Simulated square kilometre array maps from Galactic 3D-emission models

Astronomy and Astrophysics

Volumn 507, Issue 2, 2009, Pages 1087-1105

  Sun, X H ^a,b   Reich, W ^b  

^a CHINESE ACADEMY OF SCIENCES   (China)

^b MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

Author keywords

ISM: magnetic field; ISM: structure; Magnetic fields; Polarization; Radiation mechanisms: non thermal

Indexed keywords

3D MODELS; ANGULAR RESOLUTION; EMISSION MODEL; EXTRAGALACTIC SOURCES; GALACTIC EMISSION; GALACTIC LATITUDE; GALACTIC PLANE; GAUSSIANS; HIGH LATITUDES; HIGH RESOLUTION; ISM: MAGNETIC FIELDS; ISM: STRUCTURE; KOLMOGOROV; LINES-OF-SIGHT; MAGNETIC FIELD COMPONENTS; OUTER SCALE; POLARIZED EMISSIONS; POWER-LAW; RADIATION MECHANISMS: NONTHERMAL; SMALL SCALE; STEEPER SLOPES; STRUCTURE FUNCTIONS; TECHNICAL REALIZATION; TURBULENT MAGNETIC FIELDS;

COMPUTATIONAL COMPLEXITY; MAGNETIC FIELDS; MAGNETIC MATERIALS; POLARIZATION; POWER SPECTRUM; PROBABILITY DENSITY FUNCTION; SIMULATORS; WIRELESS TELECOMMUNICATION SYSTEMS;

THREE DIMENSIONAL;

EID: 70450173536     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912539     Document Type: Article

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