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Latitude and Longitude by Account--Rule- Meridian by two

Stars at Elongation-Meridian by Observation of one Circum-

polar Star at Elongation-Example of finding Meridian by Obser-

vation of one Circumpolar Star at Elongation—To Calculate the

Time of a Star's Culmination or Elongation-Example of Calcula-

tion of Time of Star's Culmination-Calculation of Star's Altitude

at Elongation-Meridian by observing the Pole-star and Alioth

in same Vertical-Meridian by observing Circumpolar Stars in

same Vertical-Test of Meridian by Time Interval between

Transits of Circumpolar Stars-Meridian by one Extra Meridian

Observation of Sun or Star-Errors in Calculated Azimuth by Sun

Observation due to given Errors in Latitude and Declination-

Example of finding Meridian by Extra Meridian Observation of

Sun-Coaltitude-Colatitude-Codeclination-Accuracy of Extra

Meridian Observation of Sun or Star-Calculation when either

Altitude, Latitude, or Declination is not known-Altitude not

known Latitude not known Declination not known-Con-

vergence of Meridians-Observations for Latitude-Latitude by

Meridian Altitude of Sun or Star-In the Northern Hemisphere

-In the Southern Hemisphere-Latitude by Meridian Altitude

of Sun-Example of finding Latitude by Meridian Altitude of

Sun-Latitude by Zenith Pair Observations of Stars-Latitude

by Extra Meridian Observations of Sun or Star-Prime Vertical

Observations for Latitude-Observations for Time --Approximate

Method of finding Time and Meridian-Time by Meridian Transit

of Sun or Star-Time by Extra Meridian Observation of Sun or

Star-To Convert Arc to Time and vice versa-To. Convert

Sidereal Time to Mean Time and vice versâ—Equation of Time—

Observations for Longitude-Longitude by Chronometer-Deter-

mination of Difference of Longitude by Watch-Example of find-

ing Difference of Longitude by Watch-Longitude by Absolute

Methods-Longitude by Eclipses of Jupiter's Satellites-Longi-

tude by Moon Culminating Stars-Longitude by Lunar Occultations

-Longitude by Lunar Distances-Solution of Spherical Triangles

-Right-angled Spherical Triangles-Oblique Spherical Triangles

-Rule of Sines-Reduction of Sides of Spherical Triangles to

Actual Linear Distances

EXPLANATION OF ASTRONOMICAL TERMS IN

CHAPTER X.

Altitude-Apparent Time-Astronomical Mean Time-Azimuth-Cir-
cumpolar Stars-Civil Mean Time-Coaltitude-Codeclination —
Colatitude-Contraction-Conjunction-Culmination― Declination
— Elongation — Equation of Time-Equator - Great Circle-

Survey-Triangles of the Ordnance Survey of Great Britain and

Ireland-Primary Triangles-Secondary Triangles-Tertiary Tri-

angles-General Form of Triangulation-Reconnaissance and

Selection of Stations-Determining necessary Heights of Stations-

Clearing out Line between two Stations not visible from each

other-Selection of Base Lines-Permanent Marking of Stations

and Base Lines-Instrument Stations and Scaffolds—Signals—

Sun Signals or Heliographs and Heliostats-Heliostats and Helio-

graphs-Gauss' Heliotrope-Wharton's Improvised Heliostat-

Night Signals-Phase of a Signal-Measurement of Base: Measure-

ment with Steel Tape—Straining Apparatus—Absolute Length of

Tape-The Coefficient of Expansion-The Modulus of Elasticity-

Correction for Sag-Correction for Pull-To Eliminate Corrections

for Sag and Pull-Correction for Temperature-Corrections for

Fractional Part of Tape Length-Measurement of Bases with

Steel and Brass Wires-Accuracy of Steel Tape Base Measure-

ments-Measurement with Rods-Broken Base-Reduction of

Base to Horizontal-Reduction of Base to Mean Sea Level-

Extending a Base-Extension of the Triangulation from the

Measured Base-Instruments-Observation of the Angles: Method

of Repetition-Method of observing Horizontal Angles adopted on

Ordnance Survey of United Kingdom-General Method of observ-

ing Angles-Time for observing Angles-Accuracy of Measure-

ments of Angles-Reduction of Angles to the Centre of Station-

Correction of the Errors of the Angles-Calculation of Spherical

Excess-Adjustment of the Angles-Example of Correction and

Adjustment of Angles of a Triangle-Correction by Reciprocals

of Number of Observations-Correction by Reciprocals of Squares

of Number of Observations-Adjustment of Angles inversely as

"Weights" of Observations-Calculation of the Sides of the

Triangles-Calculation by Spherical Trigonometry-Calculation

by Delambre's Method-Calculation by Legendre's Method--

Summary of Operations in Computation of Triangles by Legendre's

Method - Calculation of the Astronomical Co-ordinates of the

Stations-Polar Spherical Co-ordinates — Rectangular Spherical

Co-ordinates-Surveying of Interior Detail-Levelling-Cost of

Trigonometrical Surveys-Instructions for Secondary Triangulation

-Locating Stations-Reading Angles-Closing Triangles-Base

Lines-Observations for Azimuth-Stone Line Bench Marks-

Cutting Timber-Descriptions of Stations-Tertiary Triangula-

tion - Triangles - Stations Instrument Stations - Observing

Angles-Marking Stations-Map Projections-Projection to be

adopted — Rectangular Projection — Trapezoidal Projection

Simple Conic Projection-De L'Isle's Conic Projection-Bonne's

Projection—The Polyconic Projection-Projection of Maps of the

Survey of India-Projection of Maps of the Ordnance Survey of

the United Kingdom

LIST OF TABLES.

PAGES

TABLE I. FOR HEIGHTS BY MERCURIAL BAROMETER 168, 482, 484, 485

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III. FOR HEIGHTS BY BOILING POINT THERMOMETER 171, 494, 497

IV. FOR REDUCTION OF INCLINED SIGHTS IN TACHEO-
METRY OR STADIA SURVEYING

- 273, 498

TABLE FOR REDUCING MEASUREMENTS ON SLOPE TO HORI-
ZONTAL, 66 FT. CHAIN

9

TABLE FOR REDUCING MEASUREMENTS ON SLOPE TO HORI-
ZONTAL, 100 FT. CHAIN

IO

TABLE FOR CONVERSION OF DEPARTURE INTO DIFFERENCE of
LONGITUDE

348

TABLE OF LENGTHS OF A DEGREE OF LONGITUDE At Different

LATITUDES

349

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