[FPSPACE] Station-Keeping Requirements for Constellations of Free-Flying Collectors Used f
LARRY KLAES
ljk4 at msn.com
Tue Jul 3 14:33:01 EDT 2007
Station-Keeping Requirements for Constellations of Free-Flying Collectors
Used for Astronomical Imaging in Space
Authors: Ronald J. Allen
(Submitted on 2 Jul 2007)
Abstract: The accuracy requirements on station-keeping for constellations of
free-flying collectors coupled as (future) imaging arrays in space for
astrophysics applications are examined. The basic imaging element of these
arrays is the two-element interferometer. Accurate knowledge of two
quantities is required: the \textit{projected baseline length}, which is the
distance between the two interferometer elements projected on the plane
tranverse to the line of sight to the target; and the \textit{optical path
difference}, which is the difference in the distances from that transverse
plane to the beam combiner. ``Rules-of-thumb'' are determined for the
typical accuracy required on these parameters. The requirement on the
projected baseline length is a \textit{knowledge} requirement and depends on
the angular size of the targets of interest; it is generally at a level of
half a meter for typical stellar targets, decreasing to perhaps a few
centimeters only for the widest attainable fields of view. The requirement
on the optical path difference is a \textit{control} requirement and is much
tighter, depending on the bandwidth of the signal; it is at a level of half
a wavelength for narrow (few %) signal bands, decreasing to $\approx 0.2
\lambda$ for the broadest bandwidths expected to be useful. Translation of
these requirements into engineering requirements on station-keeping accuracy
depends on the specific details of the collector constellation geometry.
Several examples are provided to guide future application of the criteria
presented here. Some implications for the design of such collector
constellations and for the methods used to transform the information
acquired into images are discussed.
Comments: 13 pages, 6 figures, accepted 6/29/07 for the August 2007 issue
of PASP
Subjects: Astrophysics (astro-ph)
Cite as: arXiv:0707.0255v1 [astro-ph]
Submission history
From: Ronald J. Allen [view email]
[v1] Mon, 2 Jul 2007 15:38:06 GMT (299kb)
http://arxiv.org/abs/0707.0255
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