Multiwavelength Magnetic Field Modeling
2012 ◽
Vol 10
(H16)
◽
pp. 401-401
Keyword(s):
AbstractWe model the large-scale Galactic magnetic fields, including a spiral arm compression to generate anisotropic turbulence, by comparing polarized synchrotron and thermal dust emission. Preliminary results show that in the outer Galaxy, the dust emission comes from regions where the fields are more ordered than average while the situation is reversed in the inner Galaxy. We will attempt in subsequent work to present a more complete picture of what the comparison of these observables tells us about the distribution of the components of the magnetized ISM and about the physics of spiral arm shocks and turbulence.
Keyword(s):
1998 ◽
Vol 07
(03)
◽
pp. 331-349
◽
2008 ◽
Vol 4
(S254)
◽
pp. 95-96
Keyword(s):
Electromagnetically conducting elastic plates in a magnetic field: modeling and dynamic implications
2004 ◽
Vol 39
(5)
◽
pp. 723-739
◽
2008 ◽
Vol 4
(S259)
◽
pp. 455-466
◽
Keyword(s):
2009 ◽
Vol 114
(A10)
◽
pp. n/a-n/a
◽
Keyword(s):
2019 ◽
Vol 66
(12)
◽
pp. 9112-9121
◽
Keyword(s):