5 research outputs found
The LOFAR Magnetism Key Science Project
Measuring radio waves at low frequencies offers a new window to study cosmic
magnetism, and LOFAR is the ideal radio telescope to open this window widely.
The LOFAR Magnetism Key Science Project (MKSP) draws together expertise from
multiple fields of magnetism science and intends to use LOFAR to tackle
fundamental questions on cosmic magnetism by exploiting a variety of
observational techniques. Surveys will provide diffuse emission from the Milky
Way and from nearby galaxies, tracking the propagation of long-lived cosmic-ray
electrons through magnetic field structures, to search for radio halos around
spiral and dwarf galaxies and for magnetic fields in intergalactic space.
Targeted deep-field observations of selected nearby galaxies and suspected
intergalactic filaments allow sensitive mapping of weak magnetic fields through
Rotation Measure (RM) grids. High-resolution observations of protostellar jets
and giant radio galaxies reveal structures on small physical scales and at high
redshifts, whilst pulsar RMs map large-scale magnetic structures of the
Galactic disk and halo in revolutionary detail. The MKSP is responsible for the
development of polarization calibration and processing, thus widening the
scientific power of LOFAR.Comment: Proceedings of "Magnetic Fields in the Universe: From Laboratory and
Stars to Primordial Structures", 2011 Aug. 21-27 in Zakopane/Poland, eds. M.
Soida et a
Measuring magnetism in the Milky Way with the Square Kilometre Array
Magnetic fields in the Milky Way are present on a wide variety of sizes and
strengths, influencing many processes in the Galactic ecosystem such as star
formation, gas dynamics, jets, and evolution of supernova remnants or pulsar
wind nebulae. Observation methods are complex and indirect; the most used of
these are a grid of rotation measures of unresolved polarized extragalactic
sources, and broadband polarimetry of diffuse emission. Current studies of
magnetic fields in the Milky Way reveal a global spiral magnetic field with a
significant turbulent component; the limited sample of magnetic field
measurements in discrete objects such as supernova remnants and HII regions
shows a wide variety in field configurations; a few detections of magnetic
fields in Young Stellar Object jets have been published; and the magnetic field
structure in the Galactic Center is still under debate.
The SKA will unravel the 3D structure and configurations of magnetic fields
in the Milky Way on sub-parsec to galaxy scales, including field structure in
the Galactic Center. The global configuration of the Milky Way disk magnetic
field, probed through pulsar RMs, will resolve controversy about reversals in
the Galactic plane. Characteristics of interstellar turbulence can be
determined from the grid of background RMs. We expect to learn to understand
magnetic field structures in protostellar jets, supernova remnants, and other
discrete sources, due to the vast increase in sample sizes possible with the
SKA. This knowledge of magnetic fields in the Milky Way will not only be
crucial in understanding of the evolution and interaction of Galactic
structures, but will also help to define and remove Galactic foregrounds for a
multitude of extragalactic and cosmological studies.Comment: 19 pages, 2 figures; to appear as part of 'Cosmic Magnetism' in
Proceedings 'Advancing Astrophysics with the SKA (AASKA14)', PoS(AASKA14)09