Toward real time compensation with a combined DFP/AFCS system
Explore the source record for details and available documents.
Engineering topics
Publications and source records attributed to Vilnrotter, V..
Explore the source record for details and available documents.
In the present report, requirements and design of a prototype PPM receiver being designed for development over the next year will be elaborated.
A variety of avalanche photodiodes were tested with pulse position modulated Q-switched laser pulses incident on the detector, with varying amounts of attenuation.
An avalanche photodiode (APD) array for ground-based optical communications receivers is investigated for the reception of optical signals through the turbulent atmosphere. Kolmogorov phase screen simulations are used to generate realistic spatial distributions of the received optical field. It is shown that use of an APD array for pulse-position modulation detection can improve performance by up to 4 dB over single APD detection in the presence of turbulence, but that photon-counting detector arrays yield even greater gains.
In this article, they describe a novel adaptive optical array receiver designed to improve ground-based reception of optical signals.
Explore the source record for details and available documents.
The use of radial basis function networks for fine pointing NASA's 70-meter deep space network antennas is described and evaluated.
The structure of an optimal adaptive array receiver for ground-based optical communications is described and its performance investigated. Kolmogorov phase screen simulations are used to model the sample functions of the focal-plane signal distribution due to turbulence and to generate realistic spatial distributions of the received optical field. This novel array detector concept reduces interference from background radiation by effectively assigning higher confidence levels at each instant of time to those detector elements that contain significant signal energy and suppressing those that do not. A simpler suboptimum structure that replaces the continuous weighting function of the optimal receiver by a hard decision on the selection of the signal detector elements also is described and evaluated. Approximations and bounds to the error probability are derived and compared with the exact calculations and receiver simulation results. It is shown that, for photon-counting receivers observing Poisson-distributed signals, performance improvements of approximately 5 dB can be obtained over conventional single-detector photon-counting receivers, when operating in high background environments.
Ground-based reception of optical signals from space suffers from degradation of the optical phase-front caused by atmospheric turbulence, leading to a reduction in the effective diameter of the receiving aperture and to random fluctuations of the point spread function in the focal plane.
The current plan for DSN evolution calls for the use of Ka-band (32GHz) frequencies on large DSN antennas to increase antenna gain and useful communications bandwidth over that of current X- and S-band systems, with reduced sensitivity to plasma effects.
Explore the source record for details and available documents.
Traditional methods for carrier synchronization of digital signals are obtained from approximations made to a closed loop structure motivated by the maximum a posteriori (MAP) estimation of carrier phase.
The maximum likelihood decision statistic for detection of pulse-position modulated signals with an avalanche photodiode is derived, using the more accurate Webb density rather than Poisson or Gaussian approximations for the distribution of avalanche photodiode output electrons. It is shown that for Webb-distributed output electtrons, the maximum likelihood rule is to choose the PPM word corresponding to the slot with the maximum electron count.
The NASA Deep Space Network (DSN) is preparing to experiment with a new way to supporting highly autonomous missions. The spacecraft will have on-board intelligence to determine whether it is healthy and when ground contact is needed.
Explore the source record for details and available documents.
This paper describes the end-to-end system design, operational scenarios, performance of the ground monitor, and the DS1 experiment.
A closed-form expression for the capacity of an array of correlated Gaussian channels is derived. It is shown that when signal and noise are independent, the array of observables can be replaced with a single observable without diminishing the capacity of the array channel. Examples are provided to illustrate the dependence of channel capacity on noise correlation for two- and three-channel arrays.
A closed-form expression for the capacity of an array of correlated Gaussian channels is derived. It is shown that when signal and noise are independent, the array of observables can be replaced with a single observable without diminishing the capacity of the array channel. Examples are provided to illustrate the dependence of channel capacity on noise correlation for two- and three-channel arrays.