Solar Blind Pyrometer Temperature Measurements in High Temperature Solar Thermal Reactors: A Method for Correcting the System-Sensor Cavity Reflection Error

2005 ◽  
Vol 127 (1) ◽  
pp. 86-93 ◽  
Author(s):  
Aaron P. Freid ◽  
Paul K. Johnson ◽  
Manuela Musella ◽  
Reto Mu¨ller ◽  
Julie E. Steinbrenner ◽  
...  

We developed a method that enables one to correct solar blind pyrometer cavity temperature measurements for the system-sensor reflection error. The method is valid for measurements made on diffusely emitting and reflecting cavity surfaces when there is no participating medium between the pyrometer and the surface of interest. The surfaces’ emissivities must be known. The procedure gives the uncertainty interval associated with the correction. The procedure was validated by measuring surface temperatures in a solar reactor insulated with Yttria-stabilized Zirconia felt receiving concentrated solar radiation. The temperature range of the experimental study was from 1100–1600 K. Temperature measurements made with a pyrometer having a narrow band filter centered at 1.398 μm were compared to temperatures measured with Zirconia felt shielded thermocouples. Uncorrected pyrometer measurements differed from the thermocouple measurements by as much as 350 K. The thermocouple measurements mostly fell within the system-sensor uncertainty interval of the corrected temperature measurements. The uncertainty interval depends both on the number of surfaces probed with the pyrometer and the nature of the solar blind filter. A numerical simulation study showed that a UV filter centered at a wavelength near 0.285 μm gives tighter system-sensor uncertainty intervals than an IR filter centered at 1.398 μm.

2017 ◽  
Vol 9 (2) ◽  
pp. 1-8
Author(s):  
Chaolong Fang ◽  
Bo Dai ◽  
Qiao Xu ◽  
Qi Wang ◽  
Dawei Zhang

1998 ◽  
Vol 330 (2) ◽  
pp. 150-156 ◽  
Author(s):  
A. Andreev ◽  
Bl. Pantchev ◽  
P. Danesh ◽  
B. Zafirova ◽  
E. Karakoleva

1982 ◽  
Vol 72 (12) ◽  
pp. 1714 ◽  
Author(s):  
M. V. R. K. Murty ◽  
N. C. Das

1971 ◽  
Vol 83 ◽  
pp. 93 ◽  
Author(s):  
Torrence V. Johnson ◽  
Larry A. Lebofsky ◽  
Thomas B. McCord

2013 ◽  
Vol 33 (11) ◽  
pp. 1123003
Author(s):  
罗昕 Luo Xin ◽  
邹喜华 Zou Xihua ◽  
温坤华 Wen Kunhua ◽  
潘炜 Pan Wei ◽  
闫连山 Yan Lianshan ◽  
...  

2010 ◽  
Vol 22 (8) ◽  
pp. 1819-1822
Author(s):  
岳威 Yue Wei ◽  
洪冬梅 Hong Dongmei ◽  
刘国喜 Liu Guoxi ◽  
韩永昶 Han Yongchang ◽  
刘连泽 Liu Lianze ◽  
...  

1982 ◽  
Vol 99 ◽  
pp. 531-537
Author(s):  
Michael M. Shara ◽  
Anthony F. J. Moffat

A search to continuum magnitude B ∼ 21.5 (MB∼ −3) using a narrow band filter at λ4670å and a wide B-band filter has revealed 21 Wolf-Rayet star candidates in about half the giant Sb galaxy M31. Some weak-line WR stars, particularly WN subtypes, may have escaped detection. These numbers are compatible with the total number of luminous (i.e. massive) stars in M31. Eighteen of twenty confirmed candidate stars in M31 lie in the direction of 0B associations in the ring of prominent star formation 5–16 kpc from the center.


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