25
A Miniaturized Archimedean Spiral Antenna with Polarization Diversity Dr Jonathan M. Rigelsford, SMIEEE Department of Electronic & Electrical Engineering, The University of Sheffield, Mappin Street, Sheffield S1 3JD, United Kingdom. Email: [email protected] Tel:+44(0)114 2225584 1 19/12/2013 © The University of Sheffield

A Miniaturized Archimedean Spiral Antenna with ... · Archimedean Spiral Antenna with Polarization Diversity Dr Jonathan M. Rigelsford, SMIEEE ... The design of a 4-arm Archimedean

  • Upload
    others

  • View
    26

  • Download
    7

Embed Size (px)

Citation preview

A Miniaturized Archimedean Spiral Antenna with Polarization Diversity

Dr Jonathan M. Rigelsford, SMIEEE

Department of Electronic & Electrical Engineering, The University of Sheffield, Mappin Street, Sheffield S1 3JD, United Kingdom.Email: [email protected]:+44(0)114 2225584

1

19/12/2013 © The University of Sheffield

Overview

• Motivation for this work

• Background to the subject

• The design

• Results

• Conclusions & Comments

19/12/2013 © The University of Sheffield

2

Motivation

• How do you make large antennas smaller?

• How can you maintain their efficiency?

• How can you preserve polarization?

• Can we create a scalable design?

19/12/2013 © The University of Sheffield

3

From A to B

19/12/2013 © The University of Sheffield

4

120m

Why make antennas smaller?

• Easier to fit into devices• Smart phones

• Cars

• Reduced visual impact• Tempest

• Planning permission

• Aesthetics

• Easier to handle

19/12/2013 © The University of Sheffield

5

Background

• How do you make large antennas smaller?• Dielectric loading

• Fractals

• Meander lines

• Spirals

• Meta materials - EBG/AMC/HIS

19/12/2013 © The University of Sheffield

6

The forming of an idea…

19/12/2013 © The University of Sheffield

7

19/12/2013 © The University of Sheffield

8

… Eureka!

19/12/2013 © The University of Sheffield

9

Justification: Why a spiral?

• Easily scalable

• Easy to print

• Easy to manufacture

• For tempest applications you can use a pipe bender.

• For HF you can use radial supporting cables.

19/12/2013 © The University of Sheffield

10

The design of a 4-arm Archimedean Spiral Antenna

19/12/2013 © The University of Sheffield

11

r=r0+aφ

a=t/2π

r0

t

g

r

-21

-18

-15

-12

-9

-6

-3

0

1.4 1.6 1.8 2 2.2

Reflection coefficient (dB)

Frequency (GHz)

t=13mm

t=14mm

t=15mm

t=16mm

t=17mm

Reflection coefficient Axial Ratio

19/12/2013 © The University of Sheffield

12

0

5

10

15

20

25

1 2 3 4 5 6 7 8

Axial ratio

Frequency (GHz)

Gain Radiation pattern

19/12/2013 © The University of Sheffield

13

-6

-3

0

3

6

9

12

1.4 1.5 1.6 1.7 1.8 1.9 2 2.1 2.2 2.3

Realised Gain (dBi)

Frequency (GHz)

-30

-25

-20

-15

-10

-5

0

-180 -150 -120 -90 -60 -30 0 30 60 90 120 150 180

dB

Angle (degrees)

1.6 GHz

1.65 GHz

1.7 GHz

1.75 GHz

1.8 GHz

1.85 GHz

Results

19/12/2013 © The University of Sheffield

14

-60

-50

-40

-30

-20

-10

0

1.6 1.65 1.7 1.75 1.8 1.85 1.9 1.95 2

Reflection coefficient (dB)

Frequency (GHz)

S11

S22

S21

Summary of a Quad-arm Archimedean Spiral Antenna

• Frequency: 1.75GHz• Reflection coefficient: -20dB• Isolation: -45dB• Gain: 9dBi• Axial ratio: 38dB• Diameter: 44.5mm• Aperture reduction: 49%• Thickness: λ/4• Dielectric loading: NONE• Meta-material: NONE

19/12/2013 © The University of Sheffield

15

Dielectric loading

19/12/2013 © The University of Sheffield

16

-15

-12

-9

-6

-3

0

0 0.5 1 1.5 2 2.5 3 3.5 4

Reflection coefficient (dB)

Frequency (GHz)

1.5

2

2.5

3

3.5

4

4.5

5

Variation of S11 with different ε

Reflection coefficient of different turns spacing

Reflection coefficient of different width of arm

19/12/2013 © The University of Sheffield

17

-21

-18

-15

-12

-9

-6

-3

0

0 0.5 1 1.5 2 2.5 3 3.5 4

Reflection coefficient (dB)

Frequency (GHz)

t=13mm

t=14mm

t=15mm

t=16mm

t=17mm

-21

-18

-15

-12

-9

-6

-3

0

0 0.5 1 1.5 2 2.5 3 3.5 4

Reflection coefficient (dB)

Frequency (GHz)

0.5

1

2

Reflection coefficient of different r0

Reflection coefficient of different number of turns

19/12/2013 © The University of Sheffield

18

-21

-18

-15

-12

-9

-6

-3

0

0 0.5 1 1.5 2 2.5 3 3.5 4

Reflection coefficient (dB)

Frequency (GHz)

5

4

3

-21

-18

-15

-12

-9

-6

-3

0

0 0.5 1 1.5 2 2.5 3 3.5 4

Reflection coefficient (dB)

Frequency (GHz)

1.24

1.2

1.15

1.1

Summary of a Quad-arm Dielectrically loaded Archimedean Spiral Antenna

• Frequency: 2.75GHz• Reflection coefficient: -14dB• Diameter: 44.5mm• Aperture reduction: 45%• Thickness: λ/9• Dielectric loading: YES• Meta-material: NONE

19/12/2013 © The University of Sheffield

19

‘Polo’ Loaded

19/12/2013 © The University of Sheffield

20

-12

-11

-10

-9

-8

-7

-6

-5

-4

-3

-2

-1

0

1.5 1.7 1.9 2.1 2.3 2.5

Reflection coefficient (dB)

Frequency (GHz)

1mm larger than spiral

same as spiral

1mm smaller than spiral

2mm smaller than spiral

‘Polo’ Loaded

19/12/2013 © The University of Sheffield

21

Summary of a Quad-arm ‘Polo’ loaded Archimedean Spiral Antenna• Frequency: 2.38GHz• Reflection coefficient: -18.1dB• Isolation: -50dB• Gain: 5.9dBi• Spiral Diameter: 32.5mm• Aperture reduction: 49%• Thickness: λ/8• Dielectric loading: YES• Meta-material: NONE

19/12/2013 © The University of Sheffield

22

• Frequency: 1.52GHz• Reflection coefficient: -20dB• Isolation: -65dB• Gain: 3.7dBi• Spiral Diameter: 32.5mm• Aperture reduction: 72.5%• Thickness: λ/10• Dielectric loading: YES• Meta-material: NONE

Conclusions

With a bit of clever thinking you can:

• Design a dual polarized, miniature Archimedean spiral antenna,

• Which is highly scalable, and

• Can be made even smaller using dielectric loading.

19/12/2013 © The University of Sheffield

23

Comments/Challenges

• Still have to try and make the design even smaller using EBG/AMC/HIS.

• Design an EBG/AMC/HIS which works at 6 MHz without dielectric material.

• Be very careful with your simulations!

(suggestions and/or collaborators welcome)

19/12/2013 © The University of Sheffield

24

Thank you!

19/12/2013 © The University of Sheffield

25