Alinement of Solid Interstellar Particles by a 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

synthesis of amido alkylnaphthols using nano-magnetic particles and surfactants

we used dbsa and nano-magnetic for the synthesis of amido alkylnaphtols.

15 صفحه اول

Example : Magnetic Particles in a Magnetic Field

Recall the paramagnetic spin system we discussed in lecture 4. In this system, there are magnets with orientations parallel or antiparallel to a magnetic field. In the parallel orientation, the energy is −mB = −E, where m is the magnetic moment and B is the magnetic field. In the antiparallel orientation the energy is +mB = +E. In lecture 4, we worked out the relative numbers of parallel and an...

متن کامل

Anisotropic magnetic particles in a magnetic field

We characterize the structural properties of magnetic ellipsoidal hematite colloids with an aspect ratio ρ ≈ 2.3 using a combination of small-angle X-ray scattering and computer simulations. The evolution of the phase diagram with packing fraction ϕ and the strength of an applied magnetic field B is described, and the coupling between orientational order of magnetic ellipsoids and the bulk magn...

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

Magnetic Field Amplification by Sn-driven Interstellar Turbulence

Within the interstellar medium, supernovae are thought to be the prevailing agents in driving turbulence. Until recently, their effects on magnetic field amplification in disk galaxies remained uncertain. Analytical models based on the uncorrelated-ensemble approach predicted that any created field would be expelled from the disk before it could be amplified significantly. By means of direct si...

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: International Astronomical Union Colloquium

سال: 1965

ISSN: 0252-9211

DOI: 10.1017/s0252921100118366