Sandia’s NSTTF facilitates ground-breaking experiments this summer

Updated:2020-07-20 16:22Source:helioscsp

World’s first particle-to-supercritical COheat-exchanger system and on-sun falling particle receiver connected to a supercritical CO loop testing to take place.

Sandia National Laboratories’ National Solar Thermal Test Facility (NSTTF) will host a number of “firsts” in 2020, including testing a particle-to-supercritical CO heat-exchanger system, and the world’s first on-sun falling particle receiver connected to a supercritical CO (sCO) loop.

“SNL has been building and using supercritical CO loops for about a decade,” said Paul Gauche, Concentrating Solar Power (CSP) program manager. “There are several supercritical CO loops at the Brayton Laboratory, including one of the first three ever built, which are used for customer testing and research.” These loops demonstrated the first near-critical sCO compression, recompression Brayton cycle power generation, and trans-critical and mixed gas cycle variations, Gauche said.

In FY15, Sandia applied to the U.S. Department of Energy’s Solar Energy Technologies Office to fund a SunShot National Laboratory Multiyear Partnership (SuNLaMP) project in FY16-18. The goal of the project—a precursor to the much larger Generation 3 Particle Pilot Plant (G3P3) CSP project—was to build a falling particle receiver system with an integrated sCO loop to demonstrate the ability to heat sCO using particles heated by concentrated sunlight to temperatures above 700°C.

Dr Cliff Ho, Senior Scientist, is the Principal Investigator leading these projects. According to the researcher, this first test of the integrated test system will include the following components:

  • Falling particle receiver
  • Particle-to-sCO primary heat exchanger
  • sCO loop (to represent a closed-loop recompression sCO Brayton cycle)
  • Indirect air cooling system for the sCO loop

Although Sandia houses a megawatt-scale sCO loop, the loop that will be used for the SuNLaMP project is 150 kW to fit within the envelope of the NSTTF elevator and accommodate operation above 700°C. Ground-based testing of this system with electrical heating has exceeded 500 hours, surpassing any other loop of its size.

“The integrated system is unique because it heats the particles up to ~800°C using concentrated sunlight and then transfers that heat to a working fluid through a primary heat exchanger,” said Ho. “The heat exchanger is the world’s first to transfer heat from particles in a moving packed bed to supercritical carbon dioxide at design temperatures and pressures greater than 700°C and 20 MPa.”

Ultimately, the high-temperature sCO can be used in next-generation, high-efficiency sCO closed-loop Brayton cycles being pursued by DOE to decrease the cost to produce electricity.

“This is a ground-breaking experiment where we plan to use concentrated sunlight to transfer heat from falling particles in the receiver and into the supercritical CO loop,” Gauche said.

Heat exchanger installed in particle receiver assembly

Participants in the project include Sandia researchers Kevin Albrecht, Matt Carlson, Henk Laubscher, Francisco Alvarez, Robert Crandell, Daniel Ray, Roger Buck, Lam Banh, Rob Sharpe, Ron Hrzich, Moises Beato, and Arthur Buege, as well as partners Vacuum Processing Engineering (VPE) and Solex Thermal Science. Testing is taking place at the NSTTF using the country’s first concentrating solar tower built in 1978. The tower’s 800,000-pound-capacity elevator allows researchers to build large experiments like the SuNLaMP test and raise them to the top of the tower, which is unique in the CSP industry.

The NSTTF is also incorporating work from its Gen 3 projects by testing falling particle receiver and sCO loop control improvements.

Related Gen 3 activities include three projects:

  • G3P3 (Gen 3 Particle Pilot Plant) where researchers are working on ways to reduce heat loss and improve efficiencies in various components of the falling particle receiver system
  • Gen 3 CSP sCO Coolant Loop to simulate a 1 MWth power cycle for the Gen 3 CSP pilot plant
  • A Gen 3 Lab Call where researchers from Sandia and its partner, University of New Mexico, measure particle and heat loss from the receiver aperture using novel imaging techniques

Activities for SuNLaMP and the Gen 3 projects will continue through 2020, with the on-sun test campaign running through the summer.

(To learn more about the SuNLaMP project and G3P3, visit Gen 3 Particle-Pilot-Plant.Visit the Brayton Lab to learn more about Sandia National Laboratories’ facility.To learn more about concentrating solar power, visit Sandia’s NSTTF.By Kelly Sullivan)

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