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• http://zebu.uoregon.edu/~uochep/talks/talks05/trackrecon.pdf
• http://zebu.uoregon.edu/1998/es202/calif.html
• Means and Deviations

... Insert date: . Day: . Month: . ... This CGI -script calculates a day of week of the given date, Julian date of Greenwich noon JD and extracts from the database indices of solar activity: Wolf number for the day W , monthly W m and yealy means W y of Wolf number for month and year of the date. The prediction of Wolf number (which was made in 1998 and, hence, lost actuality) is also presented. The database uses solar activity data got from server of National Geophysical Data Center . ...

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• Datafile structure

SIMPLE = T / file does conform to FITS standard BITPIX = -32 / number of bits per data pixel NAXIS = 2 / number of data axes NAXIS1 = 1138 / length of data axis 1 NAXIS2 = 1114 / length of data axis 2 TELESCOP= 'UT1 ' PI-COI = 'C. Cesarsky' / Name of PI and COI ORIGIN = 'ESO/EIS ' / Data processed by RA = 53.0917713808546 / RA (J2000) at start (deg). ... RADECSYS= 'FK5 ' / Coordinate reference frame. ... TOT-IMAG= 125 / Total number of images. ... MOSTILES= 21 / Total number of tiles in MOSAICID. ...

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• ST-ECF Staff
• ADASS '97 Program Information
• SLITLESS (Oct97) --- ST_ECF --- SLITLESS (Oct97)

SEVENTEENTH CREW REQUIRED RESOURCES FOURTEENTH RUSSIAN VISITING CREW KAP PROJECT IMAGE VIDEO . ... EXPEDITION SIXTEEN (ISS-17) . ... During ISS-17, 182 sessions of 34 experiments are planned to be implemented. ... Breakdown of Experiments and Number of Sessions by Research Areas . Research Area . Experiment Name . Totally . ... Ascent to ISS RS: by Soyuz TMA-12 . ... ISS-17 Crew Commander S.A. Volkov (Russia) . ... RECORDING AND TRANSFER OF SCIENTIFIC DATA TO PRINCIPAL INVESTIGATORS . ...

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Next: System configuration Up: How to use CONSTRICTOR Previous: Preparation of parameter file Contents . ... DayNumber: Even though this number is in the data, some packet headers have the wrong number and it makes it a whole lot easier to have the user check and enter this number correctly. ... CONSTRICTOR will add a multiple of 24 hours to the time tag when the day number changes. Remember to set the StopTime to, say, 48 hours if you use a DayNumber of one less than the actual day number. ...

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• ESO - A number of OmegaCAM filters show vignetting in their central regions.
• OYSTER Lab
• A visual tour

For calculating model spectra of early-type helium stars in LTE, we maintain a database of atomic data for, mostly, blue-visual absorption lines of light elements. The data is sorted with one file for each ion. ... III = ++ . ... It will work on both complete linelists (including the atomic data at the start and references at the end) or raw ion files (such as Ni2.d). ... A Fortran utility to convert linelists downloaded from the Vienna Atomic Line Database into the new QUB format. synspec_qub . ...

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• Armagh Observatory
• IAJ: Contents - Volume 24 Number 1
• IAJ: Contents - Volume 24 Number 2

This page should contain a form to pass parameter value for a program producing figures illustrating the dependence of optical properties of different scatterers on their parameters. Specify the parameters and press start calculation button to produce a figure. ... Independent variable: x v a/b alpha Re(m)? another? ... Number of curves: 1 2 3 . ... Curve #1: . Particle shape: sphere spheroid another? TE/TM mode: TE TM . Other parameters: x= Re(m)= Im(m)= a/b= alpha= . ...

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• Database of Optical Constants -- Misc: computer codes
• Model realization and some results
• MBOLS: Access/Search

... The main periodicity in the Sun 's activity is the 11-year cycle called the solar cycle. ... During the cycle, changes occur in the Sun's internal magnetic field and in the surface disturbance level. ... At the beginning of a cycle the solar magnetic field resembles a dipole which axis is aligned with Sun's rotation axis. ... The sunspot number - and Sun's activity - is at maximum in the middle of a cycle, when the Sun's internal magnetic field is most chaotic. ... Space Physics Text Book of Oulu ...

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• Formulas
• The Lagrangian Point L1
• Plasma theories [Oulu]

Until recently Supernova Catalogue was stored as s filebased system. The data on SNe were connected with the data on their host galaxies in the main file of the catalogue: each string presented data on SN and on its host galaxy. ... The information on these host galaxies is presented in several lines, corresponding to each SN. ... Different galaxy catalogues can be used as source of data on SNe host galaxies, that is why the table "map" was created. ... SAI SN group | Catalogue Home | ...

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• Open Source Convention
• Torsten Martinsen's GIMP plug-ins
• Презентация PowerPoint

God Science Forum Message . Forums: . ... God and Science ћ SETI ћ Software ћ UFO ћ XEphem . ... Discussion Forums | God and Science | ... Nothing? Beyond Numbers.. Forum List | ... You do not know your future; yet it feels as if it is ALREADY known. ... 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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• How Do You Feel About Numbers? - an Astronomy Net Exploration Forum Message
• A Number Is A Very Specific Thing - an Astronomy Net Exploration Forum Message
• The Telescope's F/number - an Astronomy Net General Forum Message

Astro Space Center RadioAstron Newsletter Number 17 October 26, 2012 ====================== The process to select projects for the open RadioAstron observing time within the AO-1 period (July 2013 - June 2014) has started From the middle of 2013 RadioAstron will move to the open sky phase of its science operations. Any scientist in the world can apply for the RadioAstron observing time. ... An initial Letter of Intent (LoI) should have been directed to the Mission by 17 October 2012. ...

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• GOCG Pre-Observation Products
• Kurt Vladimir, ASC

... INTRODUCTION This data set contains fluxes and pitch angles (relative to measured magnetic field) of protons and electrons as measured in the lower half of the energy steps of the electrostatic analyzers, that is, at "<10 ev," 40 eV and 0.76 keV, 60 eV and 1.2 keV, and 100 eV and 1.8 keV. ... In the data files the values of the particle number flux is given in the data columns in units: particles per square cm per second per steradian per keV. ... FILES AND FORMAT DESCRIPTION 3.1. ...

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• The Lagrangian Point L1
• Identities
• Elements of Algebra

... In the set of letters below (which you may wish to copy onto a separate sheet far distribution to the class) are hidden a significant number of astronomy related words. ... O P L S C M T M Suggested Scoring: 25 words = Observatory S M A U R E V I Director 21 words = Astrophysics T I B T N Y T Q Professor 15 words = Assistant D E P E O A U P Professor 11 words = Graduate I P R O M R S L Student 9 words = Night J U N I D A T A Assistant Puzzle (c) 1980 Dennis Schatz . ...

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• ASP: Project ASTRO History & Evolution
• ASP's 2012 Annual Meeting
• ASP: Black Holes to Blackboards: The Sun is a Mass of Incandescent Gas

... The words are numbered according to the reference mentioned above. ... 59 WORD wSecond ; // 0 .. 59 satellite tracking start time (GMT) float fStep ; // reserved WORD wMass ; // reserved BYTE reserved [12] ; // reserved WORD wExtraBytes ; // reserved } TRAJECTORYHEADER ; NOTE: the satellite tracking start time is a hardware operating start time to follow satellite. typedef struct { // ephemeris at satellite tracking start time double time ; // Epoch time (yyddd.ddddddddd)...

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• http://smis.iki.rssi.ru/partners/esharkov/preface.doc
• Myasnyankin Andrey , Moscow Institute of Physics and Technology (MIPT),Space
• Matyushkin Evgeny, Space Research Institute (SRI)

... They were determined as a result of orbit improving on the base of all kinds of optical observations available in the catalog of observations of the Minor Planet Center on March 16, 2014 (radar observations have not been used at this stage). ... As the MPC orbits do not all were improved simultaneously with EMP orbits, only 383866 sets of elements were used for data comparison (for selected sets of elements process of improvement had started with the use of the same observations). ...

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• ENGAMPLE
• Head Litter of Minor Planet Names
• Information for Authors of Articles

. Computer Ephemeris. Lunar eclipse numerical map. Explanations. First portion of the page contains coordinates of sub-lunar points during the eclipse. Every point is represented with two numbers: geodetic longitude and geodetic latitude, both in degrees. Second portion of the page contains coordinates of the points at terminator line for the moments of contacts. There are 360 points on the lines, tens of them per line. The starting angle is indicated in the leftmost column.

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• Explanations to tables for transformation from sidereal to universal time.
• Explanation to tables for transformation from universal to sidereal time.

... 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) . ...

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• Tools (ImageJ API)
• Line (ImageJ API)
• Interpreter (ImageJ API)

from numarray import * from numarray.random_ array import * size = 8640 # Number of observations flare = 1.1 # Size of flare counts = 1208*4*4 # Number of counts in the absence of a flare threshold = 0.97 # Threshold of mean flare flux at which you claim a flare . seed() # start up the random number generator photons = poisson ( counts ,[ size ]) # set up poisson noise ...

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• http://www.mso.anu.edu.au/~fbriggs/WAARNEEM/box.sm
• Research Interests
• Mach-numbers in a simulation of convection in the sub-giant Eta Boo

New reduction of minor planets photographic plates obtained with Pulkovo Normal Astrograph A.A. Berezhnoy Pulkovo Observatory of RAS, Saint-Petersburg, Russia Minor Planet observations at Pulkovo Periodical observations of 14 bright asteroids named Selected Minor Planets (SMP) were performed at Pulkovo since 1948 within the international framework started by works of B.V. Numerov and D. Brouwer. ... 108 133 113 74 124 67 97 88 14 84 64 5 20 19 Epochs (YYYY.MM) 1200 Mean values of total obs. ...

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• The Pul-3 astrometric catalogue (Second edition). Data access form.
• The Pul_ERS astrometric catalogue. Data access form
• Pul_ERS

... ACQMODE Acquisition mode AIRMASS Air mass for current object observation BIASSEC OVERSCAN AREA BITPIX Number of bits per data pixel BSCALE Default scaling factor: REAL = TAPE*BSCALE + BZERO BZERO Offset data range to that of unsigned short CALIB Calibration CCD-TEMP CCD temperature at start of exposure in C COMMENT Comment text DATATYPE Data type DATE File creation date (YYYY-MM-DDThh:mm:ss UTC) DATE-OBS YYYY-MM-DD observation start date, UT DEC OBJECT DEC, deg:arcmin ...

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• Zeldovich-100 / International Conference / Moscow, Russia
• RTT150 Technical Description
• Second Spectrum-RG/eROSITA Conference