Solar activity is expected to be at very low levels. 

No proton events are expected at geosynchronous orbit. 

The greater than 2 MeV electron flux at geosynchronous orbit is expected to be 
at normal levels throughout the period. 

The geomagnetic field is expected to be at quiet levels through 18 January. 
Field activity is expected to increase to quiet to unsettled levels, with 
isolated active periods possible at high latitudes during 19 January due to a 
recurrent coronal hole high speed stream (CH HSS). Activity is expected to 
decrease to quiet levels during 20 - 26 January. Activity is expected to 
increase to quiet to unsettled levels, with isolated active levels possible at 
high latitudes during 27 - 30 January due to another recurrent CH HSS. Activity 
is expected to decrease to quiet levels during 31 January - 09 February.

SWPC PRF 1741 13 January 2009 
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Tilaa WRTH 2008 nyt:
http://www.hard-core-dx.com/redirect2.php?id=wrth2008
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