標題: Titlebook: Ganita-Yukti-Bhasa (Rationales Mathematical Astronomy) of Jyesthadeva; Volume II - Astronom K. V. Sarma,K. Ramasubramanian,M. S. Sriram Boo [打印本頁] 作者: Mottled 時間: 2025-3-21 19:18
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作者: Credence 時間: 2025-3-21 22:37
https://doi.org/10.1007/978-3-658-23264-1 . and five and divided by .. These two views are worth consideration. Then, (for the Moon), compute the . and apply the corrections of . and .. Then compute the . for the Sun. Compute and apply the correction of . for both the Sun and the Moon. Ascertain also the distance, at the required time, between the centres of the solar and lunar spheres.作者: Loathe 時間: 2025-3-22 01:35 作者: Immortal 時間: 2025-3-22 04:36 作者: 成績上升 時間: 2025-3-22 11:29 作者: Cholesterol 時間: 2025-3-22 16:21
Earth and Celestial Spheresr secondaries, which are used as the reference circles for describing the location of a celestial object using different co-ordinates. Finally, there is an elaborate discussion on the determination of the declination of a celestial object with latitude.作者: Cholesterol 時間: 2025-3-22 20:03 作者: progestin 時間: 2025-3-22 21:55
Computation of Planetsime period, then . where . is a constant. Given ., the radius of the planetary orbit is determined, if the time period of a planet is known. The term . refers to the number of complete revolutions made by the planet in a . consisting of 43,20,000 years. This period is also called a . and consists of four parts namely ., ., . and ..作者: fallible 時間: 2025-3-23 05:17
Eclipse longitudes are the same, it is the mid-eclipse. Now, we had.where, we approximate . by ., the true distance from the centre of the Earth in the denominator (essentially ignoring the higher order terms in .).作者: Venules 時間: 2025-3-23 05:58
Epilogueand cosine functions and also developed fast convergent approximations to them. Here, we shall discuss how the Kerala School also made equally significant discoveries in astronomy, in particular, planetary theory.作者: Terrace 時間: 2025-3-23 11:57 作者: 違反 時間: 2025-3-23 17:02
Holmer Steinfath,Claudia Wiesemannime period, then . where . is a constant. Given ., the radius of the planetary orbit is determined, if the time period of a planet is known. The term . refers to the number of complete revolutions made by the planet in a . consisting of 43,20,000 years. This period is also called a . and consists of four parts namely ., ., . and ..作者: Multiple 時間: 2025-3-23 19:41 作者: Vulnerable 時間: 2025-3-24 01:56
https://doi.org/10.1007/978-4-431-53856-1and cosine functions and also developed fast convergent approximations to them. Here, we shall discuss how the Kerala School also made equally significant discoveries in astronomy, in particular, planetary theory.作者: 易受騙 時間: 2025-3-24 06:21
Raouf Boutaba,Jin Xiao,Qi Zhang, at the confluence of the landed and watery division (of the Earth), there is a city known as .. Conceive a circular line (.) from that place, east-west, cycling round the Earth. On this line are situated four cities (including .), to the west ., to the other (diametrically opposite) side ., and to the east ..作者: Basal-Ganglia 時間: 2025-3-24 10:04 作者: FUME 時間: 2025-3-24 13:37 作者: 宮殿般 時間: 2025-3-24 18:13 作者: Pigeon 時間: 2025-3-24 20:05 作者: 莎草 時間: 2025-3-25 01:13
Ehab Al-Shaer,Jinpeng Wei,Cliff Wang is said to occur when the (magnitudes of) declinations of the Sun and Moon are equal, and when one of them is increasing and the other is decreasing. This can happen when one of these bodies is in an odd quadrant, and the other is in an even quadrant.作者: nitroglycerin 時間: 2025-3-25 03:30 作者: 親密 時間: 2025-3-25 10:40 作者: 敘述 時間: 2025-3-25 13:23
The Fifteen ProblemsNow, towards demonstrating in detail, the above-stated principles, fifteen problems are posed in relation to the divergence between the said seven (great) circles.作者: braggadocio 時間: 2025-3-25 18:24 作者: Cumbersome 時間: 2025-3-25 21:25 作者: 壓迫 時間: 2025-3-26 02:24 作者: 哀悼 時間: 2025-3-26 05:37 作者: 骯臟 時間: 2025-3-26 11:47 作者: 我說不重要 時間: 2025-3-26 13:10
Jaime Eduardo Rodríguez,Luciano A. Sposatod by solid lines in Figure 10.1. Three more circles which are referred to later in the chapter are indicated by dashed lines. In Table 10.1, the second column gives the names of the circles in Sanskrit. The third column gives their modern equivalents. In the last column we have listed the poles (vis作者: 補角 時間: 2025-3-26 17:19 作者: 庇護 時間: 2025-3-26 23:24
The Timed Autonomic Nervous System,corresponding .. The minutes of . of the Sun and Moon are to be applied, respectively, to the (true longitudes of) Sun and Moon. When the resulting true longitudes of the two are the same, that will indicate the time of the middle of the eclipse.作者: MEAN 時間: 2025-3-27 02:46
https://doi.org/10.1007/978-3-658-23264-1oon. Apply also the second true correction (.) for the Moon. Here, the view of (?rīpati, author of) . is that when the radius of the . and . circles have been ascertained, a correction has to be applied to them. The view of Mu?jāla, author of . is that the . of the Moon is to be multiplied by Moon’s作者: phase-2-enzyme 時間: 2025-3-27 07:57 作者: DECRY 時間: 2025-3-27 10:08
Autonomie und soziale Funktion der Kunst reference to the celestial equator which is revolving uniformly due to . and (iii) . — the zodiacal celestial sphere (described with reference to the ecliptic). This is followed by a discussion on the motion of equinoxes. Then, we find the description of some of the important great circles and thei作者: 間諜活動 時間: 2025-3-27 17:30 作者: 嘲弄 時間: 2025-3-27 20:02 作者: conspicuous 時間: 2025-3-28 01:31 作者: 有危險 時間: 2025-3-28 05:33
The Timed Autonomic Nervous System,corresponding .. The minutes of . of the Sun and Moon are to be applied, respectively, to the (true longitudes of) Sun and Moon. When the resulting true longitudes of the two are the same, that will indicate the time of the middle of the eclipse.作者: parasite 時間: 2025-3-28 08:27 作者: GREEN 時間: 2025-3-28 14:26 作者: NOT 時間: 2025-3-28 15:15 作者: CAB 時間: 2025-3-28 20:46 作者: Volatile-Oils 時間: 2025-3-29 02:32 作者: 拍下盜公款 時間: 2025-3-29 03:14
Ganita-Yukti-Bhasa (Rationales Mathematical Astronomy) of JyesthadevaVolume II - Astronom作者: 否決 時間: 2025-3-29 09:54
Ganita-Yukti-Bhasa (Rationales Mathematical Astronomy) of Jyesthadeva978-93-86279-37-8作者: 招人嫉妒 時間: 2025-3-29 11:37
Computation of Planets number of .-s moved per day is the same for all planets. For planets which move along smaller orbits, the circle would be completed in a shorter time. For those which move along larger orbits, the circle would be completed only in a longer period. For instance, the Moon would have completely moved 作者: Muscularis 時間: 2025-3-29 15:34 作者: 妨礙議事 時間: 2025-3-29 21:48
The Fifteen Problemsd by solid lines in Figure 10.1. Three more circles which are referred to later in the chapter are indicated by dashed lines. In Table 10.1, the second column gives the names of the circles in Sanskrit. The third column gives their modern equivalents. In the last column we have listed the poles (vis作者: EXTOL 時間: 2025-3-30 00:43
Gnomonic Shadowd spread in a circle and flow forth on all the sides uniformly. That is the indication for a level surface. On this surface draw a circle (in the following manner): Take a rod slightly bent at both ends and, with one end of the rod fixed at the centre, rotate the other end on all sides (so that a ci作者: SIT 時間: 2025-3-30 07:52 作者: CHOIR 時間: 2025-3-30 11:01 作者: arbovirus 時間: 2025-3-30 14:31
Computation of Planetsf all the planets is taken to be a constant. In other words, if . be the radius of the planetary orbit (usually given in .-s), and . be the sidereal time period, then . where . is a constant. Given ., the radius of the planetary orbit is determined, if the time period of a planet is known. The term
