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1. HwB: Accelerated Graphics Port (AGP) Connector (Offline)
AGP=Accelerated Graphics Port . ... 132 PIN EDGE CONNECTOR at the computer. ... Reserved* Ground . ... Ground . ... VCC 3.3 . ... Vddq 3.3 . ... AGP pinout at The Pin-Out directory . ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/irlab/doc/library/hwbook/connector/bus/agp.html -- 9.3 Кб -- 06.07.2001
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2. Acceleration Engineering
. Корабль Lucky Seven в представлении художника . Иллюстрация с вебсайта Spacefleet .
[ Сохраненная копия ]  Ссылки http://www.astronaut.ru/suborb/xprise/foto/acceleration2.htm -- 1.7 Кб -- 15.04.2012
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3. Stealth 64 Video 3200
Diamond's Stealth64 Video 3200 is the perfect, cost-effective choice for excellent graphics and video performance on PCI systems. ... Accelerated video playback provides smooth viewing of popular multimedia applications and digital video clips at full screen resolution at up to 30 frames per second. The Diamond Stealth64 Video 3200 continues our award-winning tradition, delivering the best price/performance multimedia accelerator available. ... 64-bit Graphics Performance . ... Video Connector: . ...
[ Сохраненная копия ]  Ссылки http://crydee.sai.msu.ru/ftproot/pub/misc/doc/stealth64video3200.html -- 5.5 Кб -- 11.08.1995
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4. http://hea.iki.rssi.ru/conf/hea2007/presentations/26.12.2007/13-istomin.pdf
... ,E_=v_B_z,B_z0 Light cylinder at RL U = electric voltage created by rotating BH I = large scale current I U LK Centrifugal acceleration in BH magnetosphere Assume `reasonable' B and E fields, from current I : Bz = 0 = v/v 1 Motion of a test particle P ( ) Light cylinder Pz() P() z() Here = 0.01 and = rc,i/RL = 0.01 Growth of particle Lorentz factor ( ) log k At light cylinder : = Here with initial value is the absolute maximal reachable by this process (ie no ...
[ Текст ]  Ссылки http://hea.iki.rssi.ru/conf/hea2007/presentations/26.12.2007/13-istomin.pdf -- 762.2 Кб -- 30.01.2008
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5. http://jet.sao.ru/~bars/Acceleration/ci-accel.htm
... CI Cam (XTE J0421+560) is an X-ray transient and a binary system the optical companion, which shows the B[e] phenomenon. ... The centroid velocities of the following emission lines were measured: FeII (5 lines), [N II] 5754.59A (NIST Database), H_alpha, H_beta, HeI (5 lines), and [O III] 5006.843A. FeII and [N II] lines that form in the cool equatorial disk wind of B[e] star have stable sharp-edge profiles. ... All the FeII lines and the [N II] line in our spectra show a linear shift with time. ...
[ Сохраненная копия ]  Ссылки http://jet.sao.ru/~bars/Acceleration/ci-accel.htm -- 6.2 Кб -- 07.02.2008
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6. http://www.adass.org/adass/proceedings/adass02/reprints/D10.pdf
Astronomical Data Analysis Software and Systems XII ASP Conference Series, Vol. ... The testbed runs under Linux and provides a web interface to selected backend NEMO modeling and analysis tools, and several integration methods which can optionally use an MD-GRAPE2 supercomputer card in the server to accelerate calculation of particle-particle forces. ... Recommendations are made for testbed enhancements. ... NEMO programs provide commonly used data models and analysis functions. ...
[ Текст ]  Ссылки http://www.adass.org/adass/proceedings/adass02/reprints/D10.pdf -- 67.9 Кб -- 11.03.2003
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7. Astrodynamics 101
. Planetary Approach . "Final Stage of the Hohmann Transfer" . Previous . Main . Next .
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/research/solarsystem/jma/approach.html -- 3.8 Кб -- 16.08.2006
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8. Личная страница Субаева Ильнура Асфалевича
In the regular experiments carried out with the RAS radio telescopes at Pushchino during 1999-2002, the study of the radial dependence of scattering of compact natural radio sources was extended to remote regions of the solar plasma environment. ... The stream in the transalfvenic region displays the same typical radial structure as observed in the transonic region, i.e., the existence of a "precursor" - a narrow band of reduced scattering preceding a wide region of enhanced scattering. ...
[ Сохраненная копия ]  Ссылки http://astra.prao.psn.ru/SUB/Abstract.htm -- 2.3 Кб -- 11.06.2005
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9. Беспроводной геймпад для Xbox 360 и PC (черный) - Microsoft Corporation -
... title='Беспроводной геймпад для Xbox 360 и PC (черный) - Microsoft Corporation - Microsoft Corporation' border='0' align='left' width='120' style='margin-right: 20px;' hspace='7' vspace='5'/> Джойстик для компьютера от Microsoft! ... Использующий оптимизированную технологию беспроводной геймпад для Xbox 360 и PC работает на расстоянии 9 метров до 40 часов от двух батарей типоразмера АА, наглядный сигнал сообщит о разрядке батарей, чтобы вы смогли подключить зарядное устройство. ... С 1 плафоном . ...
[ Сохраненная копия ]  Ссылки http://astrokuban.info/astroku571.html -- 17.7 Кб -- 14.02.2016
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10. http://lnfm1.sai.msu.ru/grav/russian/life/chteniya/sagi2007/turyshev_Anomaly.pdf
THE STUDY OF THE PIONEER ANOMALY THE STUDY OF THE PIONEER ANOMALY The Pioneer Anomaly : Effect, New Data and New Investigation Slava G. Turyshev Jet Propulsion Laboratory, California Institute of Technology Seminar at the Sternberg Astronomical Institute Moscow State University, Moscow, 6 February 2007 1 THE STUDY OF THE PIONEER ANOMALY THE STUDY OF THE PIONEER ... Are they relevant to the Pioneer anomaly? ...
[ Текст ]  Ссылки http://lnfm1.sai.msu.ru/grav/russian/life/chteniya/sagi2007/turyshev_Anomaly.pdf -- 1784.2 Кб -- 12.02.2007
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11. A Structure for Quasars
... The picture shows a 2-dimensional sketch of the outflowing wind of a quasar (Elvis 2000, Astrophysical Journal , vol.545, p.63-76). In the funnel-shaped disk wind Elvis (2000) model a wind arises from a restricted range of radii on the accretion disk around the central black hole. Initially the wind makes a large angle to the disk plane (and so is roughly cylindrical). ... Looking through the quasi-cylindrical part of the wind we see UV and X-ray warm absorbers. ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~elvis/structure.htm -- 3.5 Кб -- 01.10.2012
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12. Dawn at Ceres | Astronotes
... Planets . ... An artistтАЩs impression of Ceres located in the asteroid belt, with plumes of water vapour rising from its surface. Could Ceres have more water than on Earth? (image credit: ESA/ATG medialab) . ... Ceres, captured by the Dawn Space craft in December 2014, Dawn was 740,000 miles (1.2 million km) from Ceres at the time. (image credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA) . ... Now itтАЩs a dwarf planet. (image credit: NASA/ESA/SWRI/Cornell University/University of Maryland/STSci) . ...
[ Сохраненная копия ]  Ссылки http://www.armaghplanet.com/blog/dawn-at-ceres.html -- 49.1 Кб -- 09.04.2016
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