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NASA Scientific and Technical Aerospace Reports

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20040074322 <strong>NASA</strong> Langley Research Center, Hampton, VA, USA<br />

Parametric Studies of Square Solar Sails Using Finite Element Analysis<br />

Sleight, David W.; Muheim, Danniella M.; March 25, 2004; 13 pp.; In English; 45th AIAA/ASME/ASCE/AHS/ASC<br />

Structures, Structural Dynamics, <strong>and</strong> Materials Conference, 19-22 Apr. 2004, Palm Springs, CA, USA<br />

Contract(s)/Grant(s): 755-06-00<br />

Report No.(s): AIAA Paper 2004-1509; No Copyright; Avail: CASI; A03, Hardcopy<br />

Parametric studies are performed on two generic square solar sail designs to identify parameters of interest. The studies<br />

are performed on systems-level models of full-scale solar sails, <strong>and</strong> include geometric nonlinearity <strong>and</strong> inertia relief, <strong>and</strong> use<br />

a Newton-Raphson scheme to apply sail pre-tensioning <strong>and</strong> solar pressure. Computational strategies <strong>and</strong> difficulties<br />

encountered during the analyses are also addressed. The purpose of this paper is not to compare the benefits of one sail design<br />

over the other. Instead, the results of the parametric studies may be used to identify general response trends, <strong>and</strong> areas of<br />

potential nonlinear structural interactions for future studies. The effects of sail size, sail membrane pre-stress, sail membrane<br />

thickness, <strong>and</strong> boom stiffness on the sail membrane <strong>and</strong> boom deformations, boom loads, <strong>and</strong> vibration frequencies are<br />

studied. Over the range of parameters studied, the maximum sail deflection <strong>and</strong> boom deformations are a nonlinear function<br />

of the sail properties. In general, the vibration frequencies <strong>and</strong> modes are closely spaced. For some vibration mode shapes,<br />

local deformation patterns that dominate the response are identified. These localized patterns are attributed to the presence of<br />

negative stresses in the sail membrane that are artifacts of the assumption of ignoring the effects of wrinkling in the modeling<br />

process, <strong>and</strong> are not believed to be physically meaningful. Over the range of parameters studied, several regions of potential<br />

nonlinear modal interaction are identified.<br />

Author<br />

Solar Sails; Stresses; Vibration Mode; Design Analysis; Dynamic Structural Analysis; Membrane Structures; Computation<br />

19<br />

SPACECRAFT INSTRUMENTATION AND ASTRIONICS<br />

Includes the design, manufacture, or use of devices for the purpose of measuring, detecting, controlling, computing, recording, or<br />

processing data related to the operation of space vehicles or platforms. For related information see also 06 Avionics <strong>and</strong> Aircraft<br />

Instrumentation; for spaceborne instruments not integral to the vehicle itself see 35 Instrumentation <strong>and</strong> Photography; for spaceborne<br />

telescopes <strong>and</strong> other astronomical instruments see 89 Astronomy.<br />

20040068196 Jet Propulsion Lab., California Inst. of Tech., Pasadena, CA, USA<br />

<strong>NASA</strong> Space Cryocooler Programs: A 2003 Overview<br />

Ross, R. G., Jr.; Boyle, R. F.; Kittel, P.; International Thermal Detectors Workshop (TDW 2003); February 2004, pp. 6-1 -<br />

6-7; In English; See also 20040068186; No Copyright; Avail: CASI; A02, Hardcopy<br />

Mechanical cryocoolers represent a significant enabling technology for <strong>NASA</strong>’s Earth <strong>and</strong> Space Science missions. An<br />

overview is presented of ongoing cryocooler activities within <strong>NASA</strong> in support of current flight projects, near-term flight<br />

instruments, <strong>and</strong> long-term technology development. <strong>NASA</strong> programs in Earth <strong>and</strong> space science observe a wide range of<br />

phenomena, from crop dynamics to stellar birth. Many of the instruments require cryogenic refrigeration to improve dynamic<br />

range, extend wavelength coverage, <strong>and</strong> enable the use of advanced detectors. Although, the largest utilization of coolers over<br />

the last decade has been for instruments operating at medium to high cryogenic temperatures (55 to 150 K), reflecting the<br />

relative maturity of the technology at these temperatures, important new developments are now focusing at the lower<br />

temperature range from 4 to 20 K in support of studies of the origin of the universe <strong>and</strong> the search for planets around distant<br />

stars. <strong>NASA</strong>’s development of a 20K cryocooler for the European Planck spacecraft <strong>and</strong> its new Advanced Cryocooler<br />

Technology Development Program (ACTDP) for 6-18 K coolers are examples of the thrust to provide low temperature cooling<br />

for this class of missions.<br />

Author<br />

Cryogenic Cooling; <strong>NASA</strong> Space Programs; General Overviews; Flight Instruments; Technology Utilization<br />

20040068226 Northrop Grumman Space Technology, Redondo Beach, CA, USA<br />

Space Cryocoolers<br />

Tward, Emanuel; International Thermal Detectors Workshop (TDW 2003); February 2004, pp. 6-16; In English; See also<br />

20040068186; No Copyright; Abstract Only; Available from CASI only as part of the entire parent document<br />

Cryogenic coolers for use in space require low power <strong>and</strong> minimum weight. In this paper we describe the typical<br />

requirements <strong>and</strong> performance of a number of reliable, small, efficient, low-power, vibrationally balanced coolers designed <strong>and</strong><br />

27

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