KPL/IK LADEE UVS Instrument Kernel =============================================================================== This Instrument Kernel (IK) file contains the Field-Of-View (FOV) definitions for the Ultraviolet and Visible light Spectrometer (UVS) instrument. Version and Date ------------------------------------------------------------------------------- Version 0.0 -- October 16, 2013 -- Boris Semenov, NAIF References ------------------------------------------------------------------------------- 1. Kernel Pool Required Reading 2. GETFOV, getfoc_c, cspice_getfov headers 3. LADEE FK file, latest version 4. STK Sensor files provided by Mark Shirley, 09/25/13. Contact Information ------------------------------------------------------------------------------- Boris V. Semenov, NAIF/JPL, (818)-354-8136, Boris.Semenov@jpl.nasa.gov Implementation Notes ------------------------------------------------------------------------------- This file is used by the SPICE system as follows: programs that make use of this kernel must ``load'' the kernel, normally during program initialization. The SPICE routine FURNSH loads a kernel file into the pool as shown below. CALL FURNSH ( 'frame_kernel_name; ) -- FORTRAN furnsh_c ( "frame_kernel_name" ); -- C cspice_furnsh, frame_kernel_name -- IDL cspice_furnsh( 'frame_kernel_name' ) -- MATLAB Once the file has been loaded, the SPICE routine GETFOV (getfov_c in C, cspice_getfov in IDL and MATLAB) can be used to retrieve FOV parameters for a given instrument or structure. This file was created and may be updated with a text editor or word processor. Naming Conventions ---------------------------------------------------------- All names referencing values in this IK file start with the characters `INS' followed by the NAIF ID number for one of the UVS detectors: LADEE_UVSTEL -12400 LADEE_UVSSOL -12500 These IDs are defined in the latest LADEE FK ([3]). The remainder of the keyword name is an underscore character followed by the unique name of the data item. For example, the UVS Solar boresight direction in the UVS Solar frame is specified by: INS-12500_BORESIGHT The upper bound on the length of the name of any data item is 32 characters. Instrument Description --------------------------------------------------------- The Ultraviolet and Visible light Spectrometer (UVS) science instrument consists of a spectrometer, a limb viewing telescope, and a solar viewing optic. The instrument is operated in two modes: 1) limb viewing, using the limb viewing telescope and 2) solar occultation viewing, using the solar viewing optic. In limb viewing mode, the UVS limb telescope is pointed above the lunar surface in the direction of spacecraft (S/C) flight. In occultation mode, the UVS uses its solar viewing optic to monitor the sun as it sets/rises across the lunar limb. Mounting Alignment -------------------------------------------------------- Refer to the latest version of the LADEE Frames Definition Kernel (FK) [3] for the LADEE UVS reference frame definitions and mounting alignment information. Instrument FOVs ---------------------------------------------------------- This section defines UVS FOVs based on [4]: NAME ID HALFSIZE SHAPE BSIGHT FRAME ---------------- ------- --------- ------- ------ ---------- LADEE_UVSTEL -12400 0.25 deg cone Z LADEE_UVSTEL LADEE_UVSSOL -12500 0.25 deg cone Z LADEE_UVSSOL The FOVs are defined in this data block. \begindata INS-12400_FOV_CLASS_SPEC = 'ANGLES' INS-12400_FOV_SHAPE = 'CIRCLE' INS-12400_FOV_FRAME = 'LADEE_UVSTEL' INS-12400_BORESIGHT = ( 0.0, 0.0, 1.0 ) INS-12400_FOV_REF_VECTOR = ( 1.0, 0.0, 0.0 ) INS-12400_FOV_REF_ANGLE = ( 0.25 ) INS-12400_FOV_ANGLE_UNITS = ( 'DEGREES' ) INS-12500_FOV_CLASS_SPEC = 'ANGLES' INS-12500_FOV_SHAPE = 'CIRCLE' INS-12500_FOV_FRAME = 'LADEE_UVSSOL' INS-12500_BORESIGHT = ( 0.0, 0.0, 1.0 ) INS-12500_FOV_REF_VECTOR = ( 1.0, 0.0, 0.0 ) INS-12500_FOV_REF_ANGLE = ( 0.25 ) INS-12500_FOV_ANGLE_UNITS = ( 'DEGREES' ) \begintext End of the IK file.