[as]

[i]
[r][a]

[i]
[r][a]

[a(ll)]


Privacy Policy

Collana «Spherical and Practical Astronomy» di J. B. Lippincott & Co. in Filadelfia dal 1891
 
11:Chauvenet, WilliamManual of Spherical and Practical Astronomy 01 Vol. I. Spherical Astronomy1891
22:Chauvenet, WilliamManual of Spherical and Practical Astronomy 02 Vol. II. Theory and Use of Astronomical Instruments (Method of Least Squares)1891

2:2:0
INDICI UNIFICATI:
1[frontespizio]
2[colophon]
1863.0101;15203Preface
10Contents of Vol. I.
{titolo}
17      Chapter I.      -
17                        The Celestial Sphere-Spherical and Rectangular Co-ordinates
18                        Spherical co-ordinates
27                        Transformation of spherical co-ordinates
43                        Rectangular co-ordinates
48                        Transformation of rectangular co-ordinates
50                        Differential variations of co-ordinates
52      Chapter II.      -
52                        Time - Use of the Ephemeris - Interpolation - Star Catalogues
53                        Solar time
59                        Sidereal time
64                        Hour angles
68                        Ephemeris
79                        Interpolation by differences of any order
91                        Star catalogues
95      Chapter III.      -
95                        Figure and Dimensions of the Earth
97                        Reduction of latitude
99                        Radius of the terrestrial spheroid for given latitudes
101                        Normal, &c
103      Chapter IV.      -
103                        Reduction of Observations to the Centre of the Earth
104                        Parallax
127                        Refraction - General laws of refraction
130                                    Tables of refraction
136                                    Differential equation of the atmospheric refraction
136                                    Integration of the differential equation with Bouguer's hypothesis
143                                    Integration with Bessel's hypothesis according to the methods of Kramp and Laplace
165                                    Construction of Bessel's Table
171                                    Refraction in right ascension and declination
172                        Dip of the horizon
180                        Semidiameters of celestial bodies
183                                    Augmentation of the moon's semidiameters
184                                    Contraction of the sun's and the moon's semidiameters by refration
189                        Reduction of observed zenith distances to the centre of the earth
193      Chapter V.      -
193                        Finding the Time by Astronomical Observations
196                                    1st Method.—By transits
196                                    2st Method.—By equal altitudes
206                                    3st Method.—By a single altitude or zenith distance
213                                                Correction for second differences of zenith distance
217                                    4th Method.—By the disappearances of a star behind a terrestrial object
218                        Time of rising and setting of the stars
219                        Finding the Time at Sea
219                                    1st Method.—By a single altitude
220                                    2st Method.—By equal altitudes
223      Chapetr VI.      -
223                        Finding the Latitude by Astronomical Observations
223                                    1st Method.—By meridian altitudines or zenith distances
226                                                Combination of pairs of stars whose merdian zenith distances are nearly equal (see Vol. II, Zenith Telescope)
226                                                Meridian altitudes of circumpolar star
228                                                Meridian zenith distances of the sun near the solstices
229                                    2st Method.—By a single altitude at a given time
233                                    3st Method.—By reduction to the meridian when the time is given
235                                                Circummeridian altitudes
244                                                Gauss's method of reducing circummeridian altitudes of the sun
251                                                Limits of the reduction to the meridian
253                                    4st Method.—By the Polar Star
257                                    5st Method.—By two altitudes of the same star, or different stars, and the elapsed time between the observations
258                                                General solution
264                                                Caillet's formulae for afixed star or the sun
266                                                Correction of this method for the sun
277                                    6th Method.—By two altitudes of the same or different stars, with the difference of their azimuths
277                                    7th Method.—By two different stars observed at the same altitude, when the time is given
279                                                At nearly the same altitude, observed with the zenith telescope
280                                    8th Method.—By three stars observed at the same altitude (Gauss's method)
286                                                The same by Cagnoli's formulæ
289                                                By a number of stars observed at the same altitude, treated by the Method of Least Squares
293                                    9th Method.—By the transits of stars over vertical circles (see Vol. II., Transit Instrument in the Prime Vertical)
296                                    10th Method.—By altitudes near the meridian when the time is not known
296                        (A.)                        By two altitudes near the meridian and the chronometer times of the observations, when the rate of the chronometer is known, but not its correction
299                        (B.)                        By three altitudes near the meridian and the chronometer times of the observations, when neither the correction nor the rate of the azimuths
301                        (C.)                        By two altitudes near the meridian and the difference of the azimuths
302                        (D.)                        By three altitudes near the meridian and the differences of azimuths
303                                    11th Method.—By the rate of change of altitude near the prime vertical
304                        Finding the Latitude at Sea
304                                    1st Method.—By meridian altitude
307                                    2th Method.—By reduction to the meridian when the time is given
307                                    3th Method.—By two altitudes near the meridian when the time is not known
309                                    4th Method.—By three altitudes near the meridian when the time is not known
310                                    5th Method.—By a single altitude at a given time
311                                    6th Method.—By the change of altitude near the prime vertical
311                                    7th Method.—By the Polar Star
313                                    8th Method.—By two altitudes with the elapsed time between them
317      Chapter VII.      -
317                        Finding the Longitude by Astronomical Observations
317                                    1st Method.—By portable chronometers
323                                                Chronometric expeditions
337                                    2th Method.—By signals
337                                                Terrestrial signals
339                                                Celestial signals
339                              (a)                              Bursting of a meteor
339                              (b)                              Beginning or ending of an eclipse of the moon
339                              (c)                              Eclipses of Jupiter's satellites
339                              (d)                              Occultations of Jupiter's satellites
339                              (e)                              Transits of the satellites over Jupiter's disc
339                              (f)                              Transits of the shadows of the satellites over Jupiter's disc
339                              (g)                              Eclipses of the sun, Occultations of star and planets by the moon
341                                    3d Method.—By the electric telegraph
342                                                Method of star signals
350                                    4th Method.—By moon culminations
358                                                Peirce's method of correcting the ephemeris
363                                                Combination of moon culminations by weights
371                                    5th Method.—By azimuths of the moon, or transits of the moon and a star over the same vertical circle
382                                    6th Method.—By altitudes of the moon
383                        (A.)                        By the moon's absolute altitude
386                        (B.)                        By equal altitudes of the moon and a star observed with the Zenith Telescope
393                                    7th Method.—By lunar distances
395                        (A.)                        Rigorous method
402                        (B.)                        Approximative method
420                        Finding the Longitude at Sea
420                                    By chronometers
422                                    By lunar distances
423                                    By the eclipses of Jupiter's satellites
423                                    By the moon's altitude
424                                    By occultations of stars by the moon
424      Chapter VIII.      -
424                        Finding a Ship's Place at Sea by Circles of Position—Sumner's Method
429      Chapter IX.      -
429                        The Meridian Line and Variation of the Compass
436      Chapters X.      -
436                        Eclipses
436                        Solar Eclipses. Prediction for the earth generally
439                                    Fundamental equations
456                                    Outline of the shadows
466                                    Rising and setting limits
475                                    Curves of maximum in horizon
480                                    Northern and southern limits
491                                    Curve of central eclipse
498                                    Limits of total or annular eclipse
505                        Prediction for a given place
515                        Correction for atmospheric refraction in eclipses
517                        Correction for the height of the observer above the level of the sea
518                        Application of observed solar eclipses to the determination of terrestrial longitudes and the correction of the elements of the computation
542                        Lunar eclipses
549                        Occultations of fixed stars by the moon
550                                    Terrestrial longitudes from occultations of stars
557                                    Prediction of occultations
561                                    Limiting parallels
565                        Occultations of planets by the moon
566                                    Apparent form of a planet's disc
578                                    Terrestrial longitude from occultations of planets
591                        Transits of Venus and Mercury
592                                    Determination of the solar parallax
593                                    Prediction for the earth generally
601                        Occultation of a fixed star by a planet
602      Chapter XI.      -
602                        Precession, Nutation, Aberration, and Annual Parallax of the Fixed Stars
604                        Precession
624                        Nutation
628                        Aberration
643                        Parallax
645                        Mean and apparent places of stars
658      Chapter XII.      -
658                        Determination of the Obliquity of the Ecliptic and the Absolute Right Ascensions and Declinations of Stars by Observation
659                        Obliquity of the ecliptic
665                        Equinoctial points, and absolute right ascension an declination of the fixed stars
671      Chapter XIII.      -
671                        Determination of Astronomical Constants by Observation
671                        Constants of Refraction
673                        Constant of solar parallax
680                        Constant of lunar parallax
687                        Mean semidiameters of the planets
688                        Constant of aberration and heliocentric parallax of fixed stars
698                        Constant of nutation
701                        Constant of precession
703                        Motion of the sun in space
708_
708___
1[frontespizio]
2[colophon]
3Contents of Vol. II.
7Plates
9[titolo]
9      Chapter I.      -
9                        The Telescope
22                        
22                        Magnifying
29      Chapter II.      -
29                        Of the Measurement of Angles or Arcs in general—Circles—Micrometers—Level
29                        Graduated circles
30                        The vernier
33                        The reading microscope
37                        Eccentricity of graduated circles
42                        Periodic functions
47                        Ellipticity of the pivot of the alidade
51                        Errors of graduation
59                        The filar micrometer
70                        The level
77      Chapter III.      -
77                        Instruments for Measuring Time
77                        Chronometers
79                        Comparison of chronometers
84                        Clocks
86                        The electro-chronograph
92      Chapter IV.      -
92                        The Sextant, and other Reflecting Instruments
94                        Description of the sextant
95                        Adjustment of the sextant
101                        Method of observation
106                        Method of observation
119                        The simple reflecting circle
119                        The repeating reflecting circle
123                        Theory of its errors
127                        The prismatic reflecting circle and sextant
131      Chapter V.      -
131                        The Transit Instrument
132                        Description of the transit instrument
138                        Method of observation
139                        General formulæ
140                        The transit instrument in the meridian
141                                    Approximate adjustment
143                                    Equations of the transit instrument in the meridian
146                                    Thread intervals
149                                    Reduction to the middle thread
151                                    Reduction to the mean of the threads
153                                    Level constant
160                                    Collimation constant
169                                    Azimuth constant
174                                    Clock correction
175                                    Determination of the right ascension of stars
176                                    Transits of the moon, sun, and planets
186                                    Effect of refraction in transit observations
187                                    Meridian mark
189                                    Personal equation
193                                    Personal scale
194                                    Probable error of a transit observation
200                        Application of the method of least squares to the determination of the time with a portable instrument in the meridian
209                        The transit instrument in any virtual plane
215                        Finding the time with a portable transit instrument out of the meridian (Hansen's method)
227                        Application of the method of least squares to the determination of the time with a portable transit instrument in the vertical circle of a circumpolar star (Bessel's method)
238                        Determination of the geographical latitude by a transit instrument in the prime vertical
271                        Determination of the declinations of stars by their transits over the prime vertical
282      Chapter VI.      -
282                        The Meridian Circle
283                        Description of the meridian circle
285                        Nadir point
289                        Reduction to the meridian
293                        Horizontal point. Observations by reflection
302                        Flexure
304                        Observations of the declination of the moon
309                        Observations of the declination of a planet, or the sun
310                        Correction of the observed declination of a planet's or the moon's limb for spheroidal figure and defective illumination
315      Chapter VII.      -
315                        The Altitude and Azimuth Instrument
316                        Description (Pulkowa vertical circle)
319                        Unioversal instrument
319                        Theory of these instruments. Azimuths
326                                    Altitudes or zenith distances
333                        Correction of the observed azimuth and zenith distance of the limb of the moon or a planet for defective illumination
340      Chapter VIII.      -
340                        The Zenith Telescope
340                        Description
342                        Talcott's method of finding the latitude
344                        Correction for refraction
346                        Correction for the level
346                        Correction for the micrometer
347                        Reduction to the meridian
347                        Selection of stars
350                        Discussion of results
356                        Combination of the observations by weight
358                        Determination of the value of a division of the level
360                        Determination of the value of a revolution of the micrometer
364                        Extra-meridian observations with the zenith telescope
366                        Adaptation of the transit instrument as a zenith telescope
367      Chapter IX.      -
367                        The Equatoriaql Telescope
367                        Description (Pulkowa equatorial)
370                        General theory of the equatorial instrument
371                        Determination of the instrumental declination and hour angle to the celestial declination and hour angle
373                        Flexure
375                        Reduction of the instrumental declination and hour angle to the celestial declination and hour angle
379                        Adjustment of the equatorial with respect to the pole of the heavens, and determination of the constants
391      Chapter X.      -
391                        Micrometric Observations
391                        The Filar Micrometer—Observation of distance and position angle of two stars
392                                    Correction for errors of the equatorial instrument
395                                    Reduction of the observed position angle to the mean of the position angles at the two stars
397                                    Finding apparent difference of declination and right ascension of two stars
398                                    Correction for proper motion of one of the stars
403                        The Heliometer
405                                    Descriptio. (Königsberg heliometer)
407                                    General theory of the heliometer
420                                    Method of observation
423                                    Determinations of the constants
432                                    Observations upon the cusps of the sun in a solar eclipse
436                        The Ring Micrometer
436                                    The Ring Micrometer
441                                    Correction for the proper motion of one of the stars
445                                    Determination of the radius of the ring
450                        Correction of micrometric observations for refraction
465                        Correction of micrometric observations for precession, nutation, and aberration
469      Appendix.      Method of Least Squares
470                        Errors to which observations are liable
473                        The arithmetical mean
478                        The probability curve
485                        The measure of precision
487                        The probable error
490                        The mean of the errors, and the mean error
492                        The probable error of the arithmetical mean
493                        Determination of the mean and probable errors of given observations
497                        Determination of the mean and probable errors of functions of independent observed quantities
504                        Weight of observations
509                        Equations of condition from linear functions
512                        Normal equations
514                        Mean errors and weights of the unknown quantities
526                        Equations of condition from non-linear functions
529                        Treatment of equations of condition when the observations have different weights
530                        Elimination of the unknown quantities from the normal equations by the method of substitution, according to Gauss
534                        Determination of the weights of the unknown quantities when the elimination has been effected by the method of substitution
537                        Independent determination of each unknown quantity and its weights, according to Gauss
541                        Mean error of a linear function of the unknown quantities
549                        Conditioned observations
558                        Criterion for the rejection of doubtful observations
569      Tables.      List of tables with references to the articles in which they are explained
627Index
632_
632___
CRONOLOGIA:
 
 
1800 1800 1900 1900 2000 2000 1850 1950 2050 Chauvenet, William ( 1820.0524 - 1870.1213 ) https://en.wikipedia.org/wiki/William_Chauvenet Chauvenet, William 1720.0524 4270.1213



Generato il giorno: 2022-09-09T21:51:44+02:00 (Unix Time: 1662753104)
Precedente aggiornamento il giorno: 2022.0909
Prima registrazione il giorno: 2022.0806
Aggiornato 2 volte


Versione: 1.0.29

Privacy Policy