(B) Output data:

• (B1) decompress.sh - OS-Linux-based script for the complete decompresion of all output data (see B2) into the common subdirectory TPS_DATA (the directory must not exist before the script is run; by command: sh decompress.sh or ./decompress.sh).
• (B2) res####_$$$$.tgz - the archive of output data archives for the period ranging from #### to $$$$ Myr. After its decompression (command: tar xzvf res####_$$$$.tgz), subdirectory RES####_$$$$/ is created and following archives occur inside it:
  • (B2a) xyz@@@@_****.tgz - zipped TAR archive of the rectangular position and velocity coordinates of the integrated test particles (TPs) being in the integration region, at least for a while, during the integration period spanning from @@@@ to **** (in Myr). After a decompression (command: tar xzvf xyz@@@@_****.tgz), the files
    • -- "small&&&&.xyz" will occur. Symbol &&&& indicates the time in Myr, for which the coordinates are given. The data about each TP are written in three lines. The structure of these lines is following:
      • 1st line: identification string of the TP, epoch for which the data are given (in days from the beginning of the simulation; it corresponds to &&&&);
      • 2nd line: rectangular coordinates X, Y, Z of the TP in AU;
      • 3rd line: components of the velocity vector VX, VY, VZ of the TP in AU/day (both vectors are referred to the modified galactic heliocentric coordinate system).
  • (B2b) qew@@@@_****.tgz - zipped TAR archive of the orbital elements of the TPs being in the integration region. After a decompression, the files
    • -- "small&&&&.qew" will occur. Symbol &&&& indicates again the time, in Myr, for which the orbital elements are given. In days, this epoch is also given in the first line of the "small&&&&.qew" file. The data about the TPs are written in further lines, one line for a given TP. This line contains: perihelion distance, q [AU]; eccentricity, e; argument of perihelion, omega [deg]; longitude of ascending node, Omega [deg]; inclination, i [deg]; identification code of the given TP. The angular elements are referred to the modified galactic heliocentric coordinate system.
  • (B2c) col@@@@_****.tgz - zipped TAR archive with the files
    • -- "col&&&&.inf" containing information of which TPs collided with a massive body (Sun or planet) during the interval ranging from &&&&-1 to &&&& Myr. In a particular line, the code of a given TP is followed by information of which massive body was hit.
  • (B2d) eje@@@@_****.tgz - zipped TAR archive with the files
    • -- "eje&&&&.inf" containing the names of TPs, which were ejected into the interstellar space during the interval ranging from &&&&-1 to &&&& Myr.