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000725073 019__ $$a908088401
000725073 020__ $$a9783662446256$$qelectronic book
000725073 020__ $$a3662446251$$qelectronic book
000725073 020__ $$z9783662446249
000725073 0247_ $$a10.1007/978-3-662-44625-6$$2doi
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000725073 035__ $$aSP(OCoLC)899281196$$z(OCoLC)908088401
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000725073 049__ $$aISEA
000725073 050_4 $$aQC809.M25
000725073 08204 $$a523.01/88$$223
000725073 24500 $$aMagnetic fields in diffuse media$$h[electronic resource] /$$cAlexander Lazarian, Elisabete M. de Gouveia Dal Pino, Claudio Melioli, editors.
000725073 264_1 $$aBerlin :$$bSpringer,$$c[2014]
000725073 264_4 $$c©2015
000725073 300__ $$a1 online resource (xviii, 623 pages) :$$billustrations (some color).
000725073 336__ $$atext$$btxt$$2rdacontent
000725073 337__ $$acomputer$$bc$$2rdamedia
000725073 338__ $$aonline resource$$bcr$$2rdacarrier
000725073 4901_ $$aAstrophysics and Space Science Library,$$x0067-0057
000725073 504__ $$aIncludes bibliographical references and index.
000725073 5050_ $$aPreface; Contents; Part I Current and Forthcoming Observing Facilities; 1 Future Observations of Cosmic Magnetic Fields with LOFAR, SKA and Its Precursors; 1.1 Prospects of Future Magnetic Field Observations; 1.1.1 Diffuse Polarized Emission; 1.1.2 Rotation Measure Grids; 1.1.3 Magnetic Fields of the Milky Way; 1.1.4 Intergalactic Filaments; 1.2 Faraday Rotation Measure Synthesis; 1.3 Low Frequency Array; 1.4 Square Kilometre Array; 1.4.1 Technical Design and Development of the SKA; 1.4.2 SKA Key Science Projects; 1.4.3 SKA Timeline; 1.5 SKA Pathfinder and Precursor Telescopes; References
000725073 5058_ $$a2 Magnetic Fields with the Atacama Large Millimeter/Submillimeter Array2.1 The Atacama Large Millimeter/Submillimeter Array; 2.1.1 ALMA Specifications; 2.1.2 ALMA Science; 2.2 ALMA Polarization Calibration; 2.3 Magnetic Field Observations with ALMA; 2.3.1 (Sub-)Millimetre Polarization; 2.3.1.1 Linear Polarization; 2.3.1.2 Circular Polarization; 2.3.2 Star Formation and Molecular Clouds; 2.3.3 Evolved Stars and Planetary Nebulae; 2.3.4 Nearby Galaxies; 2.4 ALMA Polarization Analysis Tools: The ARTIST Project; Conclusion; References; Part II Techniques for Observing Cosmic Magnetic Fields
000725073 5058_ $$a3 Synchrotron Radiation and Faraday Rotation3.1 Introduction; 3.2 Synchrotron Radiation; 3.2.1 Estimation of Magnetic Field Strength; 3.3 Polarization and Faraday Rotation; 3.4 Rotation Measure Synthesis; 3.4.1 RM Synthesis Deconvolution; 3.4.2 Wavelet Based RM Synthesis; 3.5 Outlook; References; 4 Interstellar Grain Alignment: Observational Status; 4.1 Introduction; 4.2 Grain Alignment Theories; 4.2.1 Theoretical Predictions Amenable to Observational Tests; 4.2.1.1 Paramagnetic Relaxation; 4.2.1.2 Mechanical Alignment; 4.2.1.3 Radiative Alignment; 4.3 Observational Considerations
000725073 5058_ $$a4.4 Observational Constraints on Grain Alignment Mechanisms4.4.1 Davis-Greenstein Alignment; 4.4.2 Super-Paramagnetic Alignment; 4.4.3 Suprathermal Spin Alignment; 4.4.4 Mechanical (Gold) Alignment; 4.4.5 Radiative Alignment; Summary and Conclusions; References; 5 Magnetic Field Measurement with Ground State Alignment; 5.1 Introduction; 5.2 History on Studies Related to Atomic Alignment ; 5.3 Basic Physics of GSA; 5.3.1 Timescales; 5.3.2 Different Regimes; 5.4 Polarization of Absorption Lines; 5.4.1 Is There Any Circular Polarization?; 5.5 IR/Submilimetre Transitions Within Ground State
000725073 5058_ $$a5.6 Atoms with Hyperfine Structure5.7 Polarization of Resonance and Fluorescence Lines; 5.8 Influence of Magnetic field on Polarization and Line Intensity; 5.9 Observational Perspective; 5.9.1 Interstellar Absorption and 3D Magnetic Field Measurement; 5.9.2 Circumstellar Absorption; 5.9.3 Fluorescence from Reflection Nebulae; 5.9.4 Magnetic Field in PDR Regions; 5.10 Observational Tests; 5.11 GSA and Cosmological Studies; 5.11.1 Magnetic Field in the Epoch of Reionization?; 5.11.2 Influence on Abundance Studies; 5.11.3 Metal Detection in Early Universe; 5.12 Feasibility of GSA Studies
000725073 506__ $$aAccess limited to authorized users.
000725073 520__ $$aThis volume presents the current knowledge of magnetic fields in diffuse astrophysical media. Starting with an overview of 21st century instrumentation to observe astrophysical magnetic fields, the chapters cover observational techniques, origin of magnetic fields, magnetic turbulence, basic processes in magnetized fluids, the role of magnetic fields for cosmic rays, in the interstellar medium and for star formation. Written by a group of leading experts the book represents an excellent overview of the field. Nonspecialists will find sufficient background to enter the field and be able to appr.
000725073 588__ $$aOnline resource; title from PDF title page (SpringerLink, viewed January 7, 2015).
000725073 650_0 $$aCosmic magnetic fields.
000725073 650_0 $$aPlasma astrophysics.
000725073 7001_ $$aLazarian, Alexander,$$eeditor.
000725073 7001_ $$aPino, E. M. de Gouveia dal$$q(Elisabete M. de Gouveia dal),$$eeditor.
000725073 7001_ $$aMelioli, Claudio,$$eeditor.
000725073 77608 $$iPrint version:$$aLazarian, Alexander$$tMagnetic Fields in Diffuse Media$$dBerlin, Heidelberg : Springer Berlin Heidelberg,c2014$$z9783662446249
000725073 830_0 $$aAstrophysics and space science library.
000725073 852__ $$bebk
000725073 85640 $$3SpringerLink$$uhttps://univsouthin.idm.oclc.org/login?url=http://link.springer.com/10.1007/978-3-662-44625-6$$zOnline Access$$91397441.1
000725073 909CO $$ooai:library.usi.edu:725073$$pGLOBAL_SET
000725073 980__ $$aEBOOK
000725073 980__ $$aBIB
000725073 982__ $$aEbook
000725073 983__ $$aOnline
000725073 994__ $$a92$$bISE