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April 6 2003 The Air Assault of Basra coalition directed at Saddam counselors Chemical Ali in 1988 the use of poison gas against Kurdish village beaufsichtigte.BF-9E: Two 7.9 mm machine guns in the. Alcyone Ephemeris 4.3 is an accurate and fast astronomical ephemeris calculator covering the period 3000 BC to AD 3000. Look for Alcyone Ephemeris 3.5.0.81 in the list, click on it and then click Uninstall to initiate the uninstallation. Method 2: Uninstall Alcyone Ephemeris 3.5.0.81 with its.

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The visibility phenomena of the fixed stars are the same as for the superior planets, heliacal rising and setting, acronychal rising and cosmical setting. However, because stars can be at any latitude from the ecliptic, and can rise and set at any difference in azimuth from the sun, heliacal phenomena are not necessarily at the horizon close to the sun and acronychal phenomena not necessarily at the horizon opposite the sun. Consequently, a clear distinction of the arcus visionis for heliacal and acronychal phenomena may not be applicable, and intermediate values may be preferable. Further, the order of visibility phenomena can change notably from the normal sequence F, acr, cos, L, and, particularly at higher geographical latitudes, stars may have no visibility phenomena at all if they are circumpolar and either always visible or never visible.
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:

RA (J2000): right ascension in hours, minutes, and seconds for 2000 January 1, 12h UT. Dec (J2000): declination in degrees, minutes, and seconds for 2000 January 1, 12h UT. Magnitude: to two places (0.01). pm RA: proper motion in right ascension in seconds of arc per year to three places (0.001). pm Dec: proper motion in declination in seconds of arc per year to three places (0.001).

Click OK and the star appears in the star list.
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 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:

1. The formulas for calculate arcus visionis from magnitude are reset to the default values given above.
2. The set critical altitude (for all stars) is reset to the last value saved.
3. 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.

Note: The default values column is unchanged by these operations and serves as a permanent memory until it is changed either by pressing >> to set the in use values as defaults or by setting it manually. In this way, default values for all stars may be retained even when changes are made in in use values, either individually or for all stars.
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

Alcyone Ephemeris Cracked Meaning

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.

Alcyone Ephemeris Cracked Software

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.

Alcyone Ephemeris Cracked Mac