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http://www.atnf.csiro.au/computing/software/gipsy/tsk/wfits.dc1.

1. Package: vc
... unsigned int vc_alloc_colours (unsigned int num_cells, unsigned long *pixel_values, unsigned int min_cells, Kdisplay dpy_handle) . ... num_cells : The number of colourcells to store. pixel_values : The array of pixel values. reds : The array of red intensity values. greens : The array of green intensity values. blues : The array of blue intensity values. stride : The stride (in unsigned shorts) between intensity values in each array. dpy_handle : The low level display handle. ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/karma/lib/vc.html -- 9.1 Кб -- 24.12.2007
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2. block, table and array
... Meta Index / Home Page / Parameter types . Table parameters and array parameters allow a block (generic name of a table or array) and its associated dataset to be specified by a single parameter, using a colon-separated pair of the form set:table or set:array . Block parameters are used where the value may be either a table or an array. ... foo.FIT:R1SPE1 # Table R1SPE1 in set foo.FIT /data/bar.FIT:FILTER_U # Array FILTER_U in array bar.FIT . ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/8.0.0/doc/param/node11.html -- 3.9 Кб -- 01.07.2008
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3. generate_ramp.pro (JWST Pipeline routines in IDL)
... use frames summary class fields routine details file attributes . GENERATE_RAMP , time , ramp , SEED= SEED . add_cosmic_rays , CRMAP , MODE= MODE , CRPATH= CRPATH , SEED= SEED . GENERATE_DATACUBE , time , ramp , SEED= SEED , Ngroups= Ngroups . FIND_CR , CR_found . analysis , CR_found . ... time . ramp . SEED . Lines: . 50 lines . ... CR_found . ... idl verbatim . ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/~robberto/Main/Software/IDL4pipeline/generate_ramp.html -- 14.4 Кб -- 27.02.2014
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4. http://www.arcetri.astro.it/irlab/doc/library/javascript/clientreference/history.htm
... JavaScript 1.1: added current, next, and previous properties. ... To change a window's current URL without generating a history entry, you can use the Location.replace method. ... For example, if the history list contains three named entries, these entries are reflected as history[0] , history[1] , and history[2] . ... back . ... onClick="history.go('home.netscape.com')"> The following button navigates to the URL that is three entries backward in the history list: <P><INPUT TYPE="button" VALUE="Go" ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/irlab/doc/library/javascript/clientreference/history.htm -- 22.9 Кб -- 07.10.1999
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5. Calculation of errors in smoothed arrays
... Errors may be traced during the smoothing process. An error array must first be generated. This example takes errors from the same region of the original QPOE file. xs> errcreate ``xdata$rp110590.qp[6830:7029,9290:9489]'' rp90ab_err.imh # The error file is rp90ab_err.imh # The ``'' on the command line prevent IRAF's confusion with a long argument . ... errors = yes errarray = (filename of unsmoothed error array) error_out = (filename of output error array) . ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/PROS/PUG/node110.html -- 3.9 Кб -- 01.10.2012
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6. Maximum limits
... The planning and reduction programs are distributed with array sizes set large enough to let most observers work without difficulty. However, you might need to reduce a very large data set, or to deal with a very large number of passbands (9 is the nominal limit). ... The main problem is holding the matrix of normal equations during the iterations; on the other hand, star catalogs can be made quite large without paying much of a price in terms of performance. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Midas_doc/doc/94NOV/vol2/node315.html -- 6.8 Кб -- 23.02.1996
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7. exchange.h File Reference
Main Page Data Structures File List Data Fields Globals . ... Go to the source code of this file. struct . ... Data for OI_ARRAY FITS table. ... write_oi_array (fitsfile *fptr, oi_array array, int extver, int *status) . ... Data for OI_ARRAY FITS table. typedef struct _target target . ... Data for OI_TARGET FITS table. typedef struct _oi_wavelength oi_wavelength . Data for OI_WAVELENGTH FITS table. typedef struct _oi_vis_record oi_vis_record . ... fptr , . ... array data struct, see exchange.h . ...
[ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/~jsy1001/resources/exchange/html/exchange_8h.html -- 42.5 Кб -- 07.04.2003
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8. Enhanced HST Pointing and Calibration Accuracy: Generating HST Jitter Files at
Next: HST Paper Products: A New Way to Look at HST Data . ... After providing on-the-fly re-calibration of HST data to archive users, ST-ECF has embarked on a new project aiming at grouping, cosmic ray cleaning and drizzling images taken by most HST instruments. ... The production of the missing jitter files combined with the extraction of additional engineering parameters will greatly enhance the homogeneity and the scientific value of the entire archive. ... 1995, HST Data Handbook, STScI, 107 . ...
[ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/dolenskym1.html -- 9.4 Кб -- 12.06.2006
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass97/dolenskym1.html -- 9.4 Кб -- 15.05.1998
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9. Cosmological Issues for Theorists
. ___________________________________________________________________ The Electronic Universe Project e-mail: nuts@moo.uoregon.edu
[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/cosmo.html -- 6.5 Кб -- 19.04.1999
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10. Cray
Fortran 90 properties already in CF77 . ... Only the old form (fix form) of the source code is available. ... LOGICAL Default KIND number = 8 INTEGER Default int7 int15 KIND number = 6 1 2 digits = 46 7 15 radix = 2 2 2 range = 13 2 4 huge = 70368744177663 127 32767 bit_size = 46 8 16 INTEGER int31 int46 int64 KIND number = 4 6 8 digits = 31 46 63 radix = 2 2 2 range = 9 13 18 huge = 2147483647 70368744177663 9223372036854775807 bit_size = 32 46 46 REAL half Default,single double KIND ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/f77to90/cray.html -- 11.0 Кб -- 24.10.1996
[ Сохраненная копия ]  Ссылки http://crydee.sai.msu.ru/f90/cray.html -- 11.0 Кб -- 24.10.1996
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11. SCL Sfit Genetic Commands
... sfit . ... commands . scl . ... Define parameters for controlling performance of genetic algorithm . ... generations . The maximum number of generations the program will go through, before stopping, if the solution is not within the given tolerance. 10 . ... The number of parents randomly generated in the first generation, and in each subsequent generation. 50 . ... This is multiplied by the number of parameters being varied to give the total string length for each parent. 16 . ... elitism . ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/~csj/software_store/guide/scl_gen.html -- 7.9 Кб -- 30.08.2007
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12. http://www.ssau.ru/files/science/conferences/itnt2015/itnt_2015_70.pdf
TOOLS OF TEST GENERATION FOR SATELLITES CONTROL PROGRAMS Andrey Tyugashev, Ekaterina Myasnikova, Elena Sopchenko S.P. Korolyov Samara State Aerospace University (National Reseach University) The paper presents a research in the field of test automation for testing spacecraft control programs. ... Programmers or designers of spacecraft systems write tests manually. ... Tests are carried out by issuing the control actions on the spacecraft and condition monitoring systems parameters of the spacecraft. ...
[ Текст ]  Ссылки http://www.ssau.ru/files/science/conferences/itnt2015/itnt_2015_70.pdf -- 161.6 Кб -- 04.08.2015
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13. Project 5 - State Program "Condenced Matter Physics"
... The Russian Federation State Program "Physics of Condenced Matter", the "Superconductivity" division , Project code "Generation-2" . ... The multielement josephson structures are known to allow implementation of the unique properties of the Josephson junctions as electromagnetic waves sources with high change rate of generation frequency, working in the millimeter and submillimeter wavelength diapasones. ... Even the optimal type of the junction electrodynamic interconnection isn't chosen. ...
[ Сохраненная копия ]  Ссылки http://www.cplire.ru/html/oxide233/proj5.html -- 7.9 Кб -- 01.09.2005
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14. http://www.naic.edu/~tghosh/software/gauss.pro
Viewing contents of file ;'/net/www/deutsch/idl/idllib/jhuapls1r/usr/gauss.pro' ; ;------------------------------------------------------------- ;+ ; NAME: ; GAUSS ; PURPOSE: ; Return a fitted gaussian curve for a given histogram. CATEGORY: ; CALLING SEQUENCE: ; fit = gauss(x,h) ; INPUTS: ; x = array of histogram bin center values. in ; h = histogram array. in ; KEYWORD PARAMETERS: ; Keywords: ; MEAN=mn returned histogram mean. SDEV=sd returned histogram standard deviation. ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~tghosh/software/gauss.pro -- 3.4 Кб -- 24.01.2003
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15. Preparation of parameter file
Next: Parameters Up: How to use CONSTRICTOR Previous: NPOI raw data files Contents . The parameter file contains information for CONSTRICTOR on the location of the raw data files, start and stop times, integration time, etc. ... The parameter file, YYYY-MM-DD.par , can now be created using the rawlist procedure of . ... Check beginning and tail of the listing for each file. ... Next: Parameters Up: How to use CONSTRICTOR Previous: NPOI raw data files Contents Christian Hummel 2015-04-28 ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/~chummel/oyster/manual/node228.html -- 6.1 Кб -- 28.04.2015
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16. Stellarium: Extinction Class Reference
... Extinction Class Reference . ... voidљ . forward (const Vec3d *altAzPos, float *mag, const int num=1) const . ... forward (const Vec3f *altAzPos, float *mag, const int num=1) const . ... forward (const double *sinAlt, float *mag, const int num) const . ... forward (const float *sinAlt, float *mag, const int num) const . ... forward (const double *sinAlt, float *mag) const . ... forward (const float *sinAlt, float *mag) const . ... backward (const float *sinAlt, float *mag, const int num=1) const . ...
[ Сохраненная копия ]  Ссылки http://astro.uni-altai.ru/~aw/stellarium/api/classExtinction.html -- 15.3 Кб -- 28.02.2014
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17. what to do with the trace data
... Here is a sample parameter file that is set to plot the B filter trace data. ... One can generally get by with the default graph parameters. input = B.a list of images or list files to be graphed (wx1 = 3000.) left world x-coord if not autoscaling ... autoscaling (wy2 = 100.) upper world y-coord if not autoscaling (wcs = logical ) Coordinate system for images (axis = 1) axis along which projection is to be taken (transpose = no) transpose the x and y axes of the plot (pointmode = no) ...
[ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Instruments/filters/tracehelp.html -- 4.8 Кб -- 22.02.2001
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18. http://www.wdcb.ru/stp/data/geomagni.ind/pc/THULE/A_Readme/PCindex.txt
GEOMAGNETIC POLAR CAP (PC) INDEX The PC-index is a fifteen-minute index for magnetic activity in the (P)olar (C)ap. It is based on data from a single nearpolar station, and aimed to monitor the polar cap magnetic activity generated by such solar wind parameters as the southward component of the interplanetary magnetic field (IMF), the azimuthal component of the IMF (By), and the solar wind velocity (v). ... 1988), Vennerstrom (1991), and Vennerstrom et al. 1991). ...
[ Сохраненная копия ]  Ссылки http://www.wdcb.ru/stp/data/geomagni.ind/pc/THULE/A_Readme/PCindex.txt -- 2.7 Кб -- 17.03.2006
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19. CurveFitter (ImageJ API)
... public class CurveFitter . ... static int . ... Field Detail public static final int STRAIGHT_LINE . ... public static final int POLY2 . ... public static final int POLY3 . ... public static final int POLY4 . ... public static final int EXPONENTIAL . ... public static final int POWER . ... public static final int LOG . ... public static final int RODBARD . ... public static final int GAMMA_VARIATE . ... public static final int LOG2 . ... public static double f (int fit, double[] p, double x) . ...
[ Сохраненная копия ]  Ссылки http://www.astro.louisville.edu/software/astroimagej/imagej/api/ij/measure/CurveFitter.html -- 34.8 Кб -- 02.12.2010
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20. 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. ...
[ Сохраненная копия ]  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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