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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• Defining the sort field
• Sorting on a specific part of a field
• Sorting on a specific field

... 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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• New data on the cpmplex field structure of chemically peculiar stars
• Physics of Magnetic Stars 2007
• Speckle interferometry of magnetic stars

. 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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• The Chandra Multiwavelength Project (ChaMP)
• ChaMPlane
• ChaMPlane data_archive_.html

. watercolour on paper: 300 x 460 mm . signed lower left: J. Aumonier . found on ebay / Gallery Duval , March 2006 .

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• Armagh Observatory
• Abstract 205
• Conference 98

. 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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• Index of /ftproot/pub/rec/music/lyrics/cs-uwp/f/fields.of.the.nephilim
• Index of /ftproot/pub/rec/music/lyrics/cs-uwp/f/fields.dorothy
• Index of /ftproot/pub/rec/games/Cracks-Solutions-Cheats/Fields_of_Glory

... 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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• ADASS 2003 Conference Proceedings
• Starfinder: a Code for Crowded Stellar Fields Analysis
• Sky Surveys

... 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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• Laboratory for the Stellar Magnetism Study of SAO of the RAS - Magnetic stars -
• About laboratory
• Main Researches Activities

. 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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• Ekaterina's homepage
• Natural Satellites Service. Special Ephemerides

... Other Characteristics of the Sun: Variability of Rotation, Magnetism, Chemical Structure, Planetary System. ... Methods of Solar Magnetic Fields Measuring: Visual, Photografic, Photoelectric. ... Empiric Datas of Magnetic Fields in Photosphere, Chromosphere and Corona. ... Characteristics of Magnetic Field in Balanced Force Tubes by Potential and Forceless Field. ... Phenomenons in Active Region (Magnetic Field, Spots, Torches, Solar Prominences, Flares, Discharges. ... Magnetic Fields in Flares. ...

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• SET OF MAGNETIC AND ELECTRIC FIELD DETECTORS EXO-EM
• Researches of Astronomy and Space Physics Department
• aorient

Many entry fields permit sexagesimal entry (h:m:s.s or :':"). ... Sexagesimal entry is flexible in that you can specify one to three fields, as you desire. ... Offset and duration entry widgets assume that a single field is decimal arc-seconds or seconds ('.' or s.s) and two fields are (arc) minutes and seconds (':"." or m:s.s). ... You may specify one to three fields. ... Note: sexagesimal positions are entered in the same fashion, but a single field is decimal hours or degrees (h.h or . ...

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• field
• TUI:Tidbits:Entering Sexagesimal Positions
• lsst.tcc: tcc.axis.computeObj Namespace Reference

You may see figures of this paper below... or download the whole paper in PostScript or LaTeX source , everything compressed by ZIP. LaTeX notes: you would need some specific LaTeX styles . See CS-11 HomePage for more. Figures are in EPS (Encapsulated PostScript) format to be inserted using software like dvips . You can download these files via ftp. If you use GIF format, choose "Save Image As..." on the images below, or click here: first and second . Figure 1. ...

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• Anatol Cherepashchuk
• Igor Antokhin

... We have compared visualized fields of GSC and USNO A1.0 catalog with unpublished photographic finding charts that were sent by L. Plaut to the compilers of the GCVS. ... 7-15 A9 --- GCVS GCVS or NSV name 17-25 F9.4 --- GSC GSC number 26 A1 --- NoteFlag *Nonstar (GSC) flag 28-29 I2 h RA2000GSC.h Hours RA (GSC), equinox 2000.0 31-32 I2 min RA2000GSC.m Minutes RA (GSC), equinox 2000.0 34-38 F5.2 s RA2000GSC.s Seconds RA (GSC), equinox 2000.0 40 A1 --- DE2000GSC.- ... Plaut, L., 1966, Bull. ...

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• Method of search of flare current sheets in the magnetic field obtained by MHD

IBIS Data Analysis . ... IBIS . ... Flat Fielding - Introduction . The images obtained by IBIS will have intensity variations across the field of view that are not due to the solar image, but rather caused by instrumental effects that alter the observed intensity in each point of the field of view. ... IBIS Flat Fielding Techniques . ... Therefore, it is desirable to obtain the flat field measurements center on a point along the equator near the heliographic center of the solar disk. ...

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• Carlo Baffa
• Arcetri Solar Physics Group: Solar Polarimetry
• Arcetri Solar Physics Group: High Resolution Studies

... astro-ph . ... SAI VO . ... Whitespace-separated words are treated as AND ed. Show 10 50 100 articles per page in Full Compact mode . Normalized to: Fields, E. 4 article(s) in total . 61 co-authors, from 1 to 4 common article(s). ... Backus, Peter. Barott, Billy. Barott, William. ... Dreher, John. ... Fleming, Matt. Fleming, Scott W.. Forster, James R.. ... Law, Casey James. ... MacMahon, David. McMahon, Peter. ... Vitouchkine, Artyom. ... Williams, Peter K. G.. ...

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Field centres for 6dF/FLAIR observations of the 6QZ survey. # 6dF fields have radius 2.844 deg. and were defined in the # J2000 system. FLAIR fields are square and are 5x5 deg # centred on UKST survey positions and defined in the B1950 # system. # 6dF : coordinates ( B1950 ) coordinates ( J2000 ) # Field hh mm ss.ss dd mm ss.s hh mm ss.ss dd mm ss.s sgp001 21 51 31.25 -30 11 45.4 21 54 25.40 -29 57 33.0 sgp002 22 10 08.35 -29 50 17.3 22 12 59.50 -29 35 25.0 sgp003 22 30 24.34 ...

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• 2dF QSO Redshift Survey (2QZ)

Stellarium 0.12.3 . ... Classes . ... ClassљList . ClassљIndex . ... FieldConcatModel Class Reference . Allows for concatinating fields from a model for disply. ... QObject *parent=0) . ... columnCount (const QModelIndex &parent=QModelIndex()) const . ... rowCount (const QModelIndex &parent=QModelIndex()) const . ... This class allows a table model to concatinate fields for the purpose of display. ... home/aw/devel/stellarium/trunk/plugins/LogBook/src/models/ FieldConcatModel.hpp . ...

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• FIELD Home Page
• Screenshots | Jason Field
• screenshot

... Home Observing Floyd Bennett Field . ... Lecture Series 2014-2015 . ... Beyond New York City . ... Observing Resources for Amateur Astronomers - Part 1: Beginning Observers . ... A History of the First Forty Years of the Amateur Astronomers Association . ... The new observing location at Floyd Bennett Field is easy for people to find in the dark and will also be within walking distance of the Q35 bus. ... 2016 Amateur Astronomers Association of New York Designed by Press Customizr Powered by . ...

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... Satellite data ] . SMIS ] . The program is designed to process the specific AVHRR instrument data for calculation and analysis of temperature fields on the sea surface and upper level of clouds. It performs brightness correction for visible channels with regards to clouds altitude. ... The program features a wide variety of classification algorithms (including two-dimensional histogram analysis) and enables to construct personal procedures for classification. ... Back to SMIS Home Page . ...

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• Myasnyankin Andrey , Moscow Institute of Physics and Technology (MIPT),Space
• Matyushkin Evgeny, Space Research Institute (SRI)
• Proshin Andrej, Space Research Institute (SRI)

... Head of the seminar: Prof. B.V. Somov, . ... The seminar considers the questions related to generation of magnetic fields in astrophysical plasmas, effect of the magnetic reconnection and particle acceleration in strong magnetic fields, the origin and propagation of cosmic rays, the flares and other non-stationary phenomena in the solar atmosphere and solar wind, Sun Earth connections and physical processes in the heliosphere. ... On the Topological Models and Topological Trigger of the Solar Flares...

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... 3 ­ Sternberg State Astronomical Institute, Moscow, :jeanna@sai.msu.ru The graphic method of the analysis of an arrangement of linear structural elements on geographical and geological maps of continents (A.V.Dolitsky, [1]) has allowed to find out global stress fields of the past and among them one which directions (the main normal and maximal tangents) describe more than 80 % of all linear elements of a relief. ... The found poles share program way on density of an arrangement on 3-4 groups. ...

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• http://selena.sai.msu.ru/Symposium/ir_luna_e.pdf