Speaker
Mr
Jiaxin Wang
(SISSA)
Description
I would like to present my numerical work in simulating
the Galactic synchrotron emission, with the hammurabiX package,
where we have proposed fast generators for realizing
the Galactic magnetic turbulence with physical motivations
and modelings.
We find out the synchrotron B/E ratio is related to both the
spatial and spectral structure of the magnetic turbulence.
In addition, I would also like to share our work in the
IMAGINE consortium towards inferring the Galactic components
with Bayesian analysis, and our idea of the consistent numerical
approach to simulating the Galactic emissions.
Primary authors
Mr
Jiaxin Wang
(SISSA)
Prof.
Tess Jaffe
(NASA)
Co-authors
Prof.
Piero Ullio
(SISSA)
Prof.
Torsten Ensslin
(MPA)
