scholarly journals XVII. Description of a Magnetimeter, being a New Instrument for Measuring Magnetic Attractions, and Finding the Dip of the Needle; with an Account of Experiments made with it

1823 ◽  
Vol 9 (1) ◽  
pp. 243-258 ◽  
Author(s):  
William Scoresby
Keyword(s):  

About ten months ago, I had the honour of communicating to the Royal Society, a description of a new instrument for ascertaining the Magnetic Dip. Having made very considerable improvements in the apparatus, by means of which some curious results on the magnetic laws, especially those that relate to the production and annihilation of magnetism in iron, have been obtained,—I now beg leave to submit to the Society a drawing and description of my improved instrument, together with an outline of some of the most interesting experiments made with it. Many of the results appear to me to be new; if so, their importance will be my excuse for repeating some parts of the description given in the former paper. It has been long known that iron might be rendered magnetical by percussion; but I am not aware that the precise effect of position has ever been suggested, I remain, &c.

1859 ◽  
Vol 9 ◽  
pp. 194-196

In a former paper “ On the Phenomenon of Relief of the Image formed on the ground glass of the Camera Obscura,” which I com­municated to the Royal Society on the 8th of May 1856, after having investigated the cause of that extraordinary fact and tried to explain it, I found that the images produced separately by the various points of the whole aperture of an object-glass are visible only when the refracted rays are falling on the ground glass in a line nearly coinciding with the optic axes ; so that when both eyes are equally distant from the centre of the ground glass, each eye perceives only the image refracted in an oblique direction on that surface from the opposite side of the object-glass. Consequently each side of an object-glass, in proportion to its aperture, giving a different perspec­tive of a solid placed before it, the result is an illusion of relief as conspicuous as when looking naturally at the objects themselves. From the consideration of these singular facts, unnoticed before, I was led to think that it would be possible to construct a new Stereoscope, in which looking with both eyes at once on a ground glass at the point of coalescence of the two images of a stereoscopic slide, each refracted by a separate lens, we could see it on that surface in the same relief which is produced by the common stereoscope.


1875 ◽  
Vol 23 (156-163) ◽  
pp. 390-408

The mode of expressing Intervals . In the original paper presented by the writer to the Royal Society logarithms were employed as the measure of intervals, as they have been commonly employed by others. Great advantages have been found, however, to result from the adoption of the equal temperament (E. T.) mitone, which is 1/12 of an octave, as the unit of interval. It is the unit most familiar to musicians, and has been found to admit of the expression of the theory of cyclical systems by means of formulæ of the simplest character. The writer therefore devised the following rules for the transformation of ratios into E. T. semitones and vice versâ , and subsequently found that De Morgan had given rules for the same purpose which are substantially the same (Camb. Phil. Trans, vol. x. p. 129). The rules obviously depend on the form of log 2. The form of the first e affords a little more accuracy than De Morgan’s.


1874 ◽  
Vol 22 (148-155) ◽  
pp. 42-42

In a paper “On the Mechanical Conditions of the Respiratory Movements,” read before the Royal Society in November 1872, the author endeavoured to show that there is a distinct difference in the chord lengths of a sternal rib in the two positions of full inspiration and forced expiration, and that a certain degree of bending of the ribs usually takes place in forced breathing. The measurements on which these conclusions were based were made with a 3-plane stethometer, the performance of which was not sufficiently accurate to satisfy the author, who has accordingly repeated them by the aid of a new instrument, the construction and use of which are described at length in the present communication. The author considers that the new instrument gives fairly accurate results, which fully corroborate the conclusions previosly enunciated.


1972 ◽  
Vol 25 (4) ◽  
pp. 528-534
Author(s):  
Charles H. Cotter

John Hadley (1670–1744), Vice-President of the Royal Society of London, communicated his ‘Description of a new Instrument for taking Angles’ to the Society on 13 May 1731. Hadley's invention for the first time provided the navigator with an instrument by which he could measure altitudes of celestial bodies with ease and accuracy on board a lively ship at sea. It was not however until about 1750, when the instrument was to be found on board vessels of the East India Company, that Hadley's quadrant (or octant as it is sometimes called) rapidly came into general use.


1975 ◽  
Vol 8 (2) ◽  
pp. 101-126 ◽  
Author(s):  
Zev Bechler

There is no evidence to suggest that even as late as January 1672, when Newton was elected a Fellow of the Royal Society, anyone (except those unknown few who had in the previous years attended his Lucasian lectures at Cambridge) had any inkling of his new theory of colours. His name exploded on the scientific scene as the inventor and constructor of a new kind of telescope—what later became known as the reflector (which was somewhat misleading compared with its name during the seventeenth century: the catadioptrical telescope). Had the erudition of the London virtuosi been a little broader, they would have known that in fact he was not the inventor of the telescope, even though the precise form he gave it was his. Not only was the idea a hundred years old, during which period it was repeatedly suggested by various writers, but also Newton himself took the idea straight from the most recent of these suggestions, namely that included in James Gregory's Optica promota of 1663. The situation becomes even more ironic when we realize that the new instrument was admired for wrong reasons and on merits that were far from Newton's intentions. Nevertheless, admired it was, and there was a good reason for this: Newton's instrument was in fact the first reflector actually to be constructed and, moreover, for a few weeks (before its mirror became tarnished) it performed quite well. Several astonomers became interested because of the high magnifying power relative to its dimensions (about 7 inches long, with a magnification of 38).


Author(s):  
H. Tochigi ◽  
H. Uchida ◽  
S. Shirai ◽  
K. Akashi ◽  
D. J. Evins ◽  
...  

A New High Excitation Objective Lens (Second-Zone Objective Lens) was discussed at Twenty-Sixth Annual EMSA Meeting. A new commercially available Transmission Electron Microscope incorporating this new lens has been completed.Major advantages of the new instrument allow an extremely small beam to be produced on the specimen plane which minimizes specimen beam damages, reduces contamination and drift.


Author(s):  
John F. Mansfield

The current imaging trend in optical microscopy, scanning electron microscopy (SEM) or transmission electron microscopy (TEM) is to record all data digitally. Most manufacturers currently market digital acquisition systems with their microscope packages. The advantages of digital acquisition include: almost instant viewing of the data as a high-quaity positive image (a major benefit when compared to TEM images recorded onto film, where one must wait until after the microscope session to develop the images); the ability to readily quantify features in the images and measure intensities; and extremely compact storage (removable 5.25” storage devices which now can hold up to several gigabytes of data).The problem for many researchers, however, is that they have perfectly serviceable microscopes that they routinely use that have no digital imaging capabilities with little hope of purchasing a new instrument.


Author(s):  
Lee H. Veneklasen

This paper discusses some of the unique aspects of a spectroscopic emission microscope now being tested in Clausthal. The instrument is designed for the direct parallel imaging of both elastic and inelastic electrons from flat surfaces. Elastic contrast modes of the familiar LEEM include large and small angle LEED, mirror microscopy, backscatter diffraction contrast (for imaging of surface structure), and phase contrast (for imaging of step dynamics)(1). Inelastic modes include topology sensitive secondary, and work function sensitive photoemission. Most important, the new instrument will also allow analytical imaging using characteristic Auger or soft X-ray emissions. The basic instrument has been described by Bauer and Telieps (2). This configuration has been redesigned to include an airlock, and a LaB6 gun, triple condensor lens, magnetic objective lens, a double focussing separator field, an imaging energy analyzer, and a real time image processor.Fig. 1 shows the new configuration. The basic beam voltage supply Vo = 20 KV, upon which separate supplies for the gun Vg, specimen Vs, lens electrode Vf, and analyzer bias Vb float. The incident energy at the sample can be varied from Vs = 0-1 KV for elastic imaging, or from Vg + Vs = (3 + Vs) KV for inelastic imaging. The image energy window Vs±V/2 may be varied without readjusting either the illumation, or imaging/analyzer optics. The diagram shows conjugate diffraction and image planes. The apertures defining incoming Humiliation and outgoing image angles are placed below the separator magnet to allow for their independent optimization. The instrument can illuminate and image 0.5-100 μm fields at 0-1 keV emission energies with an energy window down to 0.2 eV.


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