for juicy data. For auroral oval plots I usually go to the POES satellite passes or the Ovation plots based on the DMSP pass data for the last 45mins. Well I've just found Ovation Prime, an auto-updating page of the latest DMSP data (top two plots are N Hem, your location is whatever time it is and latitude, the forecast is a blend of current DMSP and ACE data for the lead time of ~1hr ahead at the location of ACE). Now that's a useful tool for aurora hunting, presuming you're already in a tent in Scotland with a smartphone...
#27
Posted 25 January 2012 - 00:12
#28
Posted 25 January 2012 - 00:22
#29
Posted 31 January 2012 - 00:54
#30
Posted 01 February 2012 - 18:10
http://www.whitehave...ferrerPath=news
#31
Posted 07 February 2012 - 13:04

#32
Posted 07 February 2012 - 14:16
The slightly coarser but shorter time-frame Wang-Sheeley model (attached) suggests the southward (-ve) component should be with us for the next couple of days, so might be worth watching for a glow though sharp features are less likely without a disturbance to the magnetosphere.
#33
Posted 08 February 2012 - 02:47
Quote
I must say, the POES oval is looking very plump, and Ovation Prime (attached) shows quite a lot of activity at the moment. Shame about the cloud... again.
Quote
Serial Number: 1860
Issue Time: 2012 Feb 07 2033 UTC
WARNING: Geomagnetic K-index of 4 expected
Valid From: 2012 Feb 07 2040 UTC
Valid To: 2012 Feb 08 0600 UTC
Warning Condition: Onset
Potential Impacts: Area of impact primarily poleward of 65 degrees Geomagnetic Latitude. Weak power grid fluctuations can occur.
Aurora may be visible at high latitudes such as Canada and Alaska.
#34
Posted 08 February 2012 - 15:11
Also found a new indicator, 3-day detection of plasma clouds in space via the MuSTAnG muon telescope. In principal, this telescope sees the interference in Cosmic Ray detection that solar wind plasma clouds create - it sees further out than the position of ACE on 180o scans. The orientation of the detected interference is really no matter, mainly just the intensity. In this example, ACE saw a gentle negative wind slowly increase before falling away after midnight last night; but the Mustang Project saw a decline in the plasma cloud from 1030z onwards - before it was detected at the ACE point. Will have to monitor this in elevated or CME environments, but it seems to back up it's claim that it could even provide better data for Aurora Tourism (or Aurorism?).
One thing is clear, this addition is going to make Aurora Watch sound more like a scene from Top Gun. Shame they retired SuperDARN and PIXIE.
#35
Posted 12 February 2012 - 13:31
Quote
CME Arrival Time: 2012-02-13 21:25:03.0 GMT
Arival Time Confidence Level: ± 6 hours
Disturbance Duration: 12 hours
Disturbance Duration Confidence Level: ± 8 hours
Magnetopause Standoff Distance: 6.4 Re
#36
Posted 16 February 2012 - 00:19
#37
Posted 25 February 2012 - 02:03
Couldn't find a SOHO LASCO C3 gif small enough so had to make a tiny one, shown is a CME over the NE in full punch whereupon the geoeffective CME bursts up from the same area, spans about 12hrs.
Also attached are images from STEREO-Behind (to the left if looking at the sun) of both CMEs from the anim above, first the northern one then as the filament eruption tracked soutward releasing the geoeffective CME.
#38
Posted 25 February 2012 - 17:29
Quote
Solar flaring conditions are quiet and expected to remain quiet for the next 24 hours. Geomagnetic conditions have been quiet during the past 24 hours and are expected to remain quiet for the next 24 hours.
The CME that erupted yesterday 24/2 around 4UT is expected to become geoeffective in the course of Monday 27/2 between 6 and 16 UT. The magnetic field is expexted to be oriented northward, we therefore expect only active geomagnetic conditions (K=4). Another CME was observed late on 24/2 around 20 UT. It is also related to a filament eruption, this time in the south-east. This CME is not expected to have big geomagnetic consequences since it is directed mostly southward and since it is very slow (350 km/s). A glancing blow is however possible, which may lead to unsetteled conditions late on 29/2.
Found some decent imagery of the filament (upper left of disc) just before eruption (SDO retrieval was offline last night as the AIA processing offices had a power cut):
Also a movie of the event just prior to eruption, with what looks like a little plasma tornado (but isn't) right on the NE limb:
http://sdowww.lmsal....0224_212752.mov
...and a youtube movie someone generated with the Helioviewer:
#39
Posted 25 February 2012 - 18:40
#40
Posted 25 February 2012 - 18:43
#41
Posted 25 February 2012 - 20:49
Tony Sales, on 25 February 2012 - 18:43, said:
Worth keeping an eye on the 22z updates to the SWPC forecast, as they run the ENLIL-WSA-GONG model several times with more recent data to analyse plane-of-sky speeds, etc. Only the relevant ones are published online. Currently the view is unsettled to active with chances for isolated storms (geomagnetic), but it's still difficult to identify the aurora type until the CME reaches ACE and the rest of the geosatellite enviroment so we can get some real-time analysis. Even then the connection between display type and CME isn't fully understood, as detection and analysis of CMEs is still limited and hence so is forecasting.
Worth being optimistic though, or at least not missing anything.
#42
Posted 25 February 2012 - 21:44
Bazmundo, on 25 February 2012 - 20:49, said:
Worth being optimistic though, or at least not missing anything.
Cheers, I'll be watching
#43
Posted 26 February 2012 - 05:25
Five Solar Eruptions in 2 Days – CME On the Way http://www.nasa.gov/...022512-cme.html
#44
Posted 26 February 2012 - 12:10
Dave Hancox, on 26 February 2012 - 05:25, said:
He's not a reliable source IMO Dave, not worth checking with.
#45
Posted 26 February 2012 - 15:15












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