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Telescope and scanning strategy

The Archeops telescope is an off-axis Gregorian telescope with a 1.5 meter primary mirror that looks at 41 degrees of elevation. During the flight, the gondola rotates at 2 rounds per minute around its vertical axis and therefore performs scans on the sky at constant elevation. While the Earth rotates, these scans end up forming a wide annulus on the sky with scans crossing each other at various time scales allowing an efficient monitoring of systematic signals. The gondola is shown in Figure [*] and the scanning strategy in Figure [*]. The gondola is hanged below a stratospheric balloon that floats at an altitude of around 40 km. The data is taken during 24 hours nighttime winter arctic flights.

Figure: Schematic view of the Archeops gondola. The telescope observes at 41 degrees of elevation and rotates at 2 rounds per minute.
\resizebox{\hsize}{!}{\includegraphics{arch_view_eng.ps}}

Figure: Scanning strategy on the sky (Molleweide projection): a circle is plotted every hour. After 24 hours, the covered region has the shape of an annulus.
\resizebox{\hsize}{!}{\includegraphics{coverage_arch.ps}}


next up previous
Next: Cryostat, bolometers and cold Up: Archeops instrument Previous: Archeops instrument
Jean-Christophe Hamilton ISN 2001-12-01