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International Journal of Modern Engineering Research (IJMER)
Vol. 3, Issue. 5, Sep - Oct. 2013 pp-3242-3247
ISSN: 2249-6645

Analytic Model of Wind Disturbance Torque on Servo
Tracking Antenna
Tushar Golani1, Suresh Sabhapathy2
1

Spacecraft Checkout Group, ISRO Satellite Centre, Bangalore 560 017
Giant Metrewave Radio Telescope, Tata Institute of Fundamental Research, Pune 410 504

2

ABSTRACT: The paper develops an analytic wind disturbance torque model that can be used to simulate antenna servo
errors. The forces due to wind acting on antenna induce torque that creates servo errors which become significant in slow
tracking antennas. The model developed is based on the vector sum of torque acting on the antenna and is analytically
computed by disintegrating the forces due to wind in mutually orthogonal directions. The demarcation between the existing
field models of wind disturbances and the model presented in this article is brought out by the generalization of torque
induced with the only variable antenna specific parameter being the porosity.

Keywords: Antenna servo errors, antenna torque, field model, mutually orthogonal, wind disturbance
I.

INTRODUCTION

Large antennas are required to capture feeble signals, especially those received from space. Radio telescopes that
track astronomical phenomenon and inter planetary satellite tracking antennas fall under these categories. These tracking
antennas require very high pointing accuracies and thereby a robust servo control system. The large structures associated
with these antennas in ideal conditions require a second-order time invariant feedback controller1. However, these large
structures are affected by torques generated by wind disturbances. The torque results in large servo errors, which reduce the
pointing accuracies of antennas. The requirement of high pointing accuracy antennas call for wind torque disturbance models
that can accommodate the induced servo errors. The existing models2 are field models specific to antennas and thus, require
extensive fieldwork before they can be used for designing the servo control loop. The model presented here is generalized
for large antenna structures and depends only on one antenna specific parameter. The parameter is the resistance offered by
the antenna to wind and is characterized by the porosity of the antenna 2.
The article presented develops an analytic method which employs vector mechanics to calculate the torques
generated about a point. The model was conceptualized at Tata Institute of Fundamental Research during servo control
design for 45 meter Giant Meterwave Radio Telescope at Pune.

II.

THE ANALYTIC MODEL FOR WIND DISTURBANCE TORQUE

The wind disturbance generates torque that is the main cause of servo errors for tracking antenna. The wind torque
generated can be analytically expressed as vector sum of torques generated in two mutually perpendicular axes. The
determination of wind force from wind velocity is the preliminary modeling step. The force due to wind is calculated using
the pressure exerted by wind by virtue of its velocity.
2.1 Obtaining Wind Force from Wind Velocity
An antenna exposed to uniformly blowing wind is acted upon by pressure given by 1/2 𝜌𝑣 2 where
𝑤
𝜌is the density of air;
𝑣 𝑤 is the uniform velocity with which wind is blowing.
The force acting on an area A due to pressure P in quantized as the product of the P and A. Generalized force on antenna of
cross sectional area A due to wind is given by Eqn (1).
𝐹 = 𝜂1 𝜂2 𝑃𝐴

(1)

Where
𝜂1 is a measure of porosity of the antenna
𝜂2 is a factor less than 1 that takes into account the relative orientation of the wind, w.r.t. the antenna.
Fig 1 illustrates the interaction of wind with the cross sectional area of an antenna.

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3242 | Page
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International Journal of Modern Engineering Research (IJMER)
Vol. 3, Issue. 5, Sep - Oct. 2013 pp-3242-3247
ISSN: 2249-6645

Fig 1: The force generated is a function of wind velocity, area offered by the antenna against wind, porosity of the antenna
and the relative orientation of the antenna w.r.t wind.
The wind velocity so far is assumed to be constant. However, it is a function of the height above ground level. The forces
experienced by the antenna therefore, vary along the height. The unbalanced forces at the top of the antenna and bottom of
the antenna generate torque. The unbalanced force vectors are illustrated in Fig 2.

.

Fig 2: Unbalanced forces due to varying wind velocity generate torque.
The force due to wind is distributed over the entire area of the antenna. However, single vector sum of forces acting on O 1
and O2 can be calculated which shall produce the same torque as distributed forces would have produced. The vectors are
given by Eqns (2-3).
𝐹1 − 𝐹2 = 𝐹𝑢𝑝
(2)
𝐹3 − 𝐹4 = 𝐹 𝑑𝑜𝑤𝑛
(3)
O1 and O2 are points on the upper and lower half of discs, where a resultant single vector force shall produce the same
effects as distributed force.
2.2 Variation of Wind Velocity: Hellman’s Equation
Hellman‟s equation relates the velocity of wind w.r.t altitude above the earth‟s surface. (The equation is assumed
valid as long as density of air remains constant, within the altitude range or in other words, thinning of air as one goes up is
not taken into consideration).
𝑣 𝑤 ℎ = 𝑣𝑜

ℎ

𝛼

(4)

ℎ𝑜

Where
𝛼is the Hellman coefficient
𝑣 𝑜 is velocity of wind at reference altitude
𝑣 𝑤 (ℎ)is velocity of wind at height h
𝛼 can be measured on a day when winds are steady. To measure 𝛼 , velocity at two points of antenna can be measured and
the equation can be solved for 𝛼. The measurement can be repeated for precision. To further nullify the effect of wind-gusts,
velocity of wind can be taken over finite time duration and wind-gusts being random the velocity of wind will deviate
about the steady state wind velocity. Since wind gusts follow Davenport spectrum, the measured 𝛼 deviates as dictated by
Davenport spectrum.
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3243 | Page
International Journal of Modern Engineering Research (IJMER)
www.ijmer.com
Vol. 3, Issue. 5, Sep - Oct. 2013 pp-3242-3247
ISSN: 2249-6645
2.3 The Case of Face on Wind: Perpendicular Attack
The perpendicular attack case is the worst case as the whole cross-section of the antenna is exposed to the wind.
Fig 3 illustrates the case of perpendicular attack. To calculate force we need an elemental area over which the force is
constant. The area is basically a horizontal strip that is at a distance x from the center and is of width dx. The strip
subtends an angle 𝜃 at the center of parabolic disc. The strip‟s center subtends an angle𝜙 at O as illustrated
in Fig 4. The strip is the differential element for torque calculation.

Fig 3: The varying wind velocities are illustrated with different vector lengths. The shaded strip is the part of antenna that
encounters equal velocity wind. The differential element for torque calculation is the strip that faces perpendicular force of
wind.

Fig 4: The differential element subtends an angle of 𝜙at O, which is the point about which the moment is calculated. O
being d distance away from the center of disc.
Torque calculation requires calculating the force acting on the elemental strip as a function of wind velocity and distance
from the center of the parabolic disc A. Fig 5 serves as reference for further analysis.

Fig 5: The elemental strip faces constant velocity wind. The center of the circular cross-section is A. The strip subtends 𝜃 at
A, is x distance away from A and is of width dx.
The area of the elemental strip in polar coordinates is given by Eqn (5).
𝑑𝐴 = −2𝑅2 𝑠𝑖𝑛2 𝜃𝑑𝜃
(5)
The inclination of antenna is 90o w.r.t wind. Therefore, 𝜂2 is 1. Referring to Eqn (1) the force on the elemental strip can be
given as in Eqn (6).
𝑑𝐹 = 1/2 𝜂1 𝜌𝑣 2 × 𝑑𝐴
(6)
𝑤
The velocity of wind as a function of height above ground level can be substituted as per Eqn (4), while the elemental area of
the strip is substituted from Eqn (5). Eqn (6) modifies to Eqn (7).
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3244 | Page
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𝑑𝐹 = 1/2 𝜂1 𝜌 𝑣 𝑜

𝛼 2

ℎ
ℎ𝑜

International Journal of Modern Engineering Research (IJMER)
Vol. 3, Issue. 5, Sep - Oct. 2013 pp-3242-3247
ISSN: 2249-6645

× −2𝑅2 𝑠𝑖𝑛2 𝜃𝑑𝜃

(7)

If center of the circle shown in Fig 5 is taken as the reference, the height parameter in Eqn (7) equals x. Substituting x in
polar coordinates in Eqn (7) in place of h yields Eqn (8).
𝑑𝐹 = 1/2 𝜂1 𝜌 𝑣 𝑜

𝑅𝑐𝑜𝑠𝜃

𝛼 2

ℎ𝑜

× −2𝑅2 𝑠𝑖𝑛2 𝜃𝑑𝜃

(8)

The force on the differential element produces a turning moment about the hinge of antenna. The magnitude of the generated
torque is analytically found by multiplying the rotational arm length for the element or the distance of the differential
element from O with the component of dF perpendicular to the rotational arm. Fig 6 illustrates the force vectors and the
rotational arm lengths about O.

Fig 6: (a) Figure illustrating the angular span of the parabolic disc about O. The radius of the dish being R. (b) Figure
showing the resolution of forces perpendicular to the rotational arm r. (c) Figure illustrating the relation between radius R of
the antenna dish, angular span 𝜙 𝑜 and distance d.
The elemental torque (𝑑𝜏 𝑢𝑝 ) on the elemental strip in the upper half of the parabolic strip is given by Eqn (9).
𝑑𝜏 𝑢𝑝 = 𝑑𝐹𝑠𝑖𝑛𝜙 × 𝑟
(9)
The force on the elemental strip is calculated in Eqn (8) and substituting r as 𝑑 𝑐𝑜𝑠∅ from Fig 6, we have the torque on the
elemental strip as
𝑑𝜏 𝑢𝑝 = −1/2 𝜂1 𝜌 𝑣 𝑜

𝑅𝑐𝑜𝑠𝜃

𝛼 2

ℎ𝑜

× 2𝑅2 𝑠𝑖𝑛2 𝜃𝑑𝜃 × 𝑑 × 𝑡𝑎𝑛∅ × 𝑑∅

(10)

Integrating Eqn (10) with limits for 𝜃 and ∅ the torque on the upper half disc can be calculated as shown in Eqn (11).
𝜏
0

𝑑𝜏 𝑢𝑝 =

𝜋/2
𝜃 =0

𝜙𝑜
𝜂
𝜙 =0 1

𝜌 𝑣𝑜

𝑅𝑐𝑜𝑠𝜃
ℎ𝑜

𝛼 2

× 𝑅2 𝑠𝑖𝑛2 𝜃𝑑𝜃 × 𝑑 × 𝑡𝑎𝑛∅ × 𝑑∅ 𝑑𝜃

(11)

The limits for 𝜃 are reversed to absorb the negative sign in dF expression. The torque for the lower half of the dish can be
found by placing proper limits and appropriate expression for the velocity of wind. The antenna here faces the wind
perpendicularly; however, tracking antenna may be inclined at some angle to the wind velocity. The next section takes into
account the parameter 𝜂2 .
2.4 Antenna Inclined w.r.t the Wind: Angular Attack
The most generalized torque generating case is that of an inclined antenna against arbitrary direction of wind. The
assumption here is that the wind follows Hellman‟s velocity relation, only the direction is arbitrary. Consider the antenna to
be inclined at angle 𝜉as illustrated in Fig 7. Wind force is resolved into three mutually perpendicular components and torque
due to each component is measured and generalized for parameter 𝜉.

O

Fig 7: (a) Figure illustrating the inclination of the antenna w.r.t wind. (b) The resolved components of force vector. (c)
Figure illustrating the angular span of the antenna about reference O.
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3245 | Page
International Journal of Modern Engineering Research (IJMER)
www.ijmer.com
Vol. 3, Issue. 5, Sep - Oct. 2013 pp-3242-3247
ISSN: 2249-6645
The three mutually perpendicular force vectors are depicted in Fig 7 (b). Fw1 is the direction considered earlier for
perpendicular attack. Fw3 sees the parabolic lateral face analyzed in the next section and Fw2 is in the vertical direction. The
case of wind blowing vertically is seldom encountered and especially when the region experiences tornados and hurricanes.
The differential force on the element is illustrated in Fig 8. The corresponding parameters are depicted in the triangle. The
component of the force perpendicular to the moment arm is 𝑑𝐹 𝑤1 𝑠𝑖𝑛𝜙. The element is at a distance r from O. As compared
to the case of perpendicular case the element is at an inclination of 𝜉 w.r.t the wind. InΔ𝐴𝐵𝑂, the relation between sides and
angles can be determined by applying Sine Law as in Eqn (12).
𝑟
𝑑
=
(12)
𝑠𝑖𝑛𝜉

sin 𝜋− 𝜙 +𝜉

Applying Sine Law for the triangles in Fig 7 (c) we arrive at Eqns (13-14)
𝑅
𝑑
=
𝑠𝑖𝑛 𝜙 01
𝑅
𝑠𝑖𝑛 𝜙 02

sin

=

sin

(13)

𝜙 01 +𝜉
𝑑

𝜉 −𝜙 02

(14)

𝑑𝐹 𝑤1 𝑠𝑖𝑛𝜙
𝑑𝐹 𝑤1
∅
𝑟

𝑑𝐹 𝑤1 𝑐𝑜𝑠𝜙

∅

O

B

𝜉

𝑑

A

Fig 8: Figure illustrating the force vectors for the differential element. r is the distance of the element from O, d is the
distance of center A from O. and being the angle subtended by the elemental strip at O and A respectively.
The differential torque is given by Eqn (9). Substituting r from Eqn (12) and dF from Eqn (8) in Eqn (9), the
differential torque on the element can be expressed by Eqn (12).
𝑑𝜏 𝑢𝑝 = −𝜂1 𝜌 𝑣 𝑜

𝛼 2

𝑅𝑐𝑜𝑠𝜃
ℎ𝑜

× 𝑅2 𝑠𝑖𝑛2 𝜃𝑑𝜃 ×

𝑑𝑠𝑖𝑛𝜉
sin ⁡ +𝜙)
(𝜉

× 𝑠𝑖𝑛∅ × 𝑑∅

(15)

The torque on the upper half of the antenna can be obtained by integrating Eqn (15) with limits for 𝜃 and 𝜙. The limits for 𝜙
is from 0 to𝜙01 , where 𝜙01 is obtained from Eqn (13).
𝜏
0

𝑑𝜏 𝑢𝑝 =

𝜋/2
𝜃 =0

𝜙 𝑜1
𝜙 =0

𝜂1 𝜌 𝑣 𝑜

𝑅𝑐𝑜𝑠𝜃

𝛼 2

ℎ𝑜

× 𝑅2 𝑠𝑖𝑛2 𝜃𝑑𝜃 ×

𝑑𝑠𝑖𝑛𝜉
sin ⁡ +𝜙 )
(𝜉

× 𝑠𝑖𝑛∅ × 𝑑∅ 𝑑𝜃 (16)

2.5. Torque on the Lateral Surface
The antenna employed for tracking is mostly a parabolic antenna. The lateral cross- section thus is a parabola. Fig 9
shows the parameters for a parabolic cross-section. The parabola can be mathematically represented by Eqn (17).
𝐾
𝑦 = 2 𝑚2
(17)
𝑅
The elemental area in this case is the product of length of the strip with its width and can be expressed by Eqn (18)
𝑑𝐴 = 𝑙 × 𝑑𝑥
(18)
The length of the strip is mathematically the difference between the depth of the parabola K and z.
𝑙 = 𝐾− 𝑧= 𝐾 1−

𝑥2

(19)

𝑅 2 𝑐𝑜𝑠 2 𝜉

The differential area thus obtained can be substituted in the expression for torque dictated by Eqn (10). The porosity of the
antenna may differ as the lateral side now offers resistance to wind. The moment arm in this case is x as the torque is
generated about mm’
𝑑𝜏 𝑢𝑝 = 1/2 𝜂1′ 𝜌 𝑣 𝑜

𝑅𝑐𝑜𝑠𝜃

𝛼 2

ℎ𝑜

× 𝐾 1−

𝑥2
𝑅 2 𝑐𝑜𝑠 2 𝜉

× 𝑑𝑥 × 𝑥

(20)

Eqn (20) can be integrated over the upper half antenna to obtain the total torque experienced by the upper half part of the
dish. Since, this expression does not use polar coordinates the torque expression is a single integral as shown in Eqn (21).
𝜏 𝑢𝑝
0

𝑑𝜏 𝑢𝑝 =

𝑅𝑠𝑖𝑛𝜉
𝑥=0

1/2 𝜂1′ 𝜌 𝑣 𝑜

𝑅𝑐𝑜𝑠𝜃
ℎ𝑜

𝛼 2

× 𝐾 1−

𝑥2
𝑅 2 𝑐𝑜𝑠 2 𝜉

× 𝑑𝑥 × 𝑥

(21)

The torque for the lower half of the antenna can be expressed with the same equation but with different limits.

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International Journal of Modern Engineering Research (IJMER)
Vol. 3, Issue. 5, Sep - Oct. 2013 pp-3242-3247
ISSN: 2249-6645

Fig 9: Figure illustrating the lateral cross-section of the parabola with its parameters

III.

CONCLUSION AND FUTURE SCOPE

The paper develops a mathematical model for wind disturbance torque on tracking antenna. The vector approach to
torque calculation in case of antenna requires only porosity of the antenna as the variable parameter to be as compared to the
numerous antenna specific coefficients that need to be calculated while opting for field models of wind disturbance torques.
The model here has considered antenna as a single entity, however, a finite element analysis of antenna structure still needs
to be explored.

REFERENCES
[1.]
[2.]
[3.]

[4.]
[5.]
[6.]

W. Gawronski, “Wind Gust Models Derived From Field Data,” The Telecommunications and Data Acquisition Progress Report
42-123, July–September 1995, Jet Propulsion Laboratory, Pasadena, California, pp. 30–36, November 15, 1995.
W. Gawronski and J. A. Mellstrom, “Control and Dynamics of the Deep Space Network Antennas,” in Control and Dynamics
Systems, C. T. Leondes, ed.,vol.
63, San Diego, California: Academic Press.
W. Gawronski, B. Bienkiewicz, and R. E. Hill, “Pointing-Error Simulations of the DSS-13 Antenna Due to Wind Disturbances,”
The Telecommunications and Data Acquisition Progress Report 42-108, October–December 1991, Jet Propulsion Laboratory,
Pasadena, California, pp. 109–134, February 15, 1992.
Norman S. Nise, Control System Engineering, 4th edition, Wiley Education
Press.
BC Joshi,”Simulation Study of Servo Control System of 45 meter Giant
Metrewave Radio
Telescope”.
www.ncra.tifr.res.in

ABOUT THE AUTHOR
Tushar Golani received his B.Tech from Indian Institute of Space Science and Technology,
Thiruvananthapuram. He joined ISRO Satellite Centre in 2011 and is currently working in Spacecraft
Checkout Group. His areas of interest include control systems, analog and digital circuit design and
embedded systems. He is elected as a life member of the Astronautical Society of India (ASI) and
Associate Member of the Aeronautical Society of India (AeSI).
Suresh Sabhapathy is appointed as Engineer-„F‟ at the Giant Metrewave Radio Telescope facility of
TIFR. He is the group coordinator of the servo control systems group and is actively working in the
field of linear and non-linear control of large structures. He has guided several students in the field of
servo control systems.

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3247 | Page

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Analytic Model of Wind Disturbance Torque on Servo Tracking Antenna

  • 1. www.ijmer.com International Journal of Modern Engineering Research (IJMER) Vol. 3, Issue. 5, Sep - Oct. 2013 pp-3242-3247 ISSN: 2249-6645 Analytic Model of Wind Disturbance Torque on Servo Tracking Antenna Tushar Golani1, Suresh Sabhapathy2 1 Spacecraft Checkout Group, ISRO Satellite Centre, Bangalore 560 017 Giant Metrewave Radio Telescope, Tata Institute of Fundamental Research, Pune 410 504 2 ABSTRACT: The paper develops an analytic wind disturbance torque model that can be used to simulate antenna servo errors. The forces due to wind acting on antenna induce torque that creates servo errors which become significant in slow tracking antennas. The model developed is based on the vector sum of torque acting on the antenna and is analytically computed by disintegrating the forces due to wind in mutually orthogonal directions. The demarcation between the existing field models of wind disturbances and the model presented in this article is brought out by the generalization of torque induced with the only variable antenna specific parameter being the porosity. Keywords: Antenna servo errors, antenna torque, field model, mutually orthogonal, wind disturbance I. INTRODUCTION Large antennas are required to capture feeble signals, especially those received from space. Radio telescopes that track astronomical phenomenon and inter planetary satellite tracking antennas fall under these categories. These tracking antennas require very high pointing accuracies and thereby a robust servo control system. The large structures associated with these antennas in ideal conditions require a second-order time invariant feedback controller1. However, these large structures are affected by torques generated by wind disturbances. The torque results in large servo errors, which reduce the pointing accuracies of antennas. The requirement of high pointing accuracy antennas call for wind torque disturbance models that can accommodate the induced servo errors. The existing models2 are field models specific to antennas and thus, require extensive fieldwork before they can be used for designing the servo control loop. The model presented here is generalized for large antenna structures and depends only on one antenna specific parameter. The parameter is the resistance offered by the antenna to wind and is characterized by the porosity of the antenna 2. The article presented develops an analytic method which employs vector mechanics to calculate the torques generated about a point. The model was conceptualized at Tata Institute of Fundamental Research during servo control design for 45 meter Giant Meterwave Radio Telescope at Pune. II. THE ANALYTIC MODEL FOR WIND DISTURBANCE TORQUE The wind disturbance generates torque that is the main cause of servo errors for tracking antenna. The wind torque generated can be analytically expressed as vector sum of torques generated in two mutually perpendicular axes. The determination of wind force from wind velocity is the preliminary modeling step. The force due to wind is calculated using the pressure exerted by wind by virtue of its velocity. 2.1 Obtaining Wind Force from Wind Velocity An antenna exposed to uniformly blowing wind is acted upon by pressure given by 1/2 𝜌𝑣 2 where 𝑤 𝜌is the density of air; 𝑣 𝑤 is the uniform velocity with which wind is blowing. The force acting on an area A due to pressure P in quantized as the product of the P and A. Generalized force on antenna of cross sectional area A due to wind is given by Eqn (1). 𝐹 = 𝜂1 𝜂2 𝑃𝐴 (1) Where 𝜂1 is a measure of porosity of the antenna 𝜂2 is a factor less than 1 that takes into account the relative orientation of the wind, w.r.t. the antenna. Fig 1 illustrates the interaction of wind with the cross sectional area of an antenna. www.ijmer.com 3242 | Page
  • 2. www.ijmer.com International Journal of Modern Engineering Research (IJMER) Vol. 3, Issue. 5, Sep - Oct. 2013 pp-3242-3247 ISSN: 2249-6645 Fig 1: The force generated is a function of wind velocity, area offered by the antenna against wind, porosity of the antenna and the relative orientation of the antenna w.r.t wind. The wind velocity so far is assumed to be constant. However, it is a function of the height above ground level. The forces experienced by the antenna therefore, vary along the height. The unbalanced forces at the top of the antenna and bottom of the antenna generate torque. The unbalanced force vectors are illustrated in Fig 2. . Fig 2: Unbalanced forces due to varying wind velocity generate torque. The force due to wind is distributed over the entire area of the antenna. However, single vector sum of forces acting on O 1 and O2 can be calculated which shall produce the same torque as distributed forces would have produced. The vectors are given by Eqns (2-3). 𝐹1 − 𝐹2 = 𝐹𝑢𝑝 (2) 𝐹3 − 𝐹4 = 𝐹 𝑑𝑜𝑤𝑛 (3) O1 and O2 are points on the upper and lower half of discs, where a resultant single vector force shall produce the same effects as distributed force. 2.2 Variation of Wind Velocity: Hellman’s Equation Hellman‟s equation relates the velocity of wind w.r.t altitude above the earth‟s surface. (The equation is assumed valid as long as density of air remains constant, within the altitude range or in other words, thinning of air as one goes up is not taken into consideration). 𝑣 𝑤 ℎ = 𝑣𝑜 ℎ 𝛼 (4) ℎ𝑜 Where 𝛼is the Hellman coefficient 𝑣 𝑜 is velocity of wind at reference altitude 𝑣 𝑤 (ℎ)is velocity of wind at height h 𝛼 can be measured on a day when winds are steady. To measure 𝛼 , velocity at two points of antenna can be measured and the equation can be solved for 𝛼. The measurement can be repeated for precision. To further nullify the effect of wind-gusts, velocity of wind can be taken over finite time duration and wind-gusts being random the velocity of wind will deviate about the steady state wind velocity. Since wind gusts follow Davenport spectrum, the measured 𝛼 deviates as dictated by Davenport spectrum. www.ijmer.com 3243 | Page
  • 3. International Journal of Modern Engineering Research (IJMER) www.ijmer.com Vol. 3, Issue. 5, Sep - Oct. 2013 pp-3242-3247 ISSN: 2249-6645 2.3 The Case of Face on Wind: Perpendicular Attack The perpendicular attack case is the worst case as the whole cross-section of the antenna is exposed to the wind. Fig 3 illustrates the case of perpendicular attack. To calculate force we need an elemental area over which the force is constant. The area is basically a horizontal strip that is at a distance x from the center and is of width dx. The strip subtends an angle 𝜃 at the center of parabolic disc. The strip‟s center subtends an angle𝜙 at O as illustrated in Fig 4. The strip is the differential element for torque calculation. Fig 3: The varying wind velocities are illustrated with different vector lengths. The shaded strip is the part of antenna that encounters equal velocity wind. The differential element for torque calculation is the strip that faces perpendicular force of wind. Fig 4: The differential element subtends an angle of 𝜙at O, which is the point about which the moment is calculated. O being d distance away from the center of disc. Torque calculation requires calculating the force acting on the elemental strip as a function of wind velocity and distance from the center of the parabolic disc A. Fig 5 serves as reference for further analysis. Fig 5: The elemental strip faces constant velocity wind. The center of the circular cross-section is A. The strip subtends 𝜃 at A, is x distance away from A and is of width dx. The area of the elemental strip in polar coordinates is given by Eqn (5). 𝑑𝐴 = −2𝑅2 𝑠𝑖𝑛2 𝜃𝑑𝜃 (5) The inclination of antenna is 90o w.r.t wind. Therefore, 𝜂2 is 1. Referring to Eqn (1) the force on the elemental strip can be given as in Eqn (6). 𝑑𝐹 = 1/2 𝜂1 𝜌𝑣 2 × 𝑑𝐴 (6) 𝑤 The velocity of wind as a function of height above ground level can be substituted as per Eqn (4), while the elemental area of the strip is substituted from Eqn (5). Eqn (6) modifies to Eqn (7). www.ijmer.com 3244 | Page
  • 4. www.ijmer.com 𝑑𝐹 = 1/2 𝜂1 𝜌 𝑣 𝑜 𝛼 2 ℎ ℎ𝑜 International Journal of Modern Engineering Research (IJMER) Vol. 3, Issue. 5, Sep - Oct. 2013 pp-3242-3247 ISSN: 2249-6645 × −2𝑅2 𝑠𝑖𝑛2 𝜃𝑑𝜃 (7) If center of the circle shown in Fig 5 is taken as the reference, the height parameter in Eqn (7) equals x. Substituting x in polar coordinates in Eqn (7) in place of h yields Eqn (8). 𝑑𝐹 = 1/2 𝜂1 𝜌 𝑣 𝑜 𝑅𝑐𝑜𝑠𝜃 𝛼 2 ℎ𝑜 × −2𝑅2 𝑠𝑖𝑛2 𝜃𝑑𝜃 (8) The force on the differential element produces a turning moment about the hinge of antenna. The magnitude of the generated torque is analytically found by multiplying the rotational arm length for the element or the distance of the differential element from O with the component of dF perpendicular to the rotational arm. Fig 6 illustrates the force vectors and the rotational arm lengths about O. Fig 6: (a) Figure illustrating the angular span of the parabolic disc about O. The radius of the dish being R. (b) Figure showing the resolution of forces perpendicular to the rotational arm r. (c) Figure illustrating the relation between radius R of the antenna dish, angular span 𝜙 𝑜 and distance d. The elemental torque (𝑑𝜏 𝑢𝑝 ) on the elemental strip in the upper half of the parabolic strip is given by Eqn (9). 𝑑𝜏 𝑢𝑝 = 𝑑𝐹𝑠𝑖𝑛𝜙 × 𝑟 (9) The force on the elemental strip is calculated in Eqn (8) and substituting r as 𝑑 𝑐𝑜𝑠∅ from Fig 6, we have the torque on the elemental strip as 𝑑𝜏 𝑢𝑝 = −1/2 𝜂1 𝜌 𝑣 𝑜 𝑅𝑐𝑜𝑠𝜃 𝛼 2 ℎ𝑜 × 2𝑅2 𝑠𝑖𝑛2 𝜃𝑑𝜃 × 𝑑 × 𝑡𝑎𝑛∅ × 𝑑∅ (10) Integrating Eqn (10) with limits for 𝜃 and ∅ the torque on the upper half disc can be calculated as shown in Eqn (11). 𝜏 0 𝑑𝜏 𝑢𝑝 = 𝜋/2 𝜃 =0 𝜙𝑜 𝜂 𝜙 =0 1 𝜌 𝑣𝑜 𝑅𝑐𝑜𝑠𝜃 ℎ𝑜 𝛼 2 × 𝑅2 𝑠𝑖𝑛2 𝜃𝑑𝜃 × 𝑑 × 𝑡𝑎𝑛∅ × 𝑑∅ 𝑑𝜃 (11) The limits for 𝜃 are reversed to absorb the negative sign in dF expression. The torque for the lower half of the dish can be found by placing proper limits and appropriate expression for the velocity of wind. The antenna here faces the wind perpendicularly; however, tracking antenna may be inclined at some angle to the wind velocity. The next section takes into account the parameter 𝜂2 . 2.4 Antenna Inclined w.r.t the Wind: Angular Attack The most generalized torque generating case is that of an inclined antenna against arbitrary direction of wind. The assumption here is that the wind follows Hellman‟s velocity relation, only the direction is arbitrary. Consider the antenna to be inclined at angle 𝜉as illustrated in Fig 7. Wind force is resolved into three mutually perpendicular components and torque due to each component is measured and generalized for parameter 𝜉. O Fig 7: (a) Figure illustrating the inclination of the antenna w.r.t wind. (b) The resolved components of force vector. (c) Figure illustrating the angular span of the antenna about reference O. www.ijmer.com 3245 | Page
  • 5. International Journal of Modern Engineering Research (IJMER) www.ijmer.com Vol. 3, Issue. 5, Sep - Oct. 2013 pp-3242-3247 ISSN: 2249-6645 The three mutually perpendicular force vectors are depicted in Fig 7 (b). Fw1 is the direction considered earlier for perpendicular attack. Fw3 sees the parabolic lateral face analyzed in the next section and Fw2 is in the vertical direction. The case of wind blowing vertically is seldom encountered and especially when the region experiences tornados and hurricanes. The differential force on the element is illustrated in Fig 8. The corresponding parameters are depicted in the triangle. The component of the force perpendicular to the moment arm is 𝑑𝐹 𝑤1 𝑠𝑖𝑛𝜙. The element is at a distance r from O. As compared to the case of perpendicular case the element is at an inclination of 𝜉 w.r.t the wind. InΔ𝐴𝐵𝑂, the relation between sides and angles can be determined by applying Sine Law as in Eqn (12). 𝑟 𝑑 = (12) 𝑠𝑖𝑛𝜉 sin 𝜋− 𝜙 +𝜉 Applying Sine Law for the triangles in Fig 7 (c) we arrive at Eqns (13-14) 𝑅 𝑑 = 𝑠𝑖𝑛 𝜙 01 𝑅 𝑠𝑖𝑛 𝜙 02 sin = sin (13) 𝜙 01 +𝜉 𝑑 𝜉 −𝜙 02 (14) 𝑑𝐹 𝑤1 𝑠𝑖𝑛𝜙 𝑑𝐹 𝑤1 ∅ 𝑟 𝑑𝐹 𝑤1 𝑐𝑜𝑠𝜙 ∅ O B 𝜉 𝑑 A Fig 8: Figure illustrating the force vectors for the differential element. r is the distance of the element from O, d is the distance of center A from O. and being the angle subtended by the elemental strip at O and A respectively. The differential torque is given by Eqn (9). Substituting r from Eqn (12) and dF from Eqn (8) in Eqn (9), the differential torque on the element can be expressed by Eqn (12). 𝑑𝜏 𝑢𝑝 = −𝜂1 𝜌 𝑣 𝑜 𝛼 2 𝑅𝑐𝑜𝑠𝜃 ℎ𝑜 × 𝑅2 𝑠𝑖𝑛2 𝜃𝑑𝜃 × 𝑑𝑠𝑖𝑛𝜉 sin ⁡ +𝜙) (𝜉 × 𝑠𝑖𝑛∅ × 𝑑∅ (15) The torque on the upper half of the antenna can be obtained by integrating Eqn (15) with limits for 𝜃 and 𝜙. The limits for 𝜙 is from 0 to𝜙01 , where 𝜙01 is obtained from Eqn (13). 𝜏 0 𝑑𝜏 𝑢𝑝 = 𝜋/2 𝜃 =0 𝜙 𝑜1 𝜙 =0 𝜂1 𝜌 𝑣 𝑜 𝑅𝑐𝑜𝑠𝜃 𝛼 2 ℎ𝑜 × 𝑅2 𝑠𝑖𝑛2 𝜃𝑑𝜃 × 𝑑𝑠𝑖𝑛𝜉 sin ⁡ +𝜙 ) (𝜉 × 𝑠𝑖𝑛∅ × 𝑑∅ 𝑑𝜃 (16) 2.5. Torque on the Lateral Surface The antenna employed for tracking is mostly a parabolic antenna. The lateral cross- section thus is a parabola. Fig 9 shows the parameters for a parabolic cross-section. The parabola can be mathematically represented by Eqn (17). 𝐾 𝑦 = 2 𝑚2 (17) 𝑅 The elemental area in this case is the product of length of the strip with its width and can be expressed by Eqn (18) 𝑑𝐴 = 𝑙 × 𝑑𝑥 (18) The length of the strip is mathematically the difference between the depth of the parabola K and z. 𝑙 = 𝐾− 𝑧= 𝐾 1− 𝑥2 (19) 𝑅 2 𝑐𝑜𝑠 2 𝜉 The differential area thus obtained can be substituted in the expression for torque dictated by Eqn (10). The porosity of the antenna may differ as the lateral side now offers resistance to wind. The moment arm in this case is x as the torque is generated about mm’ 𝑑𝜏 𝑢𝑝 = 1/2 𝜂1′ 𝜌 𝑣 𝑜 𝑅𝑐𝑜𝑠𝜃 𝛼 2 ℎ𝑜 × 𝐾 1− 𝑥2 𝑅 2 𝑐𝑜𝑠 2 𝜉 × 𝑑𝑥 × 𝑥 (20) Eqn (20) can be integrated over the upper half antenna to obtain the total torque experienced by the upper half part of the dish. Since, this expression does not use polar coordinates the torque expression is a single integral as shown in Eqn (21). 𝜏 𝑢𝑝 0 𝑑𝜏 𝑢𝑝 = 𝑅𝑠𝑖𝑛𝜉 𝑥=0 1/2 𝜂1′ 𝜌 𝑣 𝑜 𝑅𝑐𝑜𝑠𝜃 ℎ𝑜 𝛼 2 × 𝐾 1− 𝑥2 𝑅 2 𝑐𝑜𝑠 2 𝜉 × 𝑑𝑥 × 𝑥 (21) The torque for the lower half of the antenna can be expressed with the same equation but with different limits. www.ijmer.com 3246 | Page
  • 6. www.ijmer.com International Journal of Modern Engineering Research (IJMER) Vol. 3, Issue. 5, Sep - Oct. 2013 pp-3242-3247 ISSN: 2249-6645 Fig 9: Figure illustrating the lateral cross-section of the parabola with its parameters III. CONCLUSION AND FUTURE SCOPE The paper develops a mathematical model for wind disturbance torque on tracking antenna. The vector approach to torque calculation in case of antenna requires only porosity of the antenna as the variable parameter to be as compared to the numerous antenna specific coefficients that need to be calculated while opting for field models of wind disturbance torques. The model here has considered antenna as a single entity, however, a finite element analysis of antenna structure still needs to be explored. REFERENCES [1.] [2.] [3.] [4.] [5.] [6.] W. Gawronski, “Wind Gust Models Derived From Field Data,” The Telecommunications and Data Acquisition Progress Report 42-123, July–September 1995, Jet Propulsion Laboratory, Pasadena, California, pp. 30–36, November 15, 1995. W. Gawronski and J. A. Mellstrom, “Control and Dynamics of the Deep Space Network Antennas,” in Control and Dynamics Systems, C. T. Leondes, ed.,vol. 63, San Diego, California: Academic Press. W. Gawronski, B. Bienkiewicz, and R. E. Hill, “Pointing-Error Simulations of the DSS-13 Antenna Due to Wind Disturbances,” The Telecommunications and Data Acquisition Progress Report 42-108, October–December 1991, Jet Propulsion Laboratory, Pasadena, California, pp. 109–134, February 15, 1992. Norman S. Nise, Control System Engineering, 4th edition, Wiley Education Press. BC Joshi,”Simulation Study of Servo Control System of 45 meter Giant Metrewave Radio Telescope”. www.ncra.tifr.res.in ABOUT THE AUTHOR Tushar Golani received his B.Tech from Indian Institute of Space Science and Technology, Thiruvananthapuram. He joined ISRO Satellite Centre in 2011 and is currently working in Spacecraft Checkout Group. His areas of interest include control systems, analog and digital circuit design and embedded systems. He is elected as a life member of the Astronautical Society of India (ASI) and Associate Member of the Aeronautical Society of India (AeSI). Suresh Sabhapathy is appointed as Engineer-„F‟ at the Giant Metrewave Radio Telescope facility of TIFR. He is the group coordinator of the servo control systems group and is actively working in the field of linear and non-linear control of large structures. He has guided several students in the field of servo control systems. www.ijmer.com 3247 | Page