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341. (Untitled)
. The Table on p. 5790 – 5799 includes additional data for the asteroids for which non-principal axis rotational motion (tumbling) has been reported. The data for publication in the Table were prepared by B. Warner (Palmer Divide Observatory, Colorado Springs, U.S.A.), A. W. Harris (Space Science Institute, U.S.A.) and P. Pravec (Astronomical Institute, Academy of Sciences of Czech Republic).
[ Сохраненная копия ]  Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user4tke.htm -- 1.8 Кб -- 10.04.2016
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342. (Untitled)
The table of elements represents sets of elements in increasing order of minor planet numbers. ... In the column of G (slope parameter) the default value of the parameter equal to 0.15 is indicated as “X” to distinguish it from value 0.15 obtained by photometric observations (see (89) Julia, (419) Aurelia)). ... User has possibility to save the file with elements, to print it using standard means or to turn to the construction of histograms or distributions of minor planet elements. ...
[ Сохраненная копия ]  Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user4tb9.htm -- 4.5 Кб -- 10.04.2016
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343. (Untitled)
To initiate orbital motion click on any of the icons in tool bar with red sign + or – , permitting also to speed or to slow planet motion by repeated clicking on them. ... Selecting Orbits item in menu bar and by subsequent choosing corresponding items in drop-down menu one can also fulfil the above actions. ... To enter new initial epoch or to change list of minor or major planets which are shown in the picture, select Orbits in menu bar and then select Input data in drop-down menu. ...
[ Сохраненная копия ]  Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user4rqf.htm -- 3.8 Кб -- 10.04.2016
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344. (Untitled)
... The data of the Table are based on the data published by C.-I. Lagerkvist, A. W. Harris and V. ZappalА (See: “Asteroids II machine-readable data base: March 1988 floppy disk version”, National Space Science Data Center, Greenbelt MD). The Table was updated for publication in the volume for 2014 by B. Warner (Palmer Divide Observatory, Colorado Springs, U.S.A.), A. W. Harris (Space Science Institute, U.S.A.), and P. Pravec (Astronomical Institute, Academy of Sciences of Czech Republic) . ...
[ Сохраненная копия ]  Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user4q3y.htm -- 2.2 Кб -- 10.04.2016
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345. (Untitled)
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 . ...
[ Сохраненная копия ]  Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user4oqb.htm -- 4.2 Кб -- 10.04.2016
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346. (Untitled)
... To mark coordinate net in plot, first select Plate in menu bar and then Coordinate net in drop-down menu. ... User has possibility to save plot of sky 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 plot of plate select File item in menu bar and then take advantage of options Print Preview , Print Setup , Print. ... To return to the list of centers click on x button in title bar. ...
[ Сохраненная копия ]  Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user4lys.htm -- 3.7 Кб -- 10.04.2016
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347. (Untitled)
... 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). ...
[ Сохраненная копия ]  Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user4dpi.htm -- 12.5 Кб -- 10.04.2016
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348. (Untitled)
Ephemerides of minor planets, arranged in order of opposition date, are given on p. 6462 – 23098. ... The following data are tabulated for each planet: . 1.The number and name or principal provisional designation of the minor planet, the opposition date, the mean anomaly on the fourth ephemeris date, the minimum value of the phase angle and the date of its occurrence, the last two figures of the year of the most recent astrometric observation. ...
[ Сохраненная копия ]  Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user4160.htm -- 3.1 Кб -- 10.04.2016
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349. (Untitled)
Here user should specify the origin of coordinate system (observer's position). In case of rectangular coordinates it can be center of any major planet or the Sun or any minor planet. ... For spherical coordinates the origin of coordinate system can coincide only with the center of the Earth or with any point on the Earth surface. ... a)by code of observatory in the list of observatories maintained by Minor Planet Center (see IX. Observatories ). b)by introducing name of observatory. ...
[ Сохраненная копия ]  Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user3w6q.htm -- 2.7 Кб -- 10.04.2016
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350. (Untitled)
. To continue the work mark the row with data on wonted plate by sliding bar and click first on Plate in menu bar and then on Object list or on Plot of plate in drop-down menu. The first choice will result in displaying the list of minor planets within the limits of the plate, the second one leads to displaying the image of the plate with objects. But in both cases user should specify the magnitude limit above which the objects are not inserted into the list and not displayed in the plot.
[ Сохраненная копия ]  Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user3u1z.htm -- 1.8 Кб -- 10.04.2016
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351. (Untitled)
The Table on p. 5780 – 5787 contains additional data for the lightcurves of the objects marked in the Table “Minor planet lightcurve parameters” as known or suspected binaries. The data are meant to provide a quick overview of a primary period and amplitude of the lightcurves as well as a secondary period and, if available, amplitude. ...
[ Сохраненная копия ]  Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user3rce.htm -- 1.9 Кб -- 10.04.2016
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352. (Untitled)
... To do this select File in menu bar and then Save As... in drop-down menu. As a result the Saving dialog box will appear. ... To see the list of files with desirable extension in chosen folder define the type of extension with the help of drop-down list File type at the bottom of the dialog box. ... The name of the file will appear in File name dialog box. ... In case you want to save the file with new name type it in the File name dialog box. ... Click on Save button to save the file. ...
[ Сохраненная копия ]  Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user3qef.htm -- 2.8 Кб -- 10.04.2016
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353. (Untitled)
Three different forms are possible for representing Results of calculation of spherical coordinates: . the form designated as EMP is similar to that used in the Ephemerides of Minor Planets, having formal precision of 0.01 minute of time in right ascension and 0.1 minute of arc in declination. Longitude, latitude, azimuth and altitude are also displayed with comparable formal precision. the form designated as Positions has enhanced formal precision. ...
[ Сохраненная копия ]  Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user3q9g.htm -- 2.5 Кб -- 10.04.2016
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354. (Untitled)
Information on the AMPLE integrated software package is given on p. 23494-23495. Data for the present volume of the EMP have been prepared by Yu.Chernetenko, G. R. Kastel', O. M. Kochetova, V. B. Kuznetcov, V. A. Shor, T. A. Vinogradova, and N. B. Zheleznov. ... Special system for search of necessary information on http://www.ipa.nw.ru/PAGE/DEPFUND/LSBSS/EMP/2015/emp2015.html was compiled by N. I. Alehina and N. B. Zheleznov. ...
[ Сохраненная копия ]  Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user3ods.htm -- 2.0 Кб -- 10.04.2016
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355. (Untitled)
. Present section of the package enables one to perform following actions: . — . To make selection out of the total number of elements in accordance with the conditions imposed on some element or on a variety of elements. — . to sort the set of elements in order of ascending or descending value of any element. — . to draw the histogram of element distribution for obtained selection. — . To construct dotty picture of minor planet distribution in two– or three–dimension space of elements.
[ Сохраненная копия ]  Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user3m03.htm -- 2.1 Кб -- 10.04.2016
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356. (Untitled)
... It is precisely these values that are displayed as O – C. In case computed positions of minor planet for all or some part of moments are found without accounting for perturbations, the corresponding moments are followed by asterisk (without perturbations are computed positions for all minor planets if moments of their observations lie outside the basic interval of 16 months or for ordinary ... The coordinate system and type of computed positions are indicated in status bar. ...
[ Сохраненная копия ]  Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user3khf.htm -- 2.7 Кб -- 10.04.2016
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357. (Untitled)
If necessary, the observations and corresponding O – C values belonging to some observatory can be separated from the other data. Besides, O – C satisfying some conditions imposed on their value can be separated. ... To separate O – C by value, mark O – C check box and enter positive numbers limiting absolute values of O – C from above or from bottom or both and click on Run . ... The restrictions imposed on observatory code and on O – C values are indicated in status bar. ...
[ Сохраненная копия ]  Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user39bb.htm -- 2.8 Кб -- 10.04.2016
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358. (Untitled)
User has possibility to start running the application being in any item of ephemeris menu. To do this click on Run button at the bottom of Ephemerides dialog box. The Calculation progress dialog box allows one to keep track of run. ... After inspecting them the calculations can be continued by selecting Ephemerides item in menu bar and then Continue item in drop-down box. For information about current task select Ephemerides item in menu bar and then Task Info item in drop-down box. ...
[ Сохраненная копия ]  Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user38tj.htm -- 2.0 Кб -- 10.04.2016
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359. (Untitled)
An ephemeris can be calculated with different accuracy. Calculation accuracy dialog presents three modes of accuracy. One can calculate position of a minor planet by the formulae of elliptic motion starting from the fundamental set of elements for given minor planet. ... Also there is possibility to calculate positions taking into account perturbations from different sets of perturbing bodies by numerical integration ( Integration mode). ... Accuracy of integration is equal to 10**(-10) AU. ...
[ Сохраненная копия ]  Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user34xl.htm -- 3.2 Кб -- 10.04.2016
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360. (Untitled)
To proceed to drawing tracks of some objects select Tracks item in menu bar and then select Input Data in drop-down menu. Enter initial and final dates of time interval in corresponding data fields of the Input Data dialog box Input Data . ... The frame with horizontal and vertical scales corresponding to the right ascension and declination axes appears on screen. ... Depending on specifications introduced in the Input Data dialog box the picture represents tracks up to three different objects. ...
[ Сохраненная копия ]  Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user2pnr.htm -- 3.1 Кб -- 10.04.2016
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