SV Cam comma a laboratory for X-ray eclipse experiments

We propose to observe complete orbital cycle of the short period active binaryCV Cam. Eclipses are an excellent mean as recently demonstrated by our SAXobservation of Algol to map coronal structures in eclipsing systems. CV Cam,with its short orbital period and large orbital inclination is an ideallaboratory for such study, and the high sensitivity of XMM will allow forhighresolution, phaseresolved spectroscopy to be performed. The proposedobservation will address issues such as the presence of active longitudes, ofpolar structures and of differential rotation, while at the same performing athrough Xray spectral study of the proposed target. truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]