7,358 research outputs found
Synthesis of calculational methods for the design and analysis of radiation shields for nuclear rocket systems. Volume 2 - Analysis of radiation measurements in a nuclear rocket propellant tank mockup using simulated liquid hydrogen
Calculational methods for nuclear rocket radiation shield design - analysis of radiation measurements in nuclear rocket propellant tank mockup using simulated liquid hydroge
Data report for the Siple Coast (Antarctica) project
This report presents data collected during three field seasons of glaciological studies in the Antarctica and describes the methods employed. The region investigated covers the mouths of Ice Streams B and C (the Siple Coast) and Crary Ice Rise on the Ross Ice Shelf. Measurements included in the report are as follows: surface velocity and deformation from repeated satellite geoceiver positions; surface topography from optical levelling; radar sounding of ice thickness; accumulation rates; near-surface densities and temperature profiles; and mapping from aerial photography
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A pilot study for the collaborative development of new ways of visualising seasonal climate forecasts
Radio Images of 3C 58: Expansion and Motion of its Wisp
New 1.4 GHz VLA observations of the pulsar-powered supernova remnant 3C 58
have resulted in the highest-quality radio images of this object to date. The
images show filamentary structure over the body of the nebula. The present
observations were combined with earlier ones from 1984 and 1991 to investigate
the variability of the radio emission on a variety of time-scales. No
significant changes are seen over a 110 day interval. In particular, the upper
limit on the apparent projected velocity of the wisp is 0.05c. The expansion
rate of the radio nebula was determined between 1984 and 2004, and is
0.014+/-0.003%/year, corresponding to a velocity of 630+/-70 km/s along the
major axis. If 3C 58 is the remnant of SN 1181, it must have been strongly
decelerated, which is unlikely given the absence of emission from the supernova
shell. Alternatively, the low expansion speed and a number of other arguments
suggest that 3C 58 may be several thousand years old and not be the remnant of
SN 1181.Comment: 12 pages; accepted for publication in the Astrophysical Journa
A Shell of Thermal X-ray Emission Associated with the Young Crab-like Remnant 3C58
Deep X-ray imaging spectroscopy of the bright pulsar wind nebula 3C58
confirms the existence of an embedded thermal X-ray shell surrounding the
pulsar PSR J0205+6449. Radially resolved spectra obtained with the XMM-Newton
telescope are well-characterized by a power-law model with the addition of a
soft thermal emission component in varying proportions. These fits reproduce
the well-studied increase in the spectral index with radius attributed to
synchrotron burn-off of high energy electrons. Most interestingly, a radially
resolved thermal component is shown to map out a shell-like structure ~6' in
diameter. The presence of a strong emission line corresponding to the Ne IX
He-like transition requires an overabundance of ~3 x [Ne/Ne(sun)] in the
Raymond-Smith plasma model. The best-fit temperature kT ~ 0.23 keV is
essentially independent of radius for the derived column density of N_H = (4.2
+/- 0.1)E21 per cm squared. Our result suggests that thermal shells can be
obscured in the early evolution of a supernova remnant by non-thermal pulsar
wind nebulae emission; the luminosity of the 3C58 shell is more than an order
of magnitude below the upper limit on a similar shell in the Crab Nebula. We
find the shell centroid to be offset from the pulsar location. If this neutron
star has a velocity similar to that of the Crab pulsar, we derive an age of
3700 yr and a velocity vector aligned with the long axis of the PWN. The shell
parameters and pulsar offset add to the accumulating evidence that 3C58 is not
the remnant of the supernova of CE 1181.Comment: 7 pages, 8 figures, 2 tables, Latex emulateapj style. To appear in
the Astrophysical Journa
Track Surface Optimisation - A Data Driven Approach
A summary brief on current track curation ideology and procedures as well as the proposal of a new LIDAR-based data driven approach. Prepared for and presented to Greyhound Racing Victoria
Simultaneous auroral observations described in the historical records of China, Japan and Korea from ancient times to AD 1700
International audienceEarly auroral observations recorded in various oriental histories are examined in order to search for examples of strictly simultaneous and indisputably independent observations of the aurora borealis from spatially separated sites in East Asia. In the period up to ad 1700, only five examples have been found of two or more oriental auroral observations from separate sites on the same night. These occurred during the nights of ad 1101 January 31, ad 1138 October 6, ad 1363 July 30, ad 1582 March 8 and ad 1653 March 2. The independent historical evidence describing observations of mid-latitude auroral displays at more than one site in East Asia on the same night provides virtually incontrovertible proof that auroral displays actually occurred on these five special occasions. This conclusion is corroborated by the good level of agreement between the detailed auroral descriptions recorded in the different oriental histories, which furnish essentially compatible information on both the colour (or colours) of each auroral display and its approximate position in the sky. In addition, the occurrence of auroral displays in Europe within two days of auroral displays in East Asia, on two (possibly three) out of these five special occasions, suggests that a substantial number of the mid-latitude auroral displays recorded in the oriental histories are associated with intense geomagnetic storms
Isometric Finger Pose Recognition with Sparse Channel SpatioTemporal EMG Imaging
© 2018 IEEE. High fidelity myoelectric control of prostheses and orthoses isparamount to restoring lost function to amputees and neuro-muscular disease sufferers. In this study we prove that patio-temporal imaging can be used to allow convolutional neural networks to classify sparse channel EMG samples from a consumer-grade device with over 94% accuracy. 10,572 images are generated from 960 samples of simple and complex isometric finger poses recorded from 4 fully intact subjects. Real-time classification of 12 poses is achieved with a 250ms continuous overlapping window
Tests of a Triangular Wing of Aspect Ratio 2 in the Ames 12-foot Pressure Wind Tunnel II : the Effectiveness and Hinge Moments of a Constant-chord Plain Flap
Sporadic aurorae observed in East Asia
All the accessible auroral observations recorded in Chinese and Japanese histories during the interval AD 1840&ndash;1911 are investigated in detail. Most of these auroral records have never been translated into a Western language before. The East Asian auroral reports provide information on the date and approximate location of each auroral observation, together with limited scientific information on the characteristics of the auroral luminosity such as colour, duration, extent, position in the sky and approximate time of occurrence. The full translations of the original Chinese and Japanese auroral records are presented in an appendix, which contains bibliographic details of the various historical sources. (There are no known reliable Korean observations during this interval.) A second appendix discusses a few implausible "auroral" records, which have been rejected. The salient scientific properties of all exactly dated and reliable East Asian auroral observations in the interval AD 1840&ndash;1911 are summarised succinctly. By comparing the relevant scientific information on exactly dated auroral observations with the lists of great geomagnetic storms compiled by the Royal Greenwich Observatory, and also the tabulated values of the <I>Ak</I> (Helsinki) and <I>aa</I> (Greenwich and Melbourne) magnetic indices, it is found that 5 of the great geomagnetic storms (<I>aa</I>&gt;150 or <I>Ak</I>&gt;50) during either the second half of the nineteenth century or the first decade of the twentieth century are clearly identified by extensive auroral displays observed in China or Japan. Indeed, two of these great storms produced auroral displays observed in both countries on the same night. Conversely, at least 29 (69%) of the 42 Chinese and Japanese auroral observations occurred at times of weak-to-moderate geomagnetic activity (<I>aa</I> or <I>Ak</I>&le;50). It is shown that these latter auroral displays are very similar to the more numerous (about 50) examples of sporadic aurorae observed in the United States during the interval AD 1880&ndash;1940. The localised nature and spatial structure of some sporadic aurorae observed in East Asia is indicated by the use of descriptive terms such as "lightning", "rainbow", "streak" and "grid"
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