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1
FORMATIONS NEAR THE LIBRATION POINTS:
DESIGN STRATEGIES
USING NATURAL AND NON-NATURAL ARCS
K. C. Howell and B. G. Marchand
2
Formations Near the Libration Points
Moon
1L
2L
ˆx
( )ˆ inertialX
B
θ
ˆy
Chief S/C Path
(Lissajous Orbit)
EPHEM = Sun + Earth + Moon Motion From Ephemeris w/ SRP
CR3BP = Sun + Earth/Moon barycenter Motion Assumed Circular w/o SRP
Deputy S/C
(Orbit Chief Vehicle)
3
Control Methodologies Considered
in both the CR3BP and EPHEM Models
• Continuous Control
– Linear Control
• State Feedback with Control Input Lower Bounds
• Optimal Control → Linear Quadratic Regulator (LQR)
– Nonlinear Control
• Input Feedback Linearization (State Tracking)
• Output Feedback Linearization (Constraint Tracking)
– Spherical + Aspherical Formations (i.e. Parabolic, Hyperbolic, etc.)
• Discrete Control
– Nonlinear Optimal Control
• Impulsive
• Constant Thrust Arcs
– Impulsive Targeter Schemes
• State and Range+Range Rate
– Natural Formations  Impulsive Deployment
– Hybrid Formations  Blending Natural and Non-Natural Motions
4
IMPULSIVE FORMATION KEEPING:
TARGETER METHODS
5
State Targeter:
Impulsive Control Law Formulation
1V∆
2V∆
3V∆
Segment
of Nominal
Deputy Path
0vδ −
0vδ +
0V∆
1rδ
2rδ
3rδ
STM
1 1
1 1
k kk k
k kk k k
A Br r
C Dv v V
+ +
− −
+ +
    
=    
+ ∆    

δ δ
δ δ
( )1
1k k k k k kV B r A r v− −
+∆= − −δ δ δ
Segment
of Chief S/C Path
C(t1)
C(t2)
C(t3)
D(t1)
D(t2)
D(t3)
6
State Targeter:
Radial Distance Error
( ) ˆ10 m Yρ =
DistanceErrorRelativetoNominal(cm)
Time (days)
Max.Deviation
Nominal Separation
7
State Targeter:
Achievable Accuracy
MaximumDeviationfromNominal(cm)
Formation Distance (meters)
ˆr rY=
8
State Targeter:
Maneuver Schedule
9
Range + Range Rate Targeter
Chief S/C
Deputy S/C
r
1V∆
2V∆
3V∆
( )
1/2
Range + Range Rate Constraint:
T
f f
f
T
f
f f
f
f
r r
r
g r rr
r
 
  
= =   
  
  


( ) ( ) ( )
STM
0
0 0 0
0 0
State Relationship Matrix
, ,f
r r
rr r
d g t t x t t
v V
t
r r
r r
−
∂ ∂ 
   ∂ ∂
= Φ = Φ   + ∆∂ ∂   
 
Λ
∂ ∂ 

 


δ
δ
δ
10
Comparison of Range and State Targeters
Chief S/C at Origin
Deputy S/C Path
11
DESIGN OF NON-NATURAL FORMATIONS
USING NATURAL SOLUTION ARCS
12
CR3BP Analysis of Phase Space
Eigenstructure Near Halo Orbit
( ) ( )
( ) ( ) ( )1
,0 0
0 0Jt
x t x
E t e E x−
= Φ
=
δ δ
δ
Reference Halo Orbit
Chief S/C
Deputy S/C
( ) ( ) ( ) ( ) ( ) ( )
6 6
1 1
:Solution to Variational Eqn. in terms of Floquet Modes
j j
j j
jx t x t c t E t ce t t
= =
= = =∑ ∑δ δ
Mode 1  1-D Unstable Subspace
Mode 2  1-D Stable Subspace
Modes (3,4) and (5,6)  4-D Center Subspace
Floquet Modes
13
Natural Solutions:
Periodic Halo Orbits Near Libration Points
ˆx
ˆz
ˆy
Earth
ˆx
ˆz
Sun
14
Natural Formations:
Quasi-Periodic Relative Orbits → 2-D Torus
ˆy
ˆx
ˆz
Chief S/C Centered View
(RLP Frame)
ˆy
ˆx
ˆx
ˆz
ˆy
ˆz
ˆz
ˆx
ˆy
15
Floquet Controller
(Remove Unstable + 2 Center Modes)
( )
1
2 5 6 3
1 3 4
2 5 6 3
Remove Modes 1, 3, and 4:
0r r r
v v v
x x x
x x x
x x x IV
−
  
+ +   −∆   
δ δ δα
δ δ δ
δ δ δ
( )
1
2 3 4 3
1 5 6
2 3 4 3
Remove Modes 1, 5, and 6:
0r r r
v v v
x x x
x x x
x x x IV
−
  
+ +   −∆   
δ δ δα
δ δ δ
δ δ δ
( )3
2,3,43
or
2,5 6
6
1
,
0
1
:Find that removes undesired response modes
j j
j j
j
j
V x
I
x
V
δ α δ
= =
=
 
+ ∆= + 
 
∆
∑ ∑
16
Sample Deployment into Relative Orbits:
1-∆V at Injection
Origin = Chief S/C
Deputy S/C
Quasi-Periodic
Origin = Chief S/C
3 Deputies
“Periodic”
1800 days
17
Natural Formations:
Nearly Periodic and Drifting Relative Orbits
Chief S/C @ Origin 1800 days
18
Expansion of Drifting Vertical Orbit
Origin = Chief S/C
( )0r ( )fr t
18,000 days = 100 Revolutions
19
Transitioning Natural Motions
into Non-Natural Arcs: Targeter Approach
STEP 1: Identify a suitable initial guess
Target  Orbital Drift Control
20
Application of Two Level Corrector
( )qTΓ
( )0r t
( )mr t
( ) ( )0mr t r t=
( )qV T∆
STEP 2: Apply 2-level corrector (Howell and Wilson:1996) w/ end-state constraint
STEP 3: Shift converged patch states forward by 1 period
STEP 4: Reconverge Solution
21
Drift Controlled Vertical Orbit (6 Revs)
( )
3 5 m/sec
1 maneuver/year
V∆ = −
22
Geometry of Natural Solutions
in the Ephemeris Model
w/ SRP
Inertial Frame Perspective:
Rotating Frame Perspective:
23
Transitioning Natural Motions
into Non-Natural Arcs: IFL Example
(1) Consider 1st Rev Along Orbit #4
as initial guess to simple targeter.
(2) Choose initial state on xz-plane
(3) Target next plane crossing to be ⊥
(4) Use resulting arc as half of the
reference motion.
(5) Numerically mirror solution about
xz-plane and store as nominal.
(6) Use IFL control to enforce a
closed orbit using stored nominal.
Chief S/C @ Origin
Sphere for Visualization Only
24
Hybrid Control:
Natural Motions + Continuous Control
½ Period  Natural Arc
½ Period  IFL Control
25
Concluding Remarks
• Precise Formation Keeping → Continuous Control
– Is it possible?
• Depends on hardware capabilities and nominal motion specified
• Not if thruster On/Off sequences are required & tolerances too high
• Precise Navigation → Natural Formations
– Targeter Methods
• Natural motions can be forced to follow non-natural paths
• Success depends on non-natural motion specified
– Hybrid Methods (Natural Arcs + Continuous Thrust Arcs)
• May prove beneficial for non-natural inertial formation design.
26
BACKUP SLIDES
27
Hybrid Control: Accelerations
28
( )
1/2
Range + Range Rate Constraint:
T
f f
f
T
f
f f
f
f
r r
r
g r rr
r
 
  
= =   
  
  


( ) ( ) ( ) ( )
STM
*
0 0 0 0 0
0
State Relationship Matrix
, ,f f f
r r
g x r r
d g g g x t t x t t x
r rx
r
t
x
r
δ δ δ
∂ ∂ 
 ∂ ∂ ∂ ∂
= − = = Φ = Φ 
∂ ∂∂ ∂  
 ∂
Λ
∂ 

 


*
0
0
First Order Approximation:
f f
g
g g x
x
δ
∂
= +
∂
Radial Targeter:
Control Law Formulation
*
*
Desired Range + Range Rate:
0
f
f
r
g
 
=  
 
29
Dynamical Model
( )
( ) ( )
( )
( )
2
22
2
2
3 3
1, 2,
s j j
s
js
s j j
s
P P P P
PP
N
P
PP P P P P P
sr
PI
j j s
p
r r
u tr
r r r
ft
µ
µ
= ≠
 
 − + −

=

 
 
+ +∑
Gravity Terms
Solar Radiation Pressure
Control InputGeneralized Dynamical Model for Each S/C:
( )
( )
Assumptions:
Chief S/C Evolves Along Natural Solution 0 (Nominal)
Deputy S/C Evolves Along Non-Natural Solution 0
c
d
u t
u t
→ ∴ =
→ ∴ ≠
30
Chief S/C Motion:
Natural Solutions Near L1 and L2
“Halo”OrbitsNearLi
LissajousTrajectoriesNearLi
Sun Sun
31
Controlled Deputy S/C Motion (Example 1):
Formation Fixed in the Rotating Frame
Chief S/C
Deputy S/C
ˆyρ ρ=
C(t1)
C(t2)
C(t3)
C(t4)
D(t1)
D(t2)
D(t3)
D(t4)
32
X [au]
Y[au]
Controlled Deputy S/C Motion (Example 2):
Formation Fixed in the Inertial Frame
ˆYρ ρ=Chief S/C
Deputy S/C
C(t1)
C(t2)C(t3)
C(t4)
D(t1)
D(t2)D(t3)
D(t4)
33
MAXIM:
APPLICATIONS OF IFL AND OFL
34
MAXIM Mission Sequence
35
MAXIM:
THRUSTER ON-OFF SEQUENCE
36
Free Flyer Configuration
FF2
FF1
FF3
FF4
FF5 FF6
Hub
37
Radial Error wrt. Hub S/C
Thrusters off = 100,000 sec
W Wr r− 
Nominal Radial Vector
in UVW Coordinates
Actual Radial Vector
in UVW Coordinates
38
Free Flyers
UV-Plane Angular Drift (DEG)
ν ν− 
ε ε− 
Nominal
Actual
Nominal
Actual
39
Thrust Profile
Thrusters Off Between t1 = 1 day & t2 = t1 + 100,000 sec.
A
B
C
( )O 0.05 Nµ ( )O 0.05 Nµ
3 mN≈ 3 mN≈
40
MAXIM:
FORMATION RECONFIGURATION
41
Target Reconfiguration
ˆX
ˆZ
ˆY
Detector Target #11
ˆw
1
ˆu
2
ˆw
2
ˆu
Target #2
1
ˆv
2
ˆv
Hub (t1): α = 0°, δ = 0°
Hub (t2): α = 0°, δ = 0°
42
Graphical Representation
of Reconfiguration for Free Flyers
1
ˆˆ ||w X
2
ˆ ˆ||w Y
INITIAL ORIENTATION OF UV-PLANE
FINAL ORIENTATION OF UV-PLANE
43
Thrust to Reconfigure
From α = 0o
to α = 90o
with δ = 0o
1 | ˆˆ |w X
2
ˆ ˆTarget: ||w Y
Reconfiguration Time Increased to
7 days to reduce Detector S/C Control Thrust
44
Mission Specifications
• Hold periscope positions to within 15-µm
• Detector pointing accuracy – arcminutes
• ∠ Periscope-Detector-Target alignment – µas
• Phase 1  1 Target /week
• Phase 2  1 Target/ 3 weeks
• Hub  inter. comm. port between detector & freeflyers
• Reconfiguration (Formation Slewing) Times:
– 1 Day for Phase 1
– 1 Week for Phase 2
• Propulsion
– Formation Slewing  0.02 N (Hydrazine)
– Formation keeping  0.03 mN (PPTs)
Frequent Reconfigurations
45
NATURAL FORMATIONS
46
Natural Formations:
String of Pearls
ˆx ˆy
ˆz ˆz
ˆy
ˆx
47
Deployment into Torus
(Remove Modes 1, 5, and 6)
Origin = Chief S/C
Deputy S/C
( ) [ ]
( ) [ ]
0 5 00 0 m
0 1 1 1 m/sec
r
r
=
= −
48
Deployment into Natural Orbits
(Remove Modes 1, 3, and 4)
Origin = Chief S/C
3 Deputies
( ) [ ]
( ) [ ]
00 0 0 m
0 1 1 1 m/sec
r r
r
=
= −
49
SPHERICAL FORMATIONS
50
OFL Controlled Response of Deputy S/C
Radial Distance Tracking
2 ( )
( )
( )2
, Tg r r r r r
u t r r f r
r rr
    
= − + − ∆   
   
    
3
4
( )
( )
( )2 2
,1
2
Tg r r r r
u t r f r
r r
  
= − − ∆ 
  
  
( ) ( ) ( )2
, 3
T
r r r
u t rg r r r r f r
rr
   
= − − + − ∆   
  
   
Control Law
( )
( ),
ˆ
H r r
u t r
r
=
 Geometric Approach:
Radial inputs only1
1u
3u
2u
4u
Chief S/C @ Origin (Inside Sphere)
51
OFL Controlled Response of Deputy S/C
Radial Distance + Rotation Rate Tracking
*
5 kmr =
1 rev / 6 hrs
1 rev / 1 day
Chief S/C @ Origin (Inside Sphere)
52
Impact Commanded Rotation Rate on Cost
1 rev /24 hrs 0.19 mN
1 rev /12 hrs 0.76 mN
1 rev / 6 hrs 6.40 mN
1 rev / 1 hrs 106.50 mN
→
→
→
→
700 kgsm =
53
ASPHERICAL FORMATIONS
54
Parameterization of Parabolic Formation
pa
ph
pu
ν
( )3
ˆ focal linee
1
ˆe
Nadir
q
1 2 3
ˆ ˆ ˆiCD
Er xe ye ze= + +  
Chief S/C (C)
iDeputy S/C (D )
{ }
i i
i i
CD CD
TI EE I
CD CDE I
E I
r r
C
r r
   
=   
    
: inertially fixed focal frame
: inertially fixed ephemeris frame
E
I
/ cos
/ sin
p p p
p p p
p
x a u h
y a u h
z u q
ν
ν
=
=
= +



Zenith
Transform State from Focal to Ephemeris Frame
55
Controller Development
( ) ( )
( ) ( )
( ) ( )
( )
( )( )
( )
2 2
2 2 2
2 2
2 2 2
2 2 2 2
22 2
2 2 2
0 ,
2 2 2
1 ,
0
2
u x y
x
y q x y z
z
h h h
x y g u u x y x f y f
a a au
h h h
x y u g q q x y x f y f f
a a a
u
x y xx yy xy yx
gx y x y
x y
ν ν
 
  − + + ∆ + ∆
   
   − − = + + + ∆ + ∆ − ∆   
      + −−  + ++ +   +

        

          

         
   
 
( )
( )2 2
x yy f x f
x y
 
 
 
 
 
 
 
 ∆ − ∆
 
 +
 
 
 
( ) ( ) ( )
( ) ( ) ( )
( ) ( )
* * 2 *
* * *
*
2
*
, 2
, 2
u p p p n p p n p p
q p p n
n
n
g u
g
u u u u u u
g u u q q q q
k
q
ν ν ν ω ν
ω ω
ω ω
ν
= − − − −
= − − − −
=− −
   
   
   
Desired Response for , , and :u q ν
Solve for Control Law:
, critically dampedu qδ δ →
exponential decayδθ →
56
OFL Controlled Parabolic Formation
ˆX
ˆZ
ˆY
0t
0 1.6 hrst +
0 3.8 hrst +
0 8 hrst +
0 5 dayst +
0 6 dayst +
3
ˆe
10 km
1 rev/day
500 m
500 m
Phase I: 200 m
Phase II: 300 m /1 day
Phase III: 500 m
p
p
p
p
p
q
h
a
u
u
u
ν
=
=
=
=
=
=
=


57
OFL Thrust Profile
700 kgsm =
58
New Maxim Pathfinder
Science Phase #2
High Resolution
(100 nas)
20,000 km
1 km
http://maxim.gsfc.nasa.gov/documents/SPIE-2002/spie2002.ppt
59
Maxim Configuration Example
19,500km
1 rev/day
500 m
1 km
1 km
p
p
p
q
u
h
a
ν
=
=
=
=
=

700 kgsm =
60
NONLINEAR OPTIMAL CONTROL
61
Formulation
( ) ( ) ( ) ( )
11 1
0 0
min , , , ,
i
i
tN N
N i i i N
i i t
J x L t x u x L t x u d tφ φ
+− −
= =
=+ =+∑ ∑ ∫ 
Subject to:
( ) ( )1 0, , ; Subject to 0i i i ix F t x u x x+ =
( ) ( ) ( )
( )
( )
( ) ( )
( )
1
1
1
1 1 1
0
0
min
, ,
, , ;
, ,
Subject to
0
N n N N
i i i i
i i i i
n i n i i i i
J x x t x
x F t x u
x F t x u
x t x t L t x u
x
x
φ φ+
+
+
+ + +
= + =
  
= = =  
+   
 
=  
 
 
 

Equivalent Representation as Augmented Nonlinear System:
62
Euler-Lagrange Optimality Conditions
(Based on Calculus of Variations)
( )
1
1
Condition #1: 1
Condition #2: 0 ; 0, , 1
NT T Ti
i i N
i N
Ti
i
i
i
i
i
i
xH
x x
F
x
F
N
u
H
i
u
φ
λ λ λ
λ
+
+
∂ ∂ ∂
∂
∂
= = → =  
∂ ∂ 
∂
∂
= = = −
∂



  

 
( )1 , ,T
i i i i iH F t x uλ +=  
Identify and from augmented linear system.i i
i i
F F
x u
∂ ∂
∂ ∂
 

63
Identification of Gradients
From the Linearized Model
( ) ( ) ( ) ( ) ( )x t A t x t B t u tδ δ δ= +   
( )
( ) 0
0
A t
A t L
x
 
 = ∂ 
 ∂ 
  ( )
3
3
0
0T
B t I
 
 =  
  

( )
( )
( )
( )
0
11
0, ,
;
0 0, , nn
x xf t x ux
xL t x ux ++
      
= =      
     


Augmented Nonlinear System:
Augmented Linear System:
64
Solution to Linearized Equations
( ) ( ) ( ) ( ) ( )
( ) ( ) ( ) ( )
0
0 0
0 0 0 0 7
, ,
, , ; ,
t
t
x t t t x t B u d
t t A t t t t t I
δ δ τ τ δ τ τ=Φ + Φ
Φ = Φ Φ =
∫ 
  
i
F
x
∂
∂


Relation to Gradients in E-L Optimality Conditions:
( ) ( ) ( ) ( )
1
1 1 1, ,
i
i
t
i i i i i
t
x t t x t B u dδ δ τ τ δ τ τ
+
+ + +=Φ + Φ∫ 
65
Control Gradient for Impulsive Control
( )
( )( )
( ) ( )
1 1
1
1 1
,
,
, ,
i i i i
i i i i
i i i i i i
x t t x
t t x B V
t t x t t B V
δ δ
δ
δ
− +
+ +
−
+
−
+ +
= Φ
=Φ + ∆
= Φ + Φ ∆
 
 
 
i
F
u
∂
∂

( )1,i i
i
F
t t B
u
+
∂
= Φ
∂


66
Control Gradient for Constant Thrust Arcs
( ) ( ) ( )
1
1 1 1, ,
i
i
t
i i i i i i
t
x t t x t B d uδ δ τ τ τ δ
+
+ + +
 
=Φ + Φ 
  
∫ 
i
F
u
∂
∂

( ) ( ) ( )
1
1
1, ,
i
i
t
i i i
i t
F
t t t B d
u
τ τ τ
+
−
+
 ∂
=Φ Φ 
∂   
∫

( )
( )
( )
( )
( ) ( )
( )
1
1*
, ,
, ,
,,
,,
n
i
i
ii
x f t x u
x L t x u
A t t tt t
t t Bt t
+
−
   
   
   =   ΦΦ   
   ΦΦ   


 

Equations to Integrate Numerically
67
Numerical Solution Process: Global Approach
( )
0(1) ; ( 0,1,..., 1)
(2)1-Scalar Equation to Optimize in 3 1 Control Variables
Use optimizer to identify optimal
Input , , and initia
given .
During each iteratio
l guess for
n
i
i
N i
i
i N
N
H
u
x u
u
t = −
−
∂
∂

( )
( )
( ) Sequence forward and store
of the optimizer, the following steps are followed:
( ) Evaluate cost functional,
( ) Evaluate 1
; 1
(
, , 1
N
NT N
N
N
i
N
b J x
x
c
x x
a x i N
d
φ
φ φ
λ
= … −
=
∂  ∂
= =  
∂ ∂ 
 
 

( )
) Sequence backward and compute ; 1, ,1
and used in next update of control input.
i
i
i
i
i
H
i N
u
H
e J
u
λ
∂
= −
∂
∂
∂
 
68
Formulation
( ) ( ) ( ) ( )
11 1
0 0
min , , , ,
i
i
tN N
N i i i N
i i t
J x L t x u x L t x u d tφ φ
+− −
= =
=+ =+∑ ∑ ∫ 
Subject to:
( ) ( )1 0, , ; Subject to 0i i i ix F t x u x x+ =
( ) ( ) ( )
( )
( )
( ) ( )
( )
1
1
1
1 1 1
0
0
min
, ,
, , ;
, ,
Subject to
0
N n N N
i i i i
i i i i
n i n i i i i
J x x t x
x F t x u
x F t x u
x t x t L t x u
x
x
φ φ+
+
+
+ + +
= + =
  
= = =  
+   
 
=  
 
 
 

Equivalent Representation as Augmented Nonlinear System:
69
Impulsive Optimal Control
Minimize State Error with End-State Weighting
( ) ( ) ( ) ( )
11
0
1 1
min
2 2
i
i
tN
T T
N N N N
i t
J x x W x x x x Q x x d t
+−
=
= − − + − −∑ ∫
   
70
State Corrector vs. Nonlinear Optimal Control:
Cost Function
71
State Corrector vs. Nonlinear Optimal Control:
Impulsive Maneuver Differences
72
Impulsive Radial Optimal Control
( )
11
2
0
1
min
2
i
i
tN
i t
J q r r dt
+−
=
= −∑ ∫

73
Radial Optimal Control:
Maneuver History
74
State Corrector vs. Nonlinear Optimal Control:
Cost Function
75
RANGE + RANGE RATE TARGETER
76
Comparison of Range and State Targeters
77
Range Targeter:
Spatial Behavior of Corrected Solution
Chief S/C at Origin
Deputy S/C Path

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Formations Near The Libration Points: Design Strategies Using Natural And Non-Natural Arcs

  • 1. 1 FORMATIONS NEAR THE LIBRATION POINTS: DESIGN STRATEGIES USING NATURAL AND NON-NATURAL ARCS K. C. Howell and B. G. Marchand
  • 2. 2 Formations Near the Libration Points Moon 1L 2L ˆx ( )ˆ inertialX B θ ˆy Chief S/C Path (Lissajous Orbit) EPHEM = Sun + Earth + Moon Motion From Ephemeris w/ SRP CR3BP = Sun + Earth/Moon barycenter Motion Assumed Circular w/o SRP Deputy S/C (Orbit Chief Vehicle)
  • 3. 3 Control Methodologies Considered in both the CR3BP and EPHEM Models • Continuous Control – Linear Control • State Feedback with Control Input Lower Bounds • Optimal Control → Linear Quadratic Regulator (LQR) – Nonlinear Control • Input Feedback Linearization (State Tracking) • Output Feedback Linearization (Constraint Tracking) – Spherical + Aspherical Formations (i.e. Parabolic, Hyperbolic, etc.) • Discrete Control – Nonlinear Optimal Control • Impulsive • Constant Thrust Arcs – Impulsive Targeter Schemes • State and Range+Range Rate – Natural Formations  Impulsive Deployment – Hybrid Formations  Blending Natural and Non-Natural Motions
  • 5. 5 State Targeter: Impulsive Control Law Formulation 1V∆ 2V∆ 3V∆ Segment of Nominal Deputy Path 0vδ − 0vδ + 0V∆ 1rδ 2rδ 3rδ STM 1 1 1 1 k kk k k kk k k A Br r C Dv v V + + − − + +      =     + ∆      δ δ δ δ ( )1 1k k k k k kV B r A r v− − +∆= − −δ δ δ Segment of Chief S/C Path C(t1) C(t2) C(t3) D(t1) D(t2) D(t3)
  • 6. 6 State Targeter: Radial Distance Error ( ) ˆ10 m Yρ = DistanceErrorRelativetoNominal(cm) Time (days) Max.Deviation Nominal Separation
  • 9. 9 Range + Range Rate Targeter Chief S/C Deputy S/C r 1V∆ 2V∆ 3V∆ ( ) 1/2 Range + Range Rate Constraint: T f f f T f f f f f r r r g r rr r      = =            ( ) ( ) ( ) STM 0 0 0 0 0 0 State Relationship Matrix , ,f r r rr r d g t t x t t v V t r r r r − ∂ ∂     ∂ ∂ = Φ = Φ   + ∆∂ ∂      Λ ∂ ∂       δ δ δ
  • 10. 10 Comparison of Range and State Targeters Chief S/C at Origin Deputy S/C Path
  • 11. 11 DESIGN OF NON-NATURAL FORMATIONS USING NATURAL SOLUTION ARCS
  • 12. 12 CR3BP Analysis of Phase Space Eigenstructure Near Halo Orbit ( ) ( ) ( ) ( ) ( )1 ,0 0 0 0Jt x t x E t e E x− = Φ = δ δ δ Reference Halo Orbit Chief S/C Deputy S/C ( ) ( ) ( ) ( ) ( ) ( ) 6 6 1 1 :Solution to Variational Eqn. in terms of Floquet Modes j j j j jx t x t c t E t ce t t = = = = =∑ ∑δ δ Mode 1  1-D Unstable Subspace Mode 2  1-D Stable Subspace Modes (3,4) and (5,6)  4-D Center Subspace Floquet Modes
  • 13. 13 Natural Solutions: Periodic Halo Orbits Near Libration Points ˆx ˆz ˆy Earth ˆx ˆz Sun
  • 14. 14 Natural Formations: Quasi-Periodic Relative Orbits → 2-D Torus ˆy ˆx ˆz Chief S/C Centered View (RLP Frame) ˆy ˆx ˆx ˆz ˆy ˆz ˆz ˆx ˆy
  • 15. 15 Floquet Controller (Remove Unstable + 2 Center Modes) ( ) 1 2 5 6 3 1 3 4 2 5 6 3 Remove Modes 1, 3, and 4: 0r r r v v v x x x x x x x x x IV −    + +   −∆    δ δ δα δ δ δ δ δ δ ( ) 1 2 3 4 3 1 5 6 2 3 4 3 Remove Modes 1, 5, and 6: 0r r r v v v x x x x x x x x x IV −    + +   −∆    δ δ δα δ δ δ δ δ δ ( )3 2,3,43 or 2,5 6 6 1 , 0 1 :Find that removes undesired response modes j j j j j j V x I x V δ α δ = = =   + ∆= +    ∆ ∑ ∑
  • 16. 16 Sample Deployment into Relative Orbits: 1-∆V at Injection Origin = Chief S/C Deputy S/C Quasi-Periodic Origin = Chief S/C 3 Deputies “Periodic” 1800 days
  • 17. 17 Natural Formations: Nearly Periodic and Drifting Relative Orbits Chief S/C @ Origin 1800 days
  • 18. 18 Expansion of Drifting Vertical Orbit Origin = Chief S/C ( )0r ( )fr t 18,000 days = 100 Revolutions
  • 19. 19 Transitioning Natural Motions into Non-Natural Arcs: Targeter Approach STEP 1: Identify a suitable initial guess Target  Orbital Drift Control
  • 20. 20 Application of Two Level Corrector ( )qTΓ ( )0r t ( )mr t ( ) ( )0mr t r t= ( )qV T∆ STEP 2: Apply 2-level corrector (Howell and Wilson:1996) w/ end-state constraint STEP 3: Shift converged patch states forward by 1 period STEP 4: Reconverge Solution
  • 21. 21 Drift Controlled Vertical Orbit (6 Revs) ( ) 3 5 m/sec 1 maneuver/year V∆ = −
  • 22. 22 Geometry of Natural Solutions in the Ephemeris Model w/ SRP Inertial Frame Perspective: Rotating Frame Perspective:
  • 23. 23 Transitioning Natural Motions into Non-Natural Arcs: IFL Example (1) Consider 1st Rev Along Orbit #4 as initial guess to simple targeter. (2) Choose initial state on xz-plane (3) Target next plane crossing to be ⊥ (4) Use resulting arc as half of the reference motion. (5) Numerically mirror solution about xz-plane and store as nominal. (6) Use IFL control to enforce a closed orbit using stored nominal. Chief S/C @ Origin Sphere for Visualization Only
  • 24. 24 Hybrid Control: Natural Motions + Continuous Control ½ Period  Natural Arc ½ Period  IFL Control
  • 25. 25 Concluding Remarks • Precise Formation Keeping → Continuous Control – Is it possible? • Depends on hardware capabilities and nominal motion specified • Not if thruster On/Off sequences are required & tolerances too high • Precise Navigation → Natural Formations – Targeter Methods • Natural motions can be forced to follow non-natural paths • Success depends on non-natural motion specified – Hybrid Methods (Natural Arcs + Continuous Thrust Arcs) • May prove beneficial for non-natural inertial formation design.
  • 28. 28 ( ) 1/2 Range + Range Rate Constraint: T f f f T f f f f f r r r g r rr r      = =            ( ) ( ) ( ) ( ) STM * 0 0 0 0 0 0 State Relationship Matrix , ,f f f r r g x r r d g g g x t t x t t x r rx r t x r δ δ δ ∂ ∂   ∂ ∂ ∂ ∂ = − = = Φ = Φ  ∂ ∂∂ ∂    ∂ Λ ∂       * 0 0 First Order Approximation: f f g g g x x δ ∂ = + ∂ Radial Targeter: Control Law Formulation * * Desired Range + Range Rate: 0 f f r g   =    
  • 29. 29 Dynamical Model ( ) ( ) ( ) ( ) ( ) 2 22 2 2 3 3 1, 2, s j j s js s j j s P P P P PP N P PP P P P P P sr PI j j s p r r u tr r r r ft µ µ = ≠    − + −  =      + +∑ Gravity Terms Solar Radiation Pressure Control InputGeneralized Dynamical Model for Each S/C: ( ) ( ) Assumptions: Chief S/C Evolves Along Natural Solution 0 (Nominal) Deputy S/C Evolves Along Non-Natural Solution 0 c d u t u t → ∴ = → ∴ ≠
  • 30. 30 Chief S/C Motion: Natural Solutions Near L1 and L2 “Halo”OrbitsNearLi LissajousTrajectoriesNearLi Sun Sun
  • 31. 31 Controlled Deputy S/C Motion (Example 1): Formation Fixed in the Rotating Frame Chief S/C Deputy S/C ˆyρ ρ= C(t1) C(t2) C(t3) C(t4) D(t1) D(t2) D(t3) D(t4)
  • 32. 32 X [au] Y[au] Controlled Deputy S/C Motion (Example 2): Formation Fixed in the Inertial Frame ˆYρ ρ=Chief S/C Deputy S/C C(t1) C(t2)C(t3) C(t4) D(t1) D(t2)D(t3) D(t4)
  • 37. 37 Radial Error wrt. Hub S/C Thrusters off = 100,000 sec W Wr r−  Nominal Radial Vector in UVW Coordinates Actual Radial Vector in UVW Coordinates
  • 38. 38 Free Flyers UV-Plane Angular Drift (DEG) ν ν−  ε ε−  Nominal Actual Nominal Actual
  • 39. 39 Thrust Profile Thrusters Off Between t1 = 1 day & t2 = t1 + 100,000 sec. A B C ( )O 0.05 Nµ ( )O 0.05 Nµ 3 mN≈ 3 mN≈
  • 41. 41 Target Reconfiguration ˆX ˆZ ˆY Detector Target #11 ˆw 1 ˆu 2 ˆw 2 ˆu Target #2 1 ˆv 2 ˆv Hub (t1): α = 0°, δ = 0° Hub (t2): α = 0°, δ = 0°
  • 42. 42 Graphical Representation of Reconfiguration for Free Flyers 1 ˆˆ ||w X 2 ˆ ˆ||w Y INITIAL ORIENTATION OF UV-PLANE FINAL ORIENTATION OF UV-PLANE
  • 43. 43 Thrust to Reconfigure From α = 0o to α = 90o with δ = 0o 1 | ˆˆ |w X 2 ˆ ˆTarget: ||w Y Reconfiguration Time Increased to 7 days to reduce Detector S/C Control Thrust
  • 44. 44 Mission Specifications • Hold periscope positions to within 15-µm • Detector pointing accuracy – arcminutes • ∠ Periscope-Detector-Target alignment – µas • Phase 1  1 Target /week • Phase 2  1 Target/ 3 weeks • Hub  inter. comm. port between detector & freeflyers • Reconfiguration (Formation Slewing) Times: – 1 Day for Phase 1 – 1 Week for Phase 2 • Propulsion – Formation Slewing  0.02 N (Hydrazine) – Formation keeping  0.03 mN (PPTs) Frequent Reconfigurations
  • 46. 46 Natural Formations: String of Pearls ˆx ˆy ˆz ˆz ˆy ˆx
  • 47. 47 Deployment into Torus (Remove Modes 1, 5, and 6) Origin = Chief S/C Deputy S/C ( ) [ ] ( ) [ ] 0 5 00 0 m 0 1 1 1 m/sec r r = = −
  • 48. 48 Deployment into Natural Orbits (Remove Modes 1, 3, and 4) Origin = Chief S/C 3 Deputies ( ) [ ] ( ) [ ] 00 0 0 m 0 1 1 1 m/sec r r r = = −
  • 50. 50 OFL Controlled Response of Deputy S/C Radial Distance Tracking 2 ( ) ( ) ( )2 , Tg r r r r r u t r r f r r rr      = − + − ∆             3 4 ( ) ( ) ( )2 2 ,1 2 Tg r r r r u t r f r r r    = − − ∆        ( ) ( ) ( )2 , 3 T r r r u t rg r r r r f r rr     = − − + − ∆           Control Law ( ) ( ), ˆ H r r u t r r =  Geometric Approach: Radial inputs only1 1u 3u 2u 4u Chief S/C @ Origin (Inside Sphere)
  • 51. 51 OFL Controlled Response of Deputy S/C Radial Distance + Rotation Rate Tracking * 5 kmr = 1 rev / 6 hrs 1 rev / 1 day Chief S/C @ Origin (Inside Sphere)
  • 52. 52 Impact Commanded Rotation Rate on Cost 1 rev /24 hrs 0.19 mN 1 rev /12 hrs 0.76 mN 1 rev / 6 hrs 6.40 mN 1 rev / 1 hrs 106.50 mN → → → → 700 kgsm =
  • 54. 54 Parameterization of Parabolic Formation pa ph pu ν ( )3 ˆ focal linee 1 ˆe Nadir q 1 2 3 ˆ ˆ ˆiCD Er xe ye ze= + +   Chief S/C (C) iDeputy S/C (D ) { } i i i i CD CD TI EE I CD CDE I E I r r C r r     =         : inertially fixed focal frame : inertially fixed ephemeris frame E I / cos / sin p p p p p p p x a u h y a u h z u q ν ν = = = +    Zenith Transform State from Focal to Ephemeris Frame
  • 55. 55 Controller Development ( ) ( ) ( ) ( ) ( ) ( ) ( ) ( )( ) ( ) 2 2 2 2 2 2 2 2 2 2 2 2 2 2 22 2 2 2 2 0 , 2 2 2 1 , 0 2 u x y x y q x y z z h h h x y g u u x y x f y f a a au h h h x y u g q q x y x f y f f a a a u x y xx yy xy yx gx y x y x y ν ν     − + + ∆ + ∆        − − = + + + ∆ + ∆ − ∆          + −−  + ++ +   +                                        ( ) ( )2 2 x yy f x f x y                ∆ − ∆    +       ( ) ( ) ( ) ( ) ( ) ( ) ( ) ( ) * * 2 * * * * * 2 * , 2 , 2 u p p p n p p n p p q p p n n n g u g u u u u u u g u u q q q q k q ν ν ν ω ν ω ω ω ω ν = − − − − = − − − − =− −             Desired Response for , , and :u q ν Solve for Control Law: , critically dampedu qδ δ → exponential decayδθ →
  • 56. 56 OFL Controlled Parabolic Formation ˆX ˆZ ˆY 0t 0 1.6 hrst + 0 3.8 hrst + 0 8 hrst + 0 5 dayst + 0 6 dayst + 3 ˆe 10 km 1 rev/day 500 m 500 m Phase I: 200 m Phase II: 300 m /1 day Phase III: 500 m p p p p p q h a u u u ν = = = = = = =  
  • 58. 58 New Maxim Pathfinder Science Phase #2 High Resolution (100 nas) 20,000 km 1 km http://maxim.gsfc.nasa.gov/documents/SPIE-2002/spie2002.ppt
  • 59. 59 Maxim Configuration Example 19,500km 1 rev/day 500 m 1 km 1 km p p p q u h a ν = = = = =  700 kgsm =
  • 61. 61 Formulation ( ) ( ) ( ) ( ) 11 1 0 0 min , , , , i i tN N N i i i N i i t J x L t x u x L t x u d tφ φ +− − = = =+ =+∑ ∑ ∫  Subject to: ( ) ( )1 0, , ; Subject to 0i i i ix F t x u x x+ = ( ) ( ) ( ) ( ) ( ) ( ) ( ) ( ) 1 1 1 1 1 1 0 0 min , , , , ; , , Subject to 0 N n N N i i i i i i i i n i n i i i i J x x t x x F t x u x F t x u x t x t L t x u x x φ φ+ + + + + + = + =    = = =   +      =          Equivalent Representation as Augmented Nonlinear System:
  • 62. 62 Euler-Lagrange Optimality Conditions (Based on Calculus of Variations) ( ) 1 1 Condition #1: 1 Condition #2: 0 ; 0, , 1 NT T Ti i i N i N Ti i i i i i i xH x x F x F N u H i u φ λ λ λ λ + + ∂ ∂ ∂ ∂ ∂ = = → =   ∂ ∂  ∂ ∂ = = = − ∂          ( )1 , ,T i i i i iH F t x uλ +=   Identify and from augmented linear system.i i i i F F x u ∂ ∂ ∂ ∂   
  • 63. 63 Identification of Gradients From the Linearized Model ( ) ( ) ( ) ( ) ( )x t A t x t B t u tδ δ δ= +    ( ) ( ) 0 0 A t A t L x    = ∂   ∂    ( ) 3 3 0 0T B t I    =       ( ) ( ) ( ) ( ) 0 11 0, , ; 0 0, , nn x xf t x ux xL t x ux ++        = =               Augmented Nonlinear System: Augmented Linear System:
  • 64. 64 Solution to Linearized Equations ( ) ( ) ( ) ( ) ( ) ( ) ( ) ( ) ( ) 0 0 0 0 0 0 0 7 , , , , ; , t t x t t t x t B u d t t A t t t t t I δ δ τ τ δ τ τ=Φ + Φ Φ = Φ Φ = ∫     i F x ∂ ∂   Relation to Gradients in E-L Optimality Conditions: ( ) ( ) ( ) ( ) 1 1 1 1, , i i t i i i i i t x t t x t B u dδ δ τ τ δ τ τ + + + +=Φ + Φ∫ 
  • 65. 65 Control Gradient for Impulsive Control ( ) ( )( ) ( ) ( ) 1 1 1 1 1 , , , , i i i i i i i i i i i i i i x t t x t t x B V t t x t t B V δ δ δ δ − + + + − + − + + = Φ =Φ + ∆ = Φ + Φ ∆       i F u ∂ ∂  ( )1,i i i F t t B u + ∂ = Φ ∂  
  • 66. 66 Control Gradient for Constant Thrust Arcs ( ) ( ) ( ) 1 1 1 1, , i i t i i i i i i t x t t x t B d uδ δ τ τ τ δ + + + +   =Φ + Φ     ∫  i F u ∂ ∂  ( ) ( ) ( ) 1 1 1, , i i t i i i i t F t t t B d u τ τ τ + − +  ∂ =Φ Φ  ∂    ∫  ( ) ( ) ( ) ( ) ( ) ( ) ( ) 1 1* , , , , ,, ,, n i i ii x f t x u x L t x u A t t tt t t t Bt t + −            =   ΦΦ       ΦΦ         Equations to Integrate Numerically
  • 67. 67 Numerical Solution Process: Global Approach ( ) 0(1) ; ( 0,1,..., 1) (2)1-Scalar Equation to Optimize in 3 1 Control Variables Use optimizer to identify optimal Input , , and initia given . During each iteratio l guess for n i i N i i i N N H u x u u t = − − ∂ ∂  ( ) ( ) ( ) Sequence forward and store of the optimizer, the following steps are followed: ( ) Evaluate cost functional, ( ) Evaluate 1 ; 1 ( , , 1 N NT N N N i N b J x x c x x a x i N d φ φ φ λ = … − = ∂  ∂ = =   ∂ ∂       ( ) ) Sequence backward and compute ; 1, ,1 and used in next update of control input. i i i i i H i N u H e J u λ ∂ = − ∂ ∂ ∂  
  • 68. 68 Formulation ( ) ( ) ( ) ( ) 11 1 0 0 min , , , , i i tN N N i i i N i i t J x L t x u x L t x u d tφ φ +− − = = =+ =+∑ ∑ ∫  Subject to: ( ) ( )1 0, , ; Subject to 0i i i ix F t x u x x+ = ( ) ( ) ( ) ( ) ( ) ( ) ( ) ( ) 1 1 1 1 1 1 0 0 min , , , , ; , , Subject to 0 N n N N i i i i i i i i n i n i i i i J x x t x x F t x u x F t x u x t x t L t x u x x φ φ+ + + + + + = + =    = = =   +      =          Equivalent Representation as Augmented Nonlinear System:
  • 69. 69 Impulsive Optimal Control Minimize State Error with End-State Weighting ( ) ( ) ( ) ( ) 11 0 1 1 min 2 2 i i tN T T N N N N i t J x x W x x x x Q x x d t +− = = − − + − −∑ ∫    
  • 70. 70 State Corrector vs. Nonlinear Optimal Control: Cost Function
  • 71. 71 State Corrector vs. Nonlinear Optimal Control: Impulsive Maneuver Differences
  • 72. 72 Impulsive Radial Optimal Control ( ) 11 2 0 1 min 2 i i tN i t J q r r dt +− = = −∑ ∫ 
  • 74. 74 State Corrector vs. Nonlinear Optimal Control: Cost Function
  • 75. 75 RANGE + RANGE RATE TARGETER
  • 76. 76 Comparison of Range and State Targeters
  • 77. 77 Range Targeter: Spatial Behavior of Corrected Solution Chief S/C at Origin Deputy S/C Path