2019
DOI: 10.2514/1.a34032
|View full text |Cite
|
Sign up to set email alerts
|

Space-Enhanced Terrestrial Solar Power for Equatorial Regions

Abstract: This paper investigates the concept of solar mirrors in a Earth orbit to provide large-scale terrestrial equatorial solar farms with additional solar power during the hours of darkness. A ower constellation of mirrors is considered in highly-eccentric orbits (semi-major axis=20270.4 km) in order to increase the time of visibility over the solar farms and, through this architecture, only two mirrors are needed to provide a complete night-coverage over three equatorial locations. Selecting the proper value for t… Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1

Citation Types

0
4
0

Year Published

2020
2020
2024
2024

Publication Types

Select...
5
1

Relationship

0
6

Authors

Journals

citations
Cited by 13 publications
(4 citation statements)
references
References 14 publications
0
4
0
Order By: Relevance
“…cos θ (11) where B 0 = 3.12 × 10 −5 T is the mean value of the magnetic field at the magnetic equator on the Earth's surface [18]. The angle ψ lies between the z-axis and the line of intersection between the reflector surface and the orbital plane.…”
Section: A Attitude Requirements For Simplified Reflector Systemmentioning
confidence: 99%
See 2 more Smart Citations
“…cos θ (11) where B 0 = 3.12 × 10 −5 T is the mean value of the magnetic field at the magnetic equator on the Earth's surface [18]. The angle ψ lies between the z-axis and the line of intersection between the reflector surface and the orbital plane.…”
Section: A Attitude Requirements For Simplified Reflector Systemmentioning
confidence: 99%
“…A key difference to the previous detumbling simulation is that the magnetic field direction is no longer constant, instead it's components are given by Eq. (11). Due to the constrained geometry of the system, these torques will always lie on the y-axis, and so deliver an angular acceleration around the Sun-reflector direction.…”
Section: B Attitude Control Of An Orbiting Solar Reflectormentioning
confidence: 99%
See 1 more Smart Citation
“…Further recent studies include Bonetti and McInnes who considered the use of so-called heliotropic orbits. These are elliptical equatorial orbits whose apse line is artificially precessed using solar radiation pressure to ensure that the orbit perigee is always directed to towards the Sun [15]. This enables a long dwell time for the reflectors over the night-side of the Earth at the orbit apogee.…”
Section: Introductionmentioning
confidence: 99%