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1. Autostructure

ADAS701 Autostructure The code is a full implementation of the program AUTOSTRUCTURE developed by N R Badnell The entire capability of the original program for arbitrary structure Auger rate and Radiative rate calculation has been retained However input driver file selection driver templates output selection and output routing have been enabled within the ADAS framework to simplify the production of two types of data namely dielectronic recombination rates and data for doub
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1. ADAS704: Postprocessor - Autostructure > adf18 file

ADAS704 Postprocessor Autostructure gt adf18 file This is a new code which provides one of the last links in the chain of processing required in the GCR Project for the generation of complete collisional radiative data for light elements see also ADAS807 and GCR Project bulletin no 2 The code constitutes a third post processing option on the Auger rate coefficient data output from ADAS701 Autostructure It creates a part of the cross referencing file of type
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2. Autostructure

ADAS701 Autostructure The code is a full implementation of the program AUTOSTRUCTURE developed by N R Badnell The entire capability of the original program for arbitrary structure Auger rate and Radiative rate calculation has been retained However input driver file selection driver templates output selection and output routing have been enabled within the ADAS framework to simplify the production of two types of data namely dielectronic recombination rates and data for doub
PDF Manual ENGLISH
3. ADAS703: Postprocessor - Autostructure > adf04 file

ADAS703 Postprocessor Autostructure gt adf04 file Figure 8 3 The program isolates energy level Auger rate and radiative rate data from ADAS701 calculations It assembles these into specific ion files of type adf04 which include data lines for energy levels of doubly excited states and data lines for free bound resonance capture and Auger break up These specific ion files are the precursors for doubly excited population calculation and dielectronic satellite line emissivity
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