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  • Thornthwaite, W. H. - Hints on reflecting and refracting telescopes and their accessories
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  • TABLE DES MATIÈRES
  • TABLE DES ILLUSTRATIONS
  • RECHERCHE DANS LE DOCUMENT
  • TEXTE OCÉRISÉ
  • Première image
  • PAGE DE TITRE
    • Preface to the third edition (p.R2)
    • Contents (p.R3)
    • Introduction (p.5)
    • The various forms of telescopes. Their construction and advantages (p.7)
    • Refracting telescopes (p.11)
      • The perspective and opera-glasses (p.11)
      • The ordinary refracting telescope (p.12)
      • Stands for refracting telescopes (p.16)
      • Reflecting telescopes (p.19)
        • Direct vision reflectors. The gregorian telescope (p.19)
        • The cassegrainian telescope (p.20)
      • Stands for direct vision reflectors (p.21)
        • Indirect-vision reflectors. Nasmyth's modification of the cassegrainian telescope (p.21)
        • The herschelian telescope (p.22)
        • The newtonian telescope (p.23)
        • Adjustments of a newtonian telescope (p.24)
    • Stands for indirect-vision reflectors (p.31)
      • The alt-azimuth stand (p.31)
      • Equatorial stands (p.36)
      • Horne and thornthwaite's portable equatorial (p.36)
      • Berthon's patent equatorials (p.37)
    • Equatorial adjustments (p.41)
      • To place the Polar Axis in the Méridian (p.41)
      • To correct the Declination Vernier (p.41)
      • To adjust the Polar Axis to the Latitude of Observation (p.43)
      • To test the accuracy in position of the Telescope (p.43)
        • To set the Right Ascension Vernier (p.45)
        • To find a Celestial Object by means of the Declination and Hour Circles (p.46)
        • To convert Mean into Sideral Time (p.47)
        • Table of Refractions (Bessel) (p.48)
        • To adjust the “Finder” (p.48)
    • To silver and polish glass specula (p.49)
      • Apparatus (p.49)
      • To support the Mirror in the Silvering Vessel (p.50)
      • To clean the mirror (p.51)
      • To immerse the mirror (p.51)
      • To prepare the Silvered surface for polishing (p.52)
      • To polish the Silvered surface (p.53)
      • To separete the Mirror from the Wooden Support (p.54)
      • Martin's process of silvering (p.54)
      • Dr. Henry Draper's formula for silvering (p.56)
      • The sugar of milk process for silvering (p.56)
      • General, hints on silvering (p.57)
    • Accessories to the telescope (p.58)
      • Eye-pieces (p.59)
      • Solar eye pieces (p.59)
      • Barlow's lens (p.59)
      • The micrometer (p.60)
      • The double image micrometer (p.61)
      • Berthon's dynamometer (p.61)
      • The astronomical spectroscope (p.62)
      • Horne & thornthwaite's miniature universal spectroscope (p.65)
    • Observatories (p.66)
      • To construct an observatory on the Romsey model (p.67)
      • References to illustrations (p.71)
      • Horne & thornthwaite's astronomical clock (p.72)
      • Hints on observation (p.74)
    • Defining and separating tests (p.78)
    • Light tests (p.79)
    • Catalogue of reflecting and retracting telescops and their accessories (p.81)
      • Achromatic perspective glasses (p.81)
      • Achromatic opera glasses (p.81)
      • Achromatic field glasses (p.81)
      • Achromatic telescopes (p.83)
      • Horne and thornthwaite's binocular telescopes (p.83)
      • Refracting telescopes for astronomical purposes (p.84)
      • Astronomical object glasses (p.87)
      • Astronomical reflecting telescopes (p.89)
      • Silvered-glass specula (p.93)
      • Silvered-glass diagonal mirrors (p.93)
      • The “romsey” observatory (p.93)
      • Silvering and polishing specula (p.94)
      • Apparatus for silvering (p.94)
        • Silvering vessels (p.94)
        • Glass measures (p.94)
        • Chemicals (p.94)
      • Set of silvering apparatus (p.94)
      • Astronomical eye pieces (p.95)
        • Huyghenian construction (p.95)
        • Ramsden's construction (p.95)
        • Aplanatic construction (p.95)
        • Kellner's construction (p.95)
      • Solar eye pieces (p.95)
      • Micrometers (p.95)
      • Astronomical spectroscopes (p.96)
      • Trabsit instruments (p.96)
      • Works on astronomy (p.96)
  • Dernière image
  • Première image
  • PAGE DE TITRE
    • The german equatorial stand (p.17)
    • The victoria equatorial (p.18)
    • The alt-azimuth stand (p.32)
    • Horne and Thornthwaite's equatorial reflector (p.34)
    • Horne and Thornthwaite's portable equatorial reflector (p.35)
    • The berthon equatorial (p.38)
    • The berton equatorial (p.39)
    • The victoria equatorial telescope (p.85)
    • Berthon patent equatorial stand (p.90)
    • The alt-azimuth stand (p.92)
    • Binoclar microscope (p.97)
  • Dernière image
3i

STANDS FOR INDIRECT-VISION REFLECTORS,

THE ALT-AZIMUTH STAND.

Fig. 19.

The word Alt-azimuth is a contraction of Altitude and Azimuth. These terms refer to the two movements which must be given to a telescope mounted on this plan, to enable the apparent motion of celestial objects, due to the revolution of the earth, to be followed, and thus retained in the field of view for continuous observation. When a star is due south, or, as it is technically called, “ on the meridian,” it has attained its greatest “ altitude,” or height, from the horizon. The motion preceding this meridian passage is, from the rising of the star—an ascending one—and that immediately succeeding â– —a descending one—till the star has set. To follow this ascending and descending motion, the telescope must therefore have a Vertical or Altitude Movement, which is thus applied:—The Telescope being balanced on trunnions, can be moved from an elevation approaching the Zenith to a horizontal position. In order that it may be secured anywhere between these extremes, attached to the upper part of the telescope is an iron rod, which, sliding through the end of the arm of the stand, can be there clamped. The telescope will now be clamped in Altitude. As the progression of celestial objects will apparently be very slow, resource must be had to the smoothness of motion obtained by a screw. The upper end of the Altitude rod is therefore tapped to receive a long screw with a large milled head, jointed to the telescope body ; by revolving this head, the telescope is raised or depressed accordingly as the screw is unscrewed, or the reverse. It is necessary that the screw should be withdrawn some way from the rod before clamping it, preparatory to following an object which has passed the meridian, or is setting; as, perhaps, just when the clearest vision is obtained, the observer may be annoyed by the screw action being suddenly stopped by the milled head coming in contact with the top of the rod.

When viewing objects near the zenith, the handle attached to the clamp will be found useful, as it can thereby be reached without leaving the finder. The handle may be so placed that a downward push should clamp, and an upward pull release.

We have lately introduced a great improvement on this handle, substituting for it a long rod shaped as an eccentric, and passing through




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