by Dr. Tony Phillips.


Shown here in an extreme ultraviolet photo taken Dec. 11th, the UV-dark chasm overlies more than 500 billion square kilometers of solar terrain:

Coronal holes are places in the sun’s atmosphere where the magnetic field opens up and allows solar wind to escape. A broad stream of solar wind flowing from this particular coronal hole should reach Earth on Dec. 15-17.

The last time a solar wind stream blew past Earth, on Dec. 7th, the impact sparked Northern Lights in the United States as far south as Montana and Michigan. A repeat performance could be in the offing. High-latitude sky watchers should be alert for auroras early next week.


Solar Storm Forecast 12-10-13


Published on Dec 10, 2013

Even while busy with Comet ISON, the Sun managed to launch three partially Earth-directed solar storms this week, two of which have hit the Earth causing a geomagnetic storm as of this posting. The East limb is also buzzing with new activity and 5 new sunspots have emerged on the Earth-facing solar disk in the past few days alone. All of this means more activity is in store for us this week. Find out the details of when and how this activity will affect your mobile devices and your life this week.

Follow @TamithaSkov on Twitter for Daily Space Weather Forecasts

For a more in-depth look at the data and images highlighted in this video see these links below.

Comet ISON and aurora photography:
links coming momentarily…

Solar Imaging and Analysis:
Flare Analysis:…
Computer Aided CME Tracking CACTUS:…
GOES Xray:…
NOAA Sunspot Classifications:
GONG Magnetic Maps:
LMSAL Heliophysics Events HEK

Solar Wind:
ACE Solar Wind:…
Wang-Sheeley-Arge Solar Wind Prediction Model:

Magnetosphere, Ionosphere, Atmosphere:
GOES Magnetometer:…
Ionosphere D-Region Absorption (DRAP) model:
Auroral Oval Ovation Products:
POES Auroral Global Maps:
Global 3-hr Kp index:…
Wing Kp index prediction:…
USGS Ground Magnetometers:
USGS Disturbance Storm-Time (Dst):
HAARP Data Meters:

Multi-Purpose Space Environment Sites:

Definition of Geomagnetic Storm, Radiation Storm, and Radio Blackout Levels:

None of this would be possible without the hard work and dedication of those who have provided all of this data for public use.

Images c/o NASA/ESA/CSA (most notably the superb SDO, SOHO, ACE, STEREO, CCMC, JPL & DSN teams, amazing professionals, hobbyists, institutions, organizations, agencies and amateurs such as those at the USAF/HAARP, NICT, NOAA, USGS, Environment Canada, Natural Resources Canada, Intellicast, Catatania,,,,,,, and more. Thanks for making Space Weather part of our every day dialogue.



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