Results 131 to 140 of about 37,251 (259)

Implications of Interstellar Dust and Magnetic Field at the Heliosphere [PDF]

, 2007
P. C. Frisch
openalex   +1 more source

A study of the Chamaeleon I dark cloud and T-association – VI. Interstellar polarization, grain alignment and magnetic field [PDF]

, 1994
D. C. B. Whittet, P. A. Gerakines, Arthur Lee Carkner, J. H. Hough, P. G. Martin, T. Prusti, D. Kilkenny   +6 more
openalex   +1 more source

Extreme Starlight Polarization Efficiency toward ζ Ophiuchi: A Case for Line-of-sight Foreground Subtraction

The Astronomical Journal
Despite the pervasive nature of interstellar dust and its impact on nearly all observations, most dust corrections employ line-of-sight averages over large angular scales.
Jordan A. Bartlett, Henry A. Kobulnicky
doaj   +1 more source

The Local Interstellar Magnetic Field and the IBEX Ribbon [PDF]

, 2016
R. Ratkiewicz, M. Strumik
openalex   +1 more source

Magnetic Field and Plasma Density Observations of a Pressure Front by Voyager 1 during 2020 in the Very Local Interstellar Medium [PDF]

, 2021
L. F. Burlaga, W. S. Kŭrth, D. A. Gurnett, D. B. Berdichevsky, L. K. Jian, N. F. Ness, Jeewoo Park, Á. Szabó   +7 more
openalex   +1 more source

Study of Magnetic Field and Turbulence in the TeV Halo around the Monogem Pulsar

The Astrophysical Journal
Magnetic fields are ubiquitous in the interstellar medium, including extended objects such as supernova remnants and diffuse halos around pulsars. Its turbulent characteristics govern the diffusion of cosmic rays and the multiwavelength emission from ...
Sunil Malik, Ka Ho Yuen, Huirong Yan
doaj   +1 more source

Heliosphere for a wide range of interstellar magnetic field strengths as a source of energetic neutral atoms [PDF]

, 2015
A. Czechowski, J. Grygorczuk, D. J. McComas   +2 more
openalex   +1 more source

42. Solar cosmic radiation and the interstellar magnetic field [PDF]

, 1958
A. Ehmert
openalex   +1 more source

Faraday Tomography with CHIME: The “Tadpole” Feature G137+7

The Astrophysical Journal
A direct consequence of Faraday rotation is that the polarized radio sky does not resemble the total intensity sky at long wavelengths. We analyze G137+7, which is undetectable in total intensity but appears as a depolarization feature.
Nasser Mohammed, Anna Ordog, Rebecca A. Booth, Andrea Bracco, Jo-Anne C. Brown, Ettore Carretti, John M. Dickey, Simon Foreman, Mark Halpern, Marijke Haverkorn, Alex S. Hill, Gary Hinshaw, Joseph W. Kania, Roland Kothes, T. L. Landecker, Joshua MacEachern, Kiyoshi W. Masui, Aimee Menard, Ryan R. Ransom, Wolfgang Reich, Patricia Reich, J. Richard Shaw, Seth R. Siegel, Mehrnoosh Tahani, Alec J. M. Thomson, Tristan Pinsonneault-Marotte, Haochen Wang, Jennifer L. West, Maik Wolleben, Dallas Wulf, CHIME and GMIMS Collaborations   +30 more
doaj   +1 more source

TURBULENCE AND MAGNETIC FIELD AMPLIFICATION IN SUPERNOVA REMNANTS: INTERACTIONS BETWEEN A STRONG SHOCK WAVE AND MULTIPHASE INTERSTELLAR MEDIUM [PDF]

, 2009
Tsuyoshi Inoue, Ryo Yamazaki, Shu-ichiro Inutsuka   +2 more
openalex   +1 more source