General information about SPICE I-kernels ========================================= In the SPICE system, I-kernels contains instrument parameters such as field-of-view size, shape, and orientation, timing information, detector and filter attributes, etc. The data contained in I-kernel files can be accessed and manipulated by subroutines which are part of the SPICE library, the major component of the SPICE Toolkit. The SPICE subroutines can be integrated into user application programs. For information on the SPICE Toolkit and/or how to obtain it, please consult SPICE_INST.CAT and SOFT.CAT. Refer to the KERNEL.REQ document provided with the Toolkit to get more information on how to access I-kernel data. Mars Express IK Files ===================== This file describes the contents of the DATA/IK directory of the Mars Express SPICE data set. All these IK files are produced manually with the information supplied by Mars Express teams describing the science instruments. All IK files (*.TI) contained in this directory are UNIX text files with lines terminated by only. Mars Express I-Kernels Contained in this Data Set ================================================== The following I-kernels are provided in this data set (vv refers to the version of the kernel): MEX_ASPERA_Vvv.TI SPICE Kernel (IK) that contains ASPERA geometry parameters. MEX_HRSC_Vvv.TI SPICE Kernel (IK) that contains the High Resolution Stereo Camera (HRSC) and Super Resolution Channel (SRC) camera optics, detector, and FOV parameters. MEX_MARSIS_Vvv.TI SPICE Kernel (IK) that contains MARSIS geometry, optics, detector and FOV parameters. MEX_MELACOM_Vvv.TI SPICE Kernel (IK) that contains MELACOM instrument FOV parameters. MEX_OMEGA_Vvv.TI SPICE Kernel (IK) that contains the OMEGA Visible and Near InfraRed (VNIR) and Short Wavelength InfraRed (SWIR) Sort wavelength (SWIR-S) and Long wavelength (SWIR-L) channel optics, detector, and field-of-view parameters. MEX_PFS_Vvv.TI SPICE Kernel (IK) that contains PFS geometry, optics, detector, and FOV parameters. MEX_SPICAM_Vvv.TI SPICE Kernel (IK) that contains SPICAM geometry parameters for the instrument UV and IR channels. MEX_STR_Vvv.TI SPICE Kernel (IK) that contains the Star Trackers geometry, optics, detector and FOV parameters. MEX_VMC_Vvv.TI SPICE Kernel (IK) that contains VMC geometry, optics, detector and FOV parameters. In the case that several versions of the same instrument kernel are provided, the most recent one supersedes the other versions. Kernel File Details =================== The most detailed description of the data in an IK file is provided in metadata included inside the description area of the file. This information can be viewed using any text editor program. At least a basic knowledge of the SPICE system is needed in order to use these kernels. The SPICE Toolkit provides versions in Fortran (SPICELIB), C (CSPICE), IDL (Icy), Matlab (Mice), and Java (JNISpice) and the user can choose any one that suits him/her. The SPICE routine FURNSH can be used to load a kernel file into a SPICE-based application to make kernel data usable with SPICE APIs. If two (or more) text kernels assign value(s) using the '=' operator to identical keywords, the data value(s) associated with the last loaded occurrence of the keyword are used -all earlier values have been replaced with the last loaded value(s).