The Interplanetary Network Progress Report 42-154

April-June 2003

Joseph H. Yuen
Editor in Chief


August 15, 2003

NASA Logo
National Aeronautics and
Space Administration

Jet Propulsion Laboratory
California Institute of Technology
Pasadena, California


Contents

Preface

List of Changes

Deep-Space Optical Communications Downlink Budget from Mars: System Parameters
A. Biswas and S. Piazzolla

Deep-Space Optical Communications Downlink Budget: Modulation and Coding
B. Moision and J. Hamkins

An Optical Array Receiver for Deep-Space Communication through Atmospheric Turbulence
V. Vilnrotter, C.-W. Lau, M. Srinivasan, R. Mukai, and K. Andrews

On the Use of W-Band for Deep-Space Communications
S. Shambayati

A Cross-Correlated Trellis-Coded Quadrature Modulation Representation of MIL-STD Shaped Offset Quadrature Phase-Shift Keying
M. K. Simon and L. Li

Generalized Golomb Codes and Adaptive Coding of Wavelet-Transformed Image Subbands
A. Kiely and M. Klimesh

Low-Density Parity-Check (LDPC) Codes Constructed from Protographs
J. Thorpe

Deep Space Network Receiving Systems' Operating Noise Temperature Measurements
C. T. Stelzried, R. C. Clauss, and S. M. Petty

Noise Temperature due to Reflector Surface Resistivity
T. Y. Otoshi

Phase Calibration Generator
R. Hamell, B. Tucker, and M. Calhoun

Non-Parametric Evaluation of Lifetime Data
J. Shell

Control Systems of the Large Millimeter Telescope
W. Gawronski and K. Souccar

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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