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Preface | ||
Group Photograph | ||
Polarization Surveys of the Galaxy | 3 | |
Polarization Imaging of the Galactic Emission at 1420 MHz - The Canadian Galactic Plane Survey | 9 | |
Counter-intuitive Polarization Structures | 15 | |
High Resolution Polarimetry of the Inner Galaxy | 20 | |
Low Frequency Polarization Observations of the Galactic Radio Emission | 26 | |
Polarized Microwave Emission from Dust | 32 | |
Dust Polarization from Starlight Data | 44 | |
Small Scale I, U, Q Galaxy Noise at cm. Waves | 51 | |
A Multifrequency Analysis of the Polarized Diffuse Galactic Radio Emission at Degree Scales | 54 | |
Angular Spectra of Galactic Polarized Synchrotron Emission at Arcmin Scales | 60 | |
Galactic Synchrotron Foreground and the CMB Polarization Measurements | 66 | |
Parsec-scale Structure in the Warm ISM from Polarized Galactic Radio Background Observations | 72 | |
CMB Polarization: Scientific Case and Data Analysis Issues | 78 | |
Polarized Foregrounds Power Spectra vs CMB | 84 | |
Cosmic Magnetic Fields: What We Know, What We Must Discover | 90 | |
Magnetic Fields in Our Galaxy: How Much Do We Know? (II) Halo Fields and the Global Field Structure | 96 | |
Whistlers in Interstellar Gas Dynamics | 102 | |
The SPOrt Experiment | 109 | |
The BaR-SPOrt Experiment | 115 | |
B2K: The Polarization-sensitive BOOMERanG Experiment | 122 | |
ELISA: A Small Balloon Experiment for a Large Scale Survey in the Sub-millimeter | 129 | |
Measuring CMB Polarisation with the Planck HFI | 135 | |
The Low Frequency Instrument of the Planck Mission | 144 | |
Precision and Widefield Polarimetry with the Australia Telescope Compact Array | 150 | |
AMiBA - Array for Microwave Background Anisotropy | 156 | |
QUEST - A 2.6-m mm-Wave Telescope for CMB Polarization Studies | 159 | |
The Milano Polarization Experiment Devoted to the Study of the Cosmic Microwave Background | 164 | |
The Polarimetric Observation Facility at the Medicina 32 m Parabolic Antenna | 169 | |
Millimeter Wave Passive Components for Polarization Measurements | 177 | |
Calibrating CMB Polarization Telescopes | 183 | |
The Moon as a Calibrator of Linearly Polarized Radio Emission for the SPOrt Project | 187 | |
A Destriping Technique for SPOrt Polarization Data | 193 | |
Statistical Evaluation and Processing of Uncorrelated and Correlated Outputs of the SPOrt Radiometer | 199 | |
A Code for Dust Polarized Emission Simulation | 205 | |
Some Sources of Systematic Errors on CMB Polarized Measurements with Bolometers | 209 | |
Systematics of Microwave Polarimetry with the Planck LFI | 215 | |
The ASI Science Program | 225 | |
Luigi Broglio Base Facilities and Activities: The ASI Balloon Program | 228 | |
The NASA Balloon Program: An Overview | 235 | |
The Esrange Facility in Northern Sweden - Your Partner for Successful Aerospace Operations | 239 | |
Scientific Balloons from Svalbard | 243 | |
The Rapid Prototyping Approach in the Design and Testing of Radiometric Systems | 251 | |
Calibration Techniques and Devices for Correlation Radiometers Used in Polarization Measurements | 257 | |
Synchrotron Angular Spectra at Various Galactic Latitudes and Frequencies | 261 | |
Submillimetre Polarization of M82 and the Galactic Centre: Implications for CMB Polarimetry | 267 | |
Polarization of the Cosmic Microwave Background from Non-Uniform Reionization | 271 | |
Thermal Design and Preliminary Performance Evaluation of the Cooling System for BaR-SPOrt | 275 | |
SDAMS: SPOrt Data Archiving and Management System | 279 | |
A Millimeter Polarimeter for the 45m Telescope at Nobeyama | 283 | |
Observations of Linear Polarization of Background Galactic Radio Emission in Selected Direction at 8.3 GHz | 287 | |
Radio Polarimetry: A Historical Development at Effelsberg | 291 | |
Workshop Summary and the Future | 295 | |
List of Participants | 305 | |
Author Index | 311 |
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Add 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 to the inventory that you are selling on WonderClubX
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Add 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 to your collection on WonderClub |