Author/Authors :
Alha، نويسنده , , L. and Huovelin، نويسنده , , J. and Hackman، نويسنده , , T. and Andersson، نويسنده , , H. and Howe، نويسنده , , C.J. and Esko، نويسنده , , Eero and Vننnنnen، نويسنده , , M.، نويسنده ,
Abstract :
The operation, performance, and in-flight calibrations of the X-ray Solar Monitor (XSM) on-board ESAʹs SMART-1 mission to the Moon are presented. The basic method of deriving the response and effective area of the XSM is described. The evolution of the energy resolution as a function of time is studied, and sample data of high quality broadband solar flare spectra including highly ionized Fe-lines are also presented.
Keywords :
X-ray detectors , Solar X-rays , Effective area , Spectral response
