The effects on the terrestrial atmosphere and ionosphere of energy and
momentum sources of magnetospheric origin are investigated theoretica
lly. Parameters measured by instruments on board the GGS spacecraft an
d by the GGS ground-based networks are used as inputs to the models th
at quantify the magnetosphere-ionosphere-thermosphere coupling. Images
of the aurora acquired at ultraviolet, visible and X-ray wavelengths
by instruments on board the POLAR spacecraft are particularly useful i
n this investigation by yielding good spatial coverage and high time r
esolution of the aurora.