The Interplanetary Network Progress Report

Volume 42-166

Joseph H. Yuen
Editor in Chief


August 15, 2006


National Aeronautics and
Space Administration

Jet Propulsion Laboratory
California Institute of Technology
Pasadena, California


Contents

Preface

Frequency-Agile Multi-Channel X-Band Coherent Receiver/Transmitter for the Advanced Deep Space Transponder
S. K. Smith, N. Mysoor, J. Lux, B. Cook, and B. Shah

High-Rate (130-Mb/s) Ka-Band Downlink Modulator Breadboard for the Advanced Deep Space Transponder
S. K. Smith, N. R. Mysoor, B. M. Cook, J. P. Lux, and B. N. Shah

Lunar Noise-Temperature Increase Measurements at S-Band, X-Band, and Ka-Band Using a 34-Meter-Diameter Beam-Waveguide Antenna
D. D. Morabito

Computing the Noise Temperature Increase Caused by Pointing DSS 13 at the Center of the Moon
W. A. Imbriale

Sub-10-16 Frequency Stability in Multi-Pole Linear Ion Trap Standards: Reduction of Number-Dependent Sensitivity
E. A. Burt and R. L. Tjoelker

Real-Time Wideband Telemetry Receiver Architecture and Performance
K. Andrews, J. Gin, N. Lay, K. Quirk, and M. Srinivasan

Uplink Arraying Experiment with the Mars Global Surveyor Spacecraft
V. Vilnrotter, D. Lee, T. Cornish, R. Mukai, and L. Paal

Adaptive Wavefront-Correction Algorithms Using Focal-Plane Array Intensity Measurements
R. Mukai, V. A. Vilnrotter, and C.-W. Lau

Referees


The research described in this publication was carried out by the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. Reference herein to any specific commercial product, service, process, or service by trade name, trademark, manufacturer, or otherwise, does not constitute or imply its endorsement by the United States Government or the Jet Propulsion Laboratory, California Institute of Technology.


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