During the "geodesy campaign" in May and June 1999 the wide-angle system of
the Mars Global Surveyor Mars Orbiter Camera imaged the visible surface of
Mars from latitudes 70 degreesS to 90 degreesN. Over 90% of this portion o
f the planet was covered at two viewing angles to obtain side-looking stere
o at a resolution of similar to 250 m/pixel and convergence angles of 21 de
grees -27 degrees. Continuous radiometric spacecraft tracking during this p
eriod provided precise orbit determination of spacecraft location. This dat
a set will become the basis of a new image mosaic of Mars, with the potenti
al to exceed the geodetic precision and image quality of those presently av
ailable.