29
29
Oct 9, 2017
10/17
by
Directorate of Printing, Government of India
texts
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The Gazette of India Extraordinary Gazette Published by the Directorate of Printing, Department of Publication, Ministry of Housing and Urban Affairs, Government of India Published in 1996, Issue Number 417 Ministry: Ministry not available Subject: Subject not available
Topic: Extraordinary Gazette of India
29 de Janeiro de 1996
Topics: Janeiro 29, 1996
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33
Aug 28, 2009
08/09
by
NASA/Glenn Research Center
image
eye 33
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FSDC NEEDLES FIBER SUPPORTED DROPLET COMBUSTION
24
24
Aug 28, 2009
08/09
by
NASA/Glenn Research Center
image
eye 24
favorite 0
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FSDC NEEDLES FIBER SUPPORTED DROPLET COMBUSTION
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44
Oct 15, 2009
10/09
by
NASA
image
eye 44
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A newly discovered tenth ring of Uranus is barely visible near the top of this two-frame Voyager 2 mosaic. The frames composing this picture were obtained Jan. 23, 1986, from a distance of 1.12 million kilometers (690,000 miles). The tenth ring is about midway between the bright, outermost epsilon ring and the next ring down, called delta. The tenth ring, the first such feature discovered by Voyager, orbits Uranus at a radius of about 50,000 km (30,000 mi). This places the ring close to the...
Topics: What -- Uranus, What -- Voyager 2, What -- Voyager, Where -- Jet Propulsion Laboratory (JPL)
Source: http://photojournal.jpl.nasa.gov/catalog/PIA00035
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54
Oct 15, 2009
10/09
by
NASA
image
eye 54
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This Magellan radar image is of a 'half crater' located in the rift between Rhea and Theia Montes in Beta Regio on Venus. The unnamed crater is 37 kilometers (23 miles) in diameter and is located at 29.9 degrees north latitude and 282.9 degrees east longitude. It has been cut by many fractures or faults since it was formed by the impact of a large asteroid. The eastern half of the crater was destroyed during the formation of a fault valley that is up to 20 kilometers (12 miles) wide and...
Topics: What -- Magellan, What -- Crater, What -- Rhea, What -- Venus
Source: http://photojournal.jpl.nasa.gov/catalog/PIA00100
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37
Oct 15, 2009
10/09
by
NASA
image
eye 37
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This Magellan image centered near 9.6 degrees north latitude, 189.5 degrees east longitude of an area 140 kilometers (87 miles) by 110 kilometers (68 miles) covers part of the eastern flank of the volcano Sapas Mons on the western edge of Atla Regio. The bright lobate features along the southern and the western part of the image, oriented in northeast to southwest directions, are lava flows that are rough at the 12.6 centimeter wavelength of the radar. These flows range in width from 5...
Topics: What -- Magellan, What -- Crater, What -- Venus
Source: http://photojournal.jpl.nasa.gov/catalog/PIA00099
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44
Oct 15, 2009
10/09
by
NASA
image
eye 44
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The Magellan synthetic aperture radar (SAR) imaged this unique 'triplet crater,' or 'crater field' during orbits 418-421 on 21 September 1990. These craters are 14 kilometers, 11 kilometers, and 9 kilometers in diameter, respectively, and are centered at latitude -30.1 degrees south and longitude 345.5 degrees east. The Magellan Science Team has proposed the name Stein for this crater field after the American author, Gertrude Stein. This name has not yet been approved by the International...
Topics: What -- Magellan, What -- Crater, What -- Venus
Source: http://photojournal.jpl.nasa.gov/catalog/PIA00088
133
133
Oct 15, 2009
10/09
by
NASA
image
eye 133
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This image of Neptune was taken by Voyager 2's wide-angle camera when the spacecraft was 590,000 km (370,000 miles) from the planet. The image has been processed to obtain true color balance. Additional processing was used to suppress surface brightness of the white clouds. The processing allows both the clouds' structure in the dark regions near the pole and the bright clouds east of the Great Dark Spot to be reproduced in this color photograph. Small trails of similar clouds trending east to...
Topics: What -- Neptune, What -- Voyager 2, What -- Voyager, Where -- Jet Propulsion Laboratory (JPL)
Source: http://photojournal.jpl.nasa.gov/catalog/PIA00063
118
118
Oct 15, 2009
10/09
by
NASA
image
eye 118
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This false-color mosaic of part of the Moon was constructed from 54 images taken by Galileo's imaging system as the spacecraft flew past the Moon on December 7, 1992. The mosaic images were processed to exaggerate the colors of the lunar surface for analytical purposes. Titanium-rich soils, typical of the Apollo 11 landing site, appear blue, as seen in Mare Tranquillitatis, left side; soils lower in titanium appear orange, as seen in Mare Serenitatis, center right. Most of the lunar highlands...
Topics: What -- Moon, What -- Apollo 11, What -- Galileo, What -- Jupiter, Where -- Jet Propulsion...
Source: http://photojournal.jpl.nasa.gov/catalog/PIA00129
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73
Oct 15, 2009
10/09
by
NASA
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eye 73
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These are enhanced versions of four views of the planet Venus taken by the Galileo's Solid State Imaging System at distances ranging from 1.4 to 2 million miles as the spacecraft receded from Venus. The pictures in the top row were taken about 4 and 5 days after closest approach, and those in the bottom row six days after closest approach, 2 hours apart. These show the faint Venusian cloud features especially clearly. A high-pass filter was applied to bring out broader global variations in...
Topics: What -- Venus, What -- Polar, What -- Galileo, What -- Jupiter, What -- Earth, Where -- Jet...
Source: http://photojournal.jpl.nasa.gov/catalog/PIA00110
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123
Oct 15, 2009
10/09
by
NASA
image
eye 123
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On December 16, 1992, 8 days after its encounter with Earth, the Galileo spacecraft looked back from a distance of about 6.2 million kilometers (3.9 million miles) to capture this remarkable view of the Moon in orbit about Earth. The composite photograph was constructed from images taken through visible (violet, red) and near-infrared (1.0-micron) filters. The Moon is in the foreground; its orbital path is from left to right. Brightly colored Earth contrasts strongly with the Moon, which reacts...
Topics: What -- Earth, What -- Galileo, What -- Moon, What -- Dawn
Source: http://photojournal.jpl.nasa.gov/catalog/PIA00134
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76
Oct 15, 2009
10/09
by
NASA
image
eye 76
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This Voyager 2 image of Miranda was taken Jan 24, 1986, from a distance of about 31,000 kilometers (19,000 miles), shortly before the spacecraft's closest approach to the Uranian moon. The high resolution of 600 meters (2,000 feet) reveals a bewildering variety of fractures, grooves and craters, as well as features of different albedos (reflectancea). This clear-filter, narrow-angle view encompasses areas of older, heavily cratered terrain with a wide variety of forms. The grooves and troughs...
Topics: What -- Voyager 2, What -- Miranda, What -- Moon, What -- Voyager, Where -- Jet Propulsion...
Source: http://photojournal.jpl.nasa.gov/catalog/PIA00140
36
36
Sep 18, 2013
09/13
by
E. Alfinito; M. Blasone; A. Iorio; G. Vitiello
texts
eye 36
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We show that the generator of field mixing transformations in Quantum Field Theory induces a non trivial structure in the vacuum which turns out to be a coherent state, both for bosons and for fermions, although with a different condensate structure. The Fock space for mixed fields is unitarily inequivalent to the Fock space of the massive (free) fields in the infinite volume limit. As a practical application we study neutrino mixing and oscillations. A new oscillation formula is found where...
Source: http://arxiv.org/abs/hep-ph/9601354v1
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34
texts
eye 34
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47
Sep 18, 2013
09/13
by
V. A. Kazakov; M. Staudacher; T. Wynter
texts
eye 47
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We review the recent exact solution of a matrix model which interpolates between flat and random lattices. The importance of the results is twofold: Firstly, we have developed a new large N technique capable of treating a class of matrix models previously thought to be unsolvable. Secondly, we are able to make a first precise statement about two-dimensional R^2 gravity. These notes are based on a lecture given at the Cargese summer school 1995. They contain some previously unpublished results.
Source: http://arxiv.org/abs/hep-th/9601153v1
Federal Register 1996-01-29: Volume 61 , Issue 19. Digitized from IA1532617-05 . Previous issue: sim_federal-register-find_1996-01-26_61_18 . Next issue: sim_federal-register-find_1996-01-30_61_20 .
Topics: Public Administration, Government Documents, microfilm
Source: IA1532617-05
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33
texts
eye 33
favorite 0
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FBIS Reports: Reference Aid
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20
Mar 12, 2022
03/22
by
United States Foreign Broadcast Information Service
texts
eye 20
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FBIS-WEU-96-019 Digitized from IA1176811-14-0057 .
Source: IA1176811-14
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154
Oct 15, 2009
10/09
by
NASA
image
eye 154
favorite 4
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This color image of the Earth was obtained by the Galileo spacecraft early Dec. 12, 1990, when the spacecraft was about 1.6 million miles from the Earth. The color composite used images taken through the red, green and violet filters. The Pacific Ocean covers virtually all of the visible disk of the Earth in this picture. The glint of the Sun reflected from smooth water is near the center. This is a frame of the Galileo Earth spin movie, a 500-frame time-lapse motion picture showing a 25-hour...
Topics: What -- Earth, What -- Galileo, What -- Sun, Where -- Pacific Ocean
Source: http://photojournal.jpl.nasa.gov/catalog/PIA00123
59
59
Jan 6, 2019
01/19
by
Bernd Friedmann
audio
eye 59
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https://www.discogs.com/Bernd-Friedmann-Leisure-Zones-Erholungsgebiete/release/70590
Topics: ambient, electronic, experimental, grippers.tips
Preliminary studies on a simplified kinetic model for the hydrogen flame confirm the existence of the shock-like structure in flame temperature space for the logarithm of the mass burning rate that had been discovered previously in the study of the carbon monoxide flame; notably; the mass buring rate undergoes a multiplicative jump in contrast to the additive jump in regular shock waves. jg p1
Topics: DTIC Archive, Tam, Richard, INDIANA UNIV-PURDUE UNIV AT INDIANAPOLIS DEPT OF MATHEMATICAL SCIENCES,...
16
16
Aug 2, 2018
08/18
by
Government of India
texts
eye 16
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The Gazette of India Date: 1996-1-29 Type: Extraordinary Part Number: CSL Reference Number: CSL Department: CSL Ministry: CSL Office: CSL Subject: Subject not available
Topics: Gazette of India, Extraordinary Gazette of India
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58
Sep 18, 2013
09/13
by
A. Denner; S. Dittmaier; R. Schuster
texts
eye 58
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We discuss the complete virtual and soft-photonic O(alpha) corrections to AA -> W+W- within the electroweak Standard Model for arbitrary polarized photons. In the on-shell renormalization scheme for fixed M_W no leading corrections associated with the running of alpha or heavy top-quark and Higgs-boson masses occur. The corrections turn out to be of the order of 10%, but can become much larger where the lowest-order cross-sections are suppressed.
Source: http://arxiv.org/abs/hep-ph/9601355v1
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59
Sep 18, 2013
09/13
by
M. J. Mehl; L. L. Boyer; H. T. Stokes
texts
eye 59
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This is a brief description of how to derive the local ``atomic'' potentials from the Self-Consistent Atomic Deformation (SCAD) model density function. Particular attention is paid to the spherically averaged case.
Source: http://arxiv.org/abs/mtrl-th/9601003v1
Weekly Compilation of Presidential Documents 1996-01-29: Volume 32 , Issue 4. Digitized from IA1632418-07 . Previous issue: sim_weekly-compilation-of-presidential-documents_1996-01-22_32_3 . Next issue: sim_weekly-compilation-of-presidential-documents_1996-02-05_32_5 .
Topics: Government Documents, microfilm
Source: IA1632418-07
Topics: tagesschau, Evening News, Germany
10
10.0
Apr 17, 2020
04/20
by
Government of India
texts
eye 10
favorite 0
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Gazette Type: Extra Ordinary Date: 1996-01-29 Ministry: Ministry NOT available Subject: Subject NOT available Gazette Source: URL Gazette ID: E-0305-1996-0060-11223 Download: GV_Content_Detail$ctl11$lnkflname_Pdf_Img
Topic: Extraordinary Gazette of India
27
27
Aug 28, 2009
08/09
by
NASA/Glenn Research Center
image
eye 27
favorite 0
comment 0
ENABLING PROPULSION MATERIALS NONDESTRUCTIVE EVALUATION INSPECTION
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76
Oct 15, 2009
10/09
by
NASA
image
eye 76
favorite 0
comment 0
The hemisphere of Ganymede that faces away from the Sun displays a great variety of terrain. In this Voyager 2 mosaic, photographed at a range of 300,000 kilometers, the ancient dark area of Regio Galileo lies at the upper left. Below it, the ray system is probably caused by water-ice, splashed out in a relatively recent impact.
Topics: What -- Ganymede, What -- Sun, What -- Voyager 2, What -- Galileo
Source: http://photojournal.jpl.nasa.gov/catalog/PIA00081
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54
Oct 15, 2009
10/09
by
NASA
image
eye 54
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Saturn and two of its moons, Tethys (above) and Dione, were photographed by Voyager 1 on November 3, 1980, from 13 million kilometers (8 million miles). The shadows of Saturn's three bright rings and Tethys are cast onto the cloud tops. The limb of the planet can be seen easily through the 3,500-kilometer-wide (2,170 mile) Cassini Division, which separates ring A from ring B. The view through the much narrower Encke Division, near the outer edge of ring A is less clear. Beyond the Encke...
Topics: What -- Saturn, What -- Tethys, What -- Dione, What -- Voyager 1, What -- Cassini, What -- Voyager,...
Source: http://photojournal.jpl.nasa.gov/catalog/PIA00024
27
27
Aug 28, 2009
08/09
by
NASA/Glenn Research Center
image
eye 27
favorite 0
comment 0
FSDC NEEDLES FIBER SUPPORTED DROPLET COMBUSTION
90
90
Oct 14, 2009
10/09
by
NASA
image
eye 90
favorite 0
comment 0
This color picture of Antarctica is one part of a mosaic of pictures covering the entire polar continent taken during the hours following Galileo's historic first encounter with its home planet. The view shows the Ross Ice Shelf to the right and its border with the sea. An occasional mountain can be seen poking through the ice near the McMurdo Station. It is late spring in Antarctica, so the sun never sets on the frigid, icy continent. This picture was taken about 6:20 p.m. PST on December 8,...
Topics: What -- Polar, What -- Sun
Source: http://photojournal.jpl.nasa.gov/catalog/PIA00074
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39
Oct 15, 2009
10/09
by
NASA
image
eye 39
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This color picture is made from images taken by the imaging system on the Galileo spacecraft about 14 minutes before its closest approach to asteroid 243 Ida on August 28, 1993. The range from the spacecraft was about 10,500 kilometers (6,500 miles). The images used are from the sequence in which Ida's moon was originally discovered; the moon is visible to the right of the asteroid. This picture is made from images through the 4100-angstrom (violet), 7560 A (infrared) and 9680 A (infrared)...
Topics: What -- Galileo, What -- Moon, What -- Near Infrared Mapping Spectrometer (NIMS), What -- Crater,...
Source: http://photojournal.jpl.nasa.gov/catalog/PIA00069
59
59
Oct 15, 2009
10/09
by
NASA
image
eye 59
favorite 1
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These images show changes in the clouds around Neptune's Great Dark Spot (GDS) over a four and one-half-day period. From top to bottom the images show successive rotations of the planet an interval of about 18 hours. The GDS is at a mean latitude of 20 degrees south, and covers about 30 degrees of longitude. The violet filter of the Voyager narrow angle camera was used to produce these images at distances ranging from 17 million kilometers (10.5 million miles) at the top, to 10 million...
Topics: What -- Voyager, What -- Neptune, What -- Sun, What -- Jupiter
Source: http://photojournal.jpl.nasa.gov/catalog/PIA00045
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77
Oct 15, 2009
10/09
by
NASA
image
eye 77
favorite 0
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This image of Miranda, obtained by Voyager 2 on approach, shows an unusual 'chevron' figure and regions of distinctly differing terrain on the Uranian moon. Voyager was 42,000 kilometers (26,000 miles) away when its narrow-angle camera acquired this clear-filter view. Grooved areas baring light and dark bands, distinct from other areas of mottled terrain, are visible at this resolution of about 600 meters (2,000 feet). The bright V-shaped feature in the grooved areas is the 'chevron' observed...
Topics: What -- Miranda, What -- Voyager 2, What -- Moon, What -- Voyager, Where -- Jet Propulsion...
Source: http://photojournal.jpl.nasa.gov/catalog/PIA00038
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90
Oct 15, 2009
10/09
by
NASA
image
eye 90
favorite 1
comment 0
These pictures of the Moon were taken by the Galileo spacecraft at (right photo) 6:47 p.m. PST Dec.8, 1990 from a distance of almost 220,000 miles, and at (left photo) 9:35 a.m. PST Dec. 9, 1990 at a range of more than 350,000 miles. The picture on the right shows the dark Oceanus Procellarum in the upper center, with Mare Imbrium above it and the smaller circular Mare Humorum below. The Orientale Basin, with a small mare in its center, is on the lower left near the limb or edge. Between...
Topics: What -- Moon, What -- Galileo
Source: http://photojournal.jpl.nasa.gov/catalog/PIA00077
5,138
5.1K
Feb 16, 2018
02/18
by
3D Realms
software
eye 5,138
favorite 8
comment 0
Duke Nukem 3D Disk (Shareware Version)
Topics: 3D Realms, Duke Nukem, Duke Nukem 3D, shareware CD, shareware, demo
529
529
Oct 15, 2009
10/09
by
NASA
image
eye 529
favorite 2
comment 0
During August 16 and 17, 1989, the Voyager 2 narrow-angle camera was used to photograph Neptune almost continuously, recording approximately two and one-half rotations of the planet. These images represent the most complete set of full disk Neptune images that the spacecraft will acquire. This picture from the sequence shows two of the four cloud features which have been tracked by the Voyager cameras during the past two months. The large dark oval near the western limb (the left edge) is at a...
Topics: What -- Voyager 2, What -- Neptune, What -- Voyager, Where -- Jet Propulsion Laboratory (JPL)
Source: http://photojournal.jpl.nasa.gov/catalog/PIA00046
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59
Oct 15, 2009
10/09
by
NASA
image
eye 59
favorite 0
comment 0
This bulls-eye view of Neptune's small dark spot (D2) was obtained by Voyager 2's narrow-angle camera on Aug. 24, 1989, when Voyager 2 was within 1.1 million km (680,000 miles) of the planet. The smallest structures that can be seen are 20 km (12 miles) across. This unplanned photograph was obtained when the infrared spectrograph was mapping the planet, and is the highest resolution view of the feature taken during the flyby. Banding surrounding the feature indicates unseen strong winds, while...
Topics: What -- Voyager 2, What -- Infrared Spectrograph (IRS), What -- Jupiter, What -- Neptune, What --...
Source: http://photojournal.jpl.nasa.gov/catalog/PIA00064
The goal of this investigation was to demonstrate the existence of chaotic dynamic behavior in mechanical systems that contain rotating structures and/or fluid structure interactions. Progress was made in the study of the non-linear dynamics of rotating beams (simple models of helicopter rotor blades) and fluid flow induced experimental as well as analytical and numerical simulation. The research resulted in the award of one doctoral degree and offered support to visiting Professor M....
Topics: DTIC Archive, Moon, Francis C., CORNELL UNIV ITHACA NY, *MATHEMATICAL MODELS, *CHAOS,...
This booklet features an interview conducted with Hermine Kromnik (b. 1915) and also includes acknowledgments, her family photographs, genealogy, maps, and references (n=15). The interview in the booklet is a personal testimony of Hermine's survival and the results of living in Eastern Europe during World Wars I and II. Hermine's desire was to leave a written legacy for her family. Personal interviews took place between February and May 1995 in West Chester, Pennsylvania, where Hermine lives....
Topics: ERIC Archive, Foreign Countries, Genealogy, Interviews, Oral History, Personal Narratives,...
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35
Aug 4, 2018
08/18
by
Government of Haryana
texts
eye 35
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Haryana Gazette Gazette Type: Ordinary Date: 1996-1-29 Gazette Number: 6 Department: Development and Panchayats Notification Number: 134-1ECD-I-86-399 Subject: Shri Sukhbir Singh is retired from Government Service Source URL
Topic: Haryana Gazette
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50
Sep 18, 2013
09/13
by
Eugene Lerman
texts
eye 50
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In this paper I construct, using off the shelf components, a compact symplectic manifold with a non-trivial Hamiltonian circle action that admits no Kaehler structure. The non-triviality of the action is guaranteed by the existence of an isolated fixed point. The motivation for this work comes from the program of classification of Hamiltonian group actions. The Audin-Ahara-Hattori-Karshon classification of Hamiltonian circle actions on compact symplectic 4-manifolds showed that all of such...
Source: http://arxiv.org/abs/dg-ga/9601012v1
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42
Sep 18, 2013
09/13
by
Claudio Coriano'; Lionel E. Gordon
texts
eye 42
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We calculate $O(\alpha_s)$ corrections to inclusive and isolated double prompt photon production, both for the unpolarized case, and for longitudinal polarization of the incoming hadrons. The calculation is performed using purely analytical techniques for the inclusive case, and a combination of analytical and Monte Carlo techniques to perform the phase space integration in the isolated case. A brief phenomenological study is made of the process $pp\rightarrow \gamma \gamma X$ at CMS energies...
Source: http://arxiv.org/abs/hep-ph/9601350v2
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55
Sep 18, 2013
09/13
by
P. Chiappetta; J. Layssac; F. M. Renard; C. Verzegnassi
texts
eye 55
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In order to explain possible departures from the Standard Model predictions for $b\bar b$ and $c\bar c$ production at $Z$ peak, we propose the existence of a $Z'$ vector boson with enhanced couplings to quarks. We first show that this proposal is perfectly consistent with the full set of LEP1/SLC results. In particular, $Z-Z'$ mixing effects naturally explain the fact that $\Gamma_b$ and $\Gamma_c$ deviate from the SM in opposite directions. We then show that there is a predicted range for...
Source: http://arxiv.org/abs/hep-ph/9601306v2
This research program has dealt with two projects in the field of planetary atmosphere dynamics and radiative energy transfer, one theoretical and one experimental. The first project, in radiative energy transfer, incorporated the capability to isolate and quantify the contribution of individual atmospheric components to the Venus radiative balance and thermal structure to greatly improve the current understanding of the radiative processes occurring within the Venus atmosphere. This is...
Topics: NASA Technical Reports Server (NTRS), RADIATIVE TRANSFER, ALGORITHMS, APPLICATIONS PROGRAMS...
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94
Oct 13, 2009
10/09
by
NASA
image
eye 94
favorite 1
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This Voyager 2 picture of Oberon is the best the spacecraft acquired of Uranus' outermost moon. The picture was taken shortly after 3:30 a.m. PST on Jan. 24, 1986, from a distance of 660,000 kilometers (410,000 miles). The color was reconstructed from images taken through the narrow-angle camera's violet, clear and green filters. The picture shows features as small as 12 km (7 mi) on the moon's surface. Clearly visible are several large impact craters in Oberon's icy surface surrounded by...
Topics: What -- Voyager 2, What -- Oberon, What -- Uranus, What -- Moon, What -- Callisto, What -- Crater,...
Source: http://photojournal.jpl.nasa.gov/catalog/PIA00034
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52
Sep 18, 2013
09/13
by
T. Shirafuji; G. G. L. Nashed; K. Hayashi
texts
eye 52
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We find the most general, spherically symmetric solution in a special class of tetrad theory of gravitation. The tetrad gives the Schwarzschild metric. The energy is calculated by the superpotential method and by the Euclidean continuation method. We find that unless the time-space components of the tetrad go to zero faster than ${1/\sqrt{r}}$ at infinity, the two methods give results different from each other, and that these results differ from the gravitational mass of the central gravitating...
Source: http://arxiv.org/abs/gr-qc/9601044v1
328
328
Jan 16, 2020
01/20
by
3D Realms
software
eye 328
favorite 3
comment 0
Duke Nukem 3D (Mega Drive)
Topic: dukenukem3dmegadrive
