Cultural advice

The Australian National University acknowledges, celebrates and pays our respects to the Ngunnawal and Ngambri people of the Canberra region and to all First Nations Australians on whose traditional lands we meet and work, and whose cultures are among the oldest continuing cultures in human history.

Aboriginal and Torres Strait Islander peoples are advised that ANU Library collections may include images, names, voices, and other representations of deceased persons.

Material in the collection may contain terms, language or views that reflect the period in which the item was created and may be considered inappropriate today.

Studying Galactic interstellar turbulence through fluctuations in synchrotron emission: First LOFAR Galactic foreground detection

Thumbnail Image

Date

2013

Authors

Pizzo, R
Bonafede, A
Heald, G
Kuniyoshi, M
Reich, W
Sobey, C
Asgekar, A
Bentum, M J
Bernardi, G
Best, Phillip

Journal Title

Journal ISSN

Volume Title

Publisher

Springer

Abstract

Aims. The characteristic outer scale of turbulence (i.e. the scale at which the dominant source of turbulence injects energy to the interstellar medium) and the ratio of the random to ordered components of the magnetic field are key parameters to characte

Description

Keywords

Keywords: ISM: general; ISM: magnetic fields; ISM: structure; Radio continuum: general; Radio continuum: ISM; Techniques: interferometric; Estimation; Magnetic fields; Power spectrum; Synchrotron radiation; Turbulence ISM: general; ISM: magnetic fields; ISM: structure; Radio continuum: general; Radio continuum: ISM; Techniques: interferometric

Citation

URI

http://hdl.handle.net/1885/75139

Collections

ANU Research Publications

Source

Astronomy and Astrophysics

Type

Journal article

Book Title

Entity type

Access Statement

Open Access

License Rights

DOI

10.1051/0004-6361/201322013

Restricted until

Downloads

File
Description
01_Pizzo_Studying_Galactic_interstellar_2013.pdf (1.6 MB)

DSpace software copyright © 2002-2026 LYRASIS

abcd