PDS_VERSION_ID = PDS3 ^PDF_DOCUMENT = "PFS_SWC_CALIB.PDF" PRODUCT_ID = PFS_SWC_CALIB RELEASE_ID = 0001 REVISION_ID = 0000 RECORD_TYPE = FIXED_LENGTH DATA_SET_ID = "MEX-M-PFS-2-EDR-EXT3-V1.0" PRODUCT_CREATION_TIME = 2010-12-07T12:01:24.717 OBJECT = PDF_DOCUMENT DOCUMENT_NAME = "CALIBRATION OF THE PLANETARY FOURIER SPECTROMETER SHORT WAVELENGTH CHANNEL" PUBLICATION_DATE = 2010-12-07 DOCUMENT_TOPIC_TYPE = "CALIBRATION REPORT" INTERCHANGE_FORMAT = BINARY DOCUMENT_FORMAT = "ADOBE PDF" DESCRIPTION = "The Planetary Fourier Spectrometer (PFS) experiment on board the Mars Express mission has two channels covering the 1.2 5.5 m (SWC) and the 5.5 45 m (LWC). The Short Wavelength Channel (SWC) measures part of the thermal emission spectrum and the solar reflected spectrum of Mars between 1700 cm-1 and 8200 cm-1 with a spectral resolution of 1.3 cm-1, in absence of apodization. We present here the calibration of this channel and its performance. The instrument calibration has been performed on ground, before launch, in space during Near Earth Verification (NEV) measurements, and at Mars. Special attention has been given to the problem of micro-vibrations on board the spacecraft. In order to obtain correct results, the source - instrument - detector interaction for the thermal part is studied very accurately. The instrument shows a non linear behaviour with source intensity. The SNR increases with amplification, so high gain factors are usually used. The detector is, in space, cooled by a passive radiator, and works around 210 215 K. The calibration source (an internal lamp) shows variations during a pericentre pass and therefore impose a complex procedure for the SW channel calibration. Mechanical micro vibrations strongly affect part of the spectrum. We discuss the validity of the present calibration, and indicate possible future developments. Samples of the calibrated data are given to show the performance of the experiment and its scientific potentialities." END_OBJECT = PDF_DOCUMENT END