Now showing items 1-10 of 39
Workshop material about THEMIS
Optimization of Models
(University of Alberta, 1998)
The parameters of model auroral current systems were described in the previous chapter. To model the currents at any given time, these parameters must be adjusted to provide an optimal match to the available observations. ...
May 25, 2007 Meteor
(Please contact Martin Connors for more information: email@example.com, 2007-05-31)
The file shows a view of the whole sky on Friday May 25 at 1:07:20 am with data from 1:07:24 superposed. This shows the meteor track in the southern sky, inside the box near the bottom along with the start point just ...
STEP Forward 2007-2007 Space Science Enhancement Proposal to CSA
The most effective way to exploit Canada’s ideal position for auroral zone science is to emplace instruments with sufficient density for meaningful studies. Magnetometers are useful instruments for this since their cost ...
Electrodynamic Parameters of the Auroral Oval from Combined Spacecraft and Ground Measurements
(European Space Agency, 2006)
Spacecraft traversing the auroral oval respond primarily to the field-aligned currents at its poleward and equatorward borders that are part of a solenoidal current system. If electric and magnetic field measurements are ...
Introduction on solar-terrestrial interaction.
CASCA 2006 Calgary AU Attendees
Photos showing AU attendees at CASCA 2006, held in Calgary in early June 2006.
Physical processes in near-Earth space with attention to ground and satellite magnetic fields.
Aspects of space physics data available and how to prepare it for treatment in analysis.
A Centenary Survey of Orbits of Co-Orbitals of Jupiter
Jupiter’s Trojan asteroids fulfill the prediction of Lagrange that orbits can be stable when a small body orbits in specific locations relative to its ‘parent’ planet and the Sun. The first such Trojan asteroid was discovered ...