AUTOSTRUCTURE
Created: 2010-08-04 17:50:21
Last updated: 2011-02-27 17:26:17
This is a simple workflow designed to run AUTOSTRUCTURE with an user selected input.
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 doubly excited state (satellite line) models.
More information can be found here:
- Reference Manual: http://www.adas.ac.uk/man/chap7-01.pdf
- AUTOSTRUCTURE on the Spinet client (Soaplab2): http://caoba.ivic.ve:8180/soaplab2-axis/
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Authors (2)
| Juan González / Claudio Mendoza |
| Juan González |
Titles (3)
| AUTOSTRUCTURE Workflow |
| AUTOS Workflow |
| XSTAR Workflow |
Descriptions (6)
| This workflow takes xstar input files or input file locations (URL) to execute a simple run of the routine.
AUTOSTRUCTURE is a omputer program for calculating the physical conditions and emission spectra of photoionized gases.
|
| This workflow takes xstar input files or input file locations (URL) to execute a simple run of the routine.
|
| This workflow takes autostructure input files or input file locations (URL) to execute a simple run of the routine.
AUTOSTRUCTURE is a computer program for calculating energy levels, radiative rates, autoionization rates, photoionization cross sections, plane-wave Born and distorted-wave excitation cross sections in LS- and intermediate-coupling using non- or (kappa-averaged) relativistic wavefunctions.
|
| This workflow takes xstar input files or input file locations (URL) to execute a simple run of the routine.
AUTOSTRUCTURE is a computer program for calculating energy levels, radiative rates, autoionization rates, photoionization cross sections, plane-wave Born and distorted-wave excitation cross sections in LS- and intermediate-coupling using non- or (kappa-averaged) relativistic wavefunctions.
|
| This workflow takes xstar input files or input file locations (URL) |
| This workflow takes xstar input files or input file locations (URL) to execute a simple run of the routine.
XSTAR is a omputer program for calculating the physical conditions and emission spectra of photoionized gases.
|
Dependencies (0)
Inputs (1)
| Name |
Description |
| autos_input |
The direct input port allows the user to set paramters for a single autostructure run.
The direct input port allows the user to set 21 physical paramters for a single xstar run.
|
Processors (1)
| Name |
Type |
Description |
| autostructure |
soaplab |
Endpointhttp://caoba.ivic.ve:8180/soaplab2-axis/services/testing.autostructure |
Outputs (9)
| Name |
Description |
| std_errors |
Information from the stderror stream
|
| report |
Standard report of execution
|
| olg |
|
| oic |
|
| ols |
|
| radout |
|
| tccdw |
|
| omginfic |
|
| omginfls |
|
Datalinks (10)
| Source |
Sink |
| autos_input |
autostructure:autos_input_direct_data |
| autostructure:std_errors |
std_errors |
| autostructure:report |
report |
| autostructure:olg |
olg |
| autostructure:oic |
oic |
| autostructure:ols |
ols |
| autostructure:radout |
radout |
| autostructure:tccdw |
tccdw |
| autostructure:omginfic |
omginfic |
| autostructure:omginfls |
omginfls |
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