Найдено документов: 328520 (186 сайтов) ---- Время поиска: 1.16сек. |
Показаны документы, содержащие фрагменты текста из документа
http://star.arm.ac.uk/preprints/2008/533/.
http://star.arm.ac.uk/preprints/2008/533/.
1. QSO Absorption Lines and Other Cosmological Probes
.
[
Сохраненная копия
]
Ссылки http://zebu.uoregon.edu/1997/ph410/l22.html -- 12.7 Кб -- 10.03.1997
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>427) - zebu.uoregon.edu/ )
2. Absorption line spectra of the UV bright z=2.4 QSO HE 1122-1649
... We present ultraviolet and optical spectra of the bright (V=16.5), high-redshift ( ) QSO HE1122 - 1649 (Reimers et al. 1995a,1995b). ... Keywords: absorption lines . ... The combined data are shown in Figure 1. ... The Ly profile reveals an absorbing subcomponent at in agreement with results from heavy element absorption lines detected in the high resolution optical data. ... Figure: Velocity profiles of heavy element absorption lines arising in the damped Ly system as seen in the optical data. ...
[
Сохраненная копия
]
Ссылки http://www.stsci.edu/stsci/meetings/shst2/koehlers.html -- 14.3 Кб -- 15.06.2005
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>18486) - www.stsci.edu/ )
3. Magnetic Field Lines
... Magnetic field lines similarly describe the structure of magnetic fields in three dimensions.They are defined as follows. If at any point on such a line we place an ideal compass needle, free to turn in any direction (unlike the usual compass needle, which stays horizontal) then the needle will always point along the field line (drawing below). Field lines converge where the magnetic force is strong , and spread out where it is weak. ... Exploration" home page (index) Glossary . ...
[
Сохраненная копия
]
Ссылки http://www.iki.rssi.ru/magbase/REFMAN/EAMAGSPH/wfldline.html -- 5.1 Кб -- 21.12.2007
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>1092) - www.iki.rssi.ru/ )
4. Identify the lines in one of the rows of the spectrum
Next: Wavelength calibration Up: Getting Started Previous: Detecting lines in . ... and the Calibration Starting Row will be used for the lines identifications. ... After setting these parameters, click the button. to pop up the Identify window. ... The identification starts by clicking on , which plots one row of the spectrum in the graphic window, indicates the position of the detected arc lines with blue vertical traces and gives a cursor. ... Figure: Lines Identification Window . ...
[
Сохраненная копия
]
Ссылки http://www.sao.ru/precise/Midas_doc/doc/95NOV/vol2/node533.html -- 5.7 Кб -- 23.02.1996
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>2978) - www.sao.ru/ )
5. Explosive Events
... High spectral, spatial and temporal resolution UV observations of the quiet Sun transition region show a highly structured and dynamical environment where transient supersonic flows are commonly observed. ... Estimates of the kinetic and enthalpy fluxes associated with these events show that explosive events are not important so far as solar coronal heating is concerned. ... In some cases, non-Gaussian line profiles are associated with supersonic flows in small magnetic loops. ...
[
Сохраненная копия
]
Ссылки http://star.arm.ac.uk/annrep/annrep2004/node44.html -- 8.1 Кб -- 19.04.2005
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>2966) - star.arm.ac.uk/ )
6. http://xmm.vilspa.esa.es/external/xmm_sw_cal/icwg/presentations/WS_CT.pdf
... How to calibrate the energy scale for higher energies of future gratings? Difficult to find astronomical targets with well defined lines. ... Source Energy Flux keV HZ 43 0.2 Bright Sirius B 0.2 HZ43 /10 RXJ1856 1 Faint Simplicity Var WD WD No No No No Yes Yes Extend Lines Point Point Point 1' Point Point Point No Point Point Yes No Yes Yes Yes Yes Point Point , jet Point Cont Cont Cont Cont Lines Cont Lines Lines Lines ...
[
Текст
]
Ссылки http://xmm.vilspa.esa.es/external/xmm_sw_cal/icwg/presentations/WS_CT.pdf -- 145.6 Кб -- 20.06.2006
Похожие документы
Похожие документы
7. V1494
... The spatially resolved structure near the hydrogen emission H line was found in the spectrum taken with the BTA/SCORPIO in June, 2013. ... The fragment of the Nova V1494 Aql spectrum is shown in Fig.1. ... The Nova V1494 Aql has passed the stage of the supersoft X-ray source (SSS) in the period between 218 and 516 days after the visible light maximum (Schwarz et al., ... The spectrum of Nova V1494 Aql taken on 2013 June 9 with BTA/SCORPIO . ... The vertical lines are the lines of night sky emission....
[
Сохраненная копия
]
Ссылки http://www.sao.ru/Doc-en/SciNews/2013/V1494/ -- 6.7 Кб -- 28.02.2014
[ Сохраненная копия ] Ссылки http://mavr.sao.ru/Doc-en/SciNews/2013/V1494/ -- 6.7 Кб -- 27.02.2014
Похожие документы
[ Сохраненная копия ] Ссылки http://mavr.sao.ru/Doc-en/SciNews/2013/V1494/ -- 6.7 Кб -- 27.02.2014
Похожие документы
Еще в разделе:
(Показать все результаты (>303) - mavr.sao.ru/ )
8. Magnetic Field Lines
... If at any point on such a line we place an ideal compass needle, free to turn in any direction (unlike the usual compass needle, which stays horizontal--such needles exist, see bottom of page) then the needle will always point along the field line (drawing below). ... Because of this attachment, the behavior of electrified gas ("plasma") in space, a gas of free ions and electrons, is dictated by the structure of field lines: Electric currents, for instance, find it easiest to flow along such lines. ...
[
Сохраненная копия
]
Ссылки http://www.cosmos.ru/mirrors/stern/Education/wfldline.html -- 8.6 Кб -- 24.03.2006
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>1208) - www.cosmos.ru/ )
9. A Quasar Primer
... The picture shows sketches of the optical and ultraviolet (top, left) and X-ray (top, right) spectra of a typical quasar or AGN (Active Galactic Nucleus). These spectra are full of sharp features due to the interaction of atoms with light ('atomic features'). They can be high (= bright) points, called 'emission lines' or low (= dark) points, called 'absorption lines' . ... Broad Emission Lines ("BELs") [seen in 100% of AGN], . ... Broad Absorption Lines ("BALs") [see in only 10% of AGN], . ...
[
Сохраненная копия
]
Ссылки http://hea-www.harvard.edu/~elvis/primer.htm -- 2.8 Кб -- 01.10.2012
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>3127) - hea-www.harvard.edu/ )
10. Line Disciplines and Streams Modules
Most radio and modem clocks used for a primary (stratum-1) NTP server utilize serial ports operating at speeds of 9600 baud or greater. ... In order to reduce these errors, a set of special line disciplines and stream modules can be configured in the Unix kernel. ... Note that not all Unix kernels support line disciplines and of those that do, not all support System V streams. ... There are two line disciplines and a special streams module included in the distribution. ...
[
Сохраненная копия
]
Ссылки http://www.sai.msu.su/~er/xntp/ldisc.html -- 8.3 Кб -- 21.12.2007
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>6055) - www.sai.msu.su/ )
11. A Morning Line of Stars and Planets
... A Morning Line of Stars and Planets . ... Pictured above, easily visible from left to right, were the Pleiades open star cluster, Jupiter , Venus , and the " Follower " star Aldebaran , all seen before a starry background. ... Jupiter and Venus will continue to dazzle pre-dawn strollers all over planet Earth for the rest of the month, although even now the morning planets are seen projected away from the line connecting their distant stellar sky mates . ... Publications with words: Venus - Jupiter ....
[
Сохраненная копия
]
Ссылки http://www.astronet.ru/db/xware/msg/1267189 -- 15.4 Кб -- 11.07.2012
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>118925) - www.astronet.ru/ )
12. SINGULAR POINTS IN THE SOLAR CHROMOSPHERE
SINGULAR POINTS IN THE SOLAR CHROMOSPHERE . ... In the structure of the solar chromosphere, containing information on the configuration of the magnetic field, we have found and identified all the main types of the singular points ( see Fig. 1 ), which are known as inherent features of the 2-D vector field. ... The main types of the singular points are the node, the focus, the center, and the saddle. ... Singular point of the focus type in the solar chromosphere. ...
[
Сохраненная копия
]
Ссылки http://www.izmiran.rssi.ru/info/personalia/molodensky/spoints.html -- 8.2 Кб -- 11.12.2015
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>694) - www.izmiran.rssi.ru/ )
13. Advanced Pointer Topics
... Pointers to Pointers . ... Pointers to a Function . ... We have introduced some advanced pointer issues already. This chapter brings together some topics we have briefly mentioned and others to complete our study C pointers. ... main(int argc, char **argv) . ... These are the only arguments main accepts. argc is the number of arguments typed -- including the program name. argv is an array of strings holding each command line argument -- including the program name in the first array element. ...
[
Сохраненная копия
]
Ссылки http://mavr.sao.ru/hq/sts/linux/book/c_marshall/node12.html -- 11.8 Кб -- 28.12.2007
[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/sts/linux/book/c_marshall/node12.html -- 11.8 Кб -- 02.10.2012
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/sts/linux/book/c_marshall/node12.html -- 11.8 Кб -- 02.10.2012
Похожие документы
[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/sts/linux/book/c_marshall/node12.html -- 11.8 Кб -- 02.10.2012
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/sts/linux/book/c_marshall/node12.html -- 11.8 Кб -- 02.10.2012
Похожие документы
Еще в разделе:
(Показать все результаты (>1331) - jet.sao.ru/ )
14. I-GALFA Reveals Dynamic Events in Our Galaxy
I-GALFA Reveals Dynamic Events in Our Galaxy . S. J. Gibson, J.-h. Kang, B.-C. Koo, June 2009 . ... The white stripe marks the Galactic equator ( b=0 ). ... I-GALFA three-color H I image for FVW40.0+0.5, integrated over v lsr = -100 to -90 km/s ( red ), -90 to -80 km/s ( green ), and -80 to -70 km/s ( blue ). ... I-GALFA data reveal a complex tracery of loops, filaments, and blobs hundreds of parsecs above and below the Galactic plane, with isolated compact clouds extending even higher. ...
[
Сохраненная копия
]
Ссылки http://www.naic.edu/~gibson/galfa/igalfa/gallery/dyn/ -- 7.1 Кб -- 15.12.2009
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>4724) - www.naic.edu/ )
15. A survey for redshifted molecular and atomic absorption lines. I.
We are currently undertaking a large survey for redshifted atomic and molecular absorption lines at radio frequencies. ... For the latter, no H I absorption was detected at the same redshift as the borderline OH detection. In order to determine why no clear molecular absorption was detected in any of the 13 sources searched, we investigate the properties of the five redshifted systems currently known to exhibit OH absorption. ... Australia Telescope National Facility . ... Australia . ...
[
Сохраненная копия
]
Ссылки http://www.atnf.csiro.au/people/Matthew.Whiting/papers/html_abstracts/absn1_abs.html -- 4.8 Кб -- 10.09.2008
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>28511) - www.atnf.csiro.au/ )
16. Line (ImageJ API)
... java.lang.Object ij.gui.Roi ij.gui.Line . ... public class Line . ... int . ... protected double . ... Constructor Detail public Line (int ox1, int oy1, int ox2, int oy2) . Creates a new straight line selection using the specified starting and ending offscreen integer coordinates. public Line (double ox1, double oy1, double ox2, double oy2) . Creates a new straight line selection using the specified starting and ending offscreen double coordinates. public Line (int sx, int sy, ImagePlus imp) . ...
[
Сохраненная копия
]
Ссылки http://www.astro.louisville.edu/software/astroimagej/imagej/api/ij/gui/Line.html -- 37.4 Кб -- 02.12.2010
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>413) - www.astro.louisville.edu/ )
17. Theoretical Astrophysics
Subject, Problems and Objects of Theoretical Astrophysics. ... Stellar Photospheres, Their Features. ... Physics of Continuous Radiation Absorption in Stellar Photospheres. ... Continuous Radiation Absorption in Stellar Photospheres of Various Spectral Classes. Solar Type Photospheres. ... Characterisics of Absorption Lines. ... Interstellar Absorption Lines, Their Features. ... Physical and Dynamic Features of Interstellar Medium, Which Follows from Observations of Interstellar Absorption Lines. ...
[
Сохраненная копия
]
Ссылки http://space.univ.kiev.ua/courses/teor_astroph_e.html -- 8.7 Кб -- 23.02.2005
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>101) - space.univ.kiev.ua/ )
18. IBIS: Technical Description
The following papers summarize the characterization and technical performance of IBIS : . ... Characterization of Fabry-Perot interferometers and multi-etalon transmission profiles. ... Righini, A., Cavallini, F., Reardon, K. P., 2010, Astronomy and Astrophysics , 515 , A85, . ... The filter wheel is located between the two interferometers. ... The interferometers can be rapidly tuned, simultaneously, so to allow sequential scanning of the spectral lines of interest (see movie in IBIS Intro ). ...
[
Сохраненная копия
]
Ссылки http://www.arcetri.astro.it/science/solar/IBIS/IBIS_description.html -- 33.6 Кб -- 13.12.2015
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>9786) - www.arcetri.astro.it/ )
19. Stellarium: StelCircleArcRenderer Class Reference
Stellarium 0.12.3 . ... StelCircleArcRenderer Class Reference . Provides functions to draw circle arcs using StelRenderer . ... drawGreatCircleArc (const Vec3d &start, const Vec3d &stop, const SphericalCap *clippingCap=NULL, void(*viewportEdgeIntersectCallback)(const Vec3d &screenPos, const Vec3d &direction, void *userData)=NULL, void *userData=NULL) . ... Create a circle arc renderer to draw multiple circle arcs . ... void(*)(const Vec3d &screenPos, const Vec3d &direction, void *userData)љ . ...
[
Сохраненная копия
]
Ссылки http://astro.uni-altai.ru/~aw/stellarium/api/classStelCircleArcRenderer.html -- 26.8 Кб -- 28.02.2014
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>1864) - astro.uni-altai.ru/ )
20. Synthetic Images of the Solar Corona from Octree Representation of 3-D Electron
... Empirical and theoretical modeling of 3-D structures in the solar corona is confronted by the tremendous amount of data needed to represent phenomena with a large dynamic range both in size and magnitude, and with a rapid temporal evolution. Octree representation of the 3-D coronal electron distribution offers the right compromise between resolution and size, allowing computation of synthetic images of the solar corona. ... The time interval between images is one day. ...
[
Сохраненная копия
]
Ссылки http://www.adass.org/adass/proceedings/adass96/llebariaa2.html -- 12.0 Кб -- 23.06.1998
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>1850) - www.adass.org/ )
Астронет | Научная сеть | ГАИШ МГУ | Поиск по МГУ | О проекте | Авторам
Комментарии, вопросы? Пишите: info@astronet.ru или сюда