Is LRDE Developing An Ultra-Wide-Band (UWB) AESA Radar For AMCA?
AESA radars are becoming the centrepiece of next-generation sensors suites. This new type of radar has greatly enhanced the situational awareness of modern combat aircraft. An AESA radar offers several advantages over legacy passive phased array (PESA) radar such as- higher range, beam agility, low probability of intercept (LPI), enhanced performance, increased ECCM resistance, high effective radiated power and more. An AESAR has an active phased array antenna composed of hundreds (or thousands) radiating element. These radiating elements are arranged in a geometrical pattern. The most commonly used radiating elements for phased array radar are dipoles, open-ended wave-guides, slotted wave-guide, micro-strip antenna, helix, and spiral antennas.
An active phased array radar composed of tapered slot antenna elements (TSA) undergoing testing in a anechoic chamber - Image Courtesy: Maxima Vigilantia
Electronics and Radar Development Establishment (LRDE) has already developed several advanced AESA radars such as Aslesha, Arudhra, L-STAR, Swordfish LRTR, etc. Currently, LRDE is working on several radars such as Uttam AESA radar, High Power Radar, 360° coverage AESA radar for AEW&CS India and it is also working on some futuristic RF technologies which one day might go into Indian 5th generation Advanced Medium Combat Aircraft (AMCA). One of the new technologies LRDE is working on is shared aperture radar.
What is A Shared Aperture Radar?
In simple terms, a shared aperture radar combines the functionality of multiple antennas into one, for example - using a radar antenna for electronic warfare and long-range tactical communication. The aperture can be shared in multiple ways. One way is time-interleaving, when radar functions aren't being used, the aperture can be used for other purposes. Another way is to subdivide the aperture into smaller segments, with each segment performing a specific task simultaneously, furthermore, each segment can be time-interleaved, for ex. radar segment may have interleaved modes. Finally, a shared aperture may also use multiple independent beams to perform multiple functions simultaneously. The last approach is the most advantageous as well as complex (isolating beams and inter-modulation products is a challenging task).
Primary requirements of a shared aperture radar are 1. Wide bandwidth radiating elements 2. Multiple polarisation. Isolating beams and inter-modulation products require state of the art filters and amplifiers. LRDE is developing critical components for a shared aperture radar- wideband radiating elements and associated TR module technology.
LRDE developed a 16x16 element planner array antenna to investigate the technology. The small antenna array provided sufficient functionality to study associated radiation characteristics and trade offs. Since the primary requirement is wide bandwidth ( >50% of centre frequency) and dual polarisation, it prevents the use of the common type of antennas such as microstrip patches, printed dipoles, and open-ended dipoles as the bandwidth of these antennas is <=30% of center frequency.
Therefore, TSA (Tapered slot antenna) AKA Vivaldi flared notch antenna was selected. TSA antenna meets all the requirements mentioned above. It has symmetrical radiation pattern, high gain, and wide bandwidth. The most recognisable feature of the TSA antenna is its V-shaped flared notch. The narrower region of the notch radiates RF signals of high frequency, whereas broader part radiates RF signals of low frequency.The geometry of Tapered Slot Antenna(TSA)/Vivaldi Antenna
Closeup of an active phased array radar composed of X-band TSA radiating elements
Antenna element and planks developed for wide-band TR modules by DARE
Wideband TRM developed by DARE features Vivaldi Notch Antenna Array
Due to their excellent wide-band characteristics, TSAs are well suitable for EW applications
Actual image of LRDE developed Tapered Slot Antenna (TSA)
DRDO has invested a lot of money in gallium nitride MMIC development projects and there are plans to set up a state of the art GaN foundry at IISc. It's likely that TR modules of AMCA's radar will use GaN-based solid-state RF amplifiers. GaN MMIC combined with latest LNA tech will greatly enhance detection range (greater than 200km for a 1 sqm RCS target). It also eliminates the requirement of a liquid coolant circulation based cooling system. Existing radars in IAF service use traveling wave tube amplifier (TWTA) and slotted waveguide antenna (planer array of slots). The bandwidth of these radars is relatively narrow (600-800MHz). More advanced radars such as Uttam and EL/M-2052 have a much wider bandwidth (1-3GHz). A wideband radar using TSA radiating element may have a bandwidth no less than 5 GHz and an enhanced probability of detection+classification and it's much more difficult to jam. The associated wideband/multi-channel MMIC is however very complex and expensive. It is in an early development stage and the technology in question is futuristic. If this radar tech indeed goes to the AMCA, then the development period is perfectly aligned with the timeline of the aircraft being inducted into the IAF i.e beyond 2035.
IDN wishes to thank - Disha of (ECE Department, Malaviya National Institute of Technology, Jaipur)
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