An Equilibrium State for the Interstellar Gas and Magnetic Field

نویسندگان

چکیده

برای دانلود باید عضویت طلایی داشته باشید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

The S 1 Shell and Interstellar Magnetic Field and Gas near the

The S1 subshell of the Loop I supernova remnant is consistent with observations of interstellar material close to the Sun. The magnetic field direction of the S1 shell at the Sun agrees with the field direction found from starlight polarization for stars that sample the ecliptic plane at the heliosphere nose, but is barely consistent with the field direction implied by the the offset angle betw...

متن کامل

Triangulation of the Interstellar Magnetic Field

Determining the direction of the local interstellar magnetic field (LISMF) is important for understanding the heliosphere’s global structure, the properties of the interstellar medium, and the propagation of cosmic rays in the local galactic medium. Measurements of interstellar neutral atoms by Ulysses for He and by SOHO/SWAN for H provided some of the first observational insights into the LISM...

متن کامل

Designing an approprate solenoid and magnetic field for the HZDR laser-driven beamline

Nowadays, due to the high costs and large dimensions of the conventional proton accelerators, other optimal methods for producing the proton beam have been studied. Using of Laser-driven proton accelerators is one of the important and new methods. In laser-driven ion acceleration, a highly ultra-intense laser pulse interacts with solid density targets and will create a plasma media that will ac...

متن کامل

Systematic bias in interstellar magnetic field estimates

Faraday rotation of the polarization plane in magnetized thermal plasma provides one of the most efficient methods to deduce regular magnetic fields from radio astronomical observations. Since the Faraday rotation measure RM is proportional to an integral, along the line of sight, of magnetic field weighted with thermal electron density, RM is believed to yield the regular magnetic field averag...

متن کامل

Interstellar Dust and Magnetic Field at the Heliosphere

The very weak polarization of light from nearby stars reaches a maximum near the ecliptic plane in a position offset by λ ∼ 35 from the heliosphere nose direction. The position angle for the polarization in this ecliptic-plane peak is the same for near and distant stars, to within uncertainties, indicating the interstellar magnetic field direction is relatively constant over several hundred par...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

ژورنال

عنوان ژورنال: The Astrophysical Journal

سال: 1967

ISSN: 0004-637X,1538-4357

DOI: 10.1086/149264