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Project Gutenberg's Encyclopedia, vol. 1 ( A - Andropha

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to D= 1/2 (f1+f2), known as the ``condition for oculars.'' 

If a constant of reproduction, for instance the focal length, 
be made equal for two colours, then it is not the same for 
other colours, if two different glasses are employed.  For 
example, the condition for achromatism (4) for two thin lenses 
in contact is fulfilled in only one part of the spectrum, since 
dn2/dn1 varies within the spectrum.  This fact was first 
ascertained by J. Fraunhofer, who defined the colours by means 
of the dark lines in the solar spectrum; and showed that the 
ratio of the dispersion of two glasses varied about 20% from the 
red to the violet (the variation for glass and water is about 
50%).  If, therefore, for two colours, a and b, fa = 
fb = f, then for a third colour, c, the focal length is 
different, viz. if c lie between a and b, then fc<
f, and vice versa; these algebraic results follow from 
the fact that towards the red the dispersion of the positive 
crown glass preponderates, towards the violet that of the 
negative flint.  These chromatic errors of systems, which 
are achromatic for two colours, are called the ``secondary 
spectrum,'' and depend upon the aperture and focal length 
in the same manner as the primary chromatid errors do. 

In fig. 11, taken from M. von Rohr,s Theoric und Geschichte des 
photographischen Objectivs, the abscissae are focal lengths, and the 
ordinates wave-lengths; of the latter the Fraunhofer lines used are-- 


 
 A'       C      D   Green Hg.   F    G'    Violet Hg.
 767.7  656.3  589.3  546.1    486.2 454.1  405.1 mm,
 

and the focal lengths are made equal for the lines C and F. 
In the neighbourhood of 550 mm the tangent to the curve 
is parallel to the axis of wave-lengths; and the focal 
length varies least over a fairly large range of colour, 
therefore in this neighbourhood the colour union is at its 
best.  Moreover, this region of the spectrum is that which 
appears brightest to the human eye, and consequently this 
curve of the secondary on spectrum, obtained by making 
fc = fF, is, according to the experiments of Sir G. 
G. Stokes (Proc.  Roy. Soc., 1878), the most suitable for 
visual instruments (``optical achromatism,').  In a similar 
manner, for systems used in photography, the vertex of the 
colour curve must be placed in the position of the maximum 
sensibility of the plates; this is generally supposed to be at 
G'; and to accomplish this the F and violet mercury lines are 
united.  This artifice is specially adopted in objectives for 
astronomical photography (``pure actinic achromatism'').  For 
ordinary photography, however, there is this disadvantage: 
the image on the focussing-screen and the correct adjustment 
of the photographic sensitive plate are not in register; in 
astronomical photography this difference is constant, but in 
other kinds it depends on the distance of the objects.  On this 
account the lines D and G' are united for ordinary photographic 
objectives; the optical as well as the actinic image is 
chromatically inferior, but both lie in the same place; and 
consequently the best correction lies in F (this is known as 
the ``actinic correction'' or ``freedom from chemical focus''). 

Should there be in two lenses in contact the same focal lengths 
for three colours a, b, and c, i.e. fa = fb = 
fc = f, then the relative partial dispersion (nc-
nb) (na-nb) must be equal for the two kinds of glass 
employed.  This follows by considering equation (4) for the 
two pairs of colours ac and bc. Until recently no glasses 
were known with a proportionap degree of absorption; but R. 
Blair (Trans.  Edin.  Soc., 1791, 3, p. 3), P. Barlow, and 
F. S. Archer overcame the difficulty by constructing fluid 
lenses between glass walls.  Fraunhofer prepared glasses which 
reduced the secondary spectrum; but permanent success was 
only assured on the introduction of the Jena glasses by E. 
Abbe and O. Schott.  In using glasses not having proportional 
dispersion, the deviation of a third colour can be eliminated 
by two lenses, if an interval be allowed between them; or 
by three lenses in contact, which may not all consist of 
the old glasses.  In uniting three colours an ``achromatism 
of a higher order'' is derived; there is yet a residual 
``tertiary spectrum,'' but it can always be neglected. 

The Gaussian theory is only an approximation; monochromatic 
or spherical aberrations still occur, which will be different 
for different colours; and should they be compensated for one 
colour, the image of another colour would prove disturbing.  
The most important is the chromatic difference of aberration 
of the axis point, which is still present to disturb the 
image, after par-axial rays of different colours are united 
by an appropriate combination of glasses.  If a collective 
system be corrected for the axis point for a definite 
wave-length, then, on account of the greater dispersion in 
the negative components--the flint glasses,--over-correction 
will arise for the shorter wavelengths (this being the 
error of the negative components), and under-correction for 
the longer wave-lengths (the error of crown glass lenses 
preponderating in the red).  This error was treated by 
Jean le Rond d'Alembert, and, in special detail, by C. F. 
Gauss.  It increases rapidly with the aperture, and is more 
important with medium apertures than the secondary spectrum 
of par-axial rays; consequently, spherical aberration must 
be elliminated for two colours, and if this be impossible, 
then it must be eliminated for those particular wave-lengths 
which are most effectual for the instrument in question (a 
graphical representation of this error is given in M. von Rohr, 
Theorie und Geschichte des photographischen Objectivs). 

The condition for the reproduction of a surface element in the 
place of a sharply reproduced point--the constant of the sine 
relationship must also be fulfilled with large apertures for 
several colours.  E. Abbe succeeded in computing microscope 
objectives free from error of the axis point and satisfying 
the sine condition for several colours, which therefore, 
according to his definition, were ``aplanatic for several 
colours''; such systems he termed ``apochromatic''.  While, 
however, the magnification of the individual zones is the 
same, it is not the same for red as for blue; and there is a 
chromatic difference of magnification.  This is produced in the 
same amount, but in the opposite sense, by the oculars, which 
ate used with these objectives (``compensating oculars''), so 
that it is eliminated in the image of the whole microscope.  
The best telescope objectives, and photographic objectives 
intended for three-colour work, are also apochromatic, even 
if they do not possess quite the same quality of correction 
as microscope objectives do.  The chromatic differences of 
other errors of reproduction have seldom practical importances. 

1 The investigations of E. Abbe on geometrical optics, 
originally published only in his university lectures, were 
first compiled by S. Czapski in 1893.  See below, AUTHORITIES. 
AUTHORITIES.---The standard treatise in English is H. D. 
Taylor, A System of Applied Optics (1906); reference may also 
be made to R. S. Heath, A Treatise on Geometrical Optics (2nd 
ed., 1895); and L A. Herman, A Treatise on Geometrical Optics 
(1900).  The ideas of Abbe were first dealt with in S. Czapski, 
Theorie der optischen Instrumente nach Abbe, published 
separately at Breslau in 1893, and as vol. ii. of Winkelmann's 
Handbuch der Physik in 1894; a second edition, by Czapski 
and O. Eppenstein, was published at Leipzig in 1903 with the 
title, Grundzuge der Theorie der optischen Instrumente nach 
Abbe, and in vol. ii. of the 2nd ed. of Winkelmann's Handbuch 
der Physik. The collection of the scientific staff of Carl 
Zeiss at Jena, edited by M. von Rohr, Die bilderzeugung in 
optischen Instrumenten vom Standpunkte der geometrischen 
Optik (Berlin, 1904), contains articles by A. Konig and 
M. von Rohr specially dealing with aberrations. (O. E.) 

ABERSYCHAN, an urban district in the northern parliamentary 
division of Monmouthshire, England, 11 m.  N. by W. of Newport, 
on the Great Western, London and North-Western, and Rhymney 
railways.  Pop. (1901) 17,768.  It lies in the narrow upper 
valley of the Afon Lwyd on the eastern edge of the great coal 
and iron mining district of Glamorganshire and Monmouthshire, 
and its large industrial population is occupied in the mines 
and ironworks.  The neighbourhood is wild and mountainous. 

ABERTILLERY, an urban district in the western parliamentary 
division of Monmouthshire, England, 16 m.  N.W. of Newport, on 
the Great Western railway.  Pop. (1891) 10,846; (1901) 21,945.  
It lies in the mountainous mining district of Monmouthshire 
and Glamorganshire, in the valley of the Ebbw Fach, and the 
large industrial population is mainly employed in the numerous 
coalmines, ironworks and tinplate works.  Farther up the 
valley are the mining townships of NANTYOLO and BLAINA, 
forming an urban district with a population (1901) of 13,489. 

ABERYSTWYTH, a municipal borough, market-town and seaport of 
Cardiganshire, Wales, near the confluence of the rivers Ystwyth 
and Rheidol, about the middle of Cardigan Bay. Pop. (1901) 
8013.  It is the terminal station of the Cambrian railway, 
and also of the Manchester and Milford line.  It is the 
most popular watering-place on the west coast of Wales, and 
possesses a pier, and a fine sea-front which stretches from 
Constitution Hill at the north end of the Marine Terrace to the 
mouth of the harbour.  The town is of modern appearance, and 
contains many public buildings, of which the most remarkable 
is the imposing but fantastic structure of the University 
College of Wales near the Castle Hill.  Much of the finest 
scenery in mid-Wales hes within easy reach of Aberystwyth. 

The history of Aberystwyth may be said to date from the time 
of Gilbert Strongbow, who in 1109 erected a fortress on the 
present Castle Hill.  Edward I. rebuilt Strongbow's castle 
in 1277, after its destruction by the Welsh.  Between the 
years 1404 and 1408 Aberystwyth Castle was in the hands of 
Owen Glendower, but finally surrendered to Prince Harry of 
Monmouth, and shortly after this the town was incorporated 
under the title of Ville de Lampadarn, the ancient name of the 
place being Llanbadarn Gaerog, or the fortified Llanbadarn, 
to distinguish it from Llanbadarn Fawr, the village one mile 
inland.  It is thus styled in a charter granted by Henry 
VIII., but by Elizabeth's time the town was invariably termed 
Aberystwyth in all documents.  In 1647 the parliamentarian 
troops razed the castle to the ground, so that its remains 
are now inconsiderable, though portions of three towers still 
exist.  Aberystwyth was a contributory parliamentary borough 
until 1885, when its representation was merged in that of the 
county.  In modern times Aberystwyth has become a Welsh 
educational centre, owing to the erection here of one of the 
three colleges of the university of Wales (1872), and of a 
hostel for women in connexion with it.  In 1905 it was decided 
to fix here the site of the proposed Welsh National Library. 

ABETTOR (from ``to abet,'' O. Fr. abeter, a and beter, to 
bait, urge dogs upon any one; this word is probably of Scandinavian 
origin, meaning to cause to bite), a law term implying one 
who instigates, encourages or assists another to commit an 
offence.  An abettor differs from an accessory (q.v.) in that 
he must be present at the commission of the crime; all abettors 
(with certain exceptions) are principals, and, in the absence
of specific statutory provision to the contrary, are punishable 
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