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Astrophysical Polarized Backgrounds: Workshop on Astrophysical Polarized Backgrounds Book

Astrophysical Polarized Backgrounds: Workshop on Astrophysical Polarized Backgrounds
Astrophysical Polarized Backgrounds: Workshop on Astrophysical Polarized Backgrounds, During the last decades of the past century, several experiments measuring the Cosmic Microwave Background (CMB) anisotropy spectrum (e.g. COBE, TOCO, BOOMeranG, MAXIMA, DASI, CBI) have contributed significantly to our understanding of the properties of o, Astrophysical Polarized Backgrounds: Workshop on Astrophysical Polarized Backgrounds has a rating of 3 stars
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Astrophysical Polarized Backgrounds: Workshop on Astrophysical Polarized Backgrounds, During the last decades of the past century, several experiments measuring the Cosmic Microwave Background (CMB) anisotropy spectrum (e.g. COBE, TOCO, BOOMeranG, MAXIMA, DASI, CBI) have contributed significantly to our understanding of the properties of o, Astrophysical Polarized Backgrounds: Workshop on Astrophysical Polarized Backgrounds
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  • Astrophysical Polarized Backgrounds: Workshop on Astrophysical Polarized Backgrounds
  • Written by author R. Sault
  • Published by Springer-Verlag New York, LLC, March 2002
  • During the last decades of the past century, several experiments measuring the Cosmic Microwave Background (CMB) anisotropy spectrum (e.g. COBE, TOCO, BOOMeranG, MAXIMA, DASI, CBI) have contributed significantly to our understanding of the properties of o
  • During the last decades of the past century, several experiments measuring the Cosmic Microwave Background (CMB) anisotropy spectrum (e.g. COBE, TOCO, BOOMeranG, MAXIMA, DASI, CBI) have contributed significantly to our understanding of the properties of o
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Authors

Preface
Group Photograph
Polarization Surveys of the Galaxy3
Polarization Imaging of the Galactic Emission at 1420 MHz - The Canadian Galactic Plane Survey9
Counter-intuitive Polarization Structures15
High Resolution Polarimetry of the Inner Galaxy20
Low Frequency Polarization Observations of the Galactic Radio Emission26
Polarized Microwave Emission from Dust32
Dust Polarization from Starlight Data44
Small Scale I, U, Q Galaxy Noise at cm. Waves51
A Multifrequency Analysis of the Polarized Diffuse Galactic Radio Emission at Degree Scales54
Angular Spectra of Galactic Polarized Synchrotron Emission at Arcmin Scales60
Galactic Synchrotron Foreground and the CMB Polarization Measurements66
Parsec-scale Structure in the Warm ISM from Polarized Galactic Radio Background Observations72
CMB Polarization: Scientific Case and Data Analysis Issues78
Polarized Foregrounds Power Spectra vs CMB84
Cosmic Magnetic Fields: What We Know, What We Must Discover90
Magnetic Fields in Our Galaxy: How Much Do We Know? (II) Halo Fields and the Global Field Structure96
Whistlers in Interstellar Gas Dynamics102
The SPOrt Experiment109
The BaR-SPOrt Experiment115
B2K: The Polarization-sensitive BOOMERanG Experiment122
ELISA: A Small Balloon Experiment for a Large Scale Survey in the Sub-millimeter129
Measuring CMB Polarisation with the Planck HFI135
The Low Frequency Instrument of the Planck Mission144
Precision and Widefield Polarimetry with the Australia Telescope Compact Array150
AMiBA - Array for Microwave Background Anisotropy156
QUEST - A 2.6-m mm-Wave Telescope for CMB Polarization Studies159
The Milano Polarization Experiment Devoted to the Study of the Cosmic Microwave Background164
The Polarimetric Observation Facility at the Medicina 32 m Parabolic Antenna169
Millimeter Wave Passive Components for Polarization Measurements177
Calibrating CMB Polarization Telescopes183
The Moon as a Calibrator of Linearly Polarized Radio Emission for the SPOrt Project187
A Destriping Technique for SPOrt Polarization Data193
Statistical Evaluation and Processing of Uncorrelated and Correlated Outputs of the SPOrt Radiometer199
A Code for Dust Polarized Emission Simulation205
Some Sources of Systematic Errors on CMB Polarized Measurements with Bolometers209
Systematics of Microwave Polarimetry with the Planck LFI215
The ASI Science Program225
Luigi Broglio Base Facilities and Activities: The ASI Balloon Program228
The NASA Balloon Program: An Overview235
The Esrange Facility in Northern Sweden - Your Partner for Successful Aerospace Operations239
Scientific Balloons from Svalbard243
The Rapid Prototyping Approach in the Design and Testing of Radiometric Systems251
Calibration Techniques and Devices for Correlation Radiometers Used in Polarization Measurements257
Synchrotron Angular Spectra at Various Galactic Latitudes and Frequencies261
Submillimetre Polarization of M82 and the Galactic Centre: Implications for CMB Polarimetry267
Polarization of the Cosmic Microwave Background from Non-Uniform Reionization271
Thermal Design and Preliminary Performance Evaluation of the Cooling System for BaR-SPOrt275
SDAMS: SPOrt Data Archiving and Management System279
A Millimeter Polarimeter for the 45m Telescope at Nobeyama283
Observations of Linear Polarization of Background Galactic Radio Emission in Selected Direction at 8.3 GHz287
Radio Polarimetry: A Historical Development at Effelsberg291
Workshop Summary and the Future295
List of Participants305
Author Index311


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Astrophysical Polarized Backgrounds: Workshop on Astrophysical Polarized Backgrounds, During the last decades of the past century, several experiments measuring the Cosmic Microwave Background (CMB) anisotropy spectrum (e.g. COBE, TOCO, BOOMeranG, MAXIMA, DASI, CBI) have contributed significantly to our understanding of the properties of o, Astrophysical Polarized Backgrounds: Workshop on Astrophysical Polarized Backgrounds

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Astrophysical Polarized Backgrounds: Workshop on Astrophysical Polarized Backgrounds, During the last decades of the past century, several experiments measuring the Cosmic Microwave Background (CMB) anisotropy spectrum (e.g. COBE, TOCO, BOOMeranG, MAXIMA, DASI, CBI) have contributed significantly to our understanding of the properties of o, Astrophysical Polarized Backgrounds: Workshop on Astrophysical Polarized Backgrounds

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Astrophysical Polarized Backgrounds: Workshop on Astrophysical Polarized Backgrounds, During the last decades of the past century, several experiments measuring the Cosmic Microwave Background (CMB) anisotropy spectrum (e.g. COBE, TOCO, BOOMeranG, MAXIMA, DASI, CBI) have contributed significantly to our understanding of the properties of o, Astrophysical Polarized Backgrounds: Workshop on Astrophysical Polarized Backgrounds

Astrophysical Polarized Backgrounds: Workshop on Astrophysical Polarized Backgrounds

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