CHAPTER IX

THE MAGNETIC AND METEOROLOGICAL DEPARTMENTS

Passing out of the south door of the new altazimuth building, we

come to a white cruciform erection, constructed entirely of wood.

This is the Magnet House or Magnetic Observatory, the home of a

double Department, the Magnetic and Meteorological.

This department does not, indeed, lie within the original purpose

of the Observatory as that was defined in the warrant given to

Flamsteed, and yet is so intimately connected with it, through its

bearing on navigation, that there can be no question as to its

suitability at Greenwich. Indeed, its creation is a striking example

of the thorough grasp which Airy had upon the essential principles

which should govern the great national observatory of an essentially

naval race, and of the keen insight with which he watched the new

development of science. The Magnetic Observatory, therefore, the

purpose of which was to deal with the observation of the changes in

the force and direction of the earth's magnetism--an inquiry which

the greater delicacy of modern compasses, and, in more recent times,

the use of iron instead of wood in the construction of ships has

rendered imperative--was suggested by Airy on the first possible

occasion after he entered on his office, and was sanctioned in 1837.

The Meteorological Department has a double bearing on the purpose of

the Observatory. On the one side, a knowledge of the temperature and

pressure of the atmosphere is, as we have already seen, necessary

in order to correct astronomical observations for the effect of

refraction. On the other hand, meteorology proper, the study of

the movements of the atmosphere, the elucidation of the laws which

regulate those movements, leading to accurate forecasts of storms,

are of the very first necessity for the safety of our shipping.

It is true that weather forecasts are not issued from Greenwich

Observatory, any more than the _Nautical Almanac_ is now issued from

it; but just as the Observatory furnishes the astronomical data upon

which the Almanac is based, so also it takes its part in furnishing

observations to be used by the Meteorological Office at Westminster

for its daily predictions.

Those predictions are often made the subject of much cheap ridicule;

but, however far short they may fall of the exact and accurate

predictions which we would like to have, yet they mark an enormous

advance upon the weather-lore of our immediate forefathers.

'He that is weather wise

Is seldom other wise,'

says the proverb, and the saying is not without a shrewd amount of

truth. For perhaps nowhere can we find a more striking combination

of imperfect observation and inconsequent deduction than in the

saws which form the stock-in-trade of the ordinary would-be weather

prophet. How common it is to find men full of the conviction that

the weather must change at the co-called 'changes of the moon,'

forgetful that

'If we'd no moon at all--

And that may seem strange--

We still should have weather

That's subject to change.'

They will say, truly enough, no doubt, that they have known the

weather to change at 'new' or 'full,' as the case may be, and they

argue that it, therefore, must always do so. But, in fact, they have

only noted a few chance coincidences, and have let the great number

of discordances pass by unnoticed.

But observations of this kind seem scientific and respectable

compared with those numerous weather proverbs which are based upon

the mere jingle of a rhyme, as

'If the ash is out before the oak,

You may expect a thorough soak'--

a proverb which is deftly inverted in some districts by making 'oak'

rhyme to 'choke.'

Others, again, are based upon a mere childish fancy, as, for

example, when the young moon 'lying on her back' is supposed to bode

a spell of dry weather, because it looks like a cup, and so might be

thought of as able to hold the water.

During the present reign, however, a very different method of

weather study has come into action, and the foundations of a

true weather wisdom have been laid. These have been based, not

on fancied analogies or old wives' rhymes, or a few forechosen

coincidences, but upon observations carried on for long periods of

time and over wide areas of country, and discussed in their entirety

without selection and bias. Above all, mathematical analysis has

been applied to the motions of the air, and ideas, ever gaining

in precision and exactness, have been formulated of the general

circulation of the atmosphere.

As compared with its sister science, astronomy, meteorology appears

to be still in a very undeveloped state. There is such a difference

between the power of the astronomer to foretell the precise position

of sun, moon, and planets for years, even for centuries, beforehand,

and the failure of the meteorologist to predict the weather for a

single season ahead, that the impression has been widely spread that

there is yet no true meteorological science at all. It is forgotten

that astronomy offered us, in the movements of the heavenly bodies,

the very simplest and easiest problem of related motion. Yet for how

many thousands of years did men watch the planets, and speculate

concerning their motions, before the labours of Tycho, Kepler, and

Newton culminated in the revelation of their meaning? For countless

generations it was supposed that their movements regulated the

lives, characters, and private fortunes of individual men; just as

quite recently it was fancied that a new moon falling on a Saturday,

or two full moons coming within the same calendar month, brought bad

weather!

It is still impossible to foresee the course of weather change for

long ahead; but the difference between the modern navigator, surely

and confidently making a 'bee-line' across thousands of miles of

ocean to his destination, and the timid sailor of old, creeping from

point to point of land, is hardly greater than the contrast between

the same two men, the one watching his barometer, the other trusting

in the old wives' rhymes which afforded him his only indication as

to coming storms.

It is still impossible to foresee the weather change for long ahead,

but in our own and in many other countries, especially the United

States, it has been found possible to predict the weather of the

coming four-and-twenty hours with very considerable exactness, and

often to forecast the coming of a great storm several days ahead.

This is the chief purpose of the two great observatories of the

storm-swept Indian and Chinese seas, Hong Kong and Mauritius; and

the value of the work which they have done in preventing the loss

of ships, and the consequent loss of lives and property, has been

beyond all estimate.

The Royal Observatory, Greenwich, is a meteorological as well as an

astronomical observatory, but, as remarked above, it does not itself

issue any weather forecasts. Just as the Greenwich observations

of the places of the moon and stars are sent to the _Nautical

Almanac_ Office, for use in the preparation of that ephemeris; just

as the Greenwich determinations of time are used for the issue of

signals to the Post Office, whence they are distributed over the

kingdom, so the Greenwich observations of weather are sent to the

Meteorological Office, there to be combined with similar records

from every part of the British Isles, to form the basis of the

daily forecasts which the latter office publishes. To each of these

three offices, therefore, the Royal Observatory, Greenwich, stands

in the relation of purveyor. It supplies them with the original

observations more or less in reduced and corrected form, without

which they could not carry on most important portions of their work.

Let it be noted how closely these three several departments,

the _Nautical Almanac_ Office, the Time Department, and the

Meteorological Office, are related to practical navigation. Whatever

questions of pure science--of knowledge, that is, apart from its

useful applications--may arise out of the following up of these

several inquiries, yet the first thought, the first principle of

each, is to render navigation more sure and more safe.

The first of all meteorological instruments is the barometer, which,

under its two chief forms of mercurial and aneroid, is simply a

means of measuring the pressure exerted by the atmosphere.

There are two important corrections to which its readings are

subject. The first is for the height of the station above the

level of the sea; the second is for the effect of temperature upon

the mercury in the barometer itself, lengthening the column. To

overcome these, the height of the standard barometer at Greenwich

above sea-level has been most carefully ascertained, and the

heights relative to it of the other barometers of the Observatory,

particularly those in rooms occupied by fundamental telescopes,

have also been determined, whilst the self-recording barometer is

mounted in a basement, where it is almost completely protected from

changes of temperature.

Next in importance to the barometer as a meteorological instrument

comes the thermometer. The great difficulty in the Observatory

use of the thermometer is to secure a perfectly unexceptionable

exposure, so that the thermometer may be in free and perfect contact

with the air, and yet completely sheltered from any direct ray from

the sun. This is secured in the great thermometer shed at Greenwich

by a double series of 'louvre' boards, on the east, south, and west

sides of the shed, the north side being open. The shed itself is

made a very roomy one, in order to give access to a greater body of

air.

A most important use of the thermometer is in the measurement

of the amount of moisture in the air. To obtain this, a pair of

thermometers are mounted close together, the bulb of one being

covered by damp muslin, and the other being freely exposed. If

the air is completely saturated with moisture, no evaporation

can take place from the damp muslin, and consequently the two

thermometers will read the same. But if the air be comparatively

dry, more or less evaporation will take place from the wet bulb,

and its temperature will sink to that at which the air would be

fully saturated with the moisture which it already contained. For

the higher the temperature, the greater is its power of containing

moisture. The difference of the reading of the two thermometers is,

therefore, an index of humidity. The greater the difference, the

greater the power of absorbing moisture, or, in other words, the

dryness of the air. The great shed already alluded to is devoted to

these companion thermometers.

[Illustration: THE SELF-REGISTERING THERMOMETERS.]

Very closely connected with atmospheric pressure, as shown us by the

barometer, is the study of the direction of winds. If we take a map

of the British Isles and the neighbouring countries, and put down

upon them the barometer readings from a great number of observing

stations, and then join together the different places which show the

same barometric pressure, we shall find that these lines of equal

pressure--technically called 'isobars'--are apt to run much nearer

together in some places than in others. Clearly, where the isobars

are close together it means that in a very short distance of country

we have a great difference of atmospheric pressure. In this case

we are likely to get a very strong wind blowing from the region of

high pressure to the region of low pressure, in order to restore the

balance.

If, further, we had information from these various observing

stations of the direction in which the wind was blowing, we should

soon perceive other relationships. For instance, if we found that

the barometer read about the same in a line across the country from

east to west, but that it was higher in the north of the islands

than in the south, we should then have a general set of winds from

the east, and a similar relation would hold good if the barometer

were highest in some other quarter; that is, the prevailing wind

will come from a quarter at right angles to the region of highest

barometer, or, as it is expressed in what is known as 'Buys Ballot's

law,' 'stand with your back to the wind, and the barometer will be

lower on your left hand than on your right.' This law holds good for

the northern hemisphere generally, except near to the equator; in

the southern hemisphere the right hand is the side of low barometer.

The instruments for wind observation are of two classes: vanes

to show its direction, and anemometers to show its speed and its

pressure. These may be regarded as two different modes in which the

strength of the wind manifests itself. Pressure anemometers are

usually of two forms: one in which a heavy plate is allowed to swing

by its upper edge in a position fronting the wind, the amount of its

deviation from the vertical being measured; and the other in which

the plate is supported by springs, the degree of compression of the

springs being the quantity registered in that case. Of the speed

anemometers, the best known form is the 'Robinson,' in which four

hemispherical cups are carried at the extremities of a couple of

cross bars.

For the mounting of these wind instruments the old original

Observatory, known as the Octagon Room, has proved an excellent

site, with its flat roof surmounted by two turrets in the north-east

and north-west corners, and raised some two hundred feet above

high-water mark.

[Illustration: THE ANEMOMETER ROOM, NORTH-WEST TURRET.]

The two chief remaining instruments are those for measuring the

amount of rainfall and of full sunshine. The rain gauge consists

essentially of a funnel to collect the rain, and a graduated glass

to measure it. The sunshine recorder usually consists of a large

glass globe arranged to throw an image of the sun on a piece of

specially prepared paper. This image, as the sun moves in the sky,

moves along the paper, charring it as it moves, and at the end of

the day it is easy to see, from the broken, burnt trace, at what

hours the sun was shining clear, and when it was hidden by cloud.

An amusing difficulty was encountered in an attempt to set on

foot another inquiry. The Superintendent of the Meteorological

Department at the time wished to have a measure of the rate at which

evaporation took place, and therefore exposed carefully measured

quantities of water in the open air in a shallow vessel. For a few

days the record seemed quite satisfactory. Then the evaporation

showed a sudden increase, and developed in the most erratic

and inexplicable manner, until it was found that some sparrows

had come to the conclusion that the saucer full of water was a

kindly provision for their morning 'tub,' and had made use of it

accordingly.

A large proportion of the meteorological instruments at

Greenwich and other first-class observatories are arranged to be

self-recording. It was early felt that it was necessary that the

records of the barometer and thermometer should be as nearly as

possible continuous; and at one time, within the memory of members

of the staff still living, it was the duty of the observer to read

a certain set of instruments at regular two-hour intervals during

the whole of the day and night--a work probably the most monotonous,

trying, and distasteful of any that the Observatory had to show.

The two-hour record was no doubt practically equivalent to a

continuous one, but it entailed a heavy amount of labour. Automatic

registers were, therefore, introduced whenever they were available.

The earliest of these were mechanical, and several still make their

records in this manner.

On the roof of the Octagon Room we find, beside the two turrets

already referred to, a small wooden cabin built on a platform

several feet above the roof level. This cabin and the north-western

turret contain the wind-registering instruments. Opening the turret

door, we find ourselves in a tiny room which is nearly filled by

a small table. Upon this table lies a graduated sheet of paper in

a metal frame, and as we look at it, we see that a clock set up

close to the table is slowly drawing the paper across it. Three

little pencils rest lightly on the face of the paper at different

points. One of these, and usually the most restless, is connected

with a spindle which comes down into the turret from the roof, and

which is, in fact, the spindle of the wind vane. The gearing is so

contrived that the motion on a pivot of the vane is turned into

motion in a straight line at right angles to the direction in which

the paper is drawn by the clock. A second pencil is connected with

the wind-pressure anemometer. The third pencil indicates the amount

of rain that has fallen since the last setting, the pencil being

moved by a float in the receiver of the rain gauge.

[Illustration: THE ANEMOMETER TRACE.]

An objection to all the mechanical methods of continuous

registration is that, however carefully the gearing between the

instrument itself and the pencil is contrived, however lightly

the pencil moves over the paper, yet some friction enters in

and affects the record: this is of no great moment in wind

registration, when we are dealing with so powerful an agent as

the wind, but it becomes a serious matter when the barometer is

considered, since its variations require to be registered with the

greatest minuteness. When photography, therefore, was invented,

meteorologists were very prompt to take advantage of this new ally.

A beam of light passing over the head of the column of mercury in a

thermometer or barometer could easily be made to fall upon a drum

revolving once in the twenty-four hours, and covered with a sheet

of photographic paper. In this case, when the sensitive paper is

developed, we find its upper half blackened, the lower edge of the

blackened part showing an irregular curve according as the mercury

in the thermometer or barometer rose or fell, and admitted less or

more light through the space above it.

Here we have a very perfect means of registration: the passage of

the light exercises no friction or check on the free motion of the

mercury in the tube, or on the turning of the cylinder covered by

the sensitive paper, whilst it is easy to obtain a time scale on the

register by cutting off the light for an instant--say at each hour.

In this way the wet and dry bulb thermometers in the great shed make

their registers.

The supply of material to the Meteorological Office is not the only

use of the Greenwich meteorological observations. Two elements of

meteorology, the temperature and the pressure of the atmosphere,

have the very directest bearing upon astronomical work. And this

in two ways. An instrument is sensible to heat and cold, and

undergoes changes of form, size, or scale, which, however absolutely

minute, yet become, with the increased delicacy of modern work, not

merely appreciable, but important. So too with the density of the

atmosphere: the light from a distant star, entering our atmosphere,

suffers refraction; and being thus bent out of its path, the star

appears higher in the heavens than it really is. The amount of this

bending varies with the density of the layers of air through which

the light has to pass. The two great meteorological instruments, the

thermometer and barometer, are therefore astronomical instruments as

well.

In the arrangements at Greenwich the Magnetic Department is closely

connected with the Meteorological, and it is because the two

departments have been associated together that the building devoted

to both is constructed of wood, not brick, since ordinary bricks are

made of clay which is apt to be more or less ferruginous. Copper

nails have alone been employed in the construction of the buildings.

The fire-grates, coal-scuttles, and fire-irons are all of the same

metal.

The growth of the Observatory has, however, made it necessary to

set up some of the new telescopes, into the mounting of which much

iron enters, very close to the magnetic building. The present

Astronomer-Royal has therefore erected a Magnetic Pavilion right out

in the park at an ample distance from these disturbing causes.

The double department is, therefore, the most widely scattered in

the whole Observatory. It is located for computing purposes in the

west wing of the New Observatory; many of its magnetic instruments

are in the old Magnet House, others are across the park in the new

Magnetic Pavilion; the anemometers are on the roof of the Octagon

Room, Flamsteed's original observatory, and the self-registering

thermometers are in the south ground between the old Magnet House

and the New Observatory.

[Illustration: MAGNETIC PAVILION--EXTERIOR.

(_From a photograph by Mr. Lacey._)]

The object of the Magnetic Observatory is to study the movements of

the magnetic needle. The quaintest answer that I ever received in an

examination was in reply to the question, 'What is meant by magnetic

inclination and declination?' The examinee replied:

'To make a magnet, you take a needle, and rub it on a lodestone.

If it refuses or _declines_ to become a magnet, that is magnetic

declination; if it is easily made a magnet, or is _inclined_ to

become one, that is magnetic inclination.'

One greatly regretted that it was necessary to mark the reply

according to its ignorance, and not, as one would have wished, in

proportion to its ingenuity. Magnetic declination, however, as

everybody knows, measures the deviation of the 'needle' from the

true geographical north and south direction; the inclination or dip

is the angle which a 'needle' makes with the horizon.

At one time the only method of watching the movements of the

magnetic needles was by direct observation, just precisely as it was

wont to be in the case of the barometer and thermometer. But the

same agent that has been called in to help in their case has enabled

the magnets also to give us a direct and continuous record of their

movements. In principle the arrangement is as follows: A small light

mirror is attached to the magnetic needle, and a beam of light is

arranged to fall upon the mirror, and is reflected away from it to a

drum covered with sensitive paper. If, then, the needle is perfectly

at rest, a spot of light falls on the drum and blackens the paper at

one particular point. The drum is made to revolve by clockwork once

in twenty-four hours, and the black dot is therefore lengthened out

into a straight line encircling the drum. If, however, the needle

moves, then the spot of light travels up or down, as the case may

be.

Now, if we look at one of these sheets of photographic paper after

it has been taken from the drum, we shall see that the north pole of

the magnet has moved a little, a very little, towards the west in

the early part of the day, say from sunrise to 2 p.m., and has swung

backwards from that hour till about 10 p.m., remaining fairly quiet

during the night. The extent of this daily swing is but small, but

it is greater in summer than in winter, and it varies also from year

to year.

[Illustration: MAGNETIC PAVILION--INTERIOR.

(_From a photograph by Mr. Lacey._)]

Besides this daily swing, there occasionally happen what are called

'magnetic storms;' great convulsive twitchings of the needle, as

if some unseen operator were endeavouring, whilst in a state of

intense excitement, to telegraph a message of vast importance, so

rapid and so sharp are the movements of the needle to and fro. These

great storms are felt, so far as we know, simultaneously over the

whole earth, and the more characteristic begin with a single sharp

twitch of the needle towards the east.

Besides the movements of the magnetic needle, the intensity of the

currents of electricity which are always passing through the crust

of the earth are also determined at Greenwich; but this work has

been rendered practically useless for the last few years by the

construction of the electric railway from Stockwell to the City.

Since it was opened, the photographic register of earth currents

has shown a broad blurring from the moment of the starting of the

first train in the morning to the stopping of the last train at

night. As an indication of the delicacy of modern instruments, it

may be mentioned that distinct indications of the current from this

railway have been detected as far off as North Walsham, in Norfolk,

a distance of more than a hundred miles. A further illustration of

the delicacy of the magnetic needles was afforded shortly after

the opening of the railway referred to. On one occasion the then

Superintendent of the Magnetic Department visited the Generating

Station at Stockwell, and on his return it was noticed day after day

that the traces from the magnets showed a curious deflection from 9

a.m. to 3 p.m., the hours of his attendance. This gave rise to some

speculation, as it did not seem possible that the gentleman could

himself have become magnetized. Eventually, the happy accident

of a fine day solved the mystery. That morning the Superintendent

left his umbrella at home, and the magnets were undisturbed. The

secret was out. The umbrella had become a permanent magnet, and its

presence in the lobby of the magnetic house had been sufficient to

influence the needles.

The Royal Observatory, Greenwich: A Glance at Its History and Work · 第 9 / 13 章