Data from Antarctic AGOs:
1995:

1996:

1997:

1998:

South Pole 1999

South Pole 2000

South Pole 2001

South Pole 2002

South Pole 2003

South Pole 2004

South Pole 2005

South Pole 2006

AGO and South Pole 2007

AGO and South Pole 2008

AGO and South Pole 2009

2007 THEMIS-AGO conjunctions

Geographic orientation of AGO stations
Raw All-Sky images from AGO P3 with 427.8nm imaged to the right and 630.0nm to the left. A pixels along the magnetic meridian have been extracted to create one row of the Keogram seen below.
The extracted pixels from raw images have been plotted over a full day of imaging from AGO P1 and South Pole station, creating latitude vs. time plots. Geomagnetic noon occurs around 1530 UT, consistent with the poleward contraction of the cusp.
The above keogram data are sorted according to the month and each plot shows all available stations for that day. For scientific use, especially for a zoom into a shorter time period, trasformation to geographic or geomagnetic coordinates and absolute values please contact the all-sky camera PI.

Stephen B. Mende
Space Sciences Laboratory
University of California
Berkeley, CA 94720-7450
Phone: 1.510.642.0876
Fax: 1.510.643.8302
E-mail at nospam_mende@ssl.berkeley.edu (remove nospam_ for contact)

or

Harald U. Frey
Space Science Laboratory
University of California
Berkeley, CA 94720-7450
Phone: 1.510.643.3323
Fax: 1.510.643.8302
E-mail at nospam_hfrey@ssl.berkeley.edu (remove nospam_ for contact)