HISTORY
The STEC model library was initiated in 1998
in a joint effort by DLR (German Aerospace Centre) , Sun*Lab/SANDIA (USA)
and IVTAN (Institut for High Temperatures of the Russian Academy of Science,
Russia), three scientific organisations who are active in research and
development of solar thermal power generation. TRNSYS and the STEC were
envisioned as a potential replacement for the SOLERGY code, up to then
the quasi-standard for estimating the annual performance of solar thermal
power plants, which was no longer up to date with modern standards of computing
power and user friendliness. SOLERGY is limited to energy flow calculations
of fixed (hard wired) plant configurations. Consequently, various code
adaptations arose for different plant designs and detailed modeling of
plant thermodynamics was not possible.
TRNSYS was chosen for the simulation environment
because of its modularity, user friendliness and the simplicity in adding
new component models. Moreover, the availability of the TRNSYS source code
together with its reasonable price gave rise to hope for a rapidly increasing
acceptance and usage of the STEC software developments.
In 2000 the STEC models were updated to be fully
compatible with the new TRNSYS15 and Iisibat3. This work was mainly done
by former TRNSYS engineer Nathan Blair, working under Prof. Beckman at
the University of Wisconsin, Madison. In early 2001, parts of the STEC
library were successfully validated with measurement data from the SEGS
VI plant, a commercial solar thermal power plant in the Californian dessert.
While agreement between the simulation and actual plant data was generally
within 10%, there was difficulty in modeling solar field flow rate during
transients. Later that year, Thorsten Stuetzle, Prof. Beckman and
colleagues at the University of Wisconsin performed a ground-up analysis
of the problem and developed a dynamic solar field model and new control
algorithms that can both better model existing plant behavior and offer
the possibility of more stable field outlet temperatures if implemented
in place of human control. This work was initially performed in the
EES simulation environment, but will be transferred to TRNSYS.
In September 2002 the completely revised version 2.2 of the STEC library was released containing a number of new models in the brayton, rankine and solar thermal subsection.
Today, the STEC library is distributed to more than 30 institutions world wide. The models are used in research and development as well as in commercial projects. One impulse of interest was the free distribution of the STEC library also to non-SolarPACES members in 2003. But lately, with numerous commercial solar thermal power projects emerging -mostly in Europe and the U.S.- the interest is even increasing and moving from public research to private business institutions.
STEC library users worldwide.
TRNSYS16 and the Simulation Studio were distributed in mid 2004 with significant changes especially in the model programming standard. Therefore a complete update of the source code model by model was necessary. This work was performed 2005/2006 with the great help of TRNSYS engineer Diego A. Arias.
The latest version 3.0 of the library was released in November 2006.
The status of the STEC model library is freeware with full access to the source code. This open status shall be maintained. The models are developed, written and tested by STEC-users. The distribution of the STEC library is a non-budget activity, currently conducted by DLR. Therefore, the library’s content and its quality is reliant on the contribution and collaboration of the single user. All recipients sign a user agreement and commit thermselves to improve the STEC library by adding own components or projects, by validating models with other codes or measurements or by giving comments and suggestions to the developers.