1975
DOI: 10.1364/ao.14.001509
|View full text |Cite
|
Sign up to set email alerts
|

Stationary concentrating reflector cum tracking absorber solar energy collector: optical design characteristics

Abstract: This article presents an analysis of the optical design characteristics of a stationary reflecting/tracking absorber solar energy collector. This type of collector consists of a segment of a spherical mirror placed in a stationary position facing the sun, but having a linear absorber that can track the image of the sun by a simple pivoting motion about the center of curvature of the reflector. The optical characteristics of this system and the axial variation of its concentration ratio are developed to provide… Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1
1

Citation Types

0
9
0

Year Published

1981
1981
2022
2022

Publication Types

Select...
6
3

Relationship

0
9

Authors

Journals

citations
Cited by 31 publications
(9 citation statements)
references
References 0 publications
0
9
0
Order By: Relevance
“…We obtain so the absorber characteristics as a truncated cone. This is also stated by Steward and Kreith 1975 [7]. By considering the half angle of the sun image projection …”
Section: Figmentioning
confidence: 59%
“…We obtain so the absorber characteristics as a truncated cone. This is also stated by Steward and Kreith 1975 [7]. By considering the half angle of the sun image projection …”
Section: Figmentioning
confidence: 59%
“…Unlike parabolic mirrors, spherical concentrators (or solar bowls) can be fixed using a mobile receiver [8]. Hence, these systems are also known as SRTA (stationary reflector/tracking absorber).…”
Section: The Current State Of Researchmentioning
confidence: 99%
“…The outside diameter of the coil was 75 mm, which is five times the maximal theoretical diameter. This safety factor was determined based on the optical analysis of the SRTA by Steward and Kreith (1975), which had indicated a considerably smaller (14 mm versus 75 mm) diameter possible for a perfect spherical mirror. However, in our practical mirror, the absorber diameter was determined not only by the 0.5°divergence of the solar rays but also by the imperfections of the mirror surface and the tracking system accuracy.…”
Section: The Absorbermentioning
confidence: 99%
“…The optical design characteristics of the SRTA were studied in detail by Steward and Kreith (1975). A thermal performance analysis was conducted by Kreider (1975), which identified the important design parameters influencing heat losses from the absorber.…”
Section: Introductionmentioning
confidence: 99%