3,100 research outputs found
Nonlinear Terms of MHD Equations for Homogeneous Magnetized Shear Flow
We have derived the full set of MHD equations for incompressible shear flow
of a magnetized fluid and considered their solution in the wave-vector space.
The linearized equations give the famous amplification of slow magnetosonic
waves and describe the magnetorotational instability. The nonlinear terms in
our analysis are responsible for the creation of turbulence and self-sustained
spectral density of the MHD (Alfven and pseudo-Alfven) waves. Perspectives for
numerical simulations of weak turbulence and calculation of the effective
viscosity of accretion disks are shortly discussed in k-space.Comment: 13 pages, no figures; AIP Conference Proceedings 1356, Proceedings of
the School and Workshop on Space Plasma Physics (1--12 September 2010, Kiten,
Bulgaria), American Institute of Physics, Melville, NY, 201
Spatial and Temporal Stability of Airglow Measured in the Meinel Band Window at 1191.3 nm
We report on the temporal and spatial fluctuations in the atmospheric
brightness in the narrow band between Meinel emission lines at 1191.3 nm using
an R=320 near-infrared instrument. We present the instrument design and
implementation, followed by a detailed analysis of data taken over the course
of a night from Table Mountain Observatory. The absolute sky brightness at this
wavelength is found to be 5330 +/- 30 nW m^-2 sr^-1, consistent with previous
measurements of the inter-band airglow at these wavelengths. This amplitude is
larger than simple models of the continuum component of the airglow emission at
these wavelengths, confirming that an extra emissive or scattering component is
required to explain the observations. We perform a detailed investigation of
the noise properties of the data and find no evidence for a noise component
associated with temporal instability in the inter-line continuum. This result
demonstrates that in several hours of ~100s integrations the noise performance
of the instrument does not appear to significantly degrade from expectations,
giving a proof of concept that near-IR line intensity mapping may be feasible
from ground-based sites.Comment: 15 figures, submitted to PAS
Frequency of C > T polymorphism in fourth chromosome and levels of crp in patients with atrial
Introduction. Atrial fibrillation is a heart rhythm disorder, characterized by rapid and uncoordinated atrial activation which is the most common arrhythmia in clinical practice. Atrial fibrillation is observed in 1.5 - 2% of the general population and its incidence increases with age reaching more than 8-15% by 80 years of age. Atrial fibrillation is traditionally considered as a non genetic disorder. The cause of atrial fibrillation in 10-20% of cases is unknown and it is diagnosed as idiopathic
The Cosmic Infrared Background Experiment (CIBER): Instrumentation and First Results
Ultraviolet emission from the first generation of stars in the Universe ionized the intergalactic medium in a process which was completed by z similar to 6; the wavelength of these photons has been redshifted by (1 + z) into the near infrared today and can be measured using instruments situated above the Earth's atmosphere. First flying in February 2009, the Cosmic Infrared Background ExpeRiment (CIBER) comprises four instruments housed in a single reusable sounding rocket borne payload. CIBER will measure spatial anisotropies in the extragalactic IR background caused by cosmological structure from the epoch of reionization using two broadband imaging instruments, make a detailed characterization of the spectral shape of the IR background using a low resolution spectrometer, and measure the absolute brightness of the Zodiacal light foreground with a high resolution spectrometer in each of our six science fields. The scientific motivation for CIBER and details of its first and second flight instrumentation will be discussed. First flight results on the color of the zodiacal light around 1 mu m and plans for the future will also be presented
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