APA TEGESÉ 위도관측소 ING BASA KOREA?
Klik kanggo
deleng deifinisi asli saka «위도관측소» ing bausastra Basa Korea.
Klik kanggo
deleng pertalan otomatis saka definisi ing Basa Jawa.
Definisi saka 위도관측소 ing bausastra Basa Korea
Observatorium Lintang Iki minangka observatorium sing diorganisasikake dening International Geodynamics Association taun 1899 kanggo nyinaoni gerakan kutub Bumi. Jepang, Rusia, Italia, lan Amerika Serikat. Lintang kasebut diukur kanthi metode ketinggian kaya metode heteroseksual. 위도관측소
1899년 국제측지학협회가 지구의 극운동을 연구하기 위해 조직한 관측소이다. 일본, 러시아, 이탈리아, 미국의 북위 39˚8'에 5개소가 설치되어 있다. 이성등고도법(異星等高度法)으로 위도를 측정한다.
Klik kanggo
deleng deifinisi asli saka «위도관측소» ing bausastra Basa Korea.
Klik kanggo
deleng pertalan otomatis saka definisi ing Basa Jawa.
BUKU BASA KOREA KAKAIT KARO «위도관측소»
Temukaké kagunané saka
위도관측소 ing pilihan bibliografi iki. Buku kang kakait dening
위도관측소 lan pethikan cekak kang padha kanggo nyediyakaké panggunané ing sastra Basa Korea.
1
Madras Observatory Papers. By J. Goldingham, etc - 48페이지
I shall now proceed to give some information respecting thc LATITUDE of thc Observatory. The height of the Pole i at Madras being only 13 degrees, the method by Circumpolar Stars cannot be used; and the Latitude has been found by ...
Observatory (MADRAS), John GOLDINGHAM, 1827
2
Astronomical Observations Made At The Royal Observatory Et ...
38 31 21, 045 ПВввзнь'в refractions were used, the co-latìtude would be. . . . за 81 21, 411 Hence the latitude of the Observatory is 51° 2s' 39'. The reduced latitude and corresponding radius are computed from the following formulœ: tan.
John Pond, George Biddell Airy, 1835
3
Astronomical Observations Made at the Royal Observatory, ...
Royal Observatory, Edinburgh. XXXiv INTRODUCTION- Correction of Planet's Geocentric Geocentric Heliocentric Heliocentric Longitude- Latitude- Longitude- Latitude- m II II 'm Feb- 16 -2-8 -5-2 +0-9 -2-3 20- -7-9 -2-4 +31 -10 March 4- -7-5 ...
Royal Observatory, Edinburgh, 1840
4
Report on the United States and Mexican boundary survey: ...
This latitude was obtained by a mean of results from observations with zenith telescopes by Lieutenant Michler and Senor Jimenez, at their respective observatories near the initial point, (reduced to Lieutenant Michler's observatory,) as follows ...
United States. Dept. of the Interior, William Hemsley Emory, Spencer Fullerton Baird, 1857
5
Annual Report of the Meteorological Observations Made at ...
ANNUAL REPORT OP THE METEOROLOGICAL OBSERVATIONS X MADE AT THE INTERNATIONAL LATITUDE OBSERVATORY OF MIZUSAWA FOR THE YEAR 1070 I HE UNIVEKSITY MICHIGAN AUG 2 5 1972 Ufifti LATITUDE 39°08' N., ...
Ido Kansokujo (Mizusawa-shi, Japan), 1971
6
An Introduction to Practical Astronomy ... - 332페이지
71—1) gives 37 .4: geographical miles for a degree in latitude 51° 27' M", and, consequently, of 121690 : 75858 A yards will be a degree of longitude in this parallel of latitude; but the difference of latitude between the Pagoda and Observatory ...
7
An Introduction to Practical Astronomy ...: Tables, ... - 332페이지
*H) gives 37.4 geographical miles for a degree in latitude 51°27'44", and, consequently, # of 121690 = 75853.4 yards will be a degree of longitude in this parallel of latitude; but the difference of latitude between the Pagoda and Observatory in ...
8
Astronomical observations made at the Royal Observatory at ...
The test of success was assumed to be that, on starting with an assumed latitude and longitude of one station, and with an assumed azimuth of the second station from the meridian as seen from the first, and using the angles of the triangle ...
Royal Observatory (Greenwich), 1847
9
Astronomical Observations Made at the Honorable the East ... - 73페이지
Madras Observatory ... made at Madras: thus, to render the Solsticial Observations at Madras accordant, we must diminish the Latitude of Greenwich l",65; and to reconcile the Observations at ... Difference of Latitude ofMadras and Greenwich.
10
Results of Measures Made at the Royal Observatory, ... - D-119페이지
The num-bers given in the accompanying table have been formed as íollows :The Heliographic Latitude of each Spot foreach day has been multiplied by its Area (corrected for foreshortening), and the sum of the products, for Spots North of the ...
Royal Greenwich Observatory, 1921
