Further antenna pattern measurements in the 13-mm microwave band on the goldstone space communications station 30-ft antenna
Microwave band antenna pattern measurements
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Microwave band antenna pattern measurements
The NASA JPL Deep Spae Network (DSN) of large, dual reflector antennas is subject to continuing demands for improved performance and reliabilty as a result of communications, control, and radio science requirement for future missions.
Radiation pattern direction control is one of the most important capabilities of nanoantennas required in optical wireless nano-link for emitting into or detecting from the desired direction. In this work, a novel triangle nanoantenna operating in the near-infrared region is proposed in which the angle of maximum power emission is tuned via rotating one of the triangles and fixing the remaining ones. The advantage of this theme is the result of using piezoelectricity to tune the gap between nano-particles in a nano-antenna and also the possibility of tuning the angle of the pattern up to 25°. By adding a nano-particle to the structure and varying its location, the radiation pattern can be rotated in the desired angle.
Tracking antenna for Apollo S-band communication and feed system support
Antenna system radiation patterns obtained using Surveyor I spacecraft
Indirect high impact test of cavity-backed spiral antenna
Calculated gain of advanced antenna system
Indirect impact test of cupped turnstile antenna
Orbital position and attitude tracking of ATS SPACECRAFT using parabolic ground antennas
Minkowsky electrodynamic theory and power conservation law used to calculate receiving area of dipole antenna immersed in moving ionized medium
Traveling wave V antenna, discussing parameter variation effect on radiation patterns
This work includes a simplified analysis of the radiated near to mid-field from JPL/NASA Deep Space Network (DSN) reflector antennas and uses an averaging technique over the main beam region and beyond for complying with FAA regulations in specific aviation environments. The work identifies areas that require special attention, including the implications of the very narrow beam of the DSN transmitters. The paper derives the maximum averaged power densities allowed and identifies zones where mitigation measures are required.
Photosynthesis in some phototrophic bacteria requires the PufX component of the reaction centre–light‐harvesting 1–PufX ( RC ‐ LH 1‐PufX) complex, which creates a pore for quinone/quinol (Q/ QH 2 ) exchange across the LH 1 barrier surrounding the RC . However, photosynthetic bacteria such as Thermochromatium (T.) tepidum do not require PufX because there are fewer carotenoid binding sites, which creates multiple pores in the LH 1 ring for Q/ QH 2 exchange. We show that an αTrp ‐24 →Phe alteration of the Rhodobacter (Rba.) sphaeroides LH 1 antenna impairs carotenoid binding and allows photosynthetic growth in the absence of PufX. We propose that acquisition of PufX and confining Q/ QH 2 traffic to a pore adjacent to the RC Q B site is an evolutionary upgrade that allows increased LH 1 carotenoid content for enhanced light absorption and photoprotection.
A hyperbolic metamaterial (HM) resonator is analyzed as a nano-antenna for enhancing the radiative emission of quantum emitters in its vicinity. It has been shown that the spontaneous emission rate by an emitter near a hyperbolic metamaterial substrate is enhanced dramatically due to very large density of states. However, enhanced coupling to the free-space, which is central to applications such as solid-state lighting, has not been investigated significantly. Here, we numerically demonstrate approximately 100 times enhancement of the free-space radiative emission at 660 nm wavelength by utilizing a cylindrical HM resonator with a radius of 54 nm and a height of 80 nm on top of an opaque silver-cladded substrate. We also show how the free-space radiation enhancement factor depends on the dipole orientation and the location of the emitter near the subwavelength resonator. Furthermore, we calculate that an array of HM resonators with subwavelength spacings can maintain most of the enhancement effect of a single resonator.
Large space parabolic expandable truss antenna experiment
Parabolic expandable truss antenna experiment design for Apollo applications program
Mathematical model for radio frequency circuitry of Apollo high gain antenna system
Erectable truss parabolic antenna