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Astronomy on the Personal Computer 4th ed. 2000 [Kõva köide]

  • Formaat: Hardback, 300 pages, kõrgus x laius: 229x152 mm, kaal: 670 g, XV, 300 p., 1 Hardback
  • Ilmumisaeg: 14-Apr-2000
  • Kirjastus: Springer-Verlag Berlin and Heidelberg GmbH & Co. K
  • ISBN-10: 3540672214
  • ISBN-13: 9783540672210
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  • Formaat: Hardback, 300 pages, kõrgus x laius: 229x152 mm, kaal: 670 g, XV, 300 p., 1 Hardback
  • Ilmumisaeg: 14-Apr-2000
  • Kirjastus: Springer-Verlag Berlin and Heidelberg GmbH & Co. K
  • ISBN-10: 3540672214
  • ISBN-13: 9783540672210
Astronomy on the Personal Computer provides the reader with a thorough introduction to the computation of celestial mechanics, which is of particular significance to astronomical observation. Covering everything from astronomical and computational theory to the construction of rapid and accurate applications programs, this book supplies the necessary knowledge and software solutions for determining and predicting the positions of the Sun, Moon, planets, minor planets and comets, solar eclipses, stellar occultations by the Moon, phases of the Moon and much more. This completely revised edition makes use of the widely implemented programming language C++, and individual applications may be efficiently realized through the use of a powerful module library. The material previously available on an accompanying CD-ROM, now at extras.springer.com, contains, in addition to the complete, fully documented and commented source codes, the executable programs for use with the Windows 98/2000/XP and LINUX operating systems.
Introduction
1(6)
Some Examples
1(1)
Astronomy and Computing
2(2)
Programming Languages and Techniques
4(3)
Coordinate Systems
7(28)
Making a Start
7(7)
Calendar and Julian Dates
14(3)
Ecliptic and Equatorial Coordinates
17(3)
Precession
20(5)
Geocentric Coordinates and the Orbit of the Sun
25(3)
The COCO Program
28(7)
Calculation of Rising and Setting Times
35(24)
The Observer's Horizon System
35(3)
Sun and Moon
38(1)
Sidereal Time and Hour Angle
39(2)
Universal Time and Ephemeris Time
41(3)
Parallax and Refraction
44(3)
Rising and Setting Times
47(1)
Quadratic Interpolation
48(2)
The SUNSET Program
50(7)
The PLANRISE Program
57(2)
Cometary Orbits
59(26)
Form and Orientation of the Orbit
59(2)
Position in the Orbit
61(4)
Mathematical Treatment of Kepler's Equation
65(3)
Near-Parabolic Orbits
68(4)
Gaussian Vectors
72(4)
Light-Time
76(1)
The COMET Program
77(8)
Special Perturbations
85(26)
Equation of Motion
86(3)
Planetary Coordinates
89(2)
Numerical Integration
91(6)
Osculating Elements
97(3)
The NUMINT Program
100(8)
The Asteroid Orbital Elements Database
108(3)
Planetary Orbits
111(24)
Series Expansion of the Kepler Problem
112(3)
Perturbation Terms
115(3)
Numerical Treatment of the Series Expansions
118(6)
Apparent and Astrometric Coordinates
124(5)
Aberration and Light-Time
125(2)
Nutation
127(2)
The PLANPOS Program
129(6)
Physical Ephemerides of the Planets
135(20)
Rotation
135(10)
The Position Angle of the Axis
136(2)
Planetographic Coordinates
138(7)
Illumination Conditions
145(5)
Phase and Elongation
145(2)
The Position Angle of the Sun
147(1)
Apparent Magnitude
148(2)
Apparent Diameter
150(1)
The PHYS Program
150(5)
The Orbit of the Moon
155(24)
General Description of the Lunar Orbit
155(4)
Brown's Lunar Theory
159(10)
The Chebyshev Approximation
169(5)
The LUNA Program
174(5)
Solar Eclipses
179(26)
Phases of the Moon and Eclipses
179(2)
Geometry of an Eclipse
181(5)
Geographic Coordinates and the Flattening of the Earth
186(3)
Duration of an Eclipse
189(1)
Solar and Lunar Coordinates
190(2)
The ECLIPSE Program
192(8)
Local Circumstances
200(3)
The ECLTIMER Program
203(2)
Stellar Occultations
205(26)
Apparent Positions
206(4)
Geocentric Conjunction
210(4)
The Fundamental Plane
214(2)
Disappearance and Reappearance
216(3)
The OCCULT Program
219(10)
Estimation of ΔT=ET-UT from Observations
229(2)
Orbit Determination
231(28)
Determining an Orbit from Two Position Vectors
231(8)
The Sector-Triangle Ratio
232(3)
Orbital Elements
235(4)
The Shortened Gauss Method
239(5)
The Geometry of Geocentric Observations
239(3)
Successive Improvement of the Sector-Triangle Ratios
242(1)
Multiple Solutions
243(1)
The Comprehensive Gaussian Method
244(5)
The Gauss-Lagrangian Equation
244(3)
Improved Iteration of the Triangle-Area Ratios
247(1)
Light-Time
248(1)
The GAUSS Program
249(10)
Astrometry
259(16)
Photographic Imaging
259(3)
Plate Constants
262(2)
Least Squares Adjustment
264(3)
The FOTO Program
267(5)
The Position and Proper Motion Catalogue
272(3)
Appendix 275(14)
A.1 The Accompanying CD-ROM
275(4)
A.1.1 Contents
275(2)
A.1.2 System Requirements
277(1)
A.1.3 Executing the Programs
277(2)
A.2 Compiling and Linking the Programs
279(4)
A.2.1 General Advice on Computer-Specific Modifications
279(1)
A.2.2 Microsoft Visual C++ for Windows 95/98/NT
280(1)
A.2.3 GNU C++ for Linux
281(2)
A.3 List of the Library Functions
283(6)
Symbols 289(4)
Glossary 293(4)
Bibliography 297(8)
Subject Index 305