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Computers, Materials & Continua
DOI:10.32604/cmc.2022.021852
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Article

Low Profile UHF Antenna Design for Low Earth-Observation CubeSats

Md. Amanath Ullah1, Touhidul Alam2,3, Ali F. Almutairi4,* and Mohammad Tariqul Islam5

1School of Electrical and Data Engineering, Faculty of Engineering and Information Technology, University of Technology Sydney, Ultimo NSW, 2007, Australia
2Space Science Centre (ANGKASA), Institute of Climate Change (IPI), Universiti Kebangsaan Malaysia, Bangi, 43600, Selangor, Malaysia
3Department of CSE, International Islamic University Chittagong (IIUC), Chattogram, 4318, Bangladesh
4Electrical Engineering Department, Kuwait University, 13060, KuwaitCity, Kuwait
5Department of Electrical, Electronic and Systems Engineering, Faculty of Engineering and Built Environment, Universiti Kebangsaan Malaysia, Bangi, 43600, Selangor, Malaysia
*Corresponding Author: Ali F. Almutairi. Email: ali.almut@ku.edu.kw
Received: 17 July 2021; Accepted: 03 September 2021

Abstract: This paper reveals a new design of UHF CubeSat antenna based on a modified Planar Inverted F Antenna (PIFA) for CubeSat communication. The design utilizes a CubeSat face as the ground plane. There is a gap of 5 mm beneath the radiating element that facilitates the design providing with space for solar panels. The prototype is fabricated using Aluminum metal sheet and measured. The antenna achieved resonance at 419 MHz. Response of the antenna has been investigated after placing a solar panel. Lossy properties of solar panels made the resonance shift about 20 MHz. This design addresses the frequency shifting issue after placing the antenna with the CubeSat body. This phenomenon has been analyzed considering a typical 1U and 2U CubeSat body with the antenna. The antenna achieved a positive realized gain of 0.7 dB and approximately 78% of efficiency at the resonant frequency with providing 85% of open space for solar irradiance onto the solar panel.

Keywords: CubeSat antenna; UHF antenna; small satellite; satellite communication

1  Introduction

The development of the first CubeSat in the year of 2003 unfolded a new dimension for the space researchers’ community. Space exploration missions became open for private and government organizations while attracting the research interest of universities [14]. Moreover, CubeSats are allowing developing countries to get the touch of aerospace with less expense considering the basic features of CubeSats such as low manufacturing cost, simpler design, small development duration. Moreover, CubeSats are often built with off-the-shelf components that are available commercially; the upshot, CubeSats have enabled satellite researchers for bigger mission with minimal cost [5]. Acceptance of CubeSats among researchers is increasing throughout the last five years [6]. The communication system is vital in any CubeSat since it maintains connectivity with the ground station. Antenna is one of the most important elements in any communication system. Since more than one antenna is needed in CubeSats, different antennas operating at individual frequencies are placed around the satellite body ensuring that one antenna does not affect other antenna’s performance [7]. Generally, CubeSats are launched in space using special deplorers. So, stringent requirements for weight, power, and geometry need to be followed and these three (weight, power, and geometry) are the crucial consideration issues that have a great impact on desining antenna system. Researchers are emphasizing new antenna designs that can cover the CubeSat requisites as well as maintain the performance of the antenna. Different types of antennas including patch, horn, refectory, membrane, reflector, wire etc. are reported in literature for Cu-beSat application [810]. Dipoles, monopoles, Yagi–Uda arrays, and helical antennas are several types of wire antenna. The adverse fact of using wire antennas in CubeSats is, they are required to be deployed mechanically [5,1113]. So, there is always a chance of mission failure due to improper and sophisticated deployment mechanisms, which increase mission complexity. Printed patch antennas are more convenient alternative of conventional wire antennas where deployable antennas increase mission complexity. In contrast to the deployable antenna, the Patch antenna provides low profile. However, patch antenna with partial ground plane has strong affect on metallic CubeSat structure [14]. Moreover, obtaining lower UHF operating band is a challenge due to design limitations. In addition, patch antennas are mounted on the CubeSat face that can be used for the placement of solar panels instead. Good radiation characteristics is achievable using horn antennas, but the downside, they are large in size and more suitable in higher frequency operation. In [1517], planar inverted-F antennas (PIFA) have been proposed for the CubeSat communication system.

In this paper, the design structure of a modified PIFA for UHF CubeSat communication has been revealed that can pave the way to address the shortcomings of deployable and patch antennas for the CubeSat mission. One of the faces of the typical CubeSat body is taken as the ground plane of the antenna. The design facilitates open space that can enable solar irradiance to pass through the slot of the radiating element. Design and simulation processes are performed in CST (Computer Simulation Technology) Microwave Studio. The design is simulated using 0.2 mm thick Aluminum material while the thickness of the ground plane is 0.5 mm. Finally, it has been fabricated with Aluminum sheet. The antenna performance is measured using PNA Network Analyzer. The proposed antenna resonates at 419 MHz in free space. The performance of the antenna has also been investigated with solar panels and while the antenna mounted with CubeSat backplane.

2  Antenna Design

The perspective view of the proposed Planar Inverted F Antenna (PIFA) is shown in Fig. 1a. The main radiating section is designed to deliver a larger effective length to realize resonance at desired UHF band. The rectangular shaped element at the corner has great significance in achieving resonance at 419 MHz. The width of the strip-type radiating element is 5 mm. The whole PIFA is designed using 0.2 mm Aluminum sheet. The resonant frequency can roughly be estimated by Eq. (1) [18].

f=c4(L+b) (1)

where, c is the velocity of light, b is the width of the radiating element and L is the effective length of the radiating element. Space in-between the ground plane and upper radiating structure is 5 mm. There is a gap named ‘h’ is maintained between the edge of the ground plane and the edge of radiating structure that facilitates the antenna to adjust on the CubeSat frame. There is a 2 mm distance between the feed point and the shorting wall. Parametric study on W1 and L2 has been performed to obtain the optimized design parameters of the antenna. Fig. 2 depicts the results of the parametric study. L2 has a significant impact on the resonant frequency, it can also be used to tune the antenna. Moreover, conventional shorting wall techniques is utilized to achieve lower resonance frequency and enhanced reflection coefficient. The optimization of the design parameters is performed in numerical simulation, optimized parameters as included in Tab. 1.

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Figure 1: (a) Design configuration of the proposed antenna, (b) Antenna mounted with typical CubeSat body

The radiating element of the antenna has been fabricated from commercially available 0.2 mm Aluminium (Aluminium 7075) sheet where Aluminum of 0.5 mm thickness is used to form the ground plane. The principal radiating element is shaped according to the basic design and the shorting wall is bent at its respective place. Finally, an SMA connector is soldered with the ground plane and the feed point. The possible placement of the solar panel and placement of the antenna with the CubeSat body is shown in Fig. 1b. In the simulation, Gallium Arsenide based solar panels was considered, where the dielectric constant, heat capacity and thermal conductivity was 12.94, 0.33 kJ/K/kg and 54 W/K/m, respectively. Then the performance of the antenna is investigated while the antenna is mounted with a typical 1U and 2U CubeSat.

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Figure 2: Reflection coefficient of the antenna for (a) L2 and (b) W1

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3  Results

Fig. 3a illustrates the reflection coefficient of the antenna at different conditions. The reflection coefficient of the antenna has been investigated while the antenna in free space, mounted with solar panel and mounted with both solar panel and CubeSat body. It is seen that the resonant frequency shifts as the subsystems are mounted with the antenna. The surface current distribution of the proposed antenna with solar cell is depicted in Fig. 3b, where the surface current is evenly distributed in L and W. It is also shown that significant amount of current is flowing through L2 and W1, which is responsible for shifting resonance. The fabricated prototype of the proposed antenna mounted with solar panel is shown in Fig. 4.

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Figure 3: (a) Simulated reflection coefficients of the antenna and (b) surface current distribution at 400 MHz

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Figure 4: Fabricated prototypes of the antenna with solar panel

The Fig. 5a depicts the reflection coefficient of the solar panel mounted antenna. Fig. 5b represents the reflection coefficient of the antenna mounted with the CubeSat body and solar panel. Good agreement has been achieved between simulated and measured results. The measured results are found in good alignment with the simulated results. A slight mismatch can be noticed due to fabrication tolerance, SMA connector and the RF cable that facilitates the connection with VNA, which were not considered in simulation.

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Figure 5: Reflection coefficients (a) with solar panel; (b) with solar panel and CubeSat

Performance of the antenna fluctuates due to the interaction between the lossy solar panel and radiating element of the antenna mounted on the body [19]. The antenna has been simulated and measured with solar panel to evaluate how the performance deviates. It is notable that, a significant frequency shift occurs because of the existence of solar panel. Nanosatellite patch antennas usually suffer from frequency shifting issues when they are mounted with the body. So, the reflection coefficient of the antenna mounted with nanosatellite body and solar panel has been investigated. It turned out that, the antenna’s operating frequency remained stable when it is mounted with the nanosatellite body.

Radiation patterns of the antenna have been presented in Fig. 6. The radiation patterns remained stable even after mounting the antenna with the CubeSat structure with satisfactory beamwidth to maintain communication from LEO, shown in Fig. 7. Investigation of the radiation efficiency while the antenna is mounted with solar panel has also been performed. Up to 78% efficiency is found while the antenna is mounted with solar panel with up to 0.7 dB realized gain depicted in Fig. 8. A comparison among the proposed antenna, commercial antennas [20] and some other existing small satellite antennas is presented in Tab. 2. Based on the comparison, the proposed PIFA antenna provides 0.7 dB of gain at 400 MHz with retaining lower UHF antenna design constraints. So, the proposed antenna shows potentiality for smooth Low Earth-Observation CubeSats operation.

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Figure 6: Radiation pattern of the antenna (a) at xz; (b) at yz plane

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Figure 7: Radiation patterns of the antenna (mounted with CubeSat body) (a) at xz; (b) at yz plane and (c) 3D radiation pattern with 1U and 2U CubeSats

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Figure 8: Realized gain and efficiency of the proposed UHF antenna

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4  Conclusion

This paper presents a new design approach of a modified PIFA antenna for CubeSat communication in the UHF band. The antenna operates at UHF frequency while it serves the facility of solar panel integration between the ground plane and radiating element and provides 85% free space for solar light penetration. The antenna prototype has been fabricated using Aluminum sheet. The effect of placing solar panels and CubeSat body with the antenna have been investigated in this study which is the potential for satellite communication.

Acknowledgement: The authors acknowledge the technical support with thanks to Universiti Kebangsaan Malaysia.

Funding Statement: The authors received no specific funding for this study.

Conflicts of Interest: The authors declare that they have no conflicts of interest to report regarding the present study.

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