August 7, 2024
The Growing Satellite Market
Geostationary (GEO) Systems
With the growing need for ubiquitous connectivity, the satellite communications industry is poised for explosive growth, with multiple high-capacity systems either already in orbit or planned for the near future. There are on-orbit geostationary systems like ViaSat-1 and ViaSat-2 that offer capacities of 140 GBPS and 300 GBPS, respectively. ViaSat-3 has also been recently announced and will offer 1 TBPS capacity, which in one satellite will be greater than the rest of the GEO satellite world combined. Other GEO satellites include Jupiter-1/Echostar-17 and Jupiter-2/Echostar-19, which offer capacities of 100 GBPS and 220 GBPS, respectively, with Jupiter-3/Echostar-27 launched in July 2023 with 500 GBPS capacity.
Low Earth Orbit (LEO) Systems
However, GEO satellites are not the only ones that have added significant capacity to the space industry. There are multiple low earth orbit satellite systems being designed, including Telesat, OneWeb, SpaceX, Iridium and LeoSat. These systems have constellations circling the Earth while providing coverage to parts of the planet that never before received satellite service. The sizes of these constellations vary from 100s to 1000s of satellites, so the aggregate capacity of these constellations will be enormous. Lately, SpaceX/Starlink was approved by the FCC to launch an extra 7,000 internet-beaming satellites in addition to the 4,000 that have already been approved. This will bring a total of 12,000 satellites to their constellation. These LEO satellites will be in addition to the OneWeb constellation, which is planning to have approximately 600 more satellites. Telesat will operate 292 LEO satellites with the option to grow to 512 LEO satellites. Other companies might have similar views and will be launching satellites as well. These LEO satellite systems will cover global internet broadband service for individual customers. The plan of these companies is to provide broadband access to millions of potential remote users who do not have access to it today.
Medium Earth Orbit (MEO) Systems
In the medium earth orbit systems, one finds O3b (O3b mPOWER is a communications satellite system owned and operated by SES), which is expanding its constellation of 50 deg latitude equatorial orbit satellites from 16 to 42 satellites, with the newer satellites to be deployed in inclined orbits that will provide service to the poles. Its newest seven satellites will offer a combined 10 TBPS of capacity alone.
Pros and cons of LEO, MEO and GEO Systems
These three different orbit satellite systems will provide full coverage for our everyday needs. Each orbit system has its own pros and cons, but together, they work as a whole. The GEO arc is located the farthest from Earth at about 35,800 km directly above the equator. It has the advantage of staying in one stationary position relative to the Earth and covers a bigger geographical area with fewer satellites. However, the farther the distance, the longer the latency and for GEO, it can be about 600 to 800 msec. This technology is arguably best for TV, radio, weather communications and broadcast services. In comparison, the LEO satellites orbit 500 km to 1,500 km from Earth. These satellites are much smaller and cost less to manufacture and launch. Their life cycle is shorter, and many of them are needed for global coverage. These satellites are moving at a much faster pace because of their proximity to Earth, and a larger number of them will be required to cover the entire Earth. LEO satellites spend a lot of time over the ocean, which makes them less efficient, but they do provide better communication coverage for boats and ships that are far from the shore. Communication with LEO/MEO satellites tend to be more complicated compared to GEO systems, as the ground stations need to track multiple satellites and switch between satellites during hand-offs. Another big advantage that LEO satellites offer in comparison to GEO satellites is latency. Latency is much shorter and measures from 30 to 50 msec, which makes it very attractive for gaming, video streaming, audio and fast internet communication.
The MEO satellites orbit above the Earth at about 5000 to 12000 km altitude, with latencies of 125 to 250 msec, which makes them very good for GPS use and for services that can tolerate moderate propagation delays.
This huge amount of capacity will give rise to unprecedented numbers of user terminals, most of which must have steerable antenna technology. Steerable antennas are required when either the satellite or the satellite terminal is in motion. Thus, LEO and MEO systems require steerable antennas for both fixed and mobile users. Similarly, GEO systems require steerable antennas for mobile users or even for auto-pointing applications where the antenna beam can self-point at a GEO satellite for the highest throughput performance.
Traditionally, global high-capacity satellite bands operate at 10.7-12.75 GHz or 17.7-20.2 GHz on the downlinks and 13.75-14.5 GHz and 27.5-30.0 GHz on the uplinks. So how can the satellite industry mass produce high-frequency active antennas with steerable beams in sufficient volumes to leverage the significant space resources being deployed? What is needed are antennas that are high performance, low profile, manufacturable using only 2D manufacturing methods and scalable in size to meet the various use cases from large, high throughput terminals to smaller and lower throughput terminals.
Use of Electronically Steered Active Phased Array Antennas in SATCOM
Phased array antennas can solve many of these challenges. They are an array of radiating elements fed varying phase and amplitude information to form a beam in a given direction. The beam is thus steered electronically with no moving parts. Without the need for bulky mechanical gimbals, this type of antenna is smaller, more reliable and less costly to maintain.
For the highest performance in any radio system, the power amplifier and low noise amplifier need to be placed as close to the antenna as possible to minimize front-end feed loss. In phased array antennas, the Tx/Rx plus beam steering functions need to be placed right at the radiating element. Since the distance between radiating elements in the array (the lattice) is typically one-half wavelength, the real estate available for the phased array antenna electronics is quite limited, especially at higher frequencies where the wavelengths are very short. The only monolithic technology that can provide sufficient integration of the requisite RF, analog and digital functions is silicon. Fortunately, Moore’s Law has allowed silicon to advance to the point where III-V semiconductor components like GaAs are no longer needed in the array, resulting in major cost savings and simpler construction.
Typical construction of a planar phased array uses a multi-layer printed circuit board (PCB) with antenna elements printed in metal on one side of the PCB and silicon control electronics on the opposite side of the board. The inner layers of the PCB provide beam-forming networks, DC (direct current) voltage and control signal routing. This type of construction allows simple surface mount assembly using pick-and-place machines and IR reflow. It is important to have an optimized layout from matching, loss and power perspective to achieve the best performance. Qorvo’s products are designed to enable optimized layouts with minimum board cost and complexity.
Planar phased array antennas are scalable in size, allowing larger antennas to support higher G/T or EIRP applications and smaller antennas to support lower G/T or EIRP applications. The silicon ICs that reside within the antenna lattice are just stepped and repeated across the array regardless of its size.
Qorvo ICs Enabling Next Generation of Active Phased Array Flat Panels
Qorvo’s second generation of SATCOM ICs is designed specifically for high volume, low cost phased array terminals as described herein. These parts are designed for FDD (Frequency Division Duplex) operation covering global SATCOM Ku, K and Ka bands. Each IC in the family supports four dual-polarization radiating elements with full polarization flexibility. Each channel has its own individual control of phase and gain for maximum flexibility. The gain control per element also allows the customers to adjust the gain per element to achieve a desired side lobe level. There is also power detector circuitry with an ADC (Analog to Digital Converter) on each TX element to provide an estimate of transmit output power. These ICs operate from a single supply of 1.2v and offer high gain, low noise figure and excellent DC efficiency. Additional features include gain compensation over temperature, temperature reporting and zero calibration for the array. All of these features come in a small package of 4.4 x 3.6 mm WLCSP (Wafer Level Chip Scale Package) for easy installation in planar-phased array antennas.
Qorvo’s zero calibration (ZERO-CAL®) technology removes the need for array calibration, which reduces customer test time, complexity and cost. The ICs also offer fast beam steering to enable rapid angular tracking in mobile environments and fast beam hand-offs between LEO/MEO satellites. The temperature compensation is designed to allow constant gain performance over the full range of temperature range of -40 degC to +85 degC. Finally, the ICs provide telemetry to the host system, enabling proactive maintenance by the system operator and reducing expensive truck rolls.
Qorvo’s SATCOM ICs utilize 300mm CMOS Silicon, ensuring a perfect combination of performance and low cost, which truly makes the commercialization of Active Electronically Steered Antennas for SATCOM a reality.
Conclusion
Qorvo provides ICs in every mmWave 5G, SATCOM and radar band, thereby ensuring maximum economies of scale for true low-cost and high-performance flat panel solutions. With its Ku and K/Ka-band Gen 2 SATCOM ICs, Qorvo is setting the benchmarks for high-performance and low-cost, flat panel antennas for mass commercial deployment for LEO, MEO and GEO SATCOM ground terminals and satellite-on-the-move applications. Learn More
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