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The Sky Polarization Observatory (SPOrt) Program
Ettore Carretti et al.
Istituto TeSRE/CNR, Bologna, ITALY
The main goal of the Sky Polarization Observatory (SPOrt) Pro-
gram is the measurement of the sky linear polarized emission in
the 22-90 GHz frequency range. SPOrt payload will be accom-
modated on the International Space Station in 2003-2004 for a
period of 18 months. The instrument conguration is presented
together with most relevant ground activities in support to its re-
alization. In particular, the development of hardware solutions for
high sensitive polarimetric measurements, such as those requested
by Galactic polarized emission and Cosmic Microwave Background
observations, has been addressed by the SPOrt team to match the
experiment requirements.
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