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Bestimmung der Wärmeverluste von Receiverrohren mittels transienter Thermografie

Geller, Juliane (2012) Bestimmung der Wärmeverluste von Receiverrohren mittels transienter Thermografie. Diploma, Deutsches Zentrum für Luft und Raumfahrt.

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Thermal heat losses of the receiver tube have a significant influence on the economic viability of solar thermal power plants. It is hence relevant to quantify these heat losses as accurately as possible, in order to replace aged receiver tubes if necessary. However, there is no accurate field measurement method yet available to evaluate the quality of receiver tubes in a parabolic trough power plant. In this study, transient thermography as possible measurement method is introduced. For that purpose, the receiver tube is modeled as a linear, time invariant system with respect to signal processing theory. The quality of the receiver tube can be determined from the frequency response of this system. Methods are therefore developed to compute the frequency response. In a simulation study, different ways to excitate the receiver tube are tested. The focus of this study is to determine how accurately the frequency response can be determined from the resulting temperature functions.

Item URL in elib:https://elib.dlr.de/78608/
Document Type:Thesis (Diploma)
Title:Bestimmung der Wärmeverluste von Receiverrohren mittels transienter Thermografie
AuthorsInstitution or Email of AuthorsAuthor's ORCID iDORCID Put Code
Open Access:No
Gold Open Access:No
In ISI Web of Science:No
Keywords:parabolic trough, receiver, measurement
Institution:Deutsches Zentrum für Luft und Raumfahrt
HGF - Research field:Energy
HGF - Program:Renewable Energies
HGF - Program Themes:Concentrating Solar Systems (old)
DLR - Research area:Energy
DLR - Program:E SF - Solar research
DLR - Research theme (Project):E - Qualifizierung (old)
Location: Köln-Porz
Institutes and Institutions:Institute of Solar Research > Qualifizierung
Deposited By: Kruschinski, Anja
Deposited On:17 Dec 2012 17:13
Last Modified:23 Jan 2013 15:53

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