Philipp Schramek
University of Sydney
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Featured researches published by Philipp Schramek.
Energy | 2004
Philipp Schramek; David R. Mills
Most conventional heliostats consist of a rectangular reflector which is moved around a fixed vertical axis tracking the azimuth of the sun and a second moving horizontal axis which rotates around the vertical axis to allow tracking the elevation of the sun. The maximum ground coverage possible of fields of such heliostats without colliding neighbouring reflectors is 58%. Applications of a Multi Tower Solar Array (MTSA) may need heliostat fields with ground coverage over 90%. We propose a new type of heliostat which can be set up in fields with a ground coverage of up to 100%. The maximum possible ground coverage depends on the unimpeded space volume needed by the reflector of each heliostat. The shape and the orientation of this space volume depends on the orientation of the tracking axes and on the shape of the reflector. A horizontal orientation of the fixed axis allows higher ground coverage and heliostats with rectangular reflectors can be lined up in rows with the highest density. The row density increases the longer the reflector becomes relative to its width and approximates 100% maximum ground coverage for infinite long and slim heliostats. With specially shaped hexagonal reflectors, ground coverage up to 100% is possible.
Journal of Solar Energy Engineering-transactions of The Asme | 2009
Philipp Schramek; David R. Mills; Wes Stein; Peter Le Lievre
A close-packed heliostat field of more than 800 m 2 reflector area has been installed by Solar Heat and Power for the CSIRO solar tower at the Energy Centre in Newcastle, Australia. The heliostat field has been designed with significantly greater field packing density than normally associated with heliostat fields. It can be shown that even though a heliostat field with a high ground coverage exhibits more blocking and shading, a higher annual performance can be achieved up to a certain point. The optimum ground coverage calculated for the CSIRO solar tower configuration is in the range of 53%. Other heliostat field designs usually have ground coverage below 30%. The annual optical performance of the CSIRO field per square meters of deflector is about 9% higher than a radial stagger field of 30% ground coverage for a research tower, which was optimized to have the highest perfor- mance for the time frame from 10 a.m. until 2 p.m.
Archive | 2008
David R. Mills; Philipp Schramek; David B. DeGraaff; Peter L. Johnson; Alexander Hoermann; Lars R. Johnson
Archive | 2002
David R. Mills; Philipp Schramek
Solar Energy | 2003
Philipp Schramek; David R. Mills
Solar Energy | 2006
Anne Gerd Imenes; D. Buie; David R. Mills; Philipp Schramek; Stephen Bosi
Archive | 2008
Philipp Schramek; Andrew Tanner; Lievre Peter Le
Archive | 2005
David R. Mills; Philipp Schramek; Anne Gerd Imenes; D. Buie
Archive | 2004
David R. Mills; Philipp Schramek; Stephen Bosi; Anne Gerd Imenes
publisher | None
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