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1. Magnetospheric electric fields (Oulu)
... The are two main sources of magnetospheric electric fields. The other is the solar wind related, dawn-to-dusk directed ("convection") field, and the other is the co-rotation electric field related to the rotation of the Earth along its spin axis. The electric fields have a strong effect on the drift paths of the magnetospheric plasma . ... The energetic particles, following the magnetic drifts more readily, are also affected by the convection field. ... Space Physics Text Book of Oulu ...
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Ссылки http://www.iki.rssi.ru/magbase/REFMAN/SPPHTEXT/efields.html -- 7.4 Кб -- 21.12.2007
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2. Conference Global Fields
Tsfasman and Vl\u adu\c t defined the set of invariants $\{\phi_q, q \text{ is a prime power, } \mathbb{R} \text{ or }\mathbb{C}\}$ of infinite global fields, but the properties of this sets are still not known. ... In this direction, I will talk about the constructions of infinite global fields having $n$ prescribed non-zero invariants, and of others having $n$ prescribed zero invariants. ...
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Ссылки http://www.mccme.ru/lifr/conf2007/-name=lebacque.htm -- 3.1 Кб -- 04.07.2007
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3. Southern Cross Astrophysics Conference Series
... Takuya Akahori "Faraday Rotation Measure due to the Intergalactic Magnetic Field" . Shae Brown "Cross-correlation of ATLAS and Spitzer-SWIRE Surveys: Probing intergalactic magnetic fields" . Roger Clay "Using low energy cosmic rays to investigate local galactic magnetic fields" . Roland Crocker "A new lower limit on the magnetic field around the Galactic Centre" . ... JinLin Han "Rotation measures of pulsars and radio sources for Galactic magnetic fields" . ...
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Ссылки http://www.atnf.csiro.au/research/Astro2010/attend.html -- 8.6 Кб -- 01.10.2012
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4. GOODS
... Summary of reduced ISAAC fields . ... This data release includes eight fully reduced VLT/ISAAC fields in J,H,K s bands covering 50 arcmin 2 of the GOODS region in the Chandra Deep Field South (CDFS). ... 8 ISAAC fields) . ... The 8 ISAAC fields which are part of this data release are superimposed onto a SOFI image (J+K) (part of a previous EIS data release). ... In one case (GOODS field 11/J-band), for which not enough standard stars were available, the ZP was boostrapped from previous SOFI/EIS data...
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Ссылки http://www.eso.org/science/goods/releases/20020408/ -- 21.5 Кб -- 24.03.2004
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5. Sorting on several fields
You can sort a file on several fields with the same sort command. The file is sorted on the first field; if some lines have the same value for this field they are sorted on the next field you specify and so on. ... Each field is separated by a space. ... sort -o results +3 -5 scores . ... From the first sort on field 4 (age) sort finds that Rice and Bramley are the same age so it now sorts these two lines on field 5 (score), placing Rice (67) before Bramley (75). ...
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Ссылки http://comet.sai.msu.ru/UNIXhelp/utilities2/sort3.3.html -- 2.7 Кб -- 17.01.1997
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6. I-GALFA Survey Fields
I-GALFA Survey Fields . ... Most I-GALFA fields are observed by ``nodding'' the telescope north and south along the meridian to trace out a zig-zag pattern on the sky as the Earth rotates. ... The I-GALFA fields fill the AO DEC range and overlap with each other by 20', with one field 3 degrees wide at the zenith and four others 9.3 degrees wide covering the rest of the survey. ... The LST range of each field is shown in blue. ... Field . ... The I-GALFA fields are shown in Galactic coordinates below. ...
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Ссылки http://www.naic.edu/~gibson/galfa/igalfa/fields/ -- 7.3 Кб -- 14.05.2009
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7. Bojan Nikolic -- Turbulent 3d fields and bnlib-1.3
... Bojan Nikolic web pages home . ... I've uploaded a new version the "bnlib" library that amongst other items contains the code to generate very large simulations of turbulent fields. ... http://www.mrao.cam.ac.uk/~bn204/alma/memo-turb.html#Current+version+of+library%3A+V1.3 . ... http://www.mrao.cam.ac.uk/~bn204/publications/2008/ALMASim08.pdf . Please enable JavaScript to view the comments powered by Disqus. blog comments powered by Disqus . Copyright 2012, Bojan Nikolic feedback welcome ...
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Ссылки http://www.mrao.cam.ac.uk/~bn204/blog/2009/02/turbulent-3d-fields-and-bnlib-13.html -- 4.7 Кб -- 22.11.2012
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8. Suppression of cooling by strong magnetic fields in white dwarf stars
... Astronomers of the SAO together with an international group of scientists have proposed an explanation to the long-standing mystery of why magnetic fields are more common amongst cool white dwarf stars than amongst young and hotter ones. ... As the result magnetic white dwarfs demonstrate excess in their frequencies in the temperature range below 14000K. The authors also show that the strongly magnetic white dwarfs are of the oldest stars of the Galaxy originated from intermediate-mass relic stars. ...
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Ссылки http://www.sao.ru/Doc-en/SciNews/2014/Nature/ -- 3.6 Кб -- 10.04.2016
[ Сохраненная копия ] Ссылки http://mavr.sao.ru/Doc-en/SciNews/2014/Nature/ -- 3.6 Кб -- 10.04.2016
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[ Сохраненная копия ] Ссылки http://mavr.sao.ru/Doc-en/SciNews/2014/Nature/ -- 3.6 Кб -- 10.04.2016
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9. Pulkovo database of sunspot magnetic fields
. Русская версия (Win-1251) . English version
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Ссылки http://www.gao.spb.ru/database/mfbase/ -- 1.8 Кб -- 21.05.2007
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10. Magnetic Fields
... 2 Magnetic Field . ... A magnetized bar has its power concentrated at two ends, its poles ; they are known as its north (N) and south (S) poles, because if the bar is hung by its middle from a string, its N end tends to point northwards and its S end southwards. ... That flow became known as an electric current . ... An electric current produced a magnetic force! ... The fundamental nature of magnetism was not associated with magnetic poles or iron magnets, but with electric currents . ...
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Ссылки http://www.cosmos.ru/mirrors/stern/Education/wmfield.html -- 11.1 Кб -- 24.03.2006
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11. ROSAT and EINSTEIN Calibration Fields
. Next: Image Manipulation Up: Point Response Functions Previous: On-Axis Point Response Functions . Three series of ROSAT calibration data are provided for general use. They provide examples of off-axis PRFs, and are situated in a directory with PROS alias xrcal . xecal has Einstein data. The list files in the directory provide a key to the data files (also given in the help files discussed in On-Axis Point Response Functions ). rsdc@cfa.harvard.edu . 1998-06-10
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Ссылки http://hea-www.harvard.edu/PROS/PUG/node124.html -- 3.5 Кб -- 01.10.2012
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12. James Aumonier: Cattle in the fields
. watercolour on paper: 300 x 460 mm . signed lower left: J. Aumonier . found on ebay / Gallery Duval , March 2006 .
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Ссылки http://star.arm.ac.uk/~csj/aumonier/paintings/cattle_in_fields.html -- 2.3 Кб -- 03.03.2006
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13. APOD: November 7, 1996 - Fields of Minerals on Ganymede
... Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer. November 7, 1996 . Fields of Minerals on Ganymede . Credit: NIMS , Galileo Mission , JPL , NASA . ... The leftmost photograph by Voyager shows surface features in visible light, but the rightmost photograph , taken in infrared light by Galileo, shows the locations of minerals in red and ice grains in blue. ... About APOD | ...
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Ссылки http://www.sai.msu.su/apod/ap961107.html -- 4.1 Кб -- 02.10.2012
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14. Image: Countryside. You can see rice fields in the foreground (this is the road
. Album : asv-album :: Travels to distant places and countries :: 1997/08 Kyoto, Nara (Japan) :: 24/08 Nara . Up . << Prev . Countryside. You can see rice fields in the foreground (this is the road from Nara to Kyoto). Next >> . Photo album generated by album script from MarginalHacks by Dave Madison on Tue Jun 23 14:46:24 2015 .
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Ссылки http://crydee.sai.msu.ru/album/trips/1997.08.Japan/24.Nara/tn/g07l.jpg.index.html -- 6.2 Кб -- 23.06.2015
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15. Fields of Minerals on Ganymede
... Fields of Minerals on Ganymede . ... 7.11.1996 . ... Credit: NIMS , Galileo Mission , JPL , NASA Explanation: What treasures lie on the surface of Ganymede ? Last week, NASA released a map of Jupiter's largest moon made by the Galileo Orbiter highlighting ice and minerals deposits. The leftmost photograph by Voyager shows surface features in visible light, but the rightmost photograph , taken in infrared light by Galileo, shows the locations of minerals in red and ice grains in blue. ...
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Ссылки http://www.astronet.ru/db/xware/msg/1162877 -- 12.7 Кб -- 05.10.2003
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16. Towards Optimal Analysis of HST Crowded Stellar Fields
... The improvement will be more pronounced in our crowded Wide Field Camera (WFC) images, and may be increased further through use of a more sophisticated method of combining the individual dithered images. Our analysis allows us to check for point spread function shape variations in the HST Planetary Camera (PC) field. ... In crowded field images, we are deriving information about the faint end of the luminosity function (LF) from the texture of the image background. ...
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Ссылки http://www.adass.org/adass/proceedings/adass96/lindepe.html -- 10.0 Кб -- 23.06.1998
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17. The Sun Energy Source Is Not Nuclear Fusion But Magnetic Fields. - an Astronomy
Bigbang Forum Message . Forums: . ... The Sun Energy Source Is Not Nuclear Fusion But Magnetic Fields. ... The sun is not heated by fusion reaction but by magnetic fields coming from the galactic center. The nuclear fusion is a by product of the magnetic fields heating. ... www.astronomy.net . About Astronomy Net | Advertise on Astronomy Net | ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...
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Ссылки http://www.astronomy.net/forums/bigbang/messages/882.shtml -- 14.2 Кб -- 09.04.2016
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18. Low Level Operators and Bit Fields
... Bit Fields . Bit Fields: Practical Example . ... NOTE: The combination of pointers and bit-level operators makes C useful for many low level applications and can almost replace assembly code. ... To illustrate many points of bitwise operators let us write a function, Bitcount , that counts bits set to 1 in an 8 bit number ( unsigned char ) passed as an argument to the function. int bitcount(unsigned char x) { int count; for (count=0; x != 0; x>>=1); if ( x & 01) count++; return count; } . ...
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Ссылки http://mavr.sao.ru/hq/sts/linux/book/c_marshall/node13.html -- 13.3 Кб -- 28.12.2007
[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/sts/linux/book/c_marshall/node13.html -- 13.3 Кб -- 02.10.2012
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/sts/linux/book/c_marshall/node13.html -- 13.3 Кб -- 02.10.2012
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19. How do neutron stars generate steady magnetic fields? | Astronomy.com
... Tonight's Sky . ... Observing . ... Sky this Month . ... Star Atlas . ... stars . ... Observing Podcasts . ... Astronomy for Kids . ... Observing springtime deep-sky objects with a large telescope . ... How do neutron stars generate steady magnetic fields? ... How can a neutron star exist if those neutrons are just going to pieces? Get instant access to subscriber content on Astronomy.com! ... Receive news, sky-event information, observing tips, and more from Astronomy's weekly email newsletter. ...
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Ссылки http://www.astronomy.com/magazine/ask-astro/2007/02/how-do-neutron-stars-generate-steady-magnetic-fields -- 62.8 Кб -- 10.04.2016
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20. el_fields
. Плато Шатжатмаз, здесь будет новая обсерватория ГАИШ / el_fields . Е.Ш. 31.10.2007 . 37 . 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 | 11 | 12 | 13 | 14 | 15 | 16 | 17 | 18 | 19 | 20 | 21 | 22 | 23 | 24 | 25 | 26 | 27 | 28 | 29 | 30 . el_fields.jpg .
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Ссылки http://lnfm1.sai.msu.ru/maidanak/shatzhatmaz2007/pages/el_fields.htm -- 3.6 Кб -- 31.10.2007
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