Solar Power Satellite system in formation on a common geostationary orbit
| dc.contributor.author | Salazar, F. J.T. [UNESP] | |
| dc.contributor.author | Winter, O. C. [UNESP] | |
| dc.contributor.institution | Universidade Estadual Paulista (Unesp) | |
| dc.date.accessioned | 2018-12-11T17:34:55Z | |
| dc.date.available | 2018-12-11T17:34:55Z | |
| dc.date.issued | 2017-10-25 | |
| dc.description.abstract | The diurnal day-night cycle severely limits the Terrestrial solar power. To overcome this limitation, a Solar Power Satellite (SPS) system, consisting of a sunlight reflector and a microwave energy generator-transmitter in formation, is presented in this work. The microwave transmitting satellite (MTS) is placed on a common geostationary orbit (GEO) in the Earth's equatorial plane, and the sunlight reflector uses the solar radiation pressure to achieve quasi-periodic orbits about the MTS, so that the sunlight is always redirected to the MTS, which converts the solar energy in electromagnetic power and transmits it by microwaves to an Earth-receiving antenna. Assuming the sun line direction constant at dierent seasons (i.e. autumn/spring equinoxes and winter and summer solstices), previous studies have shown the existence of a family of displaced ecliptic orbits above or below the equatorial plane of the Earth around a GEO. In this study, the position of the Sun is assumed on the ecliptic plane with a mean obliquity (inclination of Earth's equator with respect to the ecliptic) of 23.5. A linear solution as an initial condition for the full equations of motions about a GEO, which yields bounded orbit for the sunlight reflector about the MTS in the Earth-satellite two-body problem with solar radiation pressure. To redirect the sunlight to the MTS, the law of reflection is satisfied by the space mirror attitude. | en |
| dc.description.affiliation | Grupo de Dinamica Orbital and Planetologia Univ. Estadual Paulista UNESP | |
| dc.description.affiliationUnesp | Grupo de Dinamica Orbital and Planetologia Univ. Estadual Paulista UNESP | |
| dc.identifier | http://dx.doi.org/10.1088/1742-6596/911/1/012006 | |
| dc.identifier.citation | Journal of Physics: Conference Series, v. 911, n. 1, 2017. | |
| dc.identifier.doi | 10.1088/1742-6596/911/1/012006 | |
| dc.identifier.file | 2-s2.0-85034663111.pdf | |
| dc.identifier.issn | 1742-6596 | |
| dc.identifier.issn | 1742-6588 | |
| dc.identifier.scopus | 2-s2.0-85034663111 | |
| dc.identifier.uri | http://hdl.handle.net/11449/179377 | |
| dc.language.iso | eng | |
| dc.relation.ispartof | Journal of Physics: Conference Series | |
| dc.relation.ispartofsjr | 0,241 | |
| dc.relation.ispartofsjr | 0,241 | |
| dc.rights.accessRights | Acesso aberto | pt |
| dc.source | Scopus | |
| dc.title | Solar Power Satellite system in formation on a common geostationary orbit | en |
| dc.type | Trabalho apresentado em evento | pt |
| dspace.entity.type | Publication | |
| relation.isDepartmentOfPublication | cf723ce7-c9ee-4e06-b772-346bd0a102bb | |
| relation.isDepartmentOfPublication.latestForDiscovery | cf723ce7-c9ee-4e06-b772-346bd0a102bb | |
| unesp.department | Matemática - FEG | pt |
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