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Description
Alcyone Ephemeris v.1.0.1 Alcyone Ephemeris is an accurate and fast astronomial ephemeris calculator covering the period 3000 BC to AD 3500. It calculates heliocentric, geocentric, and topocentric positions of the Sun (Earth), Moon, and planets. Aug 27, 2016. 11 checkpoint safe office 1000nw firmware,MusicLabel2000 6 02 build 175 loader by EMiNENCE,fifa 15 crack 007 soundtrack,alldata 8 20 crack,life in the army. Created by experts, for experts, ALLDATA is the leading provider of OEM service and repair information to the professional automotive service and collision industries.
'Alcyone Ephemeris' is a complex, fast and accurate astronomical ephemeris calculator covering the period 3000 BC to AD 3000. I like the fact that it has many useful functions and features that help the user find the information that he or she needs. Among all these, the features that deal with visuals are of great importance, at least as far as I am concerned. Thus, I like the star charts as well as the 3D-visualization of heliocentric and..
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- Release Date:04/03/2011
- License:Shareware
- Category:Utilities
- Developer:Alcyone Software
- Downloads:128
- Size:45.4 Mb
- Price:$49.90
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System Requirements
Alcyone Ephemeris requires Windows.
Alcyone Ephemeris v.4.2.0.522 Copyright
Shareware Junction periodically updates pricing and software information of Alcyone Ephemeris v.4.2.0.522 full version from the publisher using pad file and submit from users. Software piracy is theft, Using crack, password, serial numbers, registration codes, key generators, cd key, hacks is illegal and prevent future development of Alcyone Ephemeris v.4.2.0.522 Edition. Download links are directly from our publisher sites. Links Alcyone Ephemeris v.4.2.0.522 from Bittorrent, mediafire.com, uploadfiles.com, hotfiles.com rapidshare.com, megaupload.com, netload.in, storage.to, depositfiles.com and other files hosting are not allowed. The download file is obtained directly from the publisher, not from any Peer to Peer file sharing applications such as Shareaza, Limewire, Kazaa, Imesh, eDonkey, eMule, Ares, BearShare, Overnet, Morpheus, BitTorrent Azureus and WinMX.
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Alcyone Ephemeris v.4.2.0.522
'Alcyone Ephemeris' is a complex, fast and accurate astronomical ephemeris calculator covering the period 3000 BC to AD 3000. I like the fact that it has many useful functions and features that help the user find the information that he or she needs.
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Other products of this developer Alcyone Software
Planet's Visibility v.2.0.1.61
Planet
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To compute the visibility phenomena of a star, in the object list select stars.., which opens the lists of Stars and runs a calculation for the last selected star. To compute the visibility phenomena of a different star, select it in the list and press Calculate or double-click the name of the star.
The star list gives (1) the common name of the star, (2) the constellation, (3) Bayer letter, (4) Flamsteed number, and (5) magnitude. The list may be ordered by name, by constellation and Bayer letter, or by magnitude by clicking those headings of the list. The window containing the star list remains open until it is closed by the close box so different stars may be selected and calculated directly from the list.
The star list provided with the program contains all stars through magnitude 2.5. To add a new star to the list, click the plus button, which opens the new star data window.Fill in the name of the star, the constellation, Bayer letter, Flamsteed number-if these do not exist a catalog number or other designation may be used for the name-and the following required information:
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Note: Proper motions of the faster stars can affect the dates of visibility phenomena by one or two days in antiquity, less for the last few hundred years, with the greater effect at higher geographical latitudes. The Yale Bright Star Catalogue is a convenient source of all required information.
To edit a star in the list, click the triangle button and in the edit star data window follow the procedure for adding a new star. Click OK and the edited data is saved.
To delete a star from the list, click the minus button and in the confirm window click
OK to delete record.
When a new star is added, values of the arcus visionis and critical altitude are assigned to it automatically according to the procedures described next.
Although the visibility phenomena for stars are the same as for superior planets, the visibility parameters are treated differently. In the Settings menu select visibility parameters…, select the stellar visibility page, which shows settings for the arcus visionis and critical altitude, and in the object list select the star. The computation of the arcus visionis uses the formulas for variable arcus visionis of the superior planets; however, the purpose here is not a variation in the magnitude of a single object but that the stars have a large range of magnitudes and fixed values of the arcus visionis for stars are unknown (aside from a few special cases, as Sirius). The default values for the computation are:
heliacal (first and last visibility): arcus visionis = 10.50 + 1.40 x magnitude
acronychal rising, cosmical setting: arcus visionis = 8.90 + 1.10 x magnitude
Both the constant and coefficient of magnitude are adjustable to 0.01 and the resulting arcus visionis is also calculated to 0.01 (although this is surely false precision and 0.1 is a more reasonable limit). Because differences in azimuth between stars and the sun may differ greatly from differences for planets and the sun, particularly at higher geographical latitudes, a clear distinction of arcus visionis for heliacal and acronychal phenomena may be less applicable and it may be advisable to set the arcus visionis manually, taking into account the differences of azimuth. After making any changes, click OK and the new values are saved, but are not yet applied to any stars. If the new values are not to be saved, click Cancel. Whether the values are to be saved or used without saving, the calculation of the arcus visionis is as follows:
To calculate the arcus visionis from the formulas for a single star, select the star in the name list, and press calculate arcus visionis from magnitude (for selected star). The calculated heliacal and acronychal arcus visionis then appear in the in use column and are retained and used in the computation of visibility phenomena. To make these the default values for the selected star, press >>, and the in use values appear in the default column. To make the default values, if different, the in use values, press <<, and the default values appear in the in use column. The in use and default values may also be set manually without using the formulas or arrows. These changes are retained and used in computation whether OK or Cancel is pressed to close the window. Click OK and a calculation is run for the last object calculated, which may not be the star selected and set in the stellar visibility page. To calculate visibility phenomena for the star just set, it must be selected and run from the list of Stars.
To calculate the arcus visionis from the formulas for all stars, for example, if the formulas are changed, press calculate arcus visionis from magnitude (for all stars). The calculated heliacal and acronychal arcus visionis then appear in the in use column for all stars and will be retained and used in the computation of visibility phenomena. To make these the default values, it is necessary to make the changes individually using >> or manually; the reason is that in this way default values for individual stars may be retained while the in use values are varied. These changes are retained and used in computation whether OK or Cancel is pressed to close the window. Click OK and a calculation is run for the last object calculated, which may not be a star.
The critical altitude is adjustable from 0° to 20° at intervals of 0.01° (although here also 0.1° is more reasonable precision). The default value is 0°, crossing the horizon, but it is not likely that any star is visible at the horizon so some higher value, depending upon the magnitude of the star and local conditions, should be used. To set the critical altitude for a single star, select the star in the name list and enter the critical altitude in the in use column; this value is retained and used in the computation of visibility phenomena. The values may be shifted between the in use and default columns by pressing >> and << and may also be set manually. To set the same critical altitude for all stars, enter it next to set critical altitude (for all stars) and press that button; the value then appears in the in use
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column for all stars. As for the arcus visionis, the default values must be set individually using >> or manually; in this way the in use values may be varied and default values for individual stars retained. The critical altitude, for a single star or for all stars, is retained and used in computation whether OK or Cancel is pressed to close the window. Click OK and the value assigned to set critical altitude (for all stars) is saved and a calculation is run for the last object calculated, which may not be a star.Finally, the set default values button performs the following functions:
- The formulas for calculate arcus visionis from magnitude are reset to the default values given above.
- The set critical altitude (for all stars) is reset to the last value saved.
- The in use values of the arcus visionis and critical altitude of every star are set to whatever is entered in each star's default column.
When a new star is added to the list of Stars, the in use and default values of the arcus visionis and critical altitude are automatically set using the formulas for arcus visionis and the critical altitude for all stars last saved in the stellar visibility page.
The heliacal/acronychal dates and more information windows and the command text/print are the same as for the superior planets.
The HTML files for rise, culmination, and set times of a star and the sun, and for the heliacal and acronychal phenomena of a star, are the same as for the superior planets.