To construct frequency distribution (histogram) of minor planets according to value of some element/ parameter/ function user should first select Elements item in menu bar and then Histogram in drop-down menu. ... User has possibility to save histogram or to print it using standard means. To save the file select File item in menu bar and then Save As... in drop-down menu. ... To print histogram select File item in menu bar and then take advantage of options Print Preview , Print Setup , Print . ...

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• Keywords_262
• Keywords_128
• Keywords_330

Modified 11 April 1999. The last modifications concerns to the new ground tracks selection on the base of the more wide list of the INSPIRE particpants. ... The range value was changed from 2 deg to 4 deg for the distance between lat/lon of the graund track and place of the INSPIRE members. Plots of predicted tracks under USA and Europe 11 April 1999 . April, 17, 1999 (USA) . April, 17, 1999 (EUR) . ... 11 April 1999 . ... place . ... Back to the IKI Satellite Situation Center (SSC) . ...

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• DOK-2 Results Page
• Lagrangian Points
• Multipoint correlations of the solar wind parameters observed by several

. You can check for and then change your current directory on the local host using the lcd command. For example: ftp> lcd Local directory now /u/user/eucs/eucs99 ftp> lcd REPORTS Local directory now /u/user/eucs/eucs99/REPORTS . Here, you have changed to your current directory and then moved to the subdirectory REPORTS .

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• Removing a command alias
• Changing transfer authorisation for a host
• Index: P

L1 Simulation Upgrade December 6th, 2004 BaBar Collaboration Meeting SLAC Eric Torrence University of Oregon Eric Torrence 1/15 December 2004 Phase 0 (Now) DchDigis EmcDigis EmtSim trgDC L1Accept This IS the current SP6 (14.4.X) Base simulation code unchanged, but interface elements are updated (Digis, TsfLUT) Remaining changes are inside black blob Eric Torrence 2/15 December ... Done · L1DZpdTrackDigi - cellLocation and cellPhi are not currently being simulated. ...

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• http://zebu.uoregon.edu/1998/ph101/mtr1.html
• Astronomy 123 Spring 1996
• Current Weather Conditions

The absorption of MHD waves due to the cusp (or the slow) resonance is studied numerically and the obtained results are discussed with respect to a possible application to conditions that are typical for the solar corona. The considered configuration is composed of two homogeneous regions separated by an inhomogeneous slab through which all physical parameters of the medium change continuously according to an initially prescribed distribution. ...

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• http://star.arm.ac.uk/preprints/2010/571d_OnlineII.pdf
• Armagh Observatory
• Making backups with tar

... The concept of continuous solar wind developed in 1950's. First, Biermann (1951, 1957) observed comet tails as they passed close to the Sun , and explained the observed tail deflection by a continuous flux of protons from the Sun. Then Parker (1959) showed that the solar corona must expand, and called the outward streaming coronal gas 'solar wind'. ... The expanding solar wind drags also the solar magnetic field outward, forming what is called the interplanetary magnetic field (IMF) . ...

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• ENERGETIC PARTICLE EXPERIMENT DOK-2
• INTERBALL-TAIL KP changes
• Parallax

... Up: Data Processing Systems . ... 314 Astronomical Data Analysis Software and Systems XIII, eds. F. Ochsenbein, M. Allen, & D. Egret (San Francisco: ASP), 800 . ... During early flight operation, the Chandra X-ray Observatory's Advanced CCD Imaging Spectrometer (ACIS) suffered degradation of charge transfer inefficiency (CTI) due to radiation induced charge trapping. ... We will discuss the impact of CTI on events, RMF and gain files. ... While ACIS reads out, it is still taking data. ...

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• Bias-Free Parameter Estimation with Few Counts, by Iterative Chi-Squared
• On the Need for Input Data Control in Pipeline Reductions
• Simulation of HST PSFs using Tiny Tim

Databases (NSDC) of the Natural Planetary Satellites. ... NSDC: Database of astrometric observations of Natural Planetary Satellites . ... They are thoroughly looking for observations in different sources, creating their owndatabases which are then mostly inaccessible to other researchers. ... In the file "content" with explications, the reference is given to the data source as well as the bibliographic reference. ... Data sources. ... Why a specific bibliographic database for Natural satellites? ...

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• IDL programs
• Manpage of FITSHDR_EDIT

Watching the Detective Although a lot is happening during the seasons, the facts seem to fit together. ... From these facts, we should be able to figure out the cause of the seasons. ... Facts 4, 5, and 8 indicate that the seasons have something to do with the Sun. ... Although the angle varies by the same amount at every latitude (see figure 4 ), the effect of this variation on solar heating increases with latitude, a fact you can confirm with a little trigonometry (see Geometry of the Seasons ). ...

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• ASP: What Have We Learned About Halley's Comet?
• ASP: This Restless Globe
• ASP: What If the Moon Didn't Exist?

... The change in the temperature dependence of the resistance, R ( T ), of ceramic YBa 2 Cu 3 O 7 - x as oxygen is removed from the sample has been studied. The superconducting transition temperature shifts progressively downward in the process. ... The temperature dependence of the resistivity, ( T ), is linear, with a progressively increasing slope, only at T > 400 K. It is suggested that oxygen condenses on Cu-O chains at T 400 K. PACS: 74.60.Mj, 74.70.Vy, 81.40.Rs, 72.80.Ga ...

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• http://www.issp.ac.ru/lsc/files/core_doped_1998.pdf
• http://www.issp.ac.ru/ls/Files/10345.ps
• http://www.issp.ac.ru/libm/papers/259.pdf

sw@newmail.ru THE PROBE LAYER METHOD IN THE CALCULATIONS OF CONTRIBUTION AND RESPONSE FUNCTIONS S.G.Mozharovsky Ussuriysk Astrophysical Observatory of FEB RAS, Ussuriysk, Russia sw@newmail.ru The method of probe layer for the calculation of response and contribution functions is discussed. ... This allows us to turn from the response functions to the contribution functions calculated with help of the probe layer (CFPL). ... V- VMAX . ... Solar Phys., v.136, p.239-250. ... Solar Phys., v.35, p.11-29. ...

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• http://www.uafo.ru/msg/zr_2014_08.doc
• http://www.uafo.ru/msg/6058_2014_06.doc

At the end of December 2004, the CCD was removed from the telescope and returned to Spectral Instruments in Tucson. The existing thick chip will be replaced with a thinned chip and the readout changed from 2-channel to 4-channel. ... Additional changes being made during this period include the installation of a compress air drier, collimating camera and cloud monitoring camera. Back to Recent News List . Siding Spring Survey Main Page . ... Follow-up Astrometry with the 1.0-m at SSO . ...

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• As piles of ash are removed, the courtyard has the top few cm of contaminated
• Roofing removed from walkways and outbuildings of main block.
• Removing the Farnham

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. ...

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• Optical static Fourier spectrometer
• Stellar Astronomy

The revision of the MASS/DIMM star catalogue N. Shatsky, V. Kornilov March 16, 2008 Abstract The compilation of the (updated) version of the MASS (MASS/DIMM) device target catalogue is described. ... Then the list was cleaned according to following criteria: I. Remove stars too faint for a MASS device. ... Here the color equation of the Sternb erg device was taken: M AS S mag = V mag + 0.45 (B - V ); stars with M AS S mag > 3.2 were removed. ... This was made based on the GCVS4.2 catalogue data. ...

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• http://curl.sai.msu.ru/mass/download/doc/res2007eng.pdf

Stellarium 0.12.3 . ... ScreenImageMgr Class Reference . ... createScreenImage (const QString &id, const QString &filename, float x, float y, float scale=1., bool visible=true, float alpha=1., float fadeDuration=1.) ... setImageAlpha (const QString &id, float alpha) . ... setImageXY (const QString &id, float x, float y, float duration=0.) ... virtual voidљ . ... the ID for the desired image. virtual void ScreenImageMgr::draw . ... the ID for the desired image. virtual void ScreenImageMgr::init . ...

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• Stellarium: StelButton Class Reference
• Stellarium: ShortcutsDialog Class Reference
• Stellarium: StelObjectMgr Class Reference

... Gravitational wave search provides insights into galaxy evolution and mergers . ... The double star 54 Leonis, spiral galaxy NGC 3198, and emission nebula NGC 3199 . ... Antennae Galaxies move closer . ... The Antennae Galaxies are among the closest known merging systems. ... The new, smaller distance makes the Antennae Galaxies less extreme in terms of the physics needed to explain the observed phenomena. ... Only registered members of Astronomy.com are allowed to comment on this article. ...

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• Planck steps closer to the cosmic blueprint | Astronomy.com
• Close encounters | Astronomy.com
• How close to each other do two stars have to be for one to steal material from

polimodel -- Produce model linear polarization and position angle images . ... Whether to apply random errors to output polarization and position angle values. seed = "" [integer] . ... This task produces a model linear polarization image and corresponding position angle image from an input image assumed to represent intensity (Stokes I parameter). ... A threshold for the input image can be defined such that polarization and position angle are not computed for input values less than this threshold. ...

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• Space Telescope-European Coordinating Facility
• ALIGNASN (Nov98) --- nictools --- ALIGNASN (Nov98)
• HSTPOLIMA (V1.00) --- April99 --- HSTPOLIMA (V1.00)

... Moon Shadow Moves Over Africa . ... When the Moon's shadow reached out and touched the Earth last week, the result was a solar eclipse. Such an eclipse is total only for observers located along a narrow path corresponding to the ground track of the shadow's dark central portion or umbra. ... Zimbabwe Solar Eclipse . ... On December 4th, for the second time in as many years, the Moon's shadow will track across southern Africa bringing a total solar eclipse to African skies. ... First page ] Prev. ...

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PHOTOMETRIC SEARCH FOR BLACK HOLES IN DORMANT X-RAY TRANSIENTS ґ ґ Aleksander Sadowski1 , Janusz Ziolkowski2 , and Krzysztof Belczynski3 ё Astronomical Observatory of Warsaw University, Al. ... Such definition means that our statistics for the number of expected BH X-ray binaries include both transient and persistent systems. ... If this value is 2 M , then, according to our calculations, Galaxy contains some 15 000 to 40 000 of BH X-ray binaries (and some 30 000 to 250 000 of NS X-ray binaries). ...

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• http://hea.iki.rssi.ru/conf/hea2007/bp-0.2.97/NOTES
• http://hea.iki.rssi.ru/integral06/papers/G06_Tsygankov01-22Jan07_11:45:59.pdf
• http://hea.iki.rssi.ru/integral06/papers/G31_Hjalmarsdotter03-17Apr07_14:14:42.pdf

... Astronomical Observatory, Shevchenko Park, Odessa, 65014, . ... The XVI -th G. Gamow's Odessa Astronomical Summer Соnference-School, 14-20 August, 2016, Odessa, Ukraine . ... The XV -th G. Gamow's Odessa Astronomical Summer Соnference-School, 16-23 August, 2015, Odessa, Ukraine . ... The XIV -th G. Gamow's Odessa Astronomical Summer Соnference-School, 17-23 August, 2014, Odessa, Ukraine . ... The XIII -th G. Gamow's Odessa Astronomical Summer Соnference-School, 19-25 August, 2013, Odessa, Ukraine . ...

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