Course in Astrophsics And Stellar Astronomy volume 11
Course in Astrophsics And Stellar Astronomy volume 11
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In our eReader you can find the full English version of the book. Read Course in Astrophsics And Stellar Astronomy volume 11 Online - link to read the book on full screen. Our eReader also allows you to upload and read Pdf, Txt, ePub and fb2 books. In the Mini eReder on the page below you can quickly view all pages of the book - Read Book Course in Astrophsics And Stellar Astronomy volume 11
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To quickly assess the difficulty of the text, read a short excerpt:
-^JZL _ ___. \Q I G"m 3 The universal and accurate methods of -Teasurement and reduction of astro- grams expounded ai ove sometimes require a great expenditure of time* But there are oases when it is necessary to determine as quiekly as possible the position of a single celestial object (comet, planet, variable star, et) even If the accuracy ias to suffer somewhat* In such eases it is often sufficient to Inter p >1 te the sought position of the object between two (or three) basic stars* The mea...surements are also simplified, they do not require a previous orientation of t' e plate, Suoh interpolation methods are those of Kaiser, Reger, Wolf, Schlo singer* Let K be an object on t':e rlute the position of which needs to be de- termined (Fig* 14)* Let us select two basic stars! (l)and(2) such that object K be, as close as possible to the line (l) - (2), Let us pass through star (2) the celestial meridian and through star (1) the parallel of declination (we shall neglect the error of projection of the sphere on a plrme)* He measure tho dif- ference of the coordinates with respect to some axes X, Y: Ax and Ay for the pair of basic stars.
What to read after Course in Astrophsics And Stellar Astronomy volume 11?
You can find similar books in the "Read Also" column, or choose other free books by B P Gerasimovich to read onlineMoreLess
To quickly assess the difficulty of the text, read a short excerpt:
-^JZL _ ___. \Q I G"m 3 The universal and accurate methods of -Teasurement and reduction of astro- grams expounded ai ove sometimes require a great expenditure of time* But there are oases when it is necessary to determine as quiekly as possible the position of a single celestial object (comet, planet, variable star, et) even If the accuracy ias to suffer somewhat* In such eases it is often sufficient to Inter p >1 te the sought position of the object between two (or three) basic stars* The mea...surements are also simplified, they do not require a previous orientation of t' e plate, Suoh interpolation methods are those of Kaiser, Reger, Wolf, Schlo singer* Let K be an object on t':e rlute the position of which needs to be de- termined (Fig* 14)* Let us select two basic stars! (l)and(2) such that object K be, as close as possible to the line (l) - (2), Let us pass through star (2) the celestial meridian and through star (1) the parallel of declination (we shall neglect the error of projection of the sphere on a plrme)* He measure tho dif- ference of the coordinates with respect to some axes X, Y: Ax and Ay for the pair of basic stars.
What to read after Course in Astrophsics And Stellar Astronomy volume 11?
You can find similar books in the "Read Also" column, or choose other free books by B P Gerasimovich to read onlineMoreLess
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