- #Cal.ini sd c4 install#
- #Cal.ini sd c4 serial#
- #Cal.ini sd c4 windows 10#
- #Cal.ini sd c4 pro#
- #Cal.ini sd c4 software#
The data files used were (1) the ENDF/B-IV fission product file, (2) the ENDF/B-V fission product file, (3) a file derived by substituting decay energies from JNDC into the ENDF/B-V file, and (4) a file derived by substituting decay-energies and spectra from more » the UK data file into the ENDF/B-V file. Three experiments (one from Oak Ridge and two from Los Alamos), in which samples of /sup 235/U and /sup 238/Pu were irradiated with thermal neutrons and either the total, gamma-ray, or gamma- and beta-ray fission product decay-energies were measured as functions of cooling time, were selected for comparisons with calculations made using four different fission product data files. Associated with the photon and particle radiation tables are the appropriate average energies per decay for each type of radiation, including neutrino radiation. For cases in which the multipolarities could be obtained from the file the tables also contain information on x-rays, conversion electrons, and Auger electrons. If there are spectra in the decay data file, the decay scheme is followed by tables of photon, particle, and characteristic radiation. All energies listed in this publication are in keV, and all branching ratios (BR) sum to unity. Independent fission yields are given, as well as thermal cross sections and resonance integrals as obtained from ENDF/B-IV. Uncertainties are more » given if available in the file. Following the comments is a decay scheme of the nuclide tabulating the quantities T/sub /sup 1///sub 2//, Q, branching ratio (BR), (E/sub. The detailed information for each member includes the ENDF/B-IV File 1 comments and references if available and applicable to the decay data. The heading page is followed by more detailed information on the individual members of the chain in order of increasing Z and decreasing metastable state. The fission product data have been organized by A-chains in order of ascending A from A = 72 to A = 167. For cases in which the multipolarities could be obtained from the file the tables also contain information on x rays, conversion electrons, and Auger electrons. All energies listed in this publication are in keV, and all branching ratios sum to unity.
#Cal.ini sd c4 install#
Download and Install ODIS 5.The fission product data have been organized by A-chains in order of ascending A from A = 72 to A = 167.
#Cal.ini sd c4 windows 10#
#Cal.ini sd c4 serial#
PLATFORM=PART_T (or optional _W for Wi-Fi ONLY communication)Ģ.Find out HHTWin.ini file which located in the windows MAIN folder, and then follow these:Īfter that, you need to configure serial port, LAN network or WIFI network (if you using WIFI Benz diagnostic system)įor detail register or configuration setting, please check wobd2 official blog. Find out F:ProgrammeDASbin folder in Local Disk F:/ and locate Cal.ini file, follow below steps sli by yourself.)īut you have to do following changes to convert the PartD MB Star C3 to SD Connect C4 Mux.ġ. (If you are MB Star diagnostic technician, you also can modify the cal.
#Cal.ini sd c4 software#
Replace the attached file (cal.sli) in local disk F:/ F:programmeXentrybinllist and make it Read Only after running MB Star C3 Xentry software which has connect with your SD connect C4 Multiplexer, then replace the download Cal sli.
#Cal.ini sd c4 pro#
here introduce you two ways to make your Benz Star C3 Pro ( Quality Version) work as MB SD Connect C4.Ĭonvert MB Star C3 PartD (C3) to SD connect (C4), download Convert_C3_to_C4 tool.rar, and run it on your MB star c3 Diagnosis software.
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