---------------------------------------------*/

<summary> This is the algorithm of ISO/IEC 14495-1, A.5.2, Code Segment A.11 (second else branch) It will map signed values to unsigned values. It has

** Mark black 'OLD1' objects when starting a new young collection. ** Gray objects are already in some gray list, and so will be visited ** in the ato

počet dostupných zařízení */

** When creating file handles, always creates a 'closed' file handle ** before opening the actual file; so, if there is a memory error, the ** handle

Normal

Subtract two signed integers with a wrap-around behaviour. Assumes complement-to-two signed integers. @param a @param b @return Returns a - b */

* Creates a Tier 2 handle * * @param p_image Source or destination image * @param p_cp Image coding parameters. * @

Create a new TCD handle */

** Pack integer 'n' with 'size' bytes and 'islittle' endianness. ** The final 'if' handles the case when 'size' is larger than ** the size of a Lua in

Parse CCSDS header

** Traverse a list of tests, patching their destination address and ** registers: tests producing values jump to 'vtarget' (and put their ** values in

Evaluation sum(p[i] * x^i, i, 0, N) via Horner's method. N.B. p is of length N+1.

/ @brief Generates population count (i.e., the number of set bits) * * @param [in] val is the value for which population count is sought */

* Predict absolute, observer-independent properties of the moon. * * \param time Time * \param moon Output struct * \copyright GPLv2+ **/

* Calculate RA and dec for the moon. * * \param time Time * \param ra Right ascension * \param dec Declination * \copyright GPLv2+ **/