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6581. INTERBALL-TAIL KP list
This is the short list of INTERBALL-TAIL KP . ... INTERBALL-TAIL GSE and GSM cartesian coordinates, GSE cartesian velocity (2 min). 2. "igi" . ... DOK-2 and SKA-2: Electron fluxes in 21-26, 76-95, 150-500 keV energy ranges, proton fluxes in 22-28, 1000-3000 keV energy ranges and status flags (2 min). 4. "itt" . ... MIF-M/PRAM: GSM and GSE magnetic field vector, amplitudes of magnetic fluctuations in 1-4 and 600-850 Hz ranges (2 min). ... VDP: Antisunward ion flux (2 min). 10. "itw" . ...
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Ссылки http://www.iki.rssi.ru/apetruko/kplist1.html -- 2.7 Кб -- 31.03.1999
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6582. Bill Arnett's Home Page
... I have written a number of WWW documents on various topics, mostly having to do with astronomy. Brief descriptions of each can be found on my index page . See my log page for usage stats.) This "home page" has been copied around the Net quite a bit. ... It's really no more than links to Amazon.com but if you order after going thru my links then I get a little bit of Amazon's profit. ... But then I think of all we have achieved since then and I know I have the better deal. ...
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Ссылки http://www.iki.rssi.ru/arnett.html -- 7.3 Кб -- 31.03.1999
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6583. Uranus Picture List
Uranus . ... Miranda . ... 1998 image from HST showing bright clouds html . ... Two views of Uranus' darkspot 107k gif ; 40k jpg . normal and false color views 102k gif ; 40k jpg . ... Infrared image of Uranus B 33k gif . Infrared image of Uranus 2 B 37k gif . Infrared image of Uranus 3 B 56k gif . ... Infrared image of Uranus 5 B 43k gif . Infrared image of Uranus 6 B 34k gif . Infrared image of Uranus 7 B 36k gif . ... Uranus' rings (false color) 78k gif ; 35k jpg ; 211k gif . ...
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Ссылки http://www.iki.rssi.ru/nineplanets/pxuranus.html -- 11.2 Кб -- 31.03.1999
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6584. Neptune Picture List
Neptune . ... Triton . Neptune 291k gif . Full Disk Neptune 93k gif ; 29k jpg . ... New Dark spot 25k jpg ; 113k gif ; caption ; press release . ... Another thin Crescent of Neptune 166k gif . ... low resolution shot of Neptune, possibly showing great black spot 210k gif . ... Parting view of Neptune and moon Triton 59k gif ; 17k gif ; 23k jpg . ... Small Dark Spot 190k gif ; 133k jpg . Small Dark Spot 55k gif ; 23k jpg . ... The Great Dark Spot 423k gif ; 153k gif ; 97k jpg . ...
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Ссылки http://www.iki.rssi.ru/nineplanets/pxnep.html -- 15.1 Кб -- 31.03.1999
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6585. Jupiter Picture List
Jupiter . ... HST view (true color) 1877k tiff ; 264k gif ; 96k jpg ; 34k jpg . Jupiter Storms (HST) 37k jpg ; 169k gif ; 1800k tiff ; ( caption ) . ... Jupiter and Ganymede 60k jpg . Jupiter with Narrow Angle Camera (Violet filter) 359k gif . Jupiter with Narrow Angle Camera (Violet filter) 182k gif . Jupiter with Narrow Angle Camera (Violet filter) 274k gif . Jupiter with Narrow Angle Camera (Violet filter) 291k gif . ... Jupiter with Wide Angle Camera (Orange filter) 324k gif . ...
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Ссылки http://www.iki.rssi.ru/nineplanets/pxjup.html -- 35.2 Кб -- 31.03.1999
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6586. Earth Picture List
Map projected image of Earth (AVHRR) 123k gif ; 1440k gif . Famous Apollo 11 image of Africa Europe 31k jpg . global composite of satellite images 508k gif . ... Galileo image of South America from 1st flyby 62k jpg . ... Earth by Meteosat 4 satellite (IR filter) 688k jpg . ... Ross ice sheet, Antarctica, taken by Galileo on its first pass of Earth 11k jpg . ... NOAA satellite's view of USA 322k gif . ... images of Earth from Clementine html . Earth images from weather satellites html . ...
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Ссылки http://www.iki.rssi.ru/nineplanets/pxearth.html -- 13.8 Кб -- 31.03.1999
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6587. Earth
... 0- 40 Crust 40- 400 Upper mantle 400- 650 Transition region 650-2700 Lower mantle 2700-2890 D'' layer 2890-5150 Outer core 5150-6378 Inner core The crust varies considerably in thickness, it is thinner under the oceans, thicker under the continents. ... Taken as a whole, the Earth's chemical composition (by mass) is: . ... U nlike the other terrestrial planets, Earth's crust is divided into several separate solid plates which float around independently on top of the hot mantle below. ... Moon .. ...
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Ссылки http://www.iki.rssi.ru/nineplanets/earth.html -- 18.6 Кб -- 31.03.1999
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6588. IKI SSC INTMINS APRIL98
... The predicted MIR's ground tracks, which pass near INSPIRE net, are available in this home page. The track consists from magnetic footprints calculated by magnetic mapping from MIR positions with 30 s step. ... For each time some of the INSPIRE net place are selected as soon as its coordinates are close to the MIR magnetic footprint (the geocentric angular distance between SP and footprint is less then 2.1 deg) . Back to the Top . ... Back to the IKI Satellite Situation Center (SSC) . ...
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Ссылки http://www.iki.rssi.ru/vprokhor/intmins/archive.htm -- 7.0 Кб -- 29.03.1999
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6589. http://www.iki.rssi.ru/vprokhor/intmins/april98/mm9804p2.upg
UTyymmdd:Thhmnss:Hs km:GLONS d:GLATSd:GLONF d:GLATFd:arcln:angdst: #-CC: place : 19980425 .002930 382. 123.22 38.48 -122.80 39.45 .05 1.12 7-CA Sonoma 19980425 .003000 381. ... 17.69 -40.91 -.58 50.45 3.92 .56 E4-UK London 19980425 .024630 387. 17.69 -40.91 -.58 50.45 3.92 1.28 E10-UK London 19980425 .024700 387. ... 5.40 42.37 5.36 43.60 .05 1.91 E3-IT Aosta 19980425 .092430 383. ... 1.11 49.27 1.02 50.16 .05 1.63 E10-UK London 19980425 .110100 385. ...
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Ссылки http://www.iki.rssi.ru/vprokhor/intmins/april98/mm9804p2.upg -- 18.9 Кб -- 29.03.1999
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6590. http://www.iki.rssi.ru/vprokhor/intmins/april98/mm9804p1.upg
UTyymmdd:Thhmnss:Hs km:GLONS d:GLATSd:GLONF d:GLATFd:arcln:angdst: #-CC: place : 19980418 .011300 385. 121.45 49.73 -121.06 50.26 .04 1.47 23-WA Glacier 19980418 .011730 382. ... 19.38 -43.31 -.68 51.80 4.33 .46 E10-UK London 19980418 .050730 389. ... 2.95 51.75 2.87 52.55 .05 1.95 E10-UK London 19980418 .150030 385. ... 2.64 50.95 -2.79 51.78 .05 1.75 E10-UK London 19980418 .163230 385. ... 23.47 -45.62 1.84 53.43 4.86 2.08 E10-UK London 19980419 .001800 382. ...
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Ссылки http://www.iki.rssi.ru/vprokhor/intmins/april98/mm9804p1.upg -- 26.9 Кб -- 29.03.1999
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6591. INTERBALL-TAIL KP PI list
INTERBALL Scientific Committee . Lev Zelenyi - INTERBALL Project Manager. Email: lzelenyi@iki.rssi.ru . Mikhail Nozdrachev - Tail Probe Project Scientist. Email: mnozdrch@vm1.iki.rssi.ru . George Zastenker - Tail Probe Deputy Project Scientist. ... Mikhail Mogilevsky - Auroral Probe Project Scientist. ... INTERBALL-TAIL PIs . ... Elena Budnik - SKA-2 experiment. ... Email: ingrid@irf.se . ... KP data processing . Elena Gavrilova - INTERBALL and KP preliminary data processing. ...
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Ссылки http://www.iki.rssi.ru/apetruko/whois1.html -- 3.8 Кб -- 24.03.1999
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6592. The Sun
T he Sun is an ordinary G2 star, one of more than 100 billion stars in our galaxy. diameter : 1,390,000 km . mass : 1.989e30 kg temperature : 5800 K (surface) 15,600,000 K (core) T he Sun is by far the largest object in the solar system. ... C onditions at the Sun's core are extreme. ... I n addition to heat and light, the Sun also emits a low density stream of charged particles (mostly electrons and protons) known as the solar wind which propagates throughout the solar system at about 450 km/sec. ...
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Ссылки http://www.iki.rssi.ru/nineplanets/sol.html -- 15.8 Кб -- 19.03.1999
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6593. Planetary Linguistics
... English Sun Mercury Venus Earth Moon Mars Jupiter Saturn Uranus Neptune Pluto Latin Sol Mercurius Venus Terra Luna Mars Jupiter Saturnus Uranus Neptunus Pluto French Soleil Mercure V nus Terre Lune Mars Jupiter Saturne Uranus Neptune Pluton Italian Sole Mercurio Venere Terra Luna Marte Giove Saturno Urano Nettuno Plutone Spanish Sol Mercurio ... See Peter Blinn's Planetary Gazetteer for more . ... Linguistics .. ... Bill Arnett ; last updated: 1999 Mar 17 . ...
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Ссылки http://www.iki.rssi.ru/nineplanets/days.html -- 12.4 Кб -- 18.03.1999
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6594. The Wind Spacecraft
The Wind spacecraft. ... It was designed to observe the solar wind approaching Earth, from a position near the Lagrangian point L1, and it is part of the International Solar-Terrestrial Physics (ISTP) Initiative . ... The original plan called for "Wind" to approach its final station over two years, undergoing two close encounters with the Moon to boost its speed. ... For additional details and updates, see the home page of the "Wind" mission. Exploration" home page (index) Glossary . ...
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Ссылки http://www.iki.rssi.ru/magbase/REFMAN/EAMAGSPH/wwind.html -- 7.4 Кб -- 15.03.1999
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6595. The Sun
The Sun is our nearest star and the source of energy for life on Earth. ... For centuries astronomers wondered whether they were clouds floating in the Sun's atmosphere, but we now know that they really are huge regions of magnetic field, about as intense as the field at the poles of an iron magnet. ... Such abrupt events were named solar flares , and what made them especially interesting was that occasionally, after a prominent flare, a magnetic storm would erupt on Earth. ...
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Ссылки http://www.iki.rssi.ru/magbase/REFMAN/EAMAGSPH/wsun.html -- 8.2 Кб -- 15.03.1999
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6596. The Tail of the Magnetosphere
... Most of the volume of the tail is taken up by two large bundles of nearly parallel magnetic field lines (see drawing). ... Plasma sheet" separating . tail lobes . ... Tail lobes . ... Separating the two tail lobes is the "plasma sheet", a layer of weaker magnetic field and denser plasma, centered on the equator and typically 2-6 Earth radii thick. Unlike field lines of the tail lobes, those of the plasma sheet do cross the equator, though they are quite stretched out. ...
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Ссылки http://www.iki.rssi.ru/magbase/REFMAN/EAMAGSPH/wtail.html -- 12.0 Кб -- 15.03.1999
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6597. The Polar Caps
Plasma phenomena occuring at one place in the magnetosphere also affect other locations This linkage is most pronounced between points that share the same field line, since field lines guide the motion of ions and electrons. ... It follows that the places on Earth most sensitive to distant magnetic effects are the "polar caps" , the regions around the magnetic poles. A good example is the polar aurora . ... way polar field lines . ... and to the Sun . ... Next Stop: #26H. Polar Cap--History . ...
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Ссылки http://www.iki.rssi.ru/magbase/REFMAN/EAMAGSPH/wpcap.html -- 7.7 Кб -- 15.03.1999
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6598. The Magnetosphere
... The atoms of oxygen, for instance, contain electrons with negative electric charges and protons which are positive, but the two charges balance each other andthe electric and magnetic forces cancel. Magnetic forces have almost no effect on neutral atoms. ... It can be shown that such free electrons and ions will be guided by the magnetic field lines (or "lines of force") which rise from near the southern (magnetic) pole and enter the Earth again near the northern pole. ...
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Ссылки http://www.iki.rssi.ru/magbase/REFMAN/EAMAGSPH/wms1.html -- 4.9 Кб -- 15.03.1999
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6599. The Earth's Magnetosphere
... A typical density of energetic ions is 1 per cubic cm., and the ions are matched by electrons, generally of lower energy. ... This region is almost empty of plasma--typical density 0.01 ion/cubic cm., the "best vacuum" in the Earth's vicinity--but it contains a relatively strong magnetic field which, since it fills a large volume, can store appreciable magnetic energy, Many believe that this is the storehouse from which substorms draw their energy, releasing it quite rapidly. ...
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Ссылки http://www.iki.rssi.ru/magbase/REFMAN/EAMAGSPH/wms2.html -- 6.8 Кб -- 15.03.1999
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6600. The Io Dynamo
The giant planet Jupiter has four large moons, discovered by Galileo and visible through good binoculars. ... A dynamo is created in a magnetic field by an electric circuit, part of which is moving relative to the rest (additional conditions must also be met). ... Furthermore, the plasma between them conducts electricity very well along its magnetic field lines, which act as if they were wires connecting Io and the planet (drawing). ... Exploration" home page (index) Glossary . ...
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Ссылки http://www.iki.rssi.ru/magbase/REFMAN/EAMAGSPH/wio.html -- 5.5 Кб -- 15.03.1999
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