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contributor authorTesia L. Albarado
contributor authorDavid Edwards
contributor authorCharles Semmel
contributor authorWhitney Hubbs
contributor authorWilliam A. Hollerman
date accessioned2017-05-09T00:17:51Z
date available2017-05-09T00:17:51Z
date copyrightFebruary, 2005
date issued2005
identifier issn0199-6231
identifier otherJSEEDO-28367#125_1.pdf
identifier urihttp://yetl.yabesh.ir/yetl/handle/yetl/132633
description abstractSolar sailing is a unique form of propulsion where a spacecraft gains momentum from incident photons. Since sails are not limited by reaction mass, they provide continual acceleration, reduced only by the lifetime of the lightweight film in the space environment and the distance to the Sun. Practical solar sails can expand the number of possible missions that are difficult by conventional means. The National Aeronautics and Space Administration’s Marshall Space Flight Center (MSFC) is concentrating research into the utilization of ultra lightweight materials for spacecraft propulsion. Solar sails are generally composed of a highly reflective metallic front layer, a thin polymeric substrate, and occasionally a highly emissive back surface. The Space Environmental Effects Team at MSFC is actively characterizing candidate sails to evaluate the thermo-optical and mechanical properties after exposure to electrons. This paper will discuss the preliminary results of this research.
publisherThe American Society of Mechanical Engineers (ASME)
titleElectron Exposure Measurements of Candidate Solar Sail Materials
typeJournal Paper
journal volume127
journal issue1
journal titleJournal of Solar Energy Engineering
identifier doi10.1115/1.1823495
journal fristpage125
journal lastpage130
identifier eissn1528-8986
keywordsElectrons
keywordsSolar energy
keywordsMeasurement
keywordsSpace vehicles AND Photons
treeJournal of Solar Energy Engineering:;2005:;volume( 127 ):;issue: 001
contenttypeFulltext


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