BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//Lancaster University Faculty of Science and Technology//NONSGML v1.0//EN
BEGIN:VTIMEZONE
TZID:/Europe/London
X-LIC-LOCATION:Europe/London
BEGIN:DAYLIGHT
TZOFFSETFROM:+0000
TZOFFSETTO:+0100
TZNAME:BST
DTSTART:19700329T010000
RRULE:FREQ=YEARLY;INTERVAL=1;BYDAY=-1SU;BYMONTH=3
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+0100
TZOFFSETTO:+0000
TZNAME:GMT
DTSTART:19701025T020000
RRULE:FREQ=YEARLY;INTERVAL=1;BYDAY=-1SU;BYMONTH=10
END:STANDARD
END:VTIMEZONE
BEGIN:VEVENT
UID:28
SUMMARY:Power laws in the Magnetosphere - Why are they so interesting? A data analyst's perspective
DESCRIPTION:By Dr. Gary Abel, British Antarctic Survey\nThere is a growing body of work that shows scale free behaviour in a wide range of phenomena in the Magnetosphere-Ionosphere system. These observations include the AE indices, magnetic fields, electric fields, auroral brightenings, convection flows and magnetic structures associated with reconnection. They have been analysed using a variety of techniques including spectral analysis, threshold crossings and structure function analysis. This seminar presents some analysis of convection velocities measured by the SuperDARN radar which show scale free complex behaviour. These results will be discussed in the wider context along with some of the implications of scale free behaviour in the Magnetosphere. These implications affect both the way we view the system and the framework within which we should view observations.
DTSTART:20060706T110000
DTEND:20060706T120000
LOCATION:C60 InfoLab21
END:VEVENT
END:VCALENDAR