Study of Polarization Maps from Numerical Simulations

D. Falceta-Goncalves; A. Lazarian

Study of Polarization Maps from Numerical Simulations

D. Falceta-Goncalves^*, A. Lazarian

^*Corresponding author for this work

School of Physics and Astronomy

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Abstract

In this work we performed a number of MHD numerical simulations of the ISM, for different Alfvenic and sonic Mach numbers. We used the data cubes to perform synthetic calculations of observable polarization and velocity dispersion maps. Based on these, we were able to study the statistics of polarization vectors and compare the obtained results with the different turbulent regimes.

Original language	English
Title of host publication	ASTRONOMICAL POLARIMETRY 2008: SCIENCE FROM SMALL TO LARGE TELESCOPES
Editors	P Bastien, N Manset, DP Clemens, N StLouis
Place of Publication	SAN FRANCISCO
Publisher	Astronomical Society of the Pacific
Pages	159-160
Number of pages	2
ISBN (Print)	978-1-58381-780-3
Publication status	Published - 2011
Event	Conference on Astronomical Polarimetry 2008 - Science from Small to Large Telescopes - La Malbaie, Canada Duration: 6 Jul 2008 → 11 Jul 2008

Publication series

Name	Astronomical Society of the Pacific Conference Series
Publisher	ASTRONOMICAL SOC PACIFIC
Volume	449

Conference

Conference	Conference on Astronomical Polarimetry 2008 - Science from Small to Large Telescopes
Country/Territory	Canada
City	La Malbaie
Period	6/07/08 → 11/07/08

Cite this

@inproceedings{f719e4d36e3c48e6828ba4d2f72a48c9,

title = "Study of Polarization Maps from Numerical Simulations",

abstract = "In this work we performed a number of MHD numerical simulations of the ISM, for different Alfvenic and sonic Mach numbers. We used the data cubes to perform synthetic calculations of observable polarization and velocity dispersion maps. Based on these, we were able to study the statistics of polarization vectors and compare the obtained results with the different turbulent regimes.",

author = "D. Falceta-Goncalves and A. Lazarian",

year = "2011",

language = "English",

isbn = "978-1-58381-780-3",

series = "Astronomical Society of the Pacific Conference Series",

publisher = "Astronomical Society of the Pacific",

pages = "159--160",

editor = "P Bastien and N Manset and DP Clemens and N StLouis",

booktitle = "ASTRONOMICAL POLARIMETRY 2008: SCIENCE FROM SMALL TO LARGE TELESCOPES",

note = "Conference on Astronomical Polarimetry 2008 - Science from Small to Large Telescopes ; Conference date: 06-07-2008 Through 11-07-2008",

}

Falceta-Goncalves, D & Lazarian, A 2011, Study of Polarization Maps from Numerical Simulations. in P Bastien, N Manset, DP Clemens & N StLouis (eds), ASTRONOMICAL POLARIMETRY 2008: SCIENCE FROM SMALL TO LARGE TELESCOPES. Astronomical Society of the Pacific Conference Series, vol. 449, Astronomical Society of the Pacific, SAN FRANCISCO, pp. 159-160, Conference on Astronomical Polarimetry 2008 - Science from Small to Large Telescopes, La Malbaie, Canada, 6/07/08.

Study of Polarization Maps from Numerical Simulations. / Falceta-Goncalves, D.; Lazarian, A.
ASTRONOMICAL POLARIMETRY 2008: SCIENCE FROM SMALL TO LARGE TELESCOPES. ed. / P Bastien; N Manset; DP Clemens; N StLouis. SAN FRANCISCO: Astronomical Society of the Pacific, 2011. p. 159-160 (Astronomical Society of the Pacific Conference Series; Vol. 449).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

TY - GEN

T1 - Study of Polarization Maps from Numerical Simulations

AU - Falceta-Goncalves, D.

AU - Lazarian, A.

PY - 2011

Y1 - 2011

N2 - In this work we performed a number of MHD numerical simulations of the ISM, for different Alfvenic and sonic Mach numbers. We used the data cubes to perform synthetic calculations of observable polarization and velocity dispersion maps. Based on these, we were able to study the statistics of polarization vectors and compare the obtained results with the different turbulent regimes.

AB - In this work we performed a number of MHD numerical simulations of the ISM, for different Alfvenic and sonic Mach numbers. We used the data cubes to perform synthetic calculations of observable polarization and velocity dispersion maps. Based on these, we were able to study the statistics of polarization vectors and compare the obtained results with the different turbulent regimes.

M3 - Conference contribution

SN - 978-1-58381-780-3

T3 - Astronomical Society of the Pacific Conference Series

SP - 159

EP - 160

BT - ASTRONOMICAL POLARIMETRY 2008: SCIENCE FROM SMALL TO LARGE TELESCOPES

A2 - Bastien, P

A2 - Manset, N

A2 - Clemens, DP

A2 - StLouis, N

PB - Astronomical Society of the Pacific

CY - SAN FRANCISCO

T2 - Conference on Astronomical Polarimetry 2008 - Science from Small to Large Telescopes

Y2 - 6 July 2008 through 11 July 2008

ER -

Study of Polarization Maps from Numerical Simulations

Abstract

Publication series

Conference

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