Поиск по:star.arm.ac.uk -
Поискать по всем серверам
На этой странице приведены все страницы сервера star.arm.ac.uk ,которые мы индексируем. Показаны документы 9041 - 9060 из 9197.
Упорядочить по:
URL
|
дате изменения
9041. http://star.arm.ac.uk/~ambn/rad_losses.ps
A&A manuscript no. (will be inserted by hand later) Your thesaurus codes are: 02.01.2; 02.12.1; 06.20.1; 06.21.1; 08.01.3; 08.12.1 ASTRONOMY AND ASTROPHYSICS 1.4.1996 Estimating the total radiative power output from the hot outer layers of lateґtype stellar atmospheres: How many lines are required? J.G. Doyle Armagh Observatory, College Hill, Armagh BT61 9DG, N. Ireland email: jgd@star.arm.ac.uk Received date, accepted date Abstract. ...
[
Текст
]
Ссылки http://star.arm.ac.uk/~ambn/rad_losses.ps -- 491.9 Кб -- 18.09.1996
Похожие документы
Похожие документы
9042. Yurij Shokin
Professor Yurij Shokin, born 1943, has been many years with the Computer Center and the Institute of Theoretical and Applied Mechanics (during the directorship of Academician N N Yanenko ) in Novosibirsk's scientific campus Akademgorodok and was director of the computer centre of the Soviet Academy of Sciences, Siberian Division, in Krasnoyarsk. ... He is an affiliate member of IFIP WG 2.5 and a member of the Russian Academy of Sciences. ... Russian Academy of Sciences . Siberian Division . ...
[
Сохраненная копия
]
Ссылки http://star.arm.ac.uk/f77to90/yurij.html -- 3.7 Кб -- 11.09.1996
Похожие документы
Похожие документы
9043. http://star.arm.ac.uk/~ambn/abstract223.html
We show that the flux distribution of a wind from a cool star differs considerably from what is predicted by the theory for mass loss from hot stars. ... These differences result in substantial modifications of the flux distribution and imply that care must be exercised when applying the flux predictions by e.g. Wright and Barlow (1975) to winds from cool stars. By using observational constraints we show that the mass loss from cool dwarf stars equals at most 10E-12 solar masses per year. ...
[
Сохраненная копия
]
Ссылки http://star.arm.ac.uk/~ambn/abstract223.html -- 2.6 Кб -- 10.09.1996
Похожие документы
Похожие документы
9044. http://star.arm.ac.uk/~ambn/mass_loss.ps
A&A manuscript no. (will be inserted by hand later) Your thesaurus codes are: 08(08.12.1;08.13.2;09.07.1;13.09.6;13.18.5;13.21.5) ASTRONOMY AND ASTROPHYSICS 4.9.1996 Constraints on mass loss from dMe stars: theory and observations G.H.J. van den Oord 1 and J.G. Doyle 2 1 Sterrenkundig Instituut, p.o. box 80.000, 3508 TA Utrecht, The Netherlands 2 Armagh Observatory, Armagh BT61 9DG, N. Ireland Received ;accepted Abstract. ... Constraints on mass loss from dMe stars: theory and observations Fig. ...
[
Текст
]
Ссылки http://star.arm.ac.uk/~ambn/mass_loss.ps -- 398.5 Кб -- 10.09.1996
Похожие документы
Похожие документы
9045. The historical development of Fortran
... Fortran . ... The final example shows the program in the new programming language F. program tpk(input,output); (* Pascal program for Unix *) var i : integer; y : real; a : array [0..10] of real; function f (t : real) : real; begin f := sqrt(abs(t)) + 5*t*t*t end; begin for i := 0 to 10 do read(a[i]); for i := 10 downto 0 do begin y := f(a[i]); if y > 400 then writeln(i,' TOO LARGE') else writeln(i,y); end end. ... C THE TPK ALGORITHM C FORTRAN IV STYLE DIMENSION A(11) FUN(T) = SQRT(ABS(T)) + 5.) ...
[
Сохраненная копия
]
Ссылки http://star.arm.ac.uk/f77to90/a7.html -- 14.1 Кб -- 05.09.1996
Похожие документы
Похожие документы
9046. Program units
In addition to the four old program units: PROGRAM (that is the main program), SUBROUTINE, FUNCTION and BLOCK DATA , the new concept MODULE has been added, as well as some new things in the old units. ... POSITIVE NUMBERS ASSUMED TYPE(INTERVAL), INTENT(IN) :: A, B TYPE (INTERVAL) :: INTERVAL_MULTIPLICATION INTERVAL_MULTIPLICATION%LOWER = A%LOWER * B%LOWER INTERVAL_MULTIPLICATION%UPPER = A%UPPER * B%UPPER END FUNCTION INTERVAL_MULTIPLICATION FUNCTION INTERVAL_DIVISION(A, B) ! ...
[
Сохраненная копия
]
Ссылки http://star.arm.ac.uk/f77to90/c7.html -- 11.4 Кб -- 30.08.1996
Похожие документы
Похожие документы
9047. http://star.arm.ac.uk/f77to90/code/intv_ari.f90
MODULE INTERVAL _ARITHMETICS TYPE INTERVAL REAL LOWER , UPPER END TYPE INTERVAL INTERFACE OPERATOR (+) MODULE PROCEDURE INTERVAL_ADDITION END INTERFACE INTERFACE OPERATOR (-) MODULE PROCEDURE INTERVAL _SUBTRACTION END INTERFACE INTERFACE OPERATOR (*) MODULE PROCEDURE INTERVAL_MULTIPLICATION END INTERFACE INTERFACE OPERATOR (/) MODULE PROCEDURE ...
[
Сохраненная копия
]
Ссылки http://star.arm.ac.uk/f77to90/code/intv_ari.f90 -- 2.8 Кб -- 30.08.1996
Похожие документы
Похожие документы
9048. http://star.arm.ac.uk/f77to90/code/intv.f90
USE INTERVAL_ARITHMETICS IMPLICIT NONE TYPE (INTERVAL) :: A, B, C, D, E, F A%LOWER = 6.9 A%UPPER = 7.1 B%LOWER = 10.9 B%UPPER = 11.1 WRITE (*,*) A, B C = A + B D = A - B E = A * B F = A / B WRITE (*,*) C, D WRITE (*,*) E, F END
[
Сохраненная копия
]
Ссылки http://star.arm.ac.uk/f77to90/code/intv.f90 -- 1.3 Кб -- 30.08.1996
Похожие документы
Похожие документы
9049. http://star.arm.ac.uk/~ambn/abstract215.html
The calculated flux distribution in the 300 to 400 nm region only fits the observed distribution closely for both the Sun and Arcturus when the complete ATLAS9 line list is used. ... Moreover, for Arcturus, even the sub-set of high quality lines can only provide a close fit to the observed high resolution spectrum if we include, ad hoc, an extra amount of continuous absorption opacity. ...
[
Сохраненная копия
]
Ссылки http://star.arm.ac.uk/~ambn/abstract215.html -- 1.9 Кб -- 28.08.1996
Похожие документы
Похожие документы
9050. http://star.arm.ac.uk/~ambn/ian_paper.ps
... Flux observed by Neckel and Labs: solid line (! 360 nm), dotґdashed line (? 330 nm), synthetic flux computed with: G list: triangles, PA list: squares, PM list: crosses. ... Griffin atlas: solid line , synthetic spectrum computed with: G list : dotted line , PA list : short dashed line . -- 19 -- 300 310 320 2e6 4e6 320 330 340 2e6 4e6 6e6 Physical Flux (ergs sec ґ1 cm ґ2 A ґ1 ) 340 350 360 370 2e6 4e6 6e6 8e6 370 380 390 400 2.e6 4e6 6e6 8e6 Wavelength (nm) -- 20 -- 300 310 320 ...
[
Текст
]
Ссылки http://star.arm.ac.uk/~ambn/ian_paper.ps -- 1830.2 Кб -- 28.08.1996
Похожие документы
Похожие документы
9051. http://star.arm.ac.uk/~ambn/mnras1.ps
... 000, 000--000 (0000) Printed 20 August 1996 (MN L A T E X style file v1.3) Lithium abundance in field K and M dwarfs M. Zboril 1? P.B. Byrne 1 , W.R.J.R. Rolleston 1;2 1 Armagh Observatory, Armagh, College Hill, BT61 9DG, N. Ireland 2 Queens University, Belfast, N. Ireland 20 August 1996 ABSTRACT It is widely accpted that lithium abundance in lateґtype stars correlates with other stellar characteristics, such as age, chromospheric activity and rotation. ... This is not evident in the M stars. ...
9052. Fortran 90 systems
This appendix only contains links to pages describing various Fortran 90 systems. ... Fujitsu Fortran 90 Compiler (Fujitsu WWW) . Fujitsu Fortran 90 Compiler (Unicomp WWW) . ... Fortran PowerStation 4.0 from Microsoft . Lahey Fortran 90 from Lahey Computer Systems , Nevada, USA . ... An additional compiler will be available from Absoft towards the end of 1996. ... Lahey LF90 v2.0 from Lahey Computer Systems, PO Box 6091, Incline Village, NV 89450-6091, USA, Email: sales@lahey.com . ...
[
Сохраненная копия
]
Ссылки http://star.arm.ac.uk/f77to90/a6.html -- 4.0 Кб -- 20.08.1996
Похожие документы
Похожие документы
9053. Fortran 95
... 17.1 New features . ... Pure procedures . ... A function NULL to nullify a pointer . ... Complete version of END INTERFACE Pure functions are functions without side effects, and elemental functions are pure functions with only scalar arguments and with scalar result. ... Elemental functions are pure functions with only scalar dummy arguments (not pointers or procedures) and with scalar result (not pointer). That a function is elemental can be indicated with the new ELEMENTAL prefix. ...
[
Сохраненная копия
]
Ссылки http://star.arm.ac.uk/f77to90/f95.html -- 15.4 Кб -- 20.08.1996
Похожие документы
Похожие документы
9054. Fortran 90 for the Fortran 77 Programmer, Index page
1993 and 1996, Bo Einarsson and Yurij Shokin . The tutorial has now been modified so that it either can be used directly via the network or downloaded for installation on a Unix computer, a PC running Windows 3.1 or Windows 95, or an Apple Macintosh. Main page, with links to all other pages is f77to90.html. ... Computer Exercises . ... The Russian version is available as a regular book. The textbook in Swedish on Fortran 90 is available both interactively and as a printed book. ...
[
Сохраненная копия
]
Ссылки http://star.arm.ac.uk/f77to90/ -- 3.0 Кб -- 20.08.1996
[ Сохраненная копия ] Ссылки http://star.arm.ac.uk/f77to90/index.html -- 3.0 Кб -- 20.08.1996
Похожие документы
[ Сохраненная копия ] Ссылки http://star.arm.ac.uk/f77to90/index.html -- 3.0 Кб -- 20.08.1996
Похожие документы
9055. SunSoft
... SPARCompiler(TM) Fortran 90 1.0 . FORTRAN 77 3.0.1 . ... important of these. -ansi: Report non-ANSI extensions. -c: Suppress linking, produce .o files -e: Recognize extended (132 character) source lines -fast: Specify common set of performance options - fixed : Interpret all Fortran source files according to fixed form rules -flags: Print summary of compiler options -fnonstd: Non-standard initialization of floating-point hardware -fnonstop: Execute without trapping on invalid, overflow ...
[
Сохраненная копия
]
Ссылки http://star.arm.ac.uk/f77to90/sun.html -- 7.6 Кб -- 20.08.1996
Похожие документы
Похожие документы
9056. NASoftware
NASoftware Limited Roscoe House 62 Roscoe Street Liverpool L1 9DW England marketing@nasoftwr.demon.co.uk Tel: +44 151 709 4738 Fax: +44 151 709 5645 Fortran 90 Plus is available for many computer systems, including PC (DOS, OS/2 and Windows NT), SPARC, and Transputers (T800 and 9000). They claim to have enhanced numeric capabilities, increased array functionality, standard extensions to Fortran 77, and support for in-house standards. Back to Appendix 6 . Last modified: 18 July 1996 . boein@nsc.liu.se
[
Сохраненная копия
]
Ссылки http://star.arm.ac.uk/f77to90/nas.html -- 2.0 Кб -- 20.08.1996
Похожие документы
Похожие документы
9057. Steven Fox
. Last Revised: 23 Jul. 1996 . WWW contact: webmaster@star.arm.ac.uk . Go to HOME Page
[
Сохраненная копия
]
Ссылки http://star.arm.ac.uk/staff/steven.html -- 1.6 Кб -- 16.08.1996
Похожие документы
Похожие документы
9058. http://star.arm.ac.uk/~ambn/abstract183.ps
The photosphere and chromosphere of the RS CVn star, II Peg. ... At the first epoch we have observed the three chormospheric lines, Hff, Hfi and HeI D 3 , over a single rotation and at the second epoch we observed almost the entire visible region, for a substantial fraction of one rotation, including HffґHffl and CaII H. Our photometric results show that there was an unusually complicated spot distribution at this epoch, with at least three centres of activity discernable. ...
[
Текст
]
Ссылки http://star.arm.ac.uk/~ambn/abstract183.ps -- 35.3 Кб -- 16.08.1996
Похожие документы
Похожие документы
9059. http://star.arm.ac.uk/~ambn/abstract184.ps
Theorectical emission line strengths for Ne VI compared to EUV solar observations F.P. Keenan, V.J. Foster, R.H.G. Reid. ... Electron temperatures and densities derived from ratioґratio diagrams involving the 562.7, 997.4, 999.6 and 1006.1 A lines, in conjunction with observational data for a sunspot obtained with the Harvard Sґ055 spectrometer on board Skylab, are found to be compatible, and in good agreement with plasma parameters determined using other methods. ...
[
Текст
]
Ссылки http://star.arm.ac.uk/~ambn/abstract184.ps -- 28.0 Кб -- 16.08.1996
Похожие документы
Похожие документы
9060. http://star.arm.ac.uk/~ambn/abstract185.ps
BV (RI)KC CCD photometry of the core of the young open cluster, NGC5460 D. Barrado and P.B. Byrne We present CCD photometry on the BV(RI)KC (Cape) photometric system of the core of the young open cluster, NGC5460, to a magnitude limit V ъ 19, R ъ 19.5. We give photometry for 353 stars 1 and identify 25 as cluster members along with a further 27 as possible members based on their positions in individual colourґmagnitude diagrams. ...
[
Текст
]
Ссылки http://star.arm.ac.uk/~ambn/abstract185.ps -- 26.8 Кб -- 16.08.1996
Похожие документы
Похожие документы