title: The resultant vector and principal moment of light radiation pressure upon an optically convex space structure
metadata.name: dc.contributor.author
metadata.value: Nerovny, Nikolay A.
metadata.lang: -
metadata.name: dc.date.accessioned
metadata.value: 2017-07-05T09:44:37Z
metadata.lang: -
metadata.name: dc.date.available
metadata.value: 2017-07-05T09:44:37Z
metadata.lang: -
metadata.name: dc.date.issued
metadata.value: 2017-03
metadata.lang: -
metadata.name: dc.identifier.citation
metadata.value: Nerovny N.A. The resultant vector and principal moment of light radiation pressure upon an optically convex space structure. Vestnik SPbSU. Mathematics. Mechanics. Astronomy, 2017, vol. 4 (62), issue 1, pp. 146–158.
metadata.lang: en_GB
metadata.name: dc.identifier.other
metadata.value: 10.21638/11701/spbu01.2017.117
metadata.lang: -
metadata.name: dc.identifier.uri
metadata.value: http://hdl.handle.net/11701/6696
metadata.lang: -
metadata.name: dc.description.abstract
metadata.value: In this paper we discuss the questions related to determination of light radiation pressure upon a space
  structures of optically convex shape. The equation for force from light pressure acting upon an space
  optically convex structure’s surface infinitesimal element is given with assumption that the surface may
  be shadowed partly. We derive the infinitesimal light radiation force as a series based on representation
  of absolute value function as a series of Chebyshev polynomials of first kind. We also obtain the tensor
  equations which describe the shape and the optical properties of a surface independently from its attitude.
  For these tensor equations we presented the equations for resultant vector and principal moment of light
  radiation pressure on the space structure. We also provide an example equations for flat two-sided solar
  sail. These results can be used for the analysis of dynamics of a center of gravity and around center of
  mass of a space structures, and also for the development of adaptive control systems of satellites which
  can take solar pressure into account. Refs 41. Figs 1.
metadata.lang: en_GB
metadata.name: dc.description.sponsorship
metadata.value: Работа выполнена в рамках работы над космическим экспериментом «Парус–МГТУ».
metadata.lang: en_GB
metadata.name: dc.language.iso
metadata.value: ru
metadata.lang: en_GB
metadata.name: dc.publisher
metadata.value: St Petersburg State University
metadata.lang: en_GB
metadata.name: dc.relation.ispartofseries
metadata.value: Vestnik of St Petersburg University. Mathematics. Mechanics. Astronomy;Volume 4 (62); Issue 1
metadata.lang: -
metadata.name: dc.subject
metadata.value: solar sail
metadata.lang: en_GB
metadata.name: dc.subject
metadata.value: light pressure
metadata.lang: en_GB
metadata.name: dc.subject
metadata.value: resultant vector
metadata.lang: en_GB
metadata.name: dc.subject
metadata.value: principal moment
metadata.lang: en_GB
metadata.name: dc.title
metadata.value: The resultant vector and principal moment of light radiation pressure upon an optically convex space structure
metadata.lang: en_GB
metadata.name: dc.type
metadata.value: Article
metadata.lang: en_GB
resources.filename: 17-Nerovny.pdf
resources.url: https://dspace.spbu.ru/bitstream/11701/6696/1/17-Nerovny.pdf
resources.format: Adobe PDF
resources.size: 299,75 kB