David
D. Lang1
1David D.
Lang Associates, Seattle WA.
Abstract:
This paper presents an overview of a proposed GEO-originating
deployment mission flight scenario currently under consideration to accomplish
the initial construction of a space elevator. Much as a suspension bridgeÕs
initial strand of cable must be established, so must the elevatorÕs first
strand of vertical ribbon and ballast mass be erected. Results of dynamic
simulations of initial deployment accomplished using the Generalized Tethered
Object Simulation System (GTOSS) software tool are presented via discussions
and summary graphs. A brief overview of dynamic models that constitute GTOSS
is presented, and the physical configuration of the elevator as it manifests
itself within GTOSS is characterized. A general discussion of orbital dynamics
challenges facing this initial deployment process is presented, with emphasis
on dynamic control issues and implications on the two space craft delegated
to performing the deployment. Finally, a proposed control strategy is presented
and simulated to demonstrate the possibility of a GEO originating deployment.
Currently
two different approaches to deploying the initial elevator ribbon are
identified. Both start with a space craft containing (either initially or via
build-up by multiple courier-missions) the Ribbon, Ballast mass, Ballast-end
controller (GEO craft), ribbon Anchor-end controller (Deploy craft), and
propulsion-control systems. While they differ in starting point and maneuver
strategy, they both must face the dynamics challenges of extreme tether
extension. The two scenarios are:
(a)
Start with a space-craft at GEO, thus
deploying Ribbon downward from there, in conjunction with a coordinated upward
maneuvering of the GEO craft). See Reference 1.
(b)
Start with a space-craft in LEO,
deploying the Ribbon and Ballast mass upward, creating a system
with ever-longer orbiting period, until the configuration grows to include GEO
altitude and beyond, and manifests an Òorbital periodÓ corresponding to earth
rotation rate. See Reference 6.
This paper
specifically explores the dynamics of the GEO deployment mission. A proposed
deployment control strategy is presented that serves to expose the nature of
the dynamics challenges inherent in this mission, and explores some of the
intrinsic ingredients that might constitute a successful deployment mission
design.
The
Generalized Tethered Object Simulation System is a time-domain dynamics
simulation code, conceived by the author in 1982 to provide NASA with a tool to
simulate dynamics of combinations of space objects and tethers for flight
safety certification of the Shuttle Tethered Satellite System missions. Since
then, GTOSS has undergone continuous evolution and validation, being applied at
some stage in the formulation of virtually every US tethered space experiment
flown or proposed to date. Below is an overview of GTOSS features.
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Multiple bodies, with 3 or 6 degrees of freedom, connected in arbitrary fashion
by multiple tethers, subject to natural planetary environments, including standard earth models as well as more
rudimentary models for the other planets.
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Tethers represented by either massless or massive models.
The massive tether
model is a point synthesis approach, each tether employing a
constant number of up to 500 nodes, specifiable by tether (500 is a soft system-configurable limit).
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All tethers can be deployed from, or retrieved into, objects by user-definable
scenarios. The tether model includes momentum effects of mass entering or
leaving the domain of the tether itself, and produces related forces on objects
deploying and retrieving the tether material.
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Tethers
can possess length-dependent non-uniform attributes describing elastic cross
section, aerodynamic cross section, and lineal mass density.
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Tethers are subject to distributed forces from: Subsonic and hypersonic
aerodynamics; Electrodynamics of current interaction with magnetic fields using
current-flow models incorporating effects of insulated or bare-wire conductors
interacting with a plasma environment model. With a ribbon-to-plasma contact
model, grounding-current in a conducting elevator may possibly be assessed.
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Tethers experience thermal response, gaining heat under the influence of solar
radiation, earth albedo, earth infrared radiation, aerodynamics, and electrical
currents; heat loss occurs through radiative dissipation.
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Tethers can be severed at multiple locations during simulation.
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Objects and tethers can be initialized in many ways, including creating
stabilized extremely long tether chains, attached to and rotating with a planet
(a space elevator) with due consideration for variation in longitudinally
non-uniform tether properties.
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GTOSS creates a database containing results of response to the user-defined
material configuration, initialization specifications, and environmental
options; this permanent data base can then be post processed to produce a wide variety of result displays, from
tabular data, to graph plots, to animations.
For
the GEO deployment mission, the topology consists of a Deploy craft, (as the
ribbonÕs lower body) that proceeds earth-ward during deployment and a GEO craft
(as the ribbonÕs upper body) that proceeds ballast-ward; it is the GEO craft
that contains the ribbon characterized by a dual tapered design. Deployment
occurs initially by downward ejection of the Deploy craft attached to the
earth-end of the tapered ribbon (emerging first along with the Deploy craft),
leaving the ballast-end and upper portions of the tapered ribbon stowed within
the GEO craft (as the GEO craft rises toward the ballast altitude). Figure 1
below depicts schematic snapshots of the system at various stages of
deployment.
GTOSS
characterizes the elevator ribbon with length-varying attributes of density,
elastic-area, modulus, aerodynamic-area, and damping that correspond to
baseline ribbon design (described in References 1, 2, 3, and 4), but,
appropriately modified to reflect a proposed initial deployment configuration.
This initial deployment envisions
two 20 metric ton reels of ribbon being deployed from a GEO craft (deployed
simultaneously as one ribbon, 10 cm wide in the GTOSS simulation). By
assuming that this initial ribbon would have a longitudinal taper design
identical to the mature elevator, then, corresponding ribbon properties for the
initial deployment mission can be derived as a scaled version of the mature
ribbon. Baseline mass of the mature elevator ribbon is 825 tons, so the ratio
between the initial 40 tons of ribbon and the mature ribbon yields the lineal
density ratio of the initial ribbon
in comparison to the mature ribbon. This is:
![]()
The
ribbon elastic area is also scaled per this ratio. Based on the scaled elastic cross sectional area profile and a nominal
value of the ribbon materialÕs bulk density of 1.3 gm/cm3 (CNT), the
lineal density profile was derived for use in GTOSS. Figure 2 depicts these resulting properties.

Figure 2.
Ribbon Elastic Cross Sectional Area and Lineal Density vs Altitude
This
above data combined with a nominal YoungÕs modulus of 1,300 GPa (assumed for
the CNT ribbon material) fully defined the ribbonÕs static elastic properties. Dynamic attributes were
characterized by a material-intrinsic, strain-proportional damping factor, b = 0.02,
where:
s = E(e + b e-dot)
and,
s = stress
e = strain
E = YoungÕs Modulus
Both
the GEO craft and Deploy craft were simulated as 3 degree of freedom objects,
thus no attitude control considerations were involved; this was deemed
appropriate considering the study was only focused on the overall orbital
behavior of the deploying distributed mass system, and the fact that the attitude dynamics of the end-bodies
would essentially be uncoupled from the gross orbital dynamics. Both of these
craft can loose mass due to propellant expenditure. Only the GEO craft will
loose mass due to ribbon deployment. In these preliminary studies, mass loss
specifically due to propulsion was inhibited because of many factors; for
instance the non-optimal nature of these initial controllers plus the lack of propulsion technology definition that
would be employed (with attendant specific impulse uncertainty) would likely
produce misleading propellant usage estimates.
The
initial total mass of the (upper) GEO
craft was 69,000 kg, of which
40,000 kg is ribbon mass and 29,000 kg is ribbon deployment mechanisms, control
systems, thrusters, and propellant. The initial total mass of the (lower) Deploy
craft was 1,500 kg. This entire mass
is delegated to anchor-station grappling hardware and fixtures, control
systems, thrusters, and propellant.
6. Uncontrolled
Natural Deployment Tendencies
Figure 3.
Ribbon Deploy Rate vs Range Rate
The steady increase
in tension at both ends of the ribbon is seen in Figure 4 below. The higher
tension at the GEO craft is responsible for pulling the GEO craft earthward and
a resulting significant posigrade motion of the GEO craft with respect to its
initial geosynchronous position. The sharp tension increase at the Deploy craft
near the end of deployment is due to its diving ever more rapidly into the
inverse-square gravity-well. This case clearly illustrates the potential for a
deployment to end disastrously in a crash to earth!
Figure 4. Tension at Upper and Lower Ends of Ribbon
The altitude
state of both end-objects, shown in Figures 5 and 6, exposes the sharp increase
(at 4.5 days) in the Deploy craftÕs accelerating encounter with gravity, dragging
everything down with it. Consequently, the
GEO craft vacates its geo-synchronous condition (loosing altitude as ribbon
tension increases, pulling it earthward), and simultaneously moves through
about 180 degrees of posigrade earth longitude prior to the systemÕs eventual
plunge to earth.
Figures 5 and 6.
End Object Altitude Response
The Deploy craft dips deeply into the gravity well at 4.5 days, shown in Figure 7.
Figure 7.
End Object Acceleration of Gravity
Figure 8 shows the earth longitude traversed by the GEO
craft.
Figure 8.
Earth Longitude Traversed by GEO Craft
As soon as tension manifests itself (at about ½ day) Figure 9 shows that the Deploy
craft starts to librate with respect to the GEO craft, typical of tether
deployment behavior. But this libration naturally tends toward zero amplitude,
a feature that can be used to advantage in the mission design.
Figure 9.
Libration of Deploy craft
with-respect-to the GEO Craft
7. A Controlled Fly-Away
From Earth
Figure 10.
Deploy Rate
The ultimate
failure of this deployment is clearly seen in the GEO and Deploy craft altitude
histories shown in Figure 11. The GEO craft is rising, attempting to
equilibrate tension, but at about 6 days into the mission, a vertical
instability starts manifesting itself, after a few cycles of which, the
system instability
overwhelms the control effectors, and the system irretrievably departs
controlled flight!
Figure 11.
Altitude of GEO craft and Deploy craft
In Figure 12, it is seen that the
system as a whole has failed to Òbite into the gravity wellÓ sufficiently
to prevent a centrifugal departure.
Figure 12.
Acceleration of Gravity at GEO craft and Deploy craft
Tension shown in
Figure 13 illustrates inappropriate control system design that is exciting
longitudinal ribbon dynamics and the system. These
variations are indicative of the need for an elevator ribbon deployment control
system design to be able to reject undesirable frequencies in the tension
signal so as to deduce intrinsic tension level, against which the GEO craft must fly a compensating
equilibrium-altitude maneuver.
Figure 13.
Tension at GEO craft
8.
The Deployment Venue
The
process of deploying a ribbon with physical extension on the order of the space
elevator (earth to 100,000 km) is found to be a delicate control process.
Little of the knowledge-base derived from actual orbital tether operations to
date has bearing on this procedure due to a host of attributes that make this
process unlike any yet attempted by mankind. To understand technical issues
facing deployment, one must have a grasp of the physical factors inherent in
this process, the deployment venue, as
outlined below.
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Regardless of whether deployment starts at LEO or at GEO, the final configuration must be a vertical ribbon extending from near earth
up to centrifugally effective altitudes at which net ribbon tension can be maintained to produce at least a
condition of neutral buoyancy. Such
a configuration (until actually attached to the earth) is neutrally stable;
a perturbation that moves the (neutrally) stable-state upward results in a net downward force reduction that
encourages the tendency. This is because every particle of mass becomes
attracted less toward the earth by virtue of the inverse
radius-squared gravity field, thus a
net reduction in gravity force ensues. Countering this gravity reduction, the
corresponding particles are
subject to less centrifugal effect,
however this varies as the inverse radius, thus restoration due to gravity is decreasing faster
than the centrifugal effects are decreasing, all of which contributes
to the initial upward perturbation combining to move the system higher. Conversely, if the ribbon moves closer to
earth, just the opposite of all the above ensues, and the net effect is to pull
the system lower. Small incipient departures from neutral stability may be
problematic to detect directly, that is, incipient departure may have to be
deduced from position or velocity dispersions alone.
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Note that the balance point depends upon the mass distribution of the system,
that in turn, depends upon the ribbonÕs density and taper, the amount of ribbon
deployed, and the fuel remaining in the end-craft. The ribbon must be
maintained delicately poised between the
conflicting tendencies of centrifugal and gravitational effects with no control
effectors other than (a) position state of the end-masses, (b) distributed mass
within the ribbon, and (c) onboard propulsion.
¥ Insuring stability (for anchor grappling) will require
active-propulsion since ribbon deployment,
per se, may prove ineffective for overcoming departure from the balance point.
Such imbalance can result from factors ranging from uncertainty in
state-recognition (obscuring detection of an insipient departure at deploy
termination), to the transport delays inherent in control inputs propagating
the length of the ribbon, thus attenuating the effects of control inputs
related to deploy rate modulation; note, time for tension gradients to traverse
the ribbon are about 20 minutes from earth to GEO, and 45 minutes from earth to
Ballast.
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In order to minimize the need for
onboard propellant, the progression of intermediate states comprising the
deployment must all be delicately balanced between gravitational attraction and
centrifugal effects; this becomes increasing problematic as the Deploy craft
approaches increasingly non-linear lower regions of the inverse square gravity field.
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As the ribbon is extended up, a tangential velocity make-up is required to maintain effective angular rate
consistent with the earth angular velocity; failure to do this will compromise
the necessary centrifugal counter-balance effect. At Ballast altitude the
required tangential velocity is 7292 m/s (23,900 ft/s) relative
to the anchor point (note, this is on the order of LEO insertion velocity).
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Orders of magnitude change in ribbon effective
end-to-end spring rate, length, and tension
are experienced over the course of this deployment. Initially end-to-end
spring-rate and related natural frequencies can be quite high, but, near
terminal phase (when vertical control near earth becomes critical), the ribbon
will exhibit a spring rate on the order of .004 N/m. End-mass bobbing mode frequencies,
and longitudinal and transverse string mode frequencies of the ribbon system
change drastically over the deployment. This means that control systems must
adapt to a vast range of frequencies potentially compromising control
precision.
9.
Deployment Phase Definitions and a Control Scenario
This is a summarization of a strategy and control
scenario that has proved useful for envisioning deployment of the elevator from
an initial GEO position.
Initial Phase:
This
could be accomplished by ejection of the Deploy craft with a ribbon deploy-rate
slightly greater than Deploy craft ejection rate. As the Deploy craft recedes
into the gravity field, it slowly accelerates, removing ribbon slack; Prior to
realizing tension, the Deploy craft will simply progress below and forward of
the GEO craft in accordance with relative orbital motion (per
Clohessy-Wiltshire equations). When the ribbon finally goes taut, tension will
cause the Deploy craft will begin a harmless libration relative to the GEO
craft. This libration is naturally damped, becoming inconsequential to the
overall deployment. This maneuver requires virtually no control intervention by
the Deploy craft (except minimal attitude control to avoid ribbon
entanglement). This Initial Phase is not a critical mission phase from a
dynamics standpoint. The design criteria would be to simply get some ribbon
deployed and the Deploy craft sufficiently removed from the GEO craft to enable
continuing gravity gradient driven separation. Tension would be kept to a
minimum to facilitate the growing departure between the craft. Ideally this
phase would be accomplished with minimal propulsion by both craft.
Mid Phase:
This
phase will be a long duration maneuver during which the majority of the ribbon
will be deployed. As deployment progresses towards consequential tension
buildup, the GEO craft must take action to counter this. To avoid being pulled
down, either direct equilibrating vertical thrust must be provided (with
significant fuel budget consequences), or, dynamic equilibration of this mounting tension achieved. A method to
achieve dynamic equilibration is outlined below:
- a
desired Deploy craft Altitude-rate -vs- Altitude profile is indirectly commanded as an expression of (compensated) ribbon
deploy rate,
in conjunction with the above deployment, the GEO craft is
controlled such that,
- the
GEO craft Vertical translational control algorithm attempts to achieve an
altitude at which centrifugal effects fully
equilibrate the tension and
gravitational acceleration being realized at the GEO craft.
- the
GEO craft Horizontal translational control algorithm provides tangential
velocity make-up to ensure centrifugal equilibration effectiveness and limit
libration oscillations that might adversely couple with vertical dynamic modes.
Note that for
Mid Phase deployment, vertical and horizontal control may not be necessary for
the Deploy craft. Mid Phase terminates
at the atmospheric interface. By Mid Phase termination, Deploy craft altitude
rate will have been stabilized and controllable via a combination of ribbon
fine-deployment, and propulsive control.
Atmospheric Phase:
Atmospheric
traversal may entail (a) Delaying atmospheric encounter until that time when
minimum wind conditions prevail, (b) Propulsive control closing the loop on earth position sensing. This phase was not
simulated in this paper.
Terminal Phase:
Terminal
phase consists of the combined actions of fine control of earth position, altitude, and altitude-rate.
Altitude rate control would likely be accomplished by propulsion in conjunction
with vernier ribbon deployment. This phase was not simulated in this paper.
10. Dynamics
of a Possible Control Algorithm for Deployment
The
above described deployment mission scenario demonstrates the possibility of
dynamically balancing the vertical ribbon during the course of deployment and
suppressing un-desirable dynamic ribbon responses, all by means of control
effectors of significantly less force
than the steady tensions being
managed during the deployment. This technique is an interplay of a Vertical and
Horizontal controller for the GEO craft combined with a ribbon deployment scenario that modulates the
ribbon deployment-rate as a function of the Deploy craft altitude, while paying
due regard to a supplementary deployment rate component required to compensate
for the rising altitude of the GEO craft itself. Ideally, the GEO craft
Vertical control is of such precision as to require virtually no static
propulsive-makeup against tension; in which case, a minimum propulsive impulse
would roughly correspond to the sum of the work that must be done to vertically control the GEO
craft through the gravity field from GEO to Ballast altitude (a quantity highly
sensitive to optimal design) plus tangential velocity make-up (an
essentially fixed quantity). This controller uses logic to minimize modal
interaction with the combined ribbon/end-body system, while counteracting the
intrinsic tension and gravity state; problematically, the vertical controller
can induce spurious tension transients into the ribbon system in the act of
maneuvering, then in turn, react to these very transients. For this reason the
vertical controller uses filtered tension sensor data to plan maneuvers (along with other schemes to
counteract instabilities). Details of the control algorithms and deployment
scenario follows.
GEO craft control:
For the Horizontal
axis, conventional on/off control logic was employed to maintain the GEO craft
to within a specified dead-band of a specified fixed earth longitude and
latitude. This control logic is combined with a Coriolis bias that commands a
horizontal thrust-level proportional to the altitude rate and earth rotation
rate. The maximum horizontal thrust allowed for this mode was 2200 N.
For the Vertical
axis, a conventional error/error-rate feedback proportional controller
commanding a maximum of 6500 N of thrust was used. This controller commanded an
altitude that would be consistent with equilibrating the ribbon tension with
due regard for local gravitational acceleration; this equilibration assumes a
tangential velocity corresponding to the GEO craftÕs position as though it
were on a vertical radial rotating with the earth.
Deploy craft control:
It was
determined that due to the inherent relative libration stability of space tether deployment, no active translational
control was needed on the Deploy craft for the Initial-phase and Mid-phase of this deployment.
The Ribbon Deployment:
Ribbon
deployment rate is the sum of two contributions: (a) the baseline rate profile
from a table of Deploy-rate -vs- Deploy
craft Altitude representing a desired rate
of descent for the Deploy craft, and (b) the altitude rate of the GEO craft (as it rises to equilibrate the
ever-building tension). This algorithm is configured to inhibit negative
deployment rate so as to attenuate deployer participation in longitudinal
dynamic modes and GEO craft controller-induced vertical dynamics. A strain-bias
of 0.075 (based on a reference tension of 22,000 N) accounts for the fact that
the deployer algorithm dispenses un-elongated tether, which, upon being emitted into the domain of
the tether, is destined to acquire a strain consistent with the level of stress
extant in the tether.
Figure
14 below shows the base-line deploy rate
for this example, and derived from an idealization of a possible Altitude-rate -versus- Altitude profile that might be appropriate for a Deploy craft
to experience. The ribbon deploy rate is commanded as this baseline
value, plus, the Altitude
rate of the GEO craft.
Figure 14.
Baseline Deploy Rate Component -vs- Altitude of Deploy craft
Figure 15 shows the composite ribbon deploy rate experienced
by this mission.
Figure 15.
Final Composite Deploy Rate Reflecting GEO craft Altitude Rate
Shown in Figures 16 and 17 are the actual altitude rates
achieved by the Deploy craft and GEO craft, and clearly show rate modulation
starting at about 8 days.
Figure 16. Altitude Rate of Deploy craft
Figure 17. Altitude Rate of GEO craft
The resulting altitude profiles of the GEO and Deploy craft
are seen in Figure 18.
Figure 18. Altitude of GEO craft and Deploy craft
The ribbon tension is shown in Figure 19.
Figure 19. Tension
Libration experienced by the GEO
craft is shown in Figure 20. Notice that the horizontal dead-band controller
bounds the libration at about the +1 degree dead band indicating that the
tangential velocity makeup control was slightly biased.
Figure 20. GEO craft Libration relative to Anchor
Point
Libration experienced by the Deploy craft is shown in
Figures 21. Even though the Deploy craft has no active control, its initial
libration perturbation (associated with tension onset) attenuates over time, a
behavior typical of tether deployment.
Figure 21. GEO craft Libration relative to Anchor
Point
Deploy craft position relative to the anchor is shown in Figure 22. Note, if the GEO craft were initially positioned 1.5 deg. west of the anchor, the resulting eastward dead-band bias would position the Deploy craft directly over the anchor.
Figure 22. Deploy craft Position Error Relative to
Anchor Point
11. Importance of Horizontal Control
Examination
of cases in which horizontal control was not active on the GEO craft clearly
indicates the critical need for tangential velocity compensation related to Coriolis acceleration effects. For
instance, in the example above of a successful deployment, by simply disabling
horizontal control on the GEO craft (but with the successful vertical control modes still enabled), the system crashes to earth. This is
because the centrifugal effect is the paramount mechanism in the physics of the
elevator, and as the GEO craft rises, failure to introduce tangential velocity
make-up allows the GEO craft to drift into a higher ÒorbitÓ with a corresponding
longer orbital period, hence, a lesser effective angular velocity. Thus the intrinsic centrifugal effect on which the
elevator relies is removed; under these conditions the ribbon tension can
easily pull-down the GEO craft.
Due
to the inherently unstable attributes of a tethered system whose length spans a significant portion of the
gravity field, as in the case of the space elevator, it appears that active
control effectors will be necessary to perform this mission. Failure to accomplish
such control was found to easily result in total loss of the initial elevator
system since un-attenuated vertical imbalances result in either the entire
system collapsing to earth, or flying off into an irretrievable trajectory.
While
such control can be doubtlessly accomplished given sufficient propellant
budget, the engineering challenge facing an actual deployment is to achieve
control and stability within practical levels of total propulsive impulse
expenditure. The ideal lower-bound on mission impulse could be thought of as
the sum of the impulse required to achieve tangential velocities consistent
with earth rotation, plus the impulse required to lift the ballast (and ribbon)
against the gravity potential. Since expenditure of total impulse has
mission-lapsed-time implications (analogous to gravity losses for classical
rocketry), short mission durations are desirable; however, stability and safety
of deployment speaks for long slow deployments, thus, the mission design will
likely entail compromises related
to this area of performance.
Only insignificant transverse ribbon oscillation modes were excited during the process of deployment.
While, this was not true during the engineering development process for the
various control modes and deployment strategies, it was found that as
deployment scenarios started to meet mission objectives successfully, then
simultaneously, transverse string mode deflections became inconsequential. This
was probably because successful
deployment schemes (almost axiomatically) manifested themselves as smooth deployment processes.
A
proposed control law and deployment scenario has been simulated and found to
demonstrate the possibility of effectively managing the space elevator ribbon
deployment down to the atmospheric phase interface.
13. Future Work
Many
areas of new investigation regarding initial ribbon deployment invite further
exploration. The optimization of control algorithms will be critical to
accomplishing the mission, yet expending an affordable total impulse. Transit
though the atmosphere was not addressed in this study; the effective use of
propellant in this phase of the mission may be critical. Finally the terminal
phase of the mission in which contact is made with the anchor station will require
sensitive control of altitude rate of the Deploy craft, as well as the
development of innovative grappling schemes and maneuvers.
The
potential benefits of a LEO originating deployment were not addressed in this
study. The dynamic responses of such an approach should be addressed next in
order to determine which mission scenario might be optimal for the initial
space elevator deployment.
Acknowledgements
Funding
for this work has been provided in part by the Institute for Scientific
Research, Fairmont, WV and the NASA Marshall Space Flight Center.
References
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Westling, Eric A. ÒThe Space
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2. Edwards, Bradley C.,
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4. Lang, David D., ÒApproximating Aerodynamic Response of the Space Elevator to Lower Atmospheric WindÓ, proceedings of the Space Engineering and Space Institute, 2005.
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