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DTSTAMP:20220903T060100Z
UID:1ED9B0B6-3DCF-412D-99F5-E218585D5F36
DTSTART;TZID=Australia/Sydney:20220831T190000
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DESCRIPTION:No other antenna concept has more names. At present these anten
 nas are known as Fabry-Perot resonant cavity antennas\, just Resonant Cavi
 ty Antennas (RCA)\, Partial Reflector Surface (PRS) based antennas\, Elect
 romagnetic Band Gap (EBG) Resonator antennas (ERAs) and Two Dimensional Le
 aky-Wave Antennas\, and more names are forthcoming. Yet they all have more
  or less the same configuration consisting of a resonant cavity\, formed b
 etween a partially reflecting superstructure and a fully reflecting (groun
 d) plane. The resonant cavity is excited by a small feed antenna. Hence\, 
 they are referred to as resonant cavity antennas (RCAs) in this presentati
 on. Since the concept of using a “partially reflecting sheet array” su
 perstructure to significantly enhance the directivity was disclosed by Tre
 ntini in 1956\, it has been an attractive concept to several antenna resea
 rchers for several reasons\, including its theoretical elegance\, relation
 ships to other wellresearched area such as leaky-waves\, EBG\, frequency s
 elective surfaces and metasurfaces\, and practical advantages as a low-cos
 t simple way to achieve high-gain (15-25 dBi) from an efficient planar ant
 enna without an array\, which requires a feed network. The RCA concept is 
 one of the main beneficiaries of the surge of research on electromagnetic 
 periodic structures in the last decade\, first inspired by EBG and then to
  some extent by metamaterials. As a result\, RCAs gained a tremendous impr
 ovement in performance in the last 10 years\, in addition to other advanta
 ges such as size reduction. As an example\, achieving 10% gain bandwidth f
 rom such an antenna with a PSS was a major breakthrough in 2006 but now th
 ere are prototypes with gain bandwidths greater than 50%. Until recently m
 ost RCAs required an area in the range of 25-100 square wavelengths but th
 e latest extremely wideband RCAs are very compact\, requiring only 1.5-2 s
 quare wavelengths at the lowest operating frequency. Once limited to a sel
 ect group of researchers\, these advantages have attracted many new resear
 chers to RCA research domain\, and the list is growing fast\, as demonstra
 ted by the diversity of authors in recent RCA publications. RCAs have alre
 ady replaced other types of antennas\, for example as feeds for reflectors
 .\n\nThis presentation will take the audience through historical achieveme
 nts of RCA technology\, giving emphasis to breakthroughs in the last 20 ye
 ars up to a recent method of steering its beam continuously in 2D (i.e.\, 
 azimuth and elevation).\n\nCo-sponsored by: Engineers Australia and Electr
 omagnetic Compatibility Society of Australia\n\nSpeaker(s): Professor Karu
  Esselle\, \n\nVirtual: https://events.vtools.ieee.org/m/322522
LOCATION:Virtual: https://events.vtools.ieee.org/m/322522
ORGANIZER:syed.abbas@mq.edu.au
SEQUENCE:2
SUMMARY:Many names\, many advantages – from Trentini to beam steering of 
 modern (Fabry-Perot) Resonant Cavity antennas
URL;VALUE=URI:https://events.vtools.ieee.org/m/322522
X-ALT-DESC:Description: &lt;br /&gt;&lt;p&gt;No other antenna concept has more names. A
 t present these antennas are known as Fabry-Perot resonant cavity antennas
 \, just Resonant Cavity Antennas (RCA)\, Partial Reflector Surface (PRS) b
 ased antennas\, Electromagnetic Band Gap (EBG) Resonator antennas (ERAs) a
 nd Two Dimensional Leaky-Wave Antennas\, and more names are forthcoming. Y
 et they all have more or less the same configuration consisting of a reson
 ant cavity\, formed between a partially reflecting superstructure and a fu
 lly reflecting (ground) plane. The resonant cavity is excited by a small f
 eed antenna. Hence\, they are referred to as resonant cavity antennas (RCA
 s) in this presentation. Since the concept of using a &amp;ldquo\;partially re
 flecting sheet array&amp;rdquo\; superstructure to significantly enhance the d
 irectivity was disclosed by Trentini in 1956\, it has been an attractive c
 oncept to several antenna researchers for several reasons\, including its 
 theoretical elegance\, relationships to other wellresearched area such as
  leaky-waves\, EBG\, frequency selective surfaces and metasurfaces\, and p
 ractical advantages as a low-cost simple way to achieve high-gain (15-25 d
 Bi) from an efficient planar antenna without an array\, which requires a f
 eed network. The RCA concept is one of the main&amp;nbsp\; beneficiaries of th
 e surge of research on electromagnetic periodic structures in the last dec
 ade\, first inspired by EBG and then to some extent by metamaterials. As a
  result\, RCAs gained a tremendous improvement in performance in the last 
 10 years\, in addition to other advantages such as size reduction. As an e
 xample\, achieving 10% gain bandwidth from such an antenna with a PSS was 
 a major breakthrough in 2006 but now there are prototypes with gain bandwi
 dths greater than 50%. Until recently most RCAs required an area in the ra
 nge of 25-100 square wavelengths but the latest extremely wideband RCAs ar
 e very compact\, requiring only 1.5-2 square wavelengths at the lowest ope
 rating frequency. Once limited to a select group of researchers\, these ad
 vantages have attracted many new researchers to RCA research domain\, and 
 the list is growing fast\, as demonstrated by the diversity of authors in 
 recent RCA publications. RCAs have already replaced other types of antenna
 s\, for example as feeds for reflectors.&lt;/p&gt;\n&lt;p&gt;This presentation will ta
 ke the audience through historical achievements of RCA technology\, giving
  emphasis to breakthroughs in the last 20 years up to a recent method of s
 teering its beam continuously in 2D (i.e.\, azimuth and elevation).&amp;nbsp\;
 &lt;/p&gt;
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