59 research outputs found
Eighth Annual Agricultural Marketing Conference Theme "Exporting Ohio's Agricultural Production to a Hungry World"
The proton and electron radiation belts at geosynchronous orbit: Statistics and behavior during highâspeed streamâdriven storms
The outer proton radiation belt (OPRB) and outer electron radiation belt (OERB) at geosynchronous orbit are investigated using a reanalysis of the LANL CPA (Charged Particle Analyzer) 8âsatellite 2âsolar cycle energetic particle data set from 1976 to 1995. Statistics of the OPRB and the OERB are calculated, including local time and solar cycle trends. The number density of the OPRB is about 10 times higher than the OERB, but the 1âMeV proton flux is about 1000 times less than the 1âMeV electron flux because the proton energy spectrum is softer than the electron spectrum. Using a collection of 94 highâspeed streamâdriven storms in 1976â1995, the storm time evolutions of the OPRB and OERB are studied via superposed epoch analysis. The evolution of the OERB shows the familiar sequence (1) prestorm decay of density and flux, (2) earlyâstorm dropout of density and flux, (3) sudden recovery of density, and (4) steady storm time heating to high fluxes. The evolution of the OPRB shows a sudden enhancement of density and flux early in the storm. The absence of a proton dropout when there is an electron dropout is noted. The sudden recovery of the density of the OERB and the sudden density enhancement of the OPRB are both associated with the occurrence of a substorm during the early stage of the storm when the superdense plasma sheet produces a âstrong stretching phaseâ of the storm. These storm time substorms are seen to inject electrons to 1âMeV and protons to beyond 1âMeV into geosynchronous orbit, directly producing a suddenly enhanced radiation belt population.Key PointsDuring highâspeed streamâdriven storms, the electron and proton radiation belts are directly enhanced by a single substormThe enhancing substorm occurs during the âstrong stretchingâ phase of the storm caused by the superdense plasma sheetProton and electron injection to 1 MeV is seen for these strong stretching phase substormsPeer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/133567/1/jgra52702.pdfhttp://deepblue.lib.umich.edu/bitstream/2027.42/133567/2/jgra52702_am.pd
LSST: from Science Drivers to Reference Design and Anticipated Data Products
(Abridged) We describe here the most ambitious survey currently planned in
the optical, the Large Synoptic Survey Telescope (LSST). A vast array of
science will be enabled by a single wide-deep-fast sky survey, and LSST will
have unique survey capability in the faint time domain. The LSST design is
driven by four main science themes: probing dark energy and dark matter, taking
an inventory of the Solar System, exploring the transient optical sky, and
mapping the Milky Way. LSST will be a wide-field ground-based system sited at
Cerro Pach\'{o}n in northern Chile. The telescope will have an 8.4 m (6.5 m
effective) primary mirror, a 9.6 deg field of view, and a 3.2 Gigapixel
camera. The standard observing sequence will consist of pairs of 15-second
exposures in a given field, with two such visits in each pointing in a given
night. With these repeats, the LSST system is capable of imaging about 10,000
square degrees of sky in a single filter in three nights. The typical 5
point-source depth in a single visit in will be (AB). The
project is in the construction phase and will begin regular survey operations
by 2022. The survey area will be contained within 30,000 deg with
, and will be imaged multiple times in six bands, ,
covering the wavelength range 320--1050 nm. About 90\% of the observing time
will be devoted to a deep-wide-fast survey mode which will uniformly observe a
18,000 deg region about 800 times (summed over all six bands) during the
anticipated 10 years of operations, and yield a coadded map to . The
remaining 10\% of the observing time will be allocated to projects such as a
Very Deep and Fast time domain survey. The goal is to make LSST data products,
including a relational database of about 32 trillion observations of 40 billion
objects, available to the public and scientists around the world.Comment: 57 pages, 32 color figures, version with high-resolution figures
available from https://www.lsst.org/overvie
From Sacred to Scientific: Epic Religion, Spectacular Science, and Charlton Hestonâs Science Fiction Cinema
This paper analyses how long-1960s cinema responded to and framed public discourses surrounding religion and science. This approach allows for a discussion that extends beyond a critical study of the scholarly debates that surround the place of religion in science during a transitional period. Charlton Heston was an epic actor who went from literally playing God in The Ten Commandments (1956) to playing âgodâ as a messianic scientist in The Omega Man (1971). Best known for playing Moses, Heston became an unlikely science-based cinema star during the early 1970s. He was re-imagined as a scientist, but the religiosity of his established persona was inescapable. Heston and the science-based films he starred in capitalized upon the utopian promises of real science, and also the fears of the vocal activist counterculture. Planet of the Apes (1968), Omega Man (1971), Soylent Green (1973), and other science-based films made between 1968-1977 were bleak countercultural warnings about excessive consumerism, uncontrolled science, nuclear armament, irreversible environmental damage, and eventual human extinction. In this paper I argue that Hestonâs transition from biblical epic star to science-fiction anti-hero represents the way in which the role and interpretation of science changed in post-classical cinema. Despite the shift from religious epic to science-based spectacle, religion remained a faithful component of Hollywood output indicating the ongoing connection between science and religion in US culture. I will consider the transition from sacred to science-based narratives and how religion was utilised across the production process of films that commented upon scientific advances
High-Affinity Interactions of Tumor Necrosis Factor Receptor-Associated Factors (TRAFs) and CD40 Require TRAF Trimerization and CD40 Multimerization
14,15-Dihydroxyeicosatrienoic acid relaxes bovine coronary arteries by activation of K Ca
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