in a Titan. IV or Space. Shuttle is approximately. 20-25 meters (parent reflector) in diameter. A passively controlled. 40-meter radiometer configuration requires.
: /L
Large
Phase and
Program
I:
_nolog3
Miss_Archi, e_: ....
:.
-:27:.:2.
Craig
A.
CONTRACT OCTOBER
Roge_£_Warren
NAS_ 1991 -_:5
_
_=
HI/15
_
.
NASA Contractor
Large
Phase
Technology
and
Mission
Craig
A. Rogers
and
Virginia
for
Langley Research Center under Contract NAS1-18471
National Aeronautics Space Administration
and
Office of Management Scientific and Technical Information Program 1991
Antenna
Assessment
Architecture
Polytechnic
Blacksburg,
Prepared
4410
Deployable
I:
Virginia
Report
Warren Institute
L. Stutzman and
State
University
Program
TABLE EXECUTIVE 1.
.
3.
.
OF CONTENTS
SUMMARY
INTRODUCTION 1.1
Mission
1.2
Technology
1.3
LDA
MISSION
to Planet
Objectives
REQUIREMENTS
AND
ANTENNA
FUNDAMENTALS
3.1
Overview
3.2
Main
3.3
Candidate
Reflector
AND
AND
Overview
4.2
Deployable
Trusses Truss
4.2.2
Ring
Technology
4.2.3
Design
4.2.4
New
4.3.1
4.3.2
CONFIGURATIONS
EVALUATION
Deployable
Reflector
CANDIDATE
Configurations
4.2.1
4.2.5
REQUIREMENTS
Shapes
PERFORMANCE
4.1
4.3
Needs
Program
REFLECTOR
DESIGN
Earth
Truss
Technology Review
and Performance Truss
Concepts
Overview
Evaluation for the LDA
4.2.4.1
Truss
Concepts
for a Segmented,
4.2.4.2
Truss
Concepts
for Furlable
4.2.4.3
Ring
Selected
Truss
Radiometer
Concept Structural
Rigid
Reflector
for a Membrane
Panel
LDA
Reflector
Strips Reflector
Configuration
Surfaces Rigid
Facets
4.3.1.1
Design
4.3.1.2
Manufacturing
Furlable
Evaluations Considerations
for Rigid
Facets
Surfaces
Ul
PRECEDING
PAGE
BLANK
NOT
FILMED
4.3.3
4.4
4.5
4.6
6.
Preliminary
4.3.2.2
Panel
Deployment
Membrane
Analysis
Sizing
Analysis
of Furlable
4.3.3.1
Design
4.3.3.2
Manufacturing
Surfaces
Evaluation of Furlable
4.4.1
Practically
Inextensible
Membrane
4.4.2
Membrane
Design
Material
4.4.3
Deployable
Motion
and
Reflectors Selection
Alternatives
and Controls
4.5.1
Introduction
4.5.2
LDA
4.5.3
Antenna
Motion
4.5.4
Actuator
Technology
4.5.5
Power
4.5.6
Vibration
Control
4.5.7
Summary
of Motion
4.5.8
Scan
4.5.9
A Scan
Motion
Train
AND
Requirements Systems
Considerations
Technology
Kinematics
Electromagnetic
SUMMARY
Segments
Reflectors
4.6.1 .
4.3.2.1
Selected
Scenario Designs Electromagnetic
Configurations
CONCLUSIONS
REFERENCES
iv
EXECUTIVE
The Large
SUMMARY
Deployable
availability Mission (OAET) Year
of critical
long term
The
goal
from
Program
for passive
of GCTI
specific
documentation
the 1987
goals
Sally
and understanding
Ride report
The
for the fin'st phase
of the LDA
technologies
Develop preliminary study team.
mission
study
wide
range
.
2. 3.
team
generic was
of skills
Principal Virginia
technologies
program
composed and
of university
experience,
Investigator: Polytechnic
Dr. Warren Stutzman, and State University
Dr. Craig Institute and Department
and
Astro
was
The study approach involved geosynchronous wide-scanning
The study
(rather
than
specifications)
team performed
a detailed
with
precise,
concepts
for
wide
the
Mission
the
to
referring purpose
deployable
scanning
presented
radiometer
concept
of
passive
to the study
presented
team
to the
reflectors.
researchers
Engineering,
of Mechanical
and
technologists
with a
Company, Aerospace
of Mechanical Virginia
Engineering,
Engineering,
Polytechnic Virginia
Institute
Polytechnic
Inc. Company,
Inc.
Inc. Inc.
from
determining radiometer
and enhance
to:
A. Rogers, Department State University
Aerospace
received
large,
industry
of Electrical
Mr. Ed Derby, Composite Optics, Dr. Brian Lilly, ANT Technologies,
as goals
for
the following:
Dr. John Hedgepeth, Consultant, Astro Mr. John Rule, Composite Optics, Inc.
Thomson,
large
including
Dr. Harry Robertshaw, Department Institute and State University
Additional input NASA Langley
will be required
is a concept
observations
were
for each
to support
Mr. Mark
8. 9.
the
as a system".
Administrator,
global
for
architecture
5. 7.
and demonstrate
to enable
of the earth
of the radiometer
4. 6.
which
needed
to the NASA
space-based
Determine the critical and prioritize them.
Evaluate
sensing
the technology
Review the technology state-of-readiness radiometers up to 60 GHZ.
•
to investigate
microwave
"is to provide
to the endeavor of making long-term, understanding earth system processes. The
was initiated
and for the NASA Office of Astronautics, Exploration and Technology Technology Initiative (GCTI) which is scheduled for initiation in Fiscal
observations,
Earth,
(LDA)
technologies
to Planet Earth Global Change
1991.
Planet
Antenna
the Electromagnetic
Advisory
basic operational parameters from which specific structural which
specific
technology
review, V
technologies evaluated
Panel
convened
by
and configurations for a requirements were used could
be evaluated.
the feasibility
and technology
readiness team
for a dual-reflector
also developed
IV launch
radiometer
a system
vehicle.
The
design
study
with a target
resulted
largest
deployable
stiff
IV or Space
Shuttle
A passively
controlled
thermal
controls
Segmented
'stiff'
requirements Several
with
an areal
density
concepts
have
the reflector
surface
accuracy
surface
identify
suitable
deployment
variations,
thermal
suitability
for ground
An
deployment
active
investigated •
Further
study
team
accurately support design and
goals,
the
requires
a deep
truss
and
at 40 GHz. designed
developed
to meet
using
a gore
The
manufacturing
quantify edge
scheme
surface
the surface
or
maximum
accuracy
strip
approach
to
width
to satisfy
the
techniques;
accuracy
distortions
and
for
stiff reflectors
constitutive
model
design
as a function
deployment
in the following
using
that a specific
mission
a reliable
of manufacturing
load
variations;
and
designs. antenna
assessment
mission
point
the
alloys
has been
studies.
can then With
design
vi
configurations. meter antenna for a 20-30 is needed focus,
be proposed these
to efficiently
of the
for which and
and
technology
or determination
specifications
can be completed.
designs. m antenna.
in order
state-of-readiness
of a mission
be determined. and
focus
and
selection
configurations can
memory
for further
area:
architecture Upon
shape
formulated
review and assessment of 20-30 of remote sensing requirements
electromagnetic
technology
in diameter.
testing.
configurations.
requirements
in a Titan
reflectors may be possible for sizes up to 40 meters basic fundamental investigations are still needed to
scheme;
also concluded
determine specific
control
detailed
been
develop
stresses,
is needed
Technology Determination
4. The
been
from a 40-meter
can be stowed
reflector)
configuration
Detailed EM analysis of the baseline Examination of alternative radiometric
.
2. 3.
The
of 2.4 kg/m 2.
membrane several
and a detailed
study
reflector.
to stow in a Titan
be reduced
which
(parent
requirements
3 m 2 have
down
is 12 m.
materials;
mechanical
meters
on the truss structure.
requirements
Practically inextensible in diameter. However,
20-25 radiometer
about
should
configuration
the accuracy
reflectors
'furlable'
deploying
40-meter
scaled
conclusions:
configuration
dual reflector
is approximately
to satisfy
radiometer
in the following
The deployable dual-reflector radiometer baseline to a 20-25 meter baseline. The
size of 40 m for the main
for a deployable
specific
to
of specific structural
requirements,
a
1.
INTRODUCTION
1.1
Mission
to Planet
Earth
In August of LEADERSHIP
1987, Dr. Sally K. Ride published "A Report to the Administrator" and America's Future in Space, which defined four potential U.S. space
and evaluated
them
retain
space
study
and
leadership evaluation,
exploration States
in light
and each identified
obtain
Exploration Outpost Humans program
all time
The
changes
The principal
function,
concept
accurate
- than
Mission
to Planet
Implementation proposed While
current
needed
scope
- either
the United four
selected
to Planet from
Earth,
a
space
to
Toward
with data from comprehensive
that
end,
Science
develop
of human
the
and
is to how
to evolve
of the Earth
gathered
of an integrated
by describing
be expected
to eventually
is that data
can be compared which are more
goal of this initiative System,
they may
or as a result
Earth
of Space
The
Earth
on
System,
the capability
activity."
over
a decade
or more
earth-based observations - and presumably more
guiding
principle
approach
behind
to observing
Applications)
initiative
the
the earth. has
been
[1-2]. of Aeronautics, particularly
will be necessary of CSTI
The
afforded
understanding
in order
naturally,
to Planet
(Office
us.
and how
a fundamental
is the adoption
1992
(Office
for and
restore
of Mission
use the perspective
will affect
interact,
models.
Initiative
missions,
efforts
the 5-year for the (GCTI)
OAET
near-term
technology
present-day
Year
activity."
of the entire
to that system,
occur
of this OSSA
for Fiscal
OSSA's
how they
of the Mission
Earth
if adopted,
is in support
changes
is to develop
might
would, of space
initiatives in science
on a global scale. Specifically, the mission is "an how forces shape and affect its environment, how that
those
global perspective for global change
any
report
understanding
of changes
that
candidate
achievements
and
System
that would
planet planet,
and how
challenge
from a space-based to produce models
in this
scientific
and of the consequences to predict
which
to regain
on the Moon to Mars
our home our home
components scales.
four
NASA's
desire
Earth
by the task group)
is changing,
the nation's
identified
on sphere
of the Solar
described
a comprehensive
and
group
proposal
to Planet
3.
(as described
its various
task
are:
2.
program
"builds
by the report
study and characterize initiative to understand environment
stated,
aggressive
Mission
technology
Dr. Ride
in a particular
4.
program
The they
space
of leadership
.
The
[1-1]. which is a bold,
to a position
initiatives
of the current
entitled, initiatives
[ 1-2].
the
Exploration,
and
Civil
Technology
to progress
To ensure
Space
into
availability
the next
Technology) era
of earth
of the technologies
programs
Initiative
support
(CSTI),
observation, which
new beyond
will be required
Mission to Planet Earth, OAET is developing a Global Change Technology Initiative for initiation in Fiscal Year 1991. The goal of this initiative is to provide the technology to
enable
understanding In July of 1988,
and
enhance
of the earth an Ad Hoc
the
long-term
observation,
documentation,
and
scientific
was formed
to determine
as a system. Review
Team
on Space
Technologies
what
technologiesmust be developedin the nearterm to supportMission to PlanetEarth. In their report entitled "Technology for the Mission to PlanetEarth" they describedthe major space segmentsfor the mission [t-2]. The threeproposedmission classesthat form the spacesegmentsfor the Mission to PlanetEarth are the Earth ObservingSystem(EOS), the Earth SystemExplorer missions,and the advanced GeostationaryEarth Scienceplatforms. Eachof thesespacesegmentsdescribedin detailedin the report "Technologyfor the Mission to PlanetEarth" are given below. EOS, a seriesof low earthpolar orbit platforms,eachcontainingmultiple scientificinstruments, is being planned to begin deploymentin the mid-1990s. Subsequentlauncheswill provide growth in the number and quality of remote sensingcapabilitiesthrough the year 2000, and continuousoperationof the systemat full capacityuntil at least2010. The EOS mission will createanintegratedscientificobservingsystemthatwill enablelong-termmulti-disciplinary study of the earth. The secondspacesegmentis a proposedseriesof Explorer-classmissionscalled Earth Probes, andthe useof well-establishedinstrumentsmountedon long-termplatforms suchas the space station. In additionto thepowerful synergismswithin EOS, thereare someobservingneedsthat require other low earthorbit (LEO) configurationsor dedicatedspacecraft. The third possible spacesegmentof a total systemfor global earth observationconsistsof advancedplatforms in geosynchronousearth orbit (GEO). Foremostin the advantagesthese platformswill offer overotherplatformsis thecapacityfor high temporalresolution,limited only by instrumentdesign andcost, to be brought to bearon the study of rapidly changing,global atmosphericphenomena.This type of orbit also would provide a fixed referencegeometryfor a given earth location, facilitating data analysisand interpretation; this advantagehas been demonstratedby operational geosynchronoussatellites,in service since 1974, which carry imager/sounderinstrumentsproviding high-resolutionvisible and infrared imagesof the earth. The infrared channelsof the sounding instrumentsyield frequent temperatureand moisture prof'flesover large areasof the earth. Another major advancewould be passive-microwave sensingof regionsof precipitation. For the technology program described in this report, the passive-microwave The
Ad
Hoc
sensing
instrument
Team
on Space
Review
for the geosynchronous Technologies
stated
microwave sounding is not now available because spatial resolution at GEO altitudes." This specific
current
earth
in their
focus
orbit
report
is
advanced that
on
the
platforms.
"the capability
of
of the large antenna required for adequate technology need is the motivation for this
program.
1.2 The
Technology objectives
technologies another
Needs
of the must
ad hoc group
measurement
of
technologies
have
Ad
Hoc
be developed
Review
of the Committee
precipitation so far remained
Team
on Space
in the near term to support and
soil
on Space moisture
unobservable
Research as from
2
high space
Technologies Mission
was
to Planet
(COSPAR), priority
they new
but should
to determine
what
Earth.
with
have
Along identified
technologies.
be developed
the These
to measure
global changeparameters. To determinethe technologyneedsaccurately,the scienceneeds,priorities, andrequirements must be def'med. Once the sciencerequirementsare specified, specific mission and system planningis thenpossible. The technologyreview teamidentified a lack of coherentarchitecture as hamperingtheir discussionof the Mission to PlanetEarth andGCTI's supportof it. "The committeefelt hamperedin their ability to assessOAET's GCTI plans becauseof insufficient mission andsystemplanning andanalysis." Adequatedefinition of architecturewas viewed as prerequisiteto their addressingmany technologyissues. NASA however, has had a basic assumptionthat full implementationof Mission to PlanetEarth will includeplacing observation platformsin GEO. This assumptionhasinfluencedNASA's selectionof key technologiesto be emphasizedin the GCTI. NASA's scientistsand technologistsfeel that a major advantageof GEOs for earthobserving platformsis the ability to acquirecontinuousobservationswith high temporalresolution,i.e., to be able to stare at a scene. Earth systemprocesseswhich require high temporal resolution observationsalso require high spatial resolution. Despite the substantiallygreateraltitude of GEOs over the orbits of the EOS and the Explorer-classmissions,the phenomenaobserved require the highest possible spatial resolution. This in turn meansgreaterrequirementsfor precisionpointing and platform control. Technology developmentsin precision pointing and vibration control for remote sensing instrumentsare important for the accuratepointing of multiple instruments and for large radiometric antennas. In the technologyreview teams' report they often used an 80 meter diameter antennaas a baselinefor evaluating the technologyissues. The goal of the GEO platform is to allow simultaneousandcontinuousobservationof theearthby multiple instruments with minimal interference. Advancedsensorsand detectorarrayswould permit remote sensingacrossthe electromagnetic specmamfrom the microwave to the ultraviolet. Three regions of the spectrum, the submillimeterrange(300 to 3000 GHz), the millimeter range(30 to 300GHz), andthe thermal infraredrange(5 to 20 microns),areespeciallycritical for understandingglobal climatechange. The region from 1 to 200GHz was cited as being particularly usefulfor metrology. The technologyreview teamalsoidentified a particular needfor large precisionantennas.They madethe following argumentsconcerningthe technologyneedsfor large antennasystems. "Largeprecisionantennaswouldenablemicrowavesoundingwith adequatespatial resolutionfrom geosynchronous orbit. Sinceit is estimatedthat abouthalf of the earth'srainfall occursin short-lived,small-scalestorms,resolutioncorresponding to the size of these storms (10 kin) is neededto provide complete rainfall monitoringdata. Observationsat 36 GHz with anearthfootprint of 10km require an antennadiameterof 40 meters. Theselarge antennaswould requireprecision shapecorrectionandsteeringto allow coverageof the globe,eithermechanically or throughreceiverarmyadjustments.Measurementsaboveabout36 GHz require solid surfacereflectorswhile lower frequencymeasurements can uselarge mesh reflectors. Unfilled aperture or interferometric techniquescould provide an 3
alternative approachfor the large antennasneededfor frequenciesless than 36 GHz. Special microwave-transparentstructuralmaterials may be necessaryto achievethe instrumentperformancerequirements. Array feedswill be required for effective offboresightpointing andscanning." Another related orbit
technology need Technology
environments.
developing should
and characterizing
include
subelements materials structures.
scaling
up
for large may
new and
platforms
the
High
structural
materials
characterizing
precision
not provide
Conclusions:
is advanced materials for both low earth and geosynchronous research in long-life materials and structures will be aimed
priority
promising
new
reflector
support
and
required
specific
items
for long-term
stiffness
associated
with
operation.
material
systems
structures;
into
1.3
LDA
Program
The NASA Concepts,"
and
thermal
stability
the
science
aspects
of these
Contract a program
for very
of the
for a Large
Deployable
application
of large
Antenna modular
(LDA).
The focus
reflectors
concepts/designs
for accomplishing
the mission.
components
Phase
and selection
and sketches.
this
which
the
II will consist
of a point design,
The specifications
effort,
possess
team
was
Virginia
The
charged
primary
Tech
expertise
implementation
made
mission
complete
with
objective
assembled
mission
of technology and vibration
a part
of the
identifying technologies of the LDA
suitable
detail
evaluation
Large
technologies,
of existing
hardware
specifications
the completion
of this
for follow-on
development
and
technologists
industry
and electromagnetic as well
technology
of critical
engineering
such that after
of university
readiness
(6 - 60 GHz)
Science Geophysical of the most feasible
and testing
procurement
structures,
to the focus program
and
is technology
frequency
the Earth definition
with preliminary
a team
in the areas of controls,
of these
wave
of the development
shall be of sufficient
has
of this effort
missions from oriented toward
task, these specifications can be used to initiate a new of a test article to demonstrate technology readiness. For
been
to millimeter
radiometers for future NASA Global Observation Platform (ESGP). Phase I of the program was to support
have
large
Task is entitled "Definition of Large Deployable Space Antenna Structure involving the detailed definition, assessment, and selection of conceptual
for
antenna
items
available
Objectives
designs the
All
structural
currently
included the passive microwave remote sensing which resulted in a number development needs, including advanced sensors and detectors, precision pointing controls, and advanced materials. Deployable Antenna program.
at
This research
technology.
as innovative
This
approaches
to
mission.
is to demonstrate
by means
of ground
test articles
that the technology is available for a large-deployable wide-scanning radiometer. To this end, the focus of the Phase I and II efforts is to develop concepts and configurations for such a flight article,
determine
the
state-of-readiness
technologies,
perform
articles
will demonstrate
which
can be specified
trade
in a future
studies
of the and
technology,
down-selection
the state-of-readiness RFP.
4
evaluate of alternate
and design
and
prioritize
technologies,
such items
to a degree
the
critical
select
test
that they
The test article(s)requirementsare straightforwardto determinewhen the objective of the test articles is kept in mind. It is necessaryto accommodateanticipatedmission requirements associatedwith the critical componenttechnologies. The plan for determiningthe test article requirementsfollows. 1.
Evaluateall the radiometerconfigurationsproposedby the EM Advisory Board Determine
.
.
the essential
ground-test
article
Beginning
with
NASA-LaRC, for each .
5.
critical
mission
Virginia
test article
component
architecture Tech,
technologies
specifications
the EM Advisory
component,
needed
performance
as
Board,
compiled
determine
criteria,
to be demonstrated
and
Develop
the technologies
As a starting adopted.
point,
Please
the following
note
article
that as the trade
studies
of the parameters
listed
presently
from
The
global
the
science
expended requirements
missing mission
to determine and
achievable
design
the list (e.g.,
control
been
the overall
objectives Because
upon
and
and designs there
parameters)
and
set.
of the radiometer of the complexity
specifications.
in turn,
1.3-1 begin
and
by
which
A great
will
circulate
selected
in (2)
Fig.
1.3-1
were
to appear,
that
some
are many
will be impossible
will be determined in a somewhat science and structural communities
requirements
who,
in Table
Likewise, related
agreed
goals
progress
and specifications
have
specifications.
hardware requirements the electromagnetics,
design
will be inconsequential.
requirements
requirements
that demonstrate
test
on
specifications
etc. Tech
configurations(s)
iterated
the design
Circulate the selected design specifications to Virginia to NASA-LaRC AMRB for comment and review test article
in a
must
parameters
instrument(s) of the instrument,
are
be added.
to f'trmly deal
that
determine
of
effort
and
until
is being
the necessary
the science
and
iterative fashion. Interaction between will be needed to achieve realistic and
I _,_Focal
Focal Length 60m
q.
./"7
Surface 0.1ram
Accuracy RMS
!
I_.. I-
Main Reflector 40m I_.
Diameter
1
_1 "-I Offset 40m
I y
Figure 1.3-1. Initial Test Article Requirements
6
Point
Table Test
1.3-1
Article
Design
Parameter
Goal
Frequency
Range
6 to 40 GHz
Bandwidth
Antenna Focal
Size
Consideration least two feed
for placement of at assemblies should be
given
6 to 40 GHz
to cover
Aperture)
1.0 to 2.5 (present Configuration
Offset
Dual
Reflectors
array
feed
40 m (see Fig. Surface
Reflector
GHz)
60 m
F/D
RMS
(60
40 m (Circular
Length
Antenna
Goals
Accuracy
goal is 1.5) with
an
1.3-1)
0.1mm
Surface
Lightweight
Membrane,
approx.
1 kg/m 2 Assembly
Deployable
Package
Volume
(Entire
Instrument)
Thermal Mechanical
Titan
Differential
IV (4.4
m x 15 m)
I00 °
Scan
As required
7
to achieve
scan
steering. Goal the mechanical
is to minimize motion of the
main
reflector,
subreflector
and
feed system
and
2.
MISSION
NASA
AND
Langley
September sensing
hosted
1988 issues
selected of low determine
were
vertical
water
of rapidly
evolving
vapor
events
periods
-
of the GEO
the antenna A resolution
system. From GEO very of 20 km is a long range
Without
that need
microwave
preempting
be a modest
A single
sized
from
antenna
from
out of reach
for quite
not
sensing
process
to feed
feeds
sometime.
of the
surface
GHz
(with
resulting
a hopeful
problem
designs
antenna
can
systems
Table
2-1
gives
design
from
1).
complete with
This in turn leads
global
scan
increasing
arrive
because
technology
6 to 220 GHz
characteristics
challenging Another
aspect parameter
to a narrower
(see
line
4).
can be tracked
based
of interest
mechanical
reflector
a
design,
large
especially
at the classes of the large
of antennas feed
network
microwave Also, there
from
Panel
concluded
that microwave
GHz).
be that
It may
turn
out
two completely
that
separate
and 60 to 220 GHz. of a 40-m
beamwidth large The
seems
and RF front ends is equally to an upper frequency limit of
to 60
or it could
6 to 220 GHz
diameter
circular
reflector
(see line 2).
number
required
at midband in electrical
Therefore,
of beamwidths wide
scanning
antenna. (see size
to accomplish
of scan
is required
is perhaps
the
most
of the design. to the radiometer
approaches,
Table 2-2, part a, gives physical b gives beam efficiency values smooth
upward
without
designer
is that of beam
efficiency
power in the main beam to that in the entire pattern solid angle). Beam efficiency by system configuration and surface roughness. Since surface accuracy is a strong of candidate
to
observations
For narrow beam types of reflectors.
channels
the EM Advisory
(+ 8.6 °) an increasingly
frequency
earth
events LEO
A 40-m diameter was selected because it results in a 20 krn ground resolution line 3 of the table). Note that as frequency increases the 40-m antenna increases (see line
been
is used
permit
is the radiometer
the necessary
6 to 60 GHz,
and
GEO
from
we can quickly
of similar
evolve,
goals
have
the reflector.
In addition,
be used
eventually
in
remote
beams are needed for ground resolution. This, of course, requires a large aperture
risk technology
to cover
extension
(GEO)
From
possible
components much above 60 GHz for use in the feed assembly distant in the future. Therefore, we have redirected our attention 40
6 to 220 GHz
the
orbit
as hurricanes.
narrow antenna goal at 6 GHz.
are high
used
with multiple
Platforms
meetings,
sounding
geostationary
such
remote
Arrays
array
Panel
Microwave
which introduces loss and noise problems for the radiometer. antennas, this leaves reflector antennas; there are, of course, many could
Geostationary
from
atmosphere.
something
the design
to be considered.
channels
precipitation
taken
At the heart
antenna.
the
and
data
meteorological
for long, continuous time constellation of satellites.
Frequency
through
These
Science
EM Advisory
Some channels are at atmospheric windows (frequencies surface observation, while other channels are off window
sounding
the atmosphere.
for Earth
and subsequent
discussed.
these parameters. allowing earth
temperature,
through
Workshop
At that workshop
for ESGP
for
REQUIREMENTS
the Technology
[2-I].
to observe attenuation)
frequencies
ANTENNA
feel for the numbers
must
distances for two electrical lengths for typical reflector illumination
and the same random
on the null locations
a basic
surface
for the smooth
error cases.
reflector 8
(M.C.
The beam Bailey,
(the ratio
of
is affected determinant
be introduced
early
on.
of RMS surface errors. Part for the cases of a perfectly efficiency
NASA
LaRC).
calculations Remote
were sensing
engineerswould like to haveabout95 percentbeamefficiency [2-1]. The tablerevealsthaton the order of X/50 surface accuracyis required which is about 0.1 mm for our 40 (60) GHz antenna. The parametervaluesfor the baselineantennadesignshownin the previouschapter(Fig. 1.3-1) were arrived at from remote sensingrequirementsdescribedabove,constraintson technology developmentin the future, subcontractorreview, NASA input, andEM Advisory Panelreview. The dual offset reflector with an array feed is not "the" design,but one which is rather simple in structureand hassomeevidenceof providing electronic scancapability. Table 2-1 Design Goal andCharacteristicsof a 40-meterReflectorin GEO Frequency 6
10
18
22
31
60
Main Reflector (wavelengths)
800
1,333
2,400
2,933
4,933
8,000
Half power beamwidth degx 10.2
8.16
4.90
2.72
2.22
1.32
0.82
Ground resolution(km) (23dB beamwidth)
60.2
36.1
20.0
16.4
9.7
6.0
Beamwidthsof scanfor
+105
+175
+316
+388
+652
±1054
1.00
0.60
0.33
0.27
0.16
0.10
+8.6 ° Surface error required in mm for k/50 RMS
Table of a 40-meter
Characteristics a. RMS
Surface
f I
Reflector
Antenna
Error _,
(GHz)
2-2 Circular
_./20
(mm)
I
_./50
mm
mils
I
mm
mils
6
50
2.50
98
1.0
39
37
8.1
0.41
16
0.16
6.4
50
6.0
0.30
11.8
0.12
4.7
220
1.5
0.075
3.0
0.03
1.2
b. Beam
Efficiency
Smooth Reflector 98%
L/20 Surface Error [
-70%
_./50 Surface Error [
-93%
3. REFLECTOR CONFIGURATIONS
FUNDAMENTALS
Conventional
design
antenna
developed design,
for (3)
the
consists
application
Mechanical
of
at hand
design
AND
these
CANDIDATE
steps:
(1)
(communications,
and
construction,
Performance
radar, and
(4)
specifications
or radiometry),
Measurement
are
(2) Electrical of
electrical
and
mechanical performance. This is a serial process with each step being completed before the next. In this project these steps have not been performed in a serial fashion. The research and development and
effort
mechanical
has been
designs
ongoing
were
while
performed
remote
sensing
at the same
requirements
time.
This
evolve.
was
nature of the program; it is complex and pushes the state-of-the-art components. This requires that the steps be performed iteratively. That implications of a particular electrical must be relaxed or electrical design This
section
antenna
3.1 The
identifies
design
was
reflector
configuration changed.
reveal
fundamentals
and
an inferior
candidate
electrical
because
of the
in many technology is, as the mechanical
design,
remote
configurations
sensing
from
goals
which
the
initiated.
Overview ESGP
antenna
design
design
problem
holds
that are most
many
challenges
challenging
elements
associated
antennas. Therefore, the design launch and long life in space.
then
for wide scanning. Scanning can, of course, be accomplished assembly, as is usually done on the ground. However, mechanical in space. is required;
experiments
that require
Figure
illustrates
3.1-I
a stable scanning
is that it provides
waves. 3.1-1c)
The reflector merely a parabolic reflector
rapid
However,
performance
efficiency
the reflectors
fundamentals.
no focusing
for waves
is lower
and
a large
arriving
from
such
as gain
degradation
array
directions loss
and
offers
feed
the incoming a plane wave
but with the poorest It focuses (but not
than
of Fig. 3.1-1
in the
process
must
design
be
of large
by slewing the motion creates
other
undistorted
is required
waves. arriving
to collect
The
the arriving
At the other extreme (Fig. parallel to the axis of the
than along
pattern
scanning.
the axis of the parabola,
distortion
scan properties. to a point) and
occurs.
The
parabola
The spherical reflector has scan capability. Its
that of the parabola. scanning
motion.
antenna
Electronic
feed).
trade-offs
A flat reflector
acts to redirect sharply focuses
case of no main reflector (or array
fundamental
the
scanning.
platform.
offers the best aperture efficiency of Fig. 3.1-1b is a compromise. aperture
the
with
wide
Drives and controls are required. Momentum compensation for this is a major problem on ESGP which also carries laser and other
penalty
reflector.
in mind
two
space entire
many problems antenna motion
dearly
the
size and ii) its required
It is important reflectors reflector
to have
but
are: i) its large
These would also be challenges for earth-based tempered with a goal of simplicity to facilitate
With
Also,
necessary
The
offers instantaneous beam positioning can be avoided by switching between
is achieved most
scanning
elementary (either
in the ways method switched
and even multiple beam fixed feeds as illustrated 10
illustrated
in Fig. 3.1-2
is to physically or phased)
move
for the the feed
is the alternative
that
possibilities. Mechanical motion in Fig. 3.1-2b. A full array feed
a) Flat reflector:
b) Spherical reflector:
Full scanning, no focusing
Figure
3.1-1.
a) Movement
Figure
(Fig.
3.1-2.
3.1-2c)
Scanning
of Reflectors
of the feed assembly
Implementation
b) A switched feed
of Scanning
solution
without
(assuming
full
spectrum
mentioned approach We are,
above, illustrated therefore,
configuration. reviewed.
of scanning full
methods
mechanical
Movement
available
slewing
is no clear
cut
answer
represented
is to be avoided
11
the appropriate
to compensate
are
to our
of the Main Reflector
in that
weighted
in Fig. 3.1-2 will require a very left with using a hybrid approach
There
c) Full array feed
no motion)
elements can be properly amplitude and phase well as main reflector surface distortions). The
Limited scanning, focused
Partial scanning, partial focusing
Properties
is the best
c) Parabolic reflector:
for scan degradation
in Fig.
if possible.
large array and or with finding design
problem
3.1-3. The
associated a clever in the
For
(as
reasons
electronic-scan feed network. electronic scan
literature
we have
Electronic
Mechanical
complexity
complexity
Only electronic scanning
Full slewing of antenna system Switching of feeds in under illuminated
Mechanical movement of feeds or
Mechanical movement of feeds and
aperture
subreflectors
subreflectors
Hybrid electronic/mechanical
Figure 3.1-3.
3.2
Main
There
The Trade-offs
Reflector
are a few
summarize
plane
waves
properties The
Shapes
classical
of Fig. 3.2-1
(the
focal
are summarized
parabolic
torus
of
Fig.
3.2-2
spherical
reflector
than
plane
cylindrical
which
scanning may resolution.
reflector aperture
has
along
reflector
of Fig.
because
use.
it focuses
to high gain (high
circular
3.2-4
has
array
been
aperture
In this section
incoming
aperture
a straight
feed along
used
by feed
we
(on-axis)
efficiency).
azimuth
cross-section the axial
Arecibo
displacement. larger
and
multiple
simultaneous
in applications the
with a reflector
12
in
efficiency
and separate
has
example,
scan
associated
circle
3.2-3
A linear
For
cross-section
of reduced
of Fig.
achieves
the costs
a
the focal
efficiency.
is stationary be worth
are in common
popular
This leads
the penalty
parabolic cross-section in elevation. steered to scan the beam.
important
that
is the most
point).
With
be placed in the azimuth obtained from each feed.
The
shapes
Scan
on the figure.
in elevation.
parabolic
reflector
types.
reflector
to a point
cross-section
The
main
the fundamental
The paraboloidal
in Scanning Reflector Antenna Systems
beams
may
can be
in azimuth
focal
and
line can be phase
where
1000-foot
parabolic feeds
scanning diameter
Potential than a paraboloid
for
is more spherical wide
angle
for the same
Y
Parabo
X
(Q_I¢) Civic
•Scanning
in
displacing
feed
the focal • Phase gain
point errors
AZ
and
may
however, arrays
accomplished
switching)
in the
by
linearly
plane
through
F. induced
loss and pattern
-Arrays
EL
(or feed
be used
this requires
in the aperture
during
scan
cause
degradation. to correct amplitude
3.2-1.
in AZ accomplished
switching)
along
gain aperture
phase
and phase
errors,
weighting
reduction
•Scanning
and
paraxial
or beam
phase
by feed movement
focal
arc with no scan
(or feed induced
degradation.
in EL identical
•Cylindrical
can be large.
Figure
•Scanning
to parabolic
errors
in
case.
AZ
plane
degrade
performance.
Paraboloidal
Reflector
Figure
3.2-2.
Parabolic
Torus
EL
AZ
AZ
• Scanning •Undistorted a linear •Scanning Figure
scanning
array
in AZ accomplished
(or feed
feed.
in EL identical 3.2-3.
by phase tilting
Parabolic
scan to parabola. Cylindrical
induced
• Spherical Reflector
Figure
13
in AZ and EL accomplished switching) gain
phase 3.2-4.
along reduction errors
Spherical
paraxial
or beam
degrade
by feed
focal
degradation.
performance.
Reflector
movement
sphere
with
no
3.3
Candidate
After
an extensive
Configurations literature
reflector
antenna
represent
the range
development, of possible
scanning 3.3-1.
methods
with
the
search
accompanied
several
candidate
configurations promise
configurations
available
of wide
scan
Table Candidate .
Switched
Partial
Dual
2.2 Array-Fed 2.3 Cylinder .
Electronic 3.1 Dual
Diagrams
of the configurations
companies
were
selected.
all reflector They
are
Feed
Corrected Torus
Type
Electronic
Tri-Reflector Dual
Reflector
Scanning (Foldes
Reflector
with partial
2)
Spherical
(Foldes
Type Type
1) 3)
movement
Scanning Parabolic,
Array-Fed,
3.2 Array-Fed
Dual
3.3 Array-Fed
Cylindrical
are given
Reflector
in the following
14
Gregorian (Foldes
Type
Reflector 3)
Reflector
figures
(Figs.
The
summarized
Reflector (Foldes
involved
shapes
3.3-1
Mechanical,
2.1 Array-Fed
capability.
or Moveable
1.2 Tri-Reflector 1.3 Gregorian 1.4 Parabolic
including
with
Configurations
Feed
1.1 Bifocal
.
by contacts
3.3-1-10).
with
candidates
and different in Table
o
.o_ LU_O
t--
•-_
_
rr
05 [..-
o -.--. tO.
0 OJ
0 ¢_ r.-
ea "-a
.--
¢00g
o 0
ON c-
o °-0
0
_r-
n-
.__8 i.k¢_
E
_
o
_
0
_
'_
L,L
m
c_
"0
0
r"
0") °
°
_>
g_
0
0
,-'-
• 0
15
--
U.
16
1?
._=_
o
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E
_
0
0
.o _
_
E o _
_E o
_ ._ o
0
0
0
"l_
= o
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} •-=
ogo _
___o_ _ 0.
18
..Q "13 0 t--
0
._o _. mE
,-. 9
o
t_
_8 o_
-
_
°
[
.__-_ _ .=- >o.
e_
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8o
•
19
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_ _ _
0_
o O3
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.__ 14.
4.
DESIGN
4.1
PERFORMANCE
I of the "Definition oriented
towards
the objectives
definition
will discuss
Technologies
considered
surfaces,
to the more
Many
of
the
inclusion
range
technology
evaluated
been
4.2
The
Phase
or further
been
LDA
configurations.
a LDA
evaluated
design
goals
listed
that
antennas.
based
upon
This best
in Table
reflector
their
is to say that
utilizes
its unique
1.3-1.
In the case was the
approaches to accommodating large deployable space warrants further study and will have utility in future into
Trusses
I LDA
Truss
Technology
study
has progressed
for precise
for the
approach
membrane
have
into
for the LDA.
and furlable
studied.
support
Overview with
of a reflector
semi-rigid solid surface. One may ask for reflector surfaces are often integrated is used
inextensible
by the design
an instrument.
considered
i.e. pactruss
chapter
included
such
However, not all the technologies described in this chapter will be carried of the specific performance requirements as described in Chapter 1.
Deployable
required
designs
has
was judged not to meet the stated performance requirements an attempt the maximum size of the antenna or component that would enable
Deployable
4.2.1
and physical
program
for accomplishing
to support
of conceptual
and is judged
to be utilized
missions. II because
Concepts"
concepts/designs
technology
state-of-the-art,
in this
designs
Smactures
antenna
i.e. practically
This chapter contains several novel design structures. In each case, the technology space Phase
feasible
current
discussed has
Antenna
the existing
concepts,
physical
of interest
the technology to determine
from
exploratory
characteristics
Space
of the most
and evaluating
technologies
technology
Deployable
the technologies
in preliminary
performance where made
of Large
of the LDA
This chapter
each
EVALUATION
Overview
Phase been
AND
small
solid
is attractive
used at extremely dishes by hinging
dishes
Hexagonal
Panel
and the resulting
[4.2-2]
panel-only,
concepts
on
that an area
is composed
communication
structure Ingenious segments
concepts
that
if a truss is even necessary, with the reflecting surface
flying
high frequencies. between adjacent
the assumption surface
shown
structure
will be rigid
or
since supporting structures itself. Indeed, this approach
satellites.
can be made
truss
of a segmented
The
dimensionally
simplicity stable
of this
enough
to be
concepts have been devised for deploying larger as in the TRW Sunflower [4.2-1] and the Harris in Figs.
also use well established
4.2-1
fabrication
and
4.2-2.
techniques
Integrated-structure,
and appear
or
to be of low risk.
They are, however, structurally "thin," so that small fabrication or thermally induced errors in individual parts grow into large distortions for large sizes. In addition, such structures are difficult
to test in a one-g
produce
deflections
It is therefore component measurements The
difficult
parts
experience
environment.
that are large
to passively
with enough
obtained
during
and information
Their
flexibility
in comparison achieve
precision ground obtained
to those the
desired
or by "trimming"
combines
with
acceptable
for the present
accuracy,
the gravity
either
the structure
by
loading
to
application.
fabricating
by adjustments
the
based
testing. by studies 20
and
tests over
the past two decades
have
on
_4s-- i
Deployed Figure 4.2-1. TRW Sunflower
Stowed
Deployable Reflector Concept
11
Figure 4.2-2. Harris Hexagonal Panel Deployable Reflector Concept
2l
shown
that
structural
high-precision
configurations
surfaces
than
this notion intuitively achieved with careful constructed
from
2-meter
struts
showed
an expected
had
surface
error
by testing should
in a one-g
be able
Numerous As
field
concepts
previously
for remotely
a deep-truss
support
efforts;
panel
Single-fold package
the robustness
segments
length,
poses a severe breakdown and surfaces Dynamics [4.2-11-15].
to nest,
truss
with
by a robot.
Another individual shown periphery using
a robot.
possible, One
precision that have
for
worst
of 20
of 100 cases
of the deflections
100 micrometers;
been
flew
gravity
with solid
devised
caused
compensation
reflector
for deploying
integral
surfaces large
but structurally
on the SEASAT
simplified
has been studied This arrangement
thereby
saving are
exist.
dishes
thin support.
spacecraft.
The
10.75
double
are
surface,
intelligent would
only
meter
the
deployable
Research
modules require
of the fact
truss
surface
has
for achieving
than
the
vehicle
available
configuration.
in both directions.
been
demonstrated
this is proposed
This
by General
that
and some each
aid in control
which
is
later
can be assembled Center
being
canister locking effort module
in the report.
to the deployed
on such robotic
reflectors in remote its associated support
in a deployment
would
and testing.
and by Martin Marietta with the Box Truss doubly curved panels onto a deep support truss
at Langley
would
smaller
on the launch
and the panels
deploying
hinging
diameters
the reflector
large segmented of a panel and
canister
for
structures
a concept
stowed
integration
truss geometries are notoriously difficult to attached. Stowage of flexible mesh reflector
truss
separately,
analysis,
was by
volume.
depending
to divide
fold
be made The
by One
for possible use with reflector antennas. One has the advantage that it allows the doubly
package
useful
is in progress
These
to its neighbors.
concept
variation
is supported by a deployable truss. A feature of this truss is that the radiating panels are stowed and deployed while
can be stowed
4.2-4.
Use
The
analysis
antennas
have
however,
Research
of this
large
Not only is
of magnitude.
10 to 15 meters,
deep,
of the reflector
development
with
error of 43 micrometers.
or panels
concept for constructing modules, each consisting in Fig.
lengths
error of about
it will be necessary
truss
for
7].
an RMS
using their Geo Truss [4.2-8-11] Autonomous deployment of rigid,
supporting
suitable
random
concepts
concepts
has yet to be accomplished, The
more
4, 5, 6 and
that very high precision is tetrahedral-truss structure
problem because double fold stow with rigid reflector panels
integrally
much
[4.2-3,
analyses have shown of a 20-meter-diameter
of the configuration
approximately
reflectors,
are
Refs.
This structure, which supported an L-band antenna (7L = 20 cm) 2.5 mm maximum deflection. This was achieved and demonstrated
truss-stiffened
For larger
"deep" See
Furthermore,
structure
A similar deployable truss concept of these is shown in Figs. 4.2-3. curved
surface
aperture radar antenna to the LDA application
to the truss. to better than
careful
RMS
deploying
several
with
have
an RMS
segments
long synthetic that is crucial
which
that by an order
adjacent
antenna
attached accurate
showed
mentioned,
between
are ones.
of 72 micrometers.
to decrease
hinging
"thin"
obvious, but also detailed fabrication. A simulation
micrometers, an RMS
that
are the
which each but
moves
around
to its neighbors. seems
would
the The
to be easier
be hinged,
of the canister extensively
assembly.
locations employs truss section. It is
than
so far as
motions. studied
for
various
high-precision applications is the Pactruss shown in Fig. 4.2-5. The deploying truss in this concept is very strongly synchronized and offers reliable deployment with a few actuators. The design
of the Pactruss
is flexible
in that its geometry 22
can be altered
to make
it compatible
with
i
Stowed Figure 4.2-3. Synchronously
Deployable Concept
23
B (Crest) for Stiff Panel Reflectors
Figure 4.2-4. Sequentially
Deployable Segmented
various
geometries.
types
compatible The
with rectangular
triangular,
This version parallelogram Figure
4.2-7
double-fold
of reflector or more
depicts Pactruss
stiff panel
correctly,
is compatible units on the
The
segments.
segments
form
Pactruss The
the geometry of the truss which hybrid
of the Pactruss,
or flexible
the paraUelogram
with surface
a hybrid
square
Reflector
form
strips
shown
of furlable
of the Pactruss
in Fig. 4.2-6, reflector
is shown
is composed
of six single-fold will stow around
PACTRUSS
i0
f,
,
f,,
Y U[|_UYI
panels in the
radial
beams
a central
if the figure. and six
body
_0 t_ll'
)t_w__
°
I_AN VI[W
24
I!._
I_ I'l AN V IL W U| i't IIyI
Figure 4.2-5. Pactruss Concept with Triangular Form
such
CONCEPT
0
PARIIAII
material.
in Fig. 4.2-5.
of hexagonally shaped stiff are tilted 60 degrees as shown
configuration
is
D
51t)Wt'i)
_o
Elevation
View
Perspective
View
Figure 4.2-6. Views of Pactruss for Offset Paraboloid as a feed
structure
or cryogenic
for descriptions 4.2.2
Ring
Several
of recent
Truss
types
which are held reported below. The
inflatable
a rim
that
torus
very
reliable.
sandwich
technology composite [4.2-18]. Inflatable viewed suitable
balloon, with
of precision
have
structures, as being materials needed
difficult
to "tune
Another
ring-type
wheel. As shown by stays or spokes.
while
is not a truss Examples which
ring
The
Mylar-film
being
vigorously
for very up,"
even
structure
See Ref. [4.2-16]
sheets
and
forces.
of membrane
Some
the reflector include
by
slow
the ECHO
in the space
age.
an aluminum
during
ground
that is capable
stow
without
in a radial
for lower
In addition, testing.
passive
core.
More
foil
frequency
inflatable
Adjustments
of supporting
was developed
fashion
inflation was
antennas,
are
with and
is
satellite,
a
composed recently,
antennas, in orbit
a membrane
and 25
are
by Astro deployed
once
seem
reflector
fabricated,
are
to be impossible. surface
is the wire
that is deployed state to provide
utilized
for Rockwell by
are generally
herein. The available coefficient of thermal
The folding ring approach has been at Langley Research Center.
wires
surface
Its shell
in Fig. 4.2-8, the wire wheel is composed of a folding ring The spokes also load the ring in compression in its deployed
ring
designs
since the early 1980s developing a Kevlar-epoxy on orbit after inflation. See Refs. [4.2-17] and
promoted
high precision.
reflectors
of these
membrane
inapplicable for the high frequencies being considered lack the long-term dimensional stability and super-low
folding
segments
early
support
is deployed
trusses
launched face
support
assembly
of inflatable was
for the
by distributed
but it does
load.
the appropriate stiffness and precision. of the hoop-column antenna structure A deployable
with hex-panels.
applications.
developed
work in Europe has been underway surface which is cured and hardened
expansion
The
been
configuration
a compression
100-foot-diameter of a thin
proper
type
and is compatible
Review
structures
in the
carries
intuitively
evaluations
Technology
of ring
equipment,
in the design
in the late 1970s.
a circumferential
scissors
252 Nodes 1014 Struts 264 Redundants
Stows around a central body
/
/
Pactruss
Singlefold beams
Each beam and Pactruss sector is unique for an offset configuration. Figure 4,2-7. Five Ring Hybrid Pactruss mechanism. launch 4.2.3
The
vehicle Evaluation
A simple
ring
payload
segments
space
flame
structures
which
can
be no longer
than
the
bay radius.
of Deployable
two-dimensional
are
analysis
Truss has been
performed
26
to estimate
the structural
depth
that wiU
be required for the 40-meter-diameter LDA configuration to passively maintain the required accuracy. The derivation of the equation used for this analysis was based on the lattice rectum equation
for the rise
height
of a shallow,
circular
arc.
The
f'mal form
of the equation
is:
AEL _ h -- -_
(4.2-3)
8(zXS)
where:
h is the beam AS is the rise L is the length AE is the strain
(truss) height
depth
of the arc segment differential between
the outermost
STOWED
0RUM
J,
surfaces
of a beam
ROTATION
°°* *// HIM
HINI;t
UPPER
RIM
TUSI¢
_
NN_,
(truss)
.."
_
STAY
GORE
LOWER STAY
PARTIAl.
. LOWER
DEPtOYMENT
STAY
'_R
)
RIM
TUmE
_
RIM
Figure 4.2-8. Wire Wheel Schematic
c_n. 27
STAY
For the required LDA shown that a specific deviation
from
the
configuration, RMS accuracy ideal
approximately valid localized undulations
feature
A8 can be set to 0.3 mm. This is because experience has (0.1 mm in this case) can be achieved if the maximum is approximately
whether the deviations of the surface.
three
are
due
times
to gross
the
RMS
changes
value.
This
in curvature
Shown in Fig. 4.2-9 is the relationship of the strain differential Ae to the depth, h, for the LDA to maintain a maximum deformation Ae of 0.3 mm.
required
is
or more
structural
40
35 30
25 40m Truss Depth H, m; 20
15
10
selection of truss depth of approximately 3.3 meters. _
5 _1
Microstrain
limitation imposed
by
I
I
I
I
I
I
I
I
10
15
20
25
30
35
40
45
0 0
5
Ditferential
Strain Through
50
Depth, Microstrain
Figure 4.2-9. Truss Depth and 4.0 m Panel Thickness vs. Microstrain to Limit A_ to 0.3 mm
The value of AE that is chosen represents the maximum through the depth of the structure for any reason. This maximum thermal length errors, and microstrain extensive stated structural
LDA
depth
differential that is anticipated will be a combination of the
distortion between the truss front and back, fabrication imperfections such as scatter in the CTE of the composite material. Experience has shown that 5
is a reasonable thermal insulation
in the
strain value
value for Ae, although achievement of this value may require of the structure due to the 100°C maximum thermal differential
baseline
requirements
is approximately
list.
With
the
maximum
Ae set
to 5 microstrain,
3.3 meters.
Therefore, the structural configuration required is a truss with a minimum depth of 3.0 to 3.5 meters. This depth is required to insure that the LDA requirements for passive accuracy control can be maintained.
A mass of this depth
will be composed
4.4-meter-diameter
of the
launch
convenient
STS
or Titan
vehicles,
for packaging.
28
of members which,
that are shorter
incidentally,
than
will prove
the
to be
4.2.4
New
New
Truss
truss
Concepts
concepts
generated.
for
that
one new
compatible
with
truss
has been
panel segments, furlable reflector surfaces.
semi-rigid
reflector
As explained in Section 40-meter-diameter LDA
4.2.3, a truss configuration.
highly
At least
are
the LDA
articulated.
Such
achieve
high
payload
dimensions
a doubly
a structure
reliability.
curved
The
truss
of the Titan configuration
be used to create
high
double-fold
stiffness.
a variety
4.2.4.1
Truss
studied
in some
PSR capacity,
depth
strongly folded
current
as part
rigid
membrane
type
during
vehicle.
elements
of the reflector.
concepts:
depth is required that the structure
its diameter
Finally,
for the will be
deployment
exceeds
It must such
been
to
all of the
also deploy
as standoffs
into
need
the truss should
not
be very
sections, are, in general, based on the Pactruss. satisfy the needs for reliable, highly synchronized deployment
is very
flexible
into
doubly
curved
in that its geometry
area
trusses
is readily
and
altered
to
geometries.
for a Segmented,
the Pactmss
launch
have
precision.
geometry,
the Pactruss
reflector
for one-piece
synchronized since
structural
in the following to simultaneously
of reflector
Concepts
be very
for support
packaging
requirements
for each of three
and a ring truss
be doubly
of the proper
In addition,
accommodate
must
performance
of 3.0 to 3.5 meters characteristics dictate
IV or any other
shape
achievement
The truss concepts, described The Pactruss can be designed deployment,
strips
structure These
must
LDA
conceived
so that additional
a parabolic
stiff to promote
the
Rigid
of NASA's
supports
Panel
Precision
hexagonaUy
LDA
Reflector:
Segmented shaped
The
Reflector
reflector
Pactmss
(PSR)
panels
has
program.
of optical
been In the
precision
on
three points. This panel configuration dictates a triangular Pactruss geometry such as that shown in Figs. 4.2-7. The PSR approach to attachment of the hex-panels to the truss, however, requires extravehicular
activity
Hexagonally One method 130 or more
for deployment segments
be
Due to the limitations 40-meter LDA accordion-folded meter
A concept
with
robotic
was
assembly
techniques.
and
would
be
Pactruss are
for deployment
shown
in Figs.
panels
to fill
meters
approach
have
been
A minimum the
into five rings in diameter
The depicted
chosen
and
of the
task might
more
in Figs.
4.2-5;
for further
Rectangular into the surface of 13 rows
40-meter-diameter
that are appropriate
4.2-10
panels
deployment 4.0
be staggering.
canister
reflector panels. rows on tracks built
configurations
of square
would
in Fig. 4.2-6.
required
be about
to be too complex.
rectangular
segmented into long
Additionally,
will
mechanized
also considered
such as that shown
geometry
truss.
panels complexity
the
of hex-panels,
panels
conceived
since
mechanical
with rigid, and deployed
Pactruss square
rectangular been
The
accomplished
this approach
geometry
onto a backup
is required
is 40 meters.
reasonably however,
or advanced
shaped panels do not readily lend themselves to autonomous deployment techniques. has been described in Ref. [4.2-2] and is shown in Fig. 4.2-2, but this approach is
not appropriate aperture
by Astronauts
of the
panels can be of a rectangular
and columns
LDA
for the LDA
study
aperture. requirements
of 3.1 Two have
and 4.2-11.
onto the truss
29
is shown
in Figs.
4.2-12(a-d).
This
o |
o.- = 0 O.
0 U.,.
/
/ u.O
,_,
'5 0-
0 U.
u.O
3O
deployment width must Fig.
concept is however not appropriate be less than the payload maximum
4.2-12(a)
is rotated
90 degrees
for a 40 meter aperture, diameter of 4.4 meters.
so that a larger
panel
stack
because the panel stack If the package shown in
height
is possible,
the stowed
• 6 x 6 Bay Paclruss support structure slaown
Accordian-lotdeO
l
panels
• 6 x 6 Rigid Panel Array Pactruss wilh an alongalsd
configuration
Plan View
Figure 4.2-12(a).
Square
panel deployment
concept
- slowed
Elevation
• 3 bundles
of 6 panels
attached
Figure 4.2-12(b). Square panel deployment
to Pactr,
JSS surface
battens
concept, partially deployed
surface Iongerons Deployment
tracks along
X
_
Panel bundles rotate 90_
\ Elevation
Figure 4.2-12(c). Panel deployment
concept, Truss deployment 31
complete
Pactruss
is then limited
to less
than the allowable
2 times as long as its deployed will be utilized more efficiently The
concept
Deployment 4.2-12(b). lined
provides
diameter.
A stowed
Pactruss
is about
depth. If the panels are rectangular, the payload cross-section and the panel stack height limit is the length of the payload bay.
the possibility
of truly
autonomous
deployment
with
relative
simplicity.
of the Pactruss synchronously unfolds the bundled rows of panels as shown in Fig. Once this is accomplished and the Pacmass is fully deployed, the bundled rows are
up along
one edge
to be perpendicular unfolded
payload
of the truss,
to the
accordion
style
truss
in tracks
panels
face
parallel
as shown
on the truss • Simultaneous • Sequential
deployment deployment
to the truss in Fig.
face
as shown
of all rows of two
rows
face.
4.2-12(c). in Fig.
They
must
The
panels
then
be rotated
may
then
be
4.2-12(d).
shown at a time
is an option
Figure 4.2-12(d). Square panel deployment concept, Reflector deployment Figure
4.2-13
shows
panels
in the launch
how vehicle.
the Pactruss Although
would
be stowed
autonomous
separately
deployment
from
the
3.1 meter
of this configuration
is probably
3.1m
2,0 m
Rigid panel reflector surface 145 panels 3.1 mx3.1 Paclruss 4.0 cm diameter
members
4.4m
IE = 15.3m
Figure 4.2-13. Primary Reflector Stowed on Titan IV 32
square
m x 6.0 cm
impractical,
the figure
illustrates
that
a 40 meter
diameter
rigid
paneled
primary
reflector
with
6.0 centimeter thick panels will fit into a Titan IV with little volume remaining for other constituents of a complete radiometer space craft such as the secondary reflector, feed and feed support
structure,
panels would of 145 panels
bus and
solar
arrays.
Composite
Optics
has
indicated
that
3.1 meter
require a shell and rib structure of about 12 centimeters thickness. 12 centimeters thick alone exceeds the maximum payload length
the geosynchronous launch capability. Obviously, a 40 meter diameter segmented, instrument will not be feasible until one of the following situations applies: New
.
launch
2.
Orbital
3.
Materials
4.2.4.2
Truss
vehicles
assembly
such
from
several
with several Concepts
as HLLV
orders
for
originally conceived by Composite a cigar-shaped bundle for stowage. 40-meter-long deployment. The
strips
rectangular
launch
Pactruss
vehicles
is deemed
greater
panel
Reflector
acceptable
swain
Strips:
The
accuracy/stability
are available.
furlable
concept
reflector
Optics, Inc. (COI) as a one-piece dish that can be rolled For the LDA configuration, the reflector must be cut
that can be rolled
geometry
rigid
are available
of magnitude
Furlable
square
The stack height of a Titan IV in
onto parallel
designs
tracks
described
built
into the supporting
in the previous
section
truss
and
was into into
after its
shown
in Figs.
4.2-10 and 4.2-11 are appropriate for the deployment of long, narrow, furlable strips. The rectangular truss configuration, however, requires that each furlable reflector strip have a unique figure whether it occupies a row or a column in the surface pattern of the truss. It would be desirable aperture. strips.
to have only one type of furlable strip, such as a gore, that is repeated throughout the Therefore, only one mandrel would need to be made for fabrication of all the furlable
A plan view
of a gored
truss
geometry
for an offset
aperture
is shown
in Fig. 4.2-14
The
truss
would be made from adjacent tapered beams that are identical except in length. The long edges of the beams radiate from the apex of the parent parabola. The design of a gored truss is aided by an aperture
geometry
that is significantly
together to one point at the apex. geometry; however, other geometries gored approach to deployable truss Stowage
of the Pactruss
with
furlable
furlable
packages
can be attached
vehicle
as shown
in Figs.
4.2-15.
offset.
This keeps
the truss
It may be possible to design may be found to be appropriate design. strips
is much
to the outer Figure
more
longeron
4.2-15
efficient
struts
depicts
which
furlable
edges
from
converging
such a truss using Pactruss upon careful review of the
than
with
rigid
stow vertically strips
that
panels.
The
in the launch
are one
truss
bay
wide. When the truss is deployed, the bundles of furlable strips end up in the proper position for deployment by rolling out onto tracks or ruling surfaces built onto the truss face. More detailed concepts for actual deployment forthcoming sections of this report. 4.2.4.3 designed PacRing, precision
Ring using
Truss
Concept
Pactruss
of
for a Membrane
geometry
and is shown
furlable
Reflector:
strips
A new
in Fig. 4.2-16
like the Pactruss, is highly synchronized during without the guy wires or spokes often associated 33
onto
concept
a
truss
are
for a ring
with its deployment deployment and with ring trusses.
discussed
in
truss has been sequence.
is capable
The
of high
Furled reflector (typical, others
gore not shown)
._..,
1.7m • Truss • Fuded
Figure
4.2-14.
Gored
Truss
Plan
with identical reflector
View
tapered
gores
beams
of different
roll out towards
aperture
lengths axis
Concept
A
I 4.4m
Furlable Pactruss 4.0 cm diameter
reflector
surface
12 bundles o! reflector strips 3.5×40 m
members A
L Figure
4.2-15•
Primary
-,e--35 -=, 18.3 m
Reflector
Stowed
on
Titan
IV
34
m7.0 m
! Figure 4.2-16. Pacrlng Support for Deployable Membrane Antenna 4.2.5 The
Selected
Radiometer
conclusion
radiometer
of the
can achieve
studies of the rigid within a Titan IV.
reflector
paneled
parametric
studies
described
in Section
4.2.4.1.
within the other constraints configuration, when stowed
4.3
bay.
The deployed
Reflector
4.3.1
Rigid
Configuration
studies
the required
Therefore
payload 4.2-18.
Structural
by the
surface
configuration
were
is that
that a 40 m diameter
with
determined
contractors
only
for the 40 m diameter
concluded
conducted
It was
various
precision
the rectangular that
aperture
paneled
the maximum
a rigid
aperture.
aperture
mass
paneled
Packaging will not stow
configurations
diameter
possible
of this study is approximately 28m. The maximum aperture with the feed and secondary, occupy about 14m of the Titan IV radiometer
is depicted
in Fig. 4.2-17
and
it is shown
stowed
in Fig.
Surfaces
Facets
Various
concepts
surfaces
commonly
for large
deployable
used are either
antennas
a continuous
(LDA) mesh
facets. For upcoming remote sensing applications, frequencies on the order of 40 GHz are desirable.
been
developed. of rigid,
Two
deployable
continuous
surface
reflector apertures of up to 40 meters and For these targeted frequencies, mesh surfaces
have inadequate reflectance characteristics which drives Surface accuracies for adequate performance at 40 Ghz
35
have
or an assembly
the design to a continuous solid surface. need to be on the order of. 1 mm RMS.
Focal
Point
i
÷/
l! I
I !
!
I
I 42 m
÷
i L
\Ve_ex
Flgure
4.2-17•
28 meter
LDA
radlometer
spacecraft
structural
36
Concept
--!
I
i-- H
=0.6m
=13.7m
9.5m
t 1.6m
4.4m _ 1.15m
I'
Figure 4.2-18. 28 meter radiometer structure stowed In Tltan IV
37
Composite four types. 1.
Optics
The
has manufactured
single-surface,
Communication
Spacenet,
Kevlar
Satcom,
and
graphite/epoxySizes
of these
from
2.5
to 6.1 kg/m 2.
produced accuracies
The
receive
used
and
used
that are of the following
as used
on the
master
mold,
After
reducing
for lay-up
this
from
type
from
subreflectors
with
1.0 to 3.3 meters
manufacturing
which
a
support
rib
accuracy
induced
reflective structure
Ford
with
continuous
skins is also
thermally
Compare
honeycomb this
design
shell bonded approach
.015"-thick graphite/epoxy This design yields a much of 0.11 mm RMS. 4.3.1.1 shows Astro
Design both
stowed
Pactruss.
the truss.
The
This stowed
facet
on the next
With
this deployment
and
point
employing
stable
stresses
created
front
shell
and
a
densities
reflectors
where
ranging which
achieving
are
surface
of this kind of accuracy achieved was 0.06 mm a highly
graphite/epoxy
accurate mold
in the graphite/epoxy
plaster
is replicated.
mold,
it is used
and
COI
the
cured
skin
or shell
is laid
on it and
and backup rib structure can be adjusted during of 0.070 mm RMS for 2.2 m reflectors and 0.053
can vary significantly by the design approach. of 3.4-3.8 kg/m _-. These designs use a graphite
to graphite
to the
The
Astro
the deployed
concept
utilizes
arrangement
as closely
E,
skin/Nomex
design
used
honeycomb on
the
DBS.
rib support This
structure.
design
uses
a
skin bonded to a backside rib support structure as shown in Fig. 4.3-1. reduced areal density of 2.2 kg/m 2, yet maintains a surface accuracy
Evaluations:
the
Anik
or shells.
areal weight of many graphite/epoxy reflectors ACTS reflector designs exhibit areal weights
skirt/Nomex
Satellite
Superbird,
areal
surface
to the
involves
thermal
mapped. The final accuracy of the shell manufacturing to achieve surface accuracies mm RMS for 3.3 m reflectors. The The
Broadcast
Kevlar
in aperture
of rigid
a high temperature
of the antenna
A backup
of surface
the manufacturing
Advanced
shell.
from low-density graphite/epoxy has evolved of better than 0.1 mm RMS is feasible.
Attaining
the
reflectors.
on the Direct
At Composite Optics, Incorporated, (COD, the most recent demonstration has been the 3.3-meter transmit antenna for ACTS where the accuracy RMS.
on
transmit
Satellites.
back
range
reflector
(ACTS)
reflectors
hyperbolic
stiffened
reflectors
reflectors
reflector
gridded
GSTAR
Gridded-shell-stiffened
.
Satellite
membrane-sfifened
Dual-shell-stiffened
.
continuous-surface
honeycomb-shell-stiffened
Technology
The single-surface, (DBS).
.
many
Aerospace
square, shows
deployment
arrangements rigid-facet
the rigid
concept
for a rigid-facet segments
facets
which
to be packaged
shown
in Fig.
surface
attached
deploy
sequentially
by stacking
4.3-2 to the on
one rigid
as possible.
concept,
two
antenna
aperture 38
sizes
of 40 meters
and
15 meters
were
Figure 4.3-1.2.1
Meter skin stiffened antenna for Direct Broadcast Satellite (DBS)
39
ORIGINAL OF POOR
PAGE 18 QUALITY
Slowed Stowed
truss
panels
10 packages
-
of 10 panels
each,
4.0 m)
),,
__,A,__
Panels
,Packages unfolded onto truss edge
onto
unfolded truss
I
Deployed
antenna
face
:
40m
I
t
Figure 4.3-2. Deployment investigated. the 40-meter The
goals
more facets
facet
condensed includes
required
I
Concept for Rigid Panels
For these aperture sizes, a 3.1-meter and 2.0-meter and 15-meter-aperture reflectors, respectively. for the rigid
maintaining
I
I
facet
surface
design
accuracies
were
me surface
thickness
of 0.1 mm RMS.
packaging and stowage the depth of draw which
to maintain
a minimum
square
facet
Minirnizing
facet
and
was
areal
the facet
baselined
density
thickness
for
while enables
within the launch vehicle. The total thickness of the is dictated by the F/D and the thickness of the facet
accuracy
requirements.
Feasibility of meeting a minimal areal density was also investigated. For the 40-meter-aperture antenna, a 1.0 kg/m 2 areal density was targeted to maintain a reasonable overall total launch weight.
As-manufactured
for performance A simple and
finite
3.1- meter
reflective
shell
surface
requirements element square and
accuracies
of this LDA
model facets.
was
for the rigid
were
set up to represent
element
used
orientation
the rigid
facet
concepts
plate
elements
for the backside
onto
at 0.1 mm RMS
were
for both the 2.0used
rib structure.
The
to model four
the
support
A 1-g load was assumed to compute the surface to meet the targeted surface accuracy. Several
on both configurations.
Figure 4.3-3 shows the resultant (.75-inch) thick shell consisting quasi-isotropic
baselined
A total of 40 "CQUAD4"
44 "CBAR"
performed
were
application.
points were all modeled to be simply supported. standard deviation in order to size the reflector iterations
facets
The
results
were
as follows.
design concept for the 3.1-meter square facet having a 1.9-cmof 0.25 ram-(0.01 inch) thick graphite/epoxy skins laid up in a 1.9 cm-thick
core.
For
the
purposes
of this
sizing
analysis,
aluminum core properties were used in the finite element model. The backside rib structure consists of a perimeter ring stiffener with two separate ribs crossing through the center. These ribs have a cross-section of a box beam with a 1 mm (.04 inch) wall thickness and cross-section 40
3.1
MET
NOTES:
Figure 4.3-3. 3.1 Meter square facet shell stiffened concept dimensions required The
of 5 cm (2 inches) to meet
resultant
the surface
areal
density
wide
and 10 cm (4 inches)
accuracy calculations
target
with
deep.
This deep
the four-point
for this configuration
simply
box beam supported
section
was
attachment.
as follows: Weight
Shell
skins
Shell
core
Backside
Item (2)
3.1-Meter 8.3
Interface Total The
2.0-meter
5.9
1.6
7.9
4.6
0.8
0.5
0.2
0.2
ribs
Tie clips fittings
Weight square
(Areal facet
Density)
was
23.1
of the same
(2.4 kg/m 2)
design
same
modeling
techniques
were
were
.2 cm
For each of draw desired.
(.08 inch)
thick.
of the two concepts,
The
resultant
areal
thick
in Fig.
as on the 3.1-meter
density
for the 2-meter
was computed
of draw varies depending where maximum draw on the antennas 41
facet
quasi-isotropic
4.3-3.
It had
graphite/epoxy
square
facet.
The
concept except the cross-section was smaller The wall thickness of the box beam members
the total facet thickness
for each case. The amount For these purposes, the
inch)
used on this concept
backside rib structure was the same as the 3.1-meter with 3.8 cm x 3.8 cm (1.5 in. x 1.5 in.) box beam.
10.4 (2.6 kg/m 2)
as the 3.1 meter
a 1.3mm-(.5 inch) thick shell consisting of .25mm-(.01 skins bonded to a 1.3cm-(.5 inch) thick core. The
2.0-Meter 3.5
panel
which
was
2.6 kg/m 2.
includes
the amount
on the antenna the draw is was used in the overall
thicknessdeterminationwhich is at the locationclosestto the vertex. The total panelthicknesses are summarizedas follows for eachconcept.
Maximum Draw Shell Thickness Rib Thickness
3.1-Meter SquareFacet 1.96cm 1.90cm 10.16cm
2.0-Meter SquareFacet 2.18 cm 1.27cm 3.81 cm
Total Thickness
14.02cm
7.26 cm
The resultsof thesepreliminary studiesshow thatattaining arealdensitiesof 1.0 kg/m2 are optimistic.
However,
of previous
COI
current
reflector
which
areal Panel
concept.
criteria
densities
reflectors, designs.
the 3.1-meter design
areal
of 2.0 kg/m 2 seems
densities
These
preliminary sensitive
1.
A four-point
interface
2.
Quasi-isotropic
3.
Aluminum
core
properties.
When
considering
these
baseline
future
studies
thinner
panel
design.
may
also require
antenna
sizing
to the results
Based
on the areal
improvements reduction,
studies
over
especially
results
many
of the
in the case of
are based
on the listed
obtained.
laminates
design
the rigid
These
criteria,
facet
several
design,
further
thereby
iterations
producing
could
a reduced
be performed areal
density
panel design a six-point additional ijaterface seem o
if an increased number attachment with three support
support
to offer
at the where
the most
center
assume is
all laminates
possible
where
directionalized
when
Another
of the panel
to reduced
were feasible. along each
would
areal
option
weight
(shell the
orientation
and
The core,
core COI
selection could
or using
is another propose
ribs)
backside
and panel
structure
area requiring a quasi-isotropic 42
since
be
graphite/epoxy
investigation.
tri-cell
be a center Additional
truss
supports
thickness.
core
further
designed
the cross-sectional
further
option could be thereby giving
The baseline
However,
could
higher-modulus
the design
point to the
graphite/epoxy fiber system is ideal due to its near-zero
orientation.
are quasi-isotropic. rib
One edge,
would
be supported.
laid up in a quasi-isotropic
or P120). This would benefit beam ribs could be reduced.
,
of the panel.
the center benefit
of attachments truss interfaces
The design concepts shown baseline the P75 high- modulus which is a 75- million-modulus fiber. This fiber selection CTE characteristics
in and
include:
The interface attachment to the truss is presently a four-point attachment withone at each of the comers of the rigid facet. There could be considerable improvement
.
too
densities
to the truss
graphite/epoxy
to optimize
of 2.0 kg/m 2 offer
thicknesses
are very
feasible.
made
optimization
using
material properties
In place of
concepts
the
a
more
(e.g.,
P100
of the box
of aluminum same
parent
graphite/epoxy material as the shell skins. This benefits the structure by offering uniform sandwich CTE. The core can also offer improved core shear modulus improves
the sandwich
approach
1.5 lb/ft 3, thereby
shows .
COI's
Additional
stiffness.
reducing
graphite/epoxy design
4.3-5 and 4.3-6. viable alternatives
In addition,
tri-cell
options
could
it is anticipated
the areal
densities
of the rigid
core and its possible be studied
which
These options require further requiring investigation.
( .00;8
facets.
use in applications
are
analysis
SKIt/
UPPER
that the core
REFLECTOR
SHELL
in future
studies.
They
f
--RIB
/x_
_
_
VENT
TH