Results 81 to 90 of about 988 (180)
Utilizing Planck polarized dust emission maps at 353 GHz and large-area maps of the neutral hydrogen (H i ) cold neutral medium (CNM) fraction ( f _CNM ), we investigate the relationship between dust polarization fraction ( p _353 ) and f _CNM in the ...
Minjie Lei, S. E. Clark
doaj +1 more source
Interstellar Magnetic Fields: An Observational Perspective
Abstract: Chapter 1 establishes the plausibility of “magnetic molecular clouds.” We show that the empirically known relations between spectral line width, density, and cloud size can be derived from a virial equilibrium model where gravity is balanced by the sum of magnetic and pressure support.
openaire +2 more sources
Polarization of starlight and thermal dust emission due to aligned non-spherical grains helps us to trace magnetic field ( B -field) morphology in molecular clouds and to study grain alignment mechanisms.
Saikhom Pravash +5 more
doaj +1 more source
Dust polarization induced by aligned nonspherical grains acts as an important tool to trace the magnetic field ( B -field) morphologies and strengths in molecular clouds and constrain grain properties and their alignment mechanisms.
Saikhom Pravash +7 more
doaj +1 more source
While plane-of-sky magnetic field observations in molecular clouds are now common, observations of their line-of-sight magnetic field remain limited. To address this issue, M. Tahani et al. developed a technique based on Faraday rotation.
Mehrnoosh Tahani +5 more
doaj +1 more source
Direct Samples of Interstellar and Interplanetary Material with IMAP. [PDF]
Szalay JR +21 more
europepmc +1 more source
Transport of Electrons in Tangled Magnetic Fields. [PDF]
Verscharen D +8 more
europepmc +1 more source
IMAP's Role in Understanding Particle Injection and Energization Throughout the Heliosphere. [PDF]
Cohen CMS +30 more
europepmc +1 more source
Increased and varied radiation during the Sun's encounters with cold clouds in the last 10 million years. [PDF]
Opher M +9 more
europepmc +1 more source

