Estimation of Interstitial Velocity Using a Direct Drive High‐Resolution Passive Profiler

Ground Water ◽  
2019 ◽  
Vol 57 (6) ◽  
pp. 915-924
Author(s):  
Haley A. Schneider ◽  
W. Andrew Jackson ◽  
Ken Rainwater ◽  
Danny Reible ◽  
Stephen Morse ◽  
...  
1990 ◽  
Vol 2 (6) ◽  
pp. 463-470 ◽  
Author(s):  
Tetsuo Kotoku ◽  
◽  
Erhard J. Hüsler ◽  
Kazuo Tanie ◽  
Akio Fujikawa

This paper deals with the development of a 4 degree of freedom direct drive master manipulator system which has the ability of virtually adjusting its mechanical impedance. In the field of bilateral master-slave manipulation, there are some important points to be considered when a master manipulator is designed. One point is related to how to measure the human operator’s arm motion with high accuracy (which the operator produces to teach the trajectory of tasks). Another point is how to design an effective force/torque generator to make an operator feel the constraint forces the slave arm will receive from the environments during tasks. To satisfy these requirements, a manipulator with a variable mechanical impedance structure and joints equipped with high resolution angular displacement sensors is expected to be developed. The use of the variable impedance structure provides a capability of reflecting the constraint forces to an operator not only statically, but also dynamically. This is effective to present the constraints to an operator with high fidelity. In the research, joint mechanisms and joint sensors suitable for the impedance control were discussed, while the mechanical structure of the master manipulator which is effective to construct a simple impedance control law was investigated. With these considerations in mind, a master manipulator was designed and its impedance control law was formulated. The features of the manufactured manipulator are summarized as follows; (1) each joint is driven by a direct drive torque motor with less friction and has a high resolution angular encoder attached to a processor which can provide joint angular displacement, angular velocity and angular acceleration. (2) the manipulator has the decoupled and configuration-invariant inertia structure in part which is effective to simplify impedance control law. In the paper, the design concept of the master manipulator is first discussed. Secondly, the details of the manufactured manipulator structure are explained. Finally, the results of the evaluation experiments are described and the fundamental characteristics of the system are confirmed.


2004 ◽  
Vol 11 (5) ◽  
pp. 2716-2722 ◽  
Author(s):  
Andrew J. Schmitt ◽  
D. G. Colombant ◽  
A. L. Velikovich ◽  
S. T. Zalesak ◽  
J. H. Gardner ◽  
...  

1967 ◽  
Vol 31 ◽  
pp. 45-46
Author(s):  
Carl Heiles

High-resolution 21-cm line observations in a region aroundlII= 120°,b11= +15°, have revealed four types of structure in the interstellar hydrogen: a smooth background, large sheets of density 2 atoms cm-3, clouds occurring mostly in groups, and ‘Cloudlets’ of a few solar masses and a few parsecs in size; the velocity dispersion in the Cloudlets is only 1 km/sec. Strong temperature variations in the gas are in evidence.


2019 ◽  
Vol 42 ◽  
Author(s):  
J. Alfredo Blakeley-Ruiz ◽  
Carlee S. McClintock ◽  
Ralph Lydic ◽  
Helen A. Baghdoyan ◽  
James J. Choo ◽  
...  

Abstract The Hooks et al. review of microbiota-gut-brain (MGB) literature provides a constructive criticism of the general approaches encompassing MGB research. This commentary extends their review by: (a) highlighting capabilities of advanced systems-biology “-omics” techniques for microbiome research and (b) recommending that combining these high-resolution techniques with intervention-based experimental design may be the path forward for future MGB research.


1994 ◽  
Vol 144 ◽  
pp. 593-596
Author(s):  
O. Bouchard ◽  
S. Koutchmy ◽  
L. November ◽  
J.-C. Vial ◽  
J. B. Zirker

AbstractWe present the results of the analysis of a movie taken over a small field of view in the intermediate corona at a spatial resolution of 0.5“, a temporal resolution of 1 s and a spectral passband of 7 nm. These CCD observations were made at the prime focus of the 3.6 m aperture CFHT telescope during the 1991 total solar eclipse.


1994 ◽  
Vol 144 ◽  
pp. 541-547
Author(s):  
J. Sýkora ◽  
J. Rybák ◽  
P. Ambrož

AbstractHigh resolution images, obtained during July 11, 1991 total solar eclipse, allowed us to estimate the degree of solar corona polarization in the light of FeXIV 530.3 nm emission line and in the white light, as well. Very preliminary analysis reveals remarkable differences in the degree of polarization for both sets of data, particularly as for level of polarization and its distribution around the Sun’s limb.


1988 ◽  
Vol 102 ◽  
pp. 41
Author(s):  
E. Silver ◽  
C. Hailey ◽  
S. Labov ◽  
N. Madden ◽  
D. Landis ◽  
...  

The merits of microcalorimetry below 1°K for high resolution spectroscopy has become widely recognized on theoretical grounds. By combining the high efficiency, broadband spectral sensitivity of traditional photoelectric detectors with the high resolution capabilities characteristic of dispersive spectrometers, the microcalorimeter could potentially revolutionize spectroscopic measurements of astrophysical and laboratory plasmas. In actuality, however, the performance of prototype instruments has fallen short of theoretical predictions and practical detectors are still unavailable for use as laboratory and space-based instruments. These issues are currently being addressed by the new collaborative initiative between LLNL, LBL, U.C.I., U.C.B., and U.C.D.. Microcalorimeters of various types are being developed and tested at temperatures of 1.4, 0.3, and 0.1°K. These include monolithic devices made from NTD Germanium and composite configurations using sapphire substrates with temperature sensors fabricated from NTD Germanium, evaporative films of Germanium-Gold alloy, or material with superconducting transition edges. A new approache to low noise pulse counting electronics has been developed that allows the ultimate speed of the device to be determined solely by the detector thermal response and geometry. Our laboratory studies of the thermal and resistive properties of these and other candidate materials should enable us to characterize the pulse shape and subsequently predict the ultimate performance. We are building a compact adiabatic demagnetization refrigerator for conveniently reaching 0.1°K in the laboratory and for use in future satellite-borne missions. A description of this instrument together with results from our most recent experiments will be presented.


Author(s):  
Robert M. Glaeser

It is well known that a large flux of electrons must pass through a specimen in order to obtain a high resolution image while a smaller particle flux is satisfactory for a low resolution image. The minimum particle flux that is required depends upon the contrast in the image and the signal-to-noise (S/N) ratio at which the data are considered acceptable. For a given S/N associated with statistical fluxtuations, the relationship between contrast and “counting statistics” is s131_eqn1, where C = contrast; r2 is the area of a picture element corresponding to the resolution, r; N is the number of electrons incident per unit area of the specimen; f is the fraction of electrons that contribute to formation of the image, relative to the total number of electrons incident upon the object.


Author(s):  
Glen B. Haydon

Analysis of light optical diffraction patterns produced by electron micrographs can easily lead to much nonsense. Such diffraction patterns are referred to as optical transforms and are compared with transforms produced by a variety of mathematical manipulations. In the use of light optical diffraction patterns to study periodicities in macromolecular ultrastructures, a number of potential pitfalls have been rediscovered. The limitations apply to the formation of the electron micrograph as well as its analysis.(1) The high resolution electron micrograph is itself a complex diffraction pattern resulting from the specimen, its stain, and its supporting substrate. Cowley and Moodie (Proc. Phys. Soc. B, LXX 497, 1957) demonstrated changing image patterns with changes in focus. Similar defocus images have been subjected to further light optical diffraction analysis.


Author(s):  
A. V. Crewe

The high resolution STEM is now a fact of life. I think that we have, in the last few years, demonstrated that this instrument is capable of the same resolving power as a CEM but is sufficiently different in its imaging characteristics to offer some real advantages.It seems possible to prove in a quite general way that only a field emission source can give adequate intensity for the highest resolution^ and at the moment this means operating at ultra high vacuum levels. Our experience, however, is that neither the source nor the vacuum are difficult to manage and indeed are simpler than many other systems and substantially trouble-free.


Sign in / Sign up

Export Citation Format

Share Document