_Influence of the Heat of the Soil._--It is well known that

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TROPICAL NATURE,

AND OTHER ESSAYS.

[Illustration]

TROPICAL NATURE,

AND

OTHER ESSAYS.

BY

ALFRED R. WALLACE.

AUTHOR OF “THE MALAY ARCHIPELAGO,” “THE GEOGRAPHICAL DISTRIBUTION

OF ANIMALS,”“CONTRIBUTIONS TO THE THEORY OF NATURAL SELECTION,”

ETC., ETC.

London:

MACMILLAN AND CO.

1878.

[_The Right of Translation and Reproduction is Reserved._]

LONDON:

R. CLAY, SONS, AND TAYLOR,

BREAD STREET HILL.

THE TROPICS.

Land of the Sun! where joyous green-robed Spring

And leaf-crowned Summer deck the Earth for ever;

No Winter stern their sweet embrace to sever

And numb to silence every living thing,

But bird and insect ever on the wing,

Flitting ’mid forest glades and tangled bowers,

While the life-giving orb’s effulgent beams

Through all the circling year call forth the flowers.

Here graceful palms, here luscious fruits have birth;

The fragrant coffee, life-sustaining rice,

Sweet canes, and wondrous gums, and odorous spice;

While Flora’s choicest treasures crowd the teeming earth.

Beside each cot the golden Orange stands,

And broad-leaved Plantain, pride of Tropic lands.

ENGLAND.

Sweet changing Seasons! Winter cold and stern,

Fair Spring with budding leaf and opening flower,

And Summer when the sun’s creative power

Brings leafy groves and glades of feathery fern,

The glorious blossoms of sweet-scented May,

The flowery hedgerows and the fragrant hay,

And the wide landscape’s many-tinted sheen.

Then Autumn’s yellow woods and days serene;

And when we’ve gathered in the harvest’s treasure,

The long nights bring us round the blazing hearth,

The chosen haunt of every social pleasure.

Land of green fields and flowers! Thou givest birth

To shifting scenes of beauty, which outshine

Th’ unvarying splendours of the Tropic’s clime.

PREFACE.

The luxuriance and beauty of Tropical Nature is a well-worn

theme, and there is little new to say about it. The traveller and

the naturalist have combined to praise, and not unfrequently to

exaggerate the charms of tropical life--its heat and light, its

superb vegetable forms, its brilliant tints of flower and bird

and insect. Each strange and beautiful object has been described

in detail; and both the scenery and the natural phenomena of the

tropics have been depicted by master hands and with glowing colours.

But, so far as I am aware, no one has yet attempted to give a

general view of the phenomena which are _essentially_ tropical,

or to determine the causes and conditions of those phenomena. The

local has not been separated from the general, the accidental from

the essential; and, as a natural result, many erroneous ideas have

become current as to what are really the characteristics of the

tropical as distinguished from the temperate zones.

In the present volume I have attempted to supply this want; and for

my materials have drawn chiefly on my own twelve years’ experience

of the eastern and western tropics of the equatorial zone, where

the characteristic phenomena of tropical life are fully manifested.

So many of the most remarkable forms of life are now restricted to

the tropics, and the relations of these to extinct types which once

inhabited the temperate zones open up so many interesting questions

as to the past history of the earth, that the present inquiry may be

considered a necessary preliminary to a study of the problem--how

to determine the climates of geologic periods from the character

of their organic remains. This part of the subject is however both

complex and difficult, and I have only attempted to indicate what

seem to me the special physical conditions to which the existing

peculiarities of tropical life are mainly due.

The three opening chapters treat the subject under the headings of

climate, vegetation, and animal life. The conditions and causes

of the equatorial climate are discussed in some detail, and the

somewhat complex principles on which it depends are popularly

explained. In the chapters on plant and animal life, the general

aspects and relations of their several component elements have been

dwelt upon; all botanical and zoological details and nomenclature

being excluded, except so far as was absolutely necessary to give

precision to the descriptions and to enable us to deduce from them

some conclusions of importance.

The remaining chapters have all a more or less direct connection

with the leading subject. The family of humming-birds is taken as

an illustration of the luxuriant development of allied forms in the

tropics, and as showing the special mode in which natural selection

has acted to bring about considerable changes in a limited period.

The discussion on the nature and origin of the colours of animals

and plants, is intended to show how far and in what way these are

dependent on the climate and physical conditions of the tropics. The

chapter entitled “By-paths in the Domain of Biology” contains an

account of certain curious relations of colour to locality, which

are almost exclusively manifested within the tropical zones; while

the essay on “Distribution of Animals and Geographical Changes,”

elucidates the relations of the several continents in past time,

and the probable origin of many of the groups now characteristic

of tropical or of temperate regions.

While discussing the general laws and phenomena of colour in the

organic world, and its special developments among certain groups

of animals, I have been led to a theory of the diverse colours of

the sexes and of the special ornaments and brilliant hues which

distinguish certain male birds and insects, which is directly

opposed to the view held by Mr. Darwin and so well explained and

illustrated in his great work on “The Descent of Man and on Selection

in Relation to Sex.” Being strongly impressed with the importance

and fundamental truth of this theory, I published my first sketch of

the subject in _Macmillan’s Magazine_ in order that it might have

the benefit of criticism before making it public in a more permanent

form. Taking advantage of some suggestions from Mr. Darwin and from

a few other correspondents, I have made considerable additions to

the original essay and have rearranged, and I trust strengthened

the argument, which I now hope may attract the attention of all who

are interested in the subject. I may be allowed here to remark,

that my theory cannot be properly understood without reading the

whole chapter on “The Colours of Animals;” because the view set

forth and illustrated in the first part of that chapter--that colour

in nature is normal, and that its presence hardly requires to be

accounted for so much as its absence--is an essential part of the

theory.

CROYDON, _April, 1878_.

CONTENTS.

I. The Climate and Physical Aspects of the Equatorial Zone.

The three Climatal Zones of the Earth--Temperature of the

Equatorial Zone--Causes of the Uniform High Temperature near

the Equator--Influence of the Heat of the Soil--Influence of

the Aqueous Vapour of the Atmosphere--Influence of Winds on

the Temperature of the Equator--Heat due to the Condensation

of Atmospheric Vapour--General Features of the Equatorial

Climate--Uniformity of the Equatorial Climate in all Parts of the

Globe--Effects of Vegetation on Climate--Short Twilight of the

Equatorial Zone--The Aspect of the Equatorial Heavens--Intensity

of Meteorological Phenomena at the Equator--Concluding Remarks

_pages 1-26_

II. Equatorial Vegetation.

The Equatorial Forest-belt and its Causes--General Features of the

Equatorial Forests--Low-growth Forest-trees--Flowery Trunks

and their Probable Cause--Uses of Equatorial Forest-trees--The

Climbing Plants of the Equatorial Forests--Palms--Uses of

Palm-trees and their Products--Ferns--Ginger-worts and Wild

Bananas--Arums--Screw-Pines--Orchids--Bamboos--Uses of the

Bamboo--Mangroves--Sensitive-plants--Comparative Scarcity of

Flowers--Concluding Remarks on Tropical Vegetation _pages 27-68_

III. Animal Life in the Tropical Forests.

Difficulties of the Subject--General Aspect of the Animal Life of

Equatorial Forests--Diurnal Lepidoptera or Butterflies--Peculiar

Habits of Tropical Butterflies--Ants, Wasps, and

Bees--Ants--Special Relations between Ants and Vegetation--Wasps

and Bees--Orthoptera and other Insects--Beetles--Wingless

Insects--General Observations on Tropical

Insects--Birds--Parrots--Pigeons--Picariæ--Cuckoos--Trogons,

Barbets, Toucans and Hornbills--Passeres--Reptiles

and Amphibia--Lizards--Snakes--Frogs and

Toads--Mammalia--Monkeys--Bats--Summary of the Aspects of Animal

Life in the Tropics _pages 69-123_

IV. Humming-Birds: as Illustrating the Luxuriance of Tropical Nature.

Structure--Colours and Ornaments--Descriptive Names--The

Motions and Habits of Humming-Birds--Display of Ornaments

by the Male--Food--Geographical Distribution and

Variation--Humming-Birds of Juan Fernandez as illustrating

Variation and Natural Selection--The Relations and Affinities of

Humming-Birds--How to Determine Doubtful Affinities--Resemblances

of Swifts and Humming-Birds--Differences between Sun-Birds and

Humming-Birds _pages 124-157_

V. The Colours of Animals and Sexual Selection.

General Phenomena of Colour--Theory of Heat and Light as

producing Colour--Changes of Colour in Animals produced by

Coloured Light--Classification of Organic Colours--Protective

Colours--Warning Colours--Sexual Colours--Typical Colours--The

Nature of Colour--How Animal Colours are Produced--Colour

a Normal Product of Organization--Theory of Protective

Colours--Theory of Warning Colours--Imitative Warning

Colours--The Theory of Mimicry--Theory of Sexual Colours--Colour

as a Means of Recognition--Colour proportionate to Integumentary

Development--Selection by Females not a Cause of Colour--Probable

Use of the Horns of Beetles--Cause of the greater Brilliancy of

some Female Insects--Origin of the Ornamental Plumage of Male

Birds--Theory of the Display of Ornaments by Males--Natural

Selection as neutralizing Sexual Selection--Greater Brilliancy

of some Female Birds--Colour-development as illustrated

by Humming-Birds--Theory of Typical Colours--Local Causes

of Colour-development--Summary on Colour-development in

Animals--Concluding Remarks on Causes of Bright Colour in the

Tropics _pages 158-220_

VI. The Colours of Plants and the Origin of the Colour-Sense.

Source of Colouring-matter in Plants--Protective Coloration and

Mimicry in Plants--Attractive Colours of Fruits--Protective

Colours of Fruits--Seeds how Protected--Attractive Colours of

Flowers--Attractive Odours in Flowers--Attractive Grouping

in Flowers--Why Alpine Flowers are so Beautiful--Why Allied

Species of Flowers differ in Size and Beauty--Absence of

Colours in Wind-fertilized Flowers--The same Theory of Colour

applicable to Animals and Plants--Relation of the Colours of

Flowers and their Geographical Distribution--Recent Views as

to the Direct Action of Light on the Colours of Flowers and

Fruits--Concluding Remarks on the Importance of Colour in the

Organic World--The Origin of the Colour-sense.--Supposed Increase

of Colour-perception within the Historical Period--Concluding

Remarks on the Colour-sense _pages 221-248_

VII. BY-PATHS IN THE DOMAIN OF BIOLOGY.

BEING AN ADDRESS DELIVERED TO THE BIOLOGICAL SECTION OF THE BRITISH

ASSOCIATION (GLASGOW, SEPTEMBER 6TH, 1876) AS PRESIDENT OF THE

SECTION.

Introductory Remarks--ON SOME RELATIONS OF LIVING THINGS TO

THEIR ENVIRONMENT.--The Influence of Locality on Colour in

Butterflies and Birds--Sense-perception influenced by Colour of

the Integuments--Relations of Insular Plants and Insects--RISE

AND PROGRESS OF MODERN VIEWS AS TO THE ANTIQUITY AND ORIGIN

OF MAN--Indications of Man’s Extreme Antiquity--Antiquity of

Intellectual Man--Sculptures on Easter-Island--North American

Earthworks--The Great Pyramid--Conclusion _pages 249-303_

VIII. The Distribution of Animals as Indicating Geographical Changes.

Old Opinions on Continental Changes--Theory of Oceanic

Islands--Present and Past Distribution of Land and

Sea--Zoological Regions--The Palæarctic Region--The Ethiopian

Region--The Oriental Region--Past changes of the Great Eastern

Continent--Regions of the New World--Past History of the American

Continents--The Australian Region--Summary and Conclusion

_pages 304-347_

TROPICAL NATURE,

AND OTHER ESSAYS.

I.

THE CLIMATE AND PHYSICAL ASPECTS OF THE EQUATORIAL ZONE.

The three Climatal Zones of the Earth--Temperature of the

Equatorial Zone--Causes of the Uniform High Temperature near

the Equator--Influence of the Heat of the Soil--Influence of

the Aqueous Vapour of the Atmosphere--Influence of Winds on

the Temperature of the Equator--Heat due to the Condensation

of Atmospheric Vapour--General features of the Equatorial

Climate--Uniformity of the Equatorial Climate in all parts of the

globe--Effects of Vegetation on Climate--Short Twilight of the

Equatorial Zone--The aspect of the Equatorial Heavens--Intensity

of meteorological phenomena at the Equator--Concluding Remarks.

It is difficult for an inhabitant of our temperate land to realize

either the sudden and violent contrasts of the arctic seasons or the

wonderful uniformity of the equatorial climate. The lengthening or

the shortening days, the ever-changing tints of spring, summer, and

autumn, succeeded by the leafless boughs of winter, are constantly

recurring phenomena which represent to us the established course

of nature. At the equator none of these changes occur; there is

a perpetual equinox and a perpetual summer, and were it not for

variations in the quantity of rain, in the direction and strength

of the winds, and in the amount of sunshine, accompanied by

corresponding slight changes in the development of vegetable and

animal life, the monotony of nature would be extreme.

In the present chapter it is proposed to describe the chief

peculiarities which distinguish the equatorial from the temperate

climate, and to explain the causes of the difference between

them,--causes which are by no means of so simple a nature as are

usually imagined.

The three great divisions of the earth--the tropical, the

temperate, and the frigid zones, may be briefly defined as the

regions of uniform, of variable, and of extreme physical conditions

respectively. They are primarily determined by the circumstance

of the earth’s axis not being perpendicular to the plane in which

it moves round the sun; whence it follows that during one half

of its revolution the north pole, and during the other half the

south pole, is turned at a considerable angle towards the source

of light and heat. This inclination of the axis on which the earth

rotates is usually defined by the inclination of the equator to

the plane of the orbit, termed the obliquity of the ecliptic. The

amount of this obliquity is 23½ degrees, and this measures the

extent on each side of the equator of what are called the tropics,

because within these limits the sun becomes vertical at noon twice

a year, and at the extreme limit once a year, while beyond this

distance it is never vertical. It will be evident, however, from

the nature of the case, that the two lines which mark the limits of

the geographical “tropics” will not define any abrupt change of

climate or physical conditions, such as characterise the tropical

and temperate zones in their full development. There will be a

gradual transition from one to the other, and in order to study

them separately and contrast their special features we must only

take into account the portion of each in which these are most fully

exhibited. For the temperate zone we may take all countries situated

between 35° and 60° of latitude, which in Europe will include

every place between Christiania and Algiers, the districts further

south forming a transitional belt in which temperate and tropical

features are combined. In order to study the special features of

tropical nature, on the other hand, it will be advisable to confine

our attention mainly to that portion of the globe which extends for

about twelve degrees on each side of the equator, in which all the

chief tropical phenomena dependent on astronomical causes are most

fully manifested, and which we may distinguish as the “equatorial

zone.” In the debateable ground between these two well contrasted

belts local causes have a preponderating influence; and it would not

be difficult to point out localities within the temperate zone of

our maps, which exhibit all the chief characteristics of tropical

nature to a greater degree than other localities which are, as

regards geographical position, tropical.

_Temperature of the Equatorial Zone._--The most characteristic,

as it is the most important feature in the physical conditions

of the great equatorial zone is the wonderful uniformity of its

temperature, alike throughout the changes of day and night, and from

one part of the year to another. As a general rule, the greatest

heat of the day does not exceed 90° or 91° Fahr., while it seldom

falls during the night below 74° Fahr. It has been found by hourly

observations carried on for three years at the meteorological

observatory established by the Dutch government at Batavia, that

the extreme range of temperature in that period was only 27° Fahr.,

the maximum being 95° and the minimum 68°. But this is, of course,

very much beyond the usual daily range of the thermometer, which

is, on the average, only a little more than 11° Fahr.; being 12·6°

in September when it is greatest, and only 8·1° in January, when

it is least.

Batavia, being situated between six and seven degrees south of the

equator, may be taken as affording a fair example of the climate

of the equatorial zone; though, being in an island, it is somewhat

less extreme than many continental localities. Observations made

at Para, which is continental and close to the equator, agree

however very closely with those at Batavia; but at the latter place

all the observations were made with extreme care and with the

best instruments, and are therefore preferred as being thoroughly

trustworthy.[1] The accompanying diagram, showing by curves the

monthly means of the highest and lowest daily temperatures at Batavia

and London, is very instructive; more especially when we consider

that the maximum of temperature is by no means remarkably different

in the two places, 90° Fahr, being sometimes reached with us and

not being often very much exceeded at Batavia.

[1] “Observations Made at the Magnetical and Meteorological

Observatory at Batavia. Published by order of the Government of

Netherlands India. Vol. I. Meteorological, from Jan. 1866 to Dec.

1868; and Magnetical, from July 1867 to June 1870. By Dr. P. A.

Bergsma. Batavia, 1871.” This fine work is entirely in English.

[Illustration: _Monthly Mean Temperature at Batavia & London._]

_Causes of the Uniform High Temperature near the Equator._--It is

popularly supposed that the uniform high temperature of the tropics

is sufficiently explained by the greater altitude, and therefore

greater heating-power, of the midday sun; but a little consideration

will show that this alone by no means accounts for the phenomenon.

The island of Java is situated in from six and a half to eight and

a half degrees of south latitude, and in the month of June the

sun’s altitude at noon will not be more than from 58° to 60°. In

the same month at London, which is fifty-two and a half degrees

of north latitude, the sun’s noonday altitude is 62°. But besides

this difference of altitude in favour of London there is a still

more important difference; for in Java the day is only about eleven

and a half hours long in the month of June, while at London it is

sixteen hours long, so that the total amount of sun-heat received by

the earth must be then very much greater at London than at Batavia.

Yet at the former place the mean temperature of the day and night

is under 60° Fahr., while in the latter place it is 80° Fahr., the

daily maximum being on the average in the one case about 68° and

in the other about 89°.

Neither does the temperature at the same place depend upon the

height of the sun at noon; for at Batavia it is nearly vertical

during October and February, but these are far from being the

hottest months, which are May, June, and September; while December,

January, and February are the coldest months, although then the sun

attains nearly its greatest altitude. It is evident, therefore,

that a difference of 30° in the altitude of the sun at noon has no

apparent influence in raising the temperature of a place near the

equator, and we must therefore conclude that other agencies are at

work which often completely neutralise the effect which increased

altitude must undoubtedly exert.

There is another important difference between the temperate and

tropical zones, in the direct heating effect of the sun’s rays

independently of altitude. In England the noonday sun in the month of

June rarely inconveniences us or produces any burning of the skin;

while in the tropics, at almost any hour of the day, and when the

sun has an elevation of only 40° or 50°, exposure to it for a few

minutes will scorch a European so that the skin turns red, becomes

painful, and often blisters or peels off. Almost every visitor to the

tropics suffers from incautious exposure of the neck, the leg, or

some other part of the body to the sun’s rays, which there possess

a power as new, as it is at first sight inexplicable, for it is

not accompanied by any extraordinary increase in the temperature

of the air.

These very different effects, produced by the same amount of sun-heat

poured upon the earth in different latitudes is due to a combination

of causes. The most important of these are, probably,--the constant

high temperature of the soil and of the surface-waters of the

ocean,--the great amount of aqueous vapour in the atmosphere,--the

great extent of the intertropical regions which cause the winds that

reach the equatorial zone to be always warm,--and the latent heat

given out during the formation of rain and dew. We will briefly

consider the manner in which each of these causes contributes to

the degree and the uniformity of the equatorial temperature.

_Influence of the Heat of the Soil._--It is well known that at

a very moderate depth the soil maintains a uniform temperature

during the twenty-four hours; while at a greater depth even the

annual inequalities disappear, and a uniform temperature, which is

almost exactly the mean temperature of the locality, is constantly

maintained throughout the year. The depth at which this uniform

temperature is reached is greater as the annual range of temperature

is greater, so that it is least near the equator, and greatest in

localities near the arctic circle where the greatest difference

between summer and winter temperature prevails. In the vicinity of

the equator, where the annual range of the thermometer is so small

as we have seen that it is at Batavia, the mean temperature of about

80° Fahr. is reached at a depth of four or five feet. The surplus

heat received during the day is therefore conducted downwards very

slowly, the surface soil becomes greatly superheated, and a large

portion of this heat is given out at night and thus keeps up the

high temperature of the air when the sun has ceased to warm the

earth. In the temperate zones, on the other hand, the stratum of

uniform earth-temperature lies very deep. At Geneva it is not less

than from thirty to forty feet, and with us it is probably fifty or

sixty feet, and the temperature found there is nearly forty degrees

lower than at the equator. This great body of cool earth absorbs a

large portion of the surface heat during the summer, and conducts

it downwards with comparative rapidity, and it is only late in the

year (in July and August) when the upper layers of the soil have

accumulated a surplus store of solar heat that a sufficient quantity

is radiated at night to keep up a high temperature in the absence

of the sun. At the equator, on the other hand, this radiation is

always going on, and earth-heat is one of the most important of

the agencies which tend to equalise the equatorial climate.

_Influence of the Aqueous Vapour of the Atmosphere._--The aqueous

vapour which is always present in considerable quantities in the

atmosphere, exhibits a singular and very important relation to

solar and terrestrial heat. The rays of the sun pass through it

unobstructed to the earth; but the warmth given off by the heated

earth is very largely absorbed by it, thus raising the temperature

of the air; and as it is the lower strata of air which contain most

vapour these act as a blanket to the earth, preventing it from losing

heat at night by radiation into space. During a large part of the

year the air in the equatorial zone is nearly saturated with vapour,

so that, notwithstanding the heat, salt and sugar become liquid,

and all articles of iron get thickly coated with rust. Complete

saturation being represented by 100, the daily average of greatest

humidity at Batavia reaches 96 in January and 92 in December. In

January, which is the dampest month, the range of humidity is small

(77 to 96), and at this time the range of temperature is also

least; while in September, with a greater daily range of humidity

(62 to 92) the range of temperature is the greatest, and the lowest

temperatures are recorded in this and the preceding month. It is a

curious fact, that in many parts of England the degree of humidity

as measured by the comparative saturation of the air, is as great

as that of Batavia or even greater. A register kept at Clifton

during the years 1853-1862 shows a mean humidity in January of 90,

while the highest monthly mean for the four years at Batavia was

88; and while the lowest of the monthly means at Clifton was 79·1,

the lowest at Batavia was 78·9. These figures however represent

an immense difference in the _quantity_ of vapour in every cubic

foot of air. In January at Clifton, with a temperature of 35° to

40° Fahr., there would be only about 4 to 4½ grains of vapour per

cubic foot of air, while at Batavia, with a temperature from 80°

to 90° Fahr., there would be about 20 grains in the same quantity

of air. The most important fact however is, that the capacity of

air for holding vapour in suspension increases more rapidly than

temperature increases, so that a fall of ten degrees at 50° Fahr.

will lead to the condensation of about 1½ grains of vapour, while

a similar fall at 90° Fahr. will set free 6½ grains. We can thus

understand how it is that the very moderate fall of the thermometer

during a tropical night causes heavier dews and a greater amount

of sensible moisture than are ever experienced during much greater

variations of temperature in the temperate zone. It is this large

quantity of vapour in the equatorial atmosphere that keeps up a

genial warmth throughout the night by preventing the radiation into

space of the heat absorbed by the surface soil during the day. That

this is really the case is strikingly proved by what occurs in the

plains of Northern India, where the daily maximum of heat is far

beyond anything experienced near the equator, yet, owing to the

extreme dryness of the atmosphere, the clear nights are very cold,

radiation being sometimes so rapid that water placed in shallow

pans becomes frozen over.

As the heated earth, and everything upon its surface, does not cool

so fast when surrounded by moist as by dry air, it follows, that

even if the quantity and intensity of the solar rays falling upon

two given portions of the earth’s surface are exactly equal, yet the

sensible and effective heat produced in the two localities may be

very different according as the atmosphere contains much or little

vapour. In the one case the heat is absorbed more rapidly than it

can escape by radiation; in the other case it radiates away into

space, and is lost, more rapidly than it is being absorbed. In both

cases an equilibrium will be arrived at, but in the one case the

resulting mean temperature will be much higher than in the other.

_Influence of Winds on the Temperature of the Equator._--The distance

from the northern to the southern tropics being considerably more

than three thousand miles, and the area of the intertropical

zone more than one-third the whole area of the globe, it becomes

hardly possible for any currents of air to reach the equatorial

belt without being previously warmed by contact with the earth or

ocean, or by mixture with the heated surface-air which is found in

all intertropical and subtropical lands. This warming of the air

is rendered more certain and more effective by the circumstance,

that all currents of air coming from the north or south have their

direction changed owing to the increasing rapidity of the earth’s

rotational velocity, so that they reach the equator as easterly

winds, and thus pass obliquely over a great extent of the heated

surface of the globe. The causes that produce the westerly monsoons

act in a similar manner, so that on the equator direct north or

south winds, except as local land and sea breezes, are almost

unknown. The Batavia observations show, that for ten months in

the year the average direction of the wind varies only between 5°

and 30° from due east or west, and these are also the strongest

winds. In the two months--March and October--when the winds are

northerly, they are very light, and are probably in great part

local sea-breezes, which, from the position of Batavia, must come

from the north. As a rule, therefore, every current of air at or

near the equator has passed obliquely over an immense extent of

tropical surface and is thus necessarily a warm wind.

In the north temperate zone, on the other hand, the winds are always

cool, and often of very low temperature even in the height of

summer, due probably to their coming from colder northern regions as

easterly winds, or from the upper parts of the atmosphere as westerly

winds; and this constant supply of cool air, combined with quick

radiation through a dryer atmosphere, carries off the solar heat

so rapidly that an equilibrium is only reached at a comparatively

low temperature. In the equatorial zone, on the contrary, the heat

accumulates, on account of the absence of any medium of sufficiently

low temperature to carry it off rapidly, and it thus soon reaches

a point high enough to produce those scorching effects which are

so puzzling when the altitude of the sun or the indications of

the thermometer are alone considered. Whenever, as is sometimes

the case, exceptional cold occurs near the equator, it can almost

always be traced to the influence of currents of air of unusually

low temperature. Thus in July near the Aru islands, the writer

experienced a strong south-east wind which almost neutralised the

usual effects of tropical heat although the weather was bright and

sunny. But the wind, coming direct from the southern ocean during

its winter without acquiring heat by passing over land, was of an

unusually low temperature. Again, Mr. Bates informs us that in the

Upper Amazon in the month of May there is a regularly recurring

south wind which produces a remarkable lowering of the usual

equatorial temperature. But owing to the increased velocity of the

earth’s surface at the equator a south wind there must have been

a south-west wind at its origin, and this would bring it directly

from the high chain of the Peruvian Andes during the winter of the

southern hemisphere. It is therefore probably a cold mountain wind,

and blowing as it does over a continuous forest it has been unable

to acquire the usual tropical warmth.

The cause of the striking contrast between the climates of equatorial

and temperate lands at times when both are receiving an approximately

equal amount of solar heat may perhaps be made clearer by an

illustration. Let us suppose there to be two reservoirs of water,

each supplied by a pipe which pours into it a thousand gallons a

day, but which runs only during the daytime, being cut off at night.

The reservoirs are both leaky, but while the one loses at the rate

of nine hundred gallons in the twenty-four hours the other loses

at the rate of eleven hundred gallons in the same time, supposing

that both are kept exactly half full and thus subjected to the same

uniform water-pressure. If now both are left to be supplied by the

above-mentioned pipes the result will be, that in the one which

loses by leakage less than it receives the water will rise day by

day, till the increased pressure causes the leakage to increase so

as exactly to balance the supply; while in the other the water will

sink till the decreasing pressure causes the leakage to decrease

so as to balance the supply, when both will remain stationary, the

one at a high the other at a low average level, each rising during

the day and sinking again at night. Just the same thing occurs

with that great heat-reservoir the earth, whose actual temperature

at any spot will depend, not alone upon the quantity of heat it

receives, but on the balance between its constantly varying waste

and supply. We can thus understand how it is that, although in the

months of June and July Scotland in latitude 57° north receives as

much sun-heat as Angola or Timor in latitude 10° south, and for

a much greater number of hours daily, yet in the latter the mean

temperature will be about 80° Fahr., with a daily maximum of 90°

to 95°, while in the former the mean will be about 60° Fahr. with

a daily maximum of 70° or 75°; and, while in Scotland exposure to

the full noonday sun produces no unpleasant heat-sensations, a

similar exposure in Timor at any time between 9 A.M. and 3 P.M.

would blister the skin in a few minutes almost as effectually as

the application of scalding water.

_Heat Due to the Condensation of Atmospheric Vapour._--Another cause

which tends to keep up a uniform high temperature in the equatorial,

as compared with the variable temperatures of the extra-tropical

zones, is the large amount of heat liberated during the condensation

of the aqueous vapour of the atmosphere in the form of rain and dew.

Owing to the frequent near approach of the equatorial atmosphere

to the saturation point, and the great weight of vapour its high

temperature enables it to hold in suspension, a very slight fall

of the thermometer is accompanied by the condensation of a large

absolute quantity of atmospheric vapour, so that copious dews and

heavy showers of rain are produced at comparatively high temperatures

and low altitudes. The drops of rain rapidly increase in size while

falling through the saturated atmosphere; and during this process

as well as by the formation of dew, the heat which retained the

water in the gaseous form, and was insensible while doing so, is

liberated, and thus helps to keep up the high temperature of the air.

This production of heat is almost always going on. In fine weather

the nights are always dewy, and the diagram on the preceding page

showing the mean monthly rainfall at Batavia and Greenwich proves

that this source of increased temperature is present during every

month in the year, since the lowest monthly fall at the former

place is almost equal to the highest monthly fall at the latter.

[Illustration: _Monthly Rainfall at London and Batavia._]

It may perhaps be objected, that evaporation must absorb as much heat

as is afterwards liberated by condensation, and this is true; but as

evaporation and condensation occur usually at different times and

in different places, the equalising effect is still very important.

Evaporation occurs chiefly during the hottest sunshine, when it

tends to moderate the extreme heat, while condensation takes place

chiefly at night in the form of dew and rain, when the liberated

heat helps to make up for the loss of the direct rays of the sun.

Again, the most copious condensation both of dew and rain is greatly

influenced by vegetation and especially by forests, and also by the

presence of hills and mountains, and is therefore greater on land

than on the ocean; while evaporation is much greater on the ocean,

both on account of the less amount of cloudy weather and because

the air is more constantly in motion. This is particularly the case

throughout that large portion of the tropical and subtropical

zones where the trade-winds constantly blow, as the evaporation

must there be enormous while the quantity of rain is very small.

It follows, then, that on the equatorial land-surface there will

be a considerable balance of condensation over evaporation which

must tend to the general raising of the temperature, and, owing to

the condensation being principally at night, not less powerfully

to its equalisation.

_General Features of the Equatorial Climate._--The various causes now

enumerated are sufficient to enable us to understand how the great

characteristic features of the climate of the equatorial zone are

brought about; how it is that so high a temperature is maintained

during the absence of the sun at night, and why so little effect

is produced by the sun’s varying altitude during its passage from

the northern to the southern tropic. In this favoured zone the heat

is never oppressive, as it so often becomes on the borders of the

tropics; and the large absolute amount of moisture always present

in the air, is almost as congenial to the health of man as it is

favourable to the growth and development of vegetation.[2] Again,

the lowering of the temperature at night is so regular and yet so

strictly limited in amount, that, although never cold enough to be

unpleasant, the nights are never so oppressively hot as to prevent

sleep. During the wettest months of the year, it is rare to have

many days in succession without some hours of sunshine, while

even in the driest months there are occasional showers to cool

and refresh the overheated earth. As a result of this condition

of the earth and atmosphere, there is no check to vegetation, and

little if any demarcation of the seasons. Plants are all evergreen;

flowers and fruits, although more abundant at certain seasons, are

never altogether absent; while many annual food-plants as well as

some fruit-trees produce two crops a year. In other cases, more

than one complete year is required to mature the large and massive

fruits, so that it is not uncommon for fruit to be ripe at the same

time that the tree is covered with flowers, in preparation for the

succeeding crop. This is the case with the Brazil nut tree, in the

forests of the Amazon, and with many other tropical as with a few

temperate fruits.

[2] Where the inhabitants adapt their mode of life to the

peculiarities of the climate, as is the case with the Dutch in

the Malay Archipelago, they enjoy as robust health as in Europe,

both in the case of persons born in Europe and of those who for

generations have lived under a vertical sun.

_Uniformity of the Equatorial Climate in all Parts of the

Globe._--The description of the climatal phenomena of the equatorial

zone here given, has been in great part drawn from long personal

experience in South America and in the Malay Archipelago. Over

a large portion of these countries the same general features

prevail, only modified by varying local conditions. Whether we

are at Singapore or Batavia; in the Moluccas, or New Guinea; at

Para, at the sources of the Rio Negro, or on the Upper Amazon, the

equatorial climate is essentially the same, and we have no reason

to believe that it materially differs in Guinea or the Congo. In

certain localities, however, a more contrasted wet and dry season

prevails, with a somewhat greater range of the thermometer. This is

generally associated with a sandy soil, and a less dense forest,

or with an open and more cultivated country. The open sandy

country with scattered trees and shrubs or occasional thickets,

which is found at Santarem and Monte-Alegre on the lower Amazon,

are examples, as well as the open cultivated plains of Southern

Celebes; but in both cases the forest country in adjacent districts

has a moister and more uniform climate, so that it seems probable

that the nature of the soil or the artificial clearing away of the

forests, are important agents in producing the departure from the

typical equatorial climate observed in such districts. The almost

rainless district of Ceara on the North-East coast of Brazil and

only a few degrees south of the equator, is a striking example

of the need of vegetation to react on the rainfall. We have here

no apparent cause but the sandy soil and bare hills, which when

heated by the equatorial sun produce ascending currents of warm

air and thus prevent the condensation of the atmospheric vapour,

to account for such an anomaly; and there is probably no district

where judicious planting would produce such striking and beneficial

effects. In Central India the scanty and intermittent rainfall,

with its fearful accompaniment of famine, is no doubt in great part

due to the absence of a sufficient proportion of forest-covering

to the earth’s surface; and it is to a systematic planting of all

the hill tops, elevated ridges, and higher slopes that we can alone

look for a radical cure of the evil. This would almost certainly

induce an increased rainfall; but even more important and more

certain, is the action of forests in checking evaporation from the

soil and causing perennial springs to flow, which may be collected

in vast storage tanks and will serve to fertilise a great extent

of country; whereas tanks without regular rainfall or permanent

springs to supply them are worthless. In the colder parts of the

temperate zones, the absence of forests is not so much felt, because

the hills and uplands are naturally clothed with a thick coating

of turf which absorbs moisture and does not become overheated by

the sun’s rays, and the rains are seldom violent enough to strip

this protective covering from the surface. In tropical and even

in south-temperate countries, on the other hand, the rains are

periodical and often of excessive violence for a short period;

and when the forests are cleared away the torrents of rain soon

strip off the vegetable soil, and thus destroy in a few years the

fertility which has been the growth of many centuries. The bare

subsoil becoming heated by the sun, every particle of moisture

which does not flow off is evaporated, and this again reacts on the

climate, producing long-continued droughts only relieved by sudden

and violent storms, which add to the destruction and render all

attempts at cultivation unavailing. Wide tracts of fertile land in

the south of Europe have been devastated in this manner, and have

become absolutely uninhabitable. Knowingly to produce such disastrous

results would be a far more serious offence than any destruction of

property which human labour has produced and can replace; yet we

ignorantly allow such extensive clearings for coffee cultivation

in India and Ceylon, as to cause the destruction of much fertile

soil which generations cannot replace, and which will surely, if

not checked in time, lead to the deterioration of the climate and

the permanent impoverishment of the country.[3]

[3] For a terrible picture of the irreparable devastation caused

by the reckless clearing of forests see the third chapter of Mr.

Marsh’s work _The Earth as Modified by Human Action_.

_Short Twilight of the Equatorial Zone._--One of the phenomena

which markedly distinguish the equatorial from the temperate and

polar zones, is the shortness of the twilight and consequent

rapid transition from day to night and from night to day. As this

depends only on the fact of the sun descending vertically instead

of obliquely below the horizon, the difference is most marked when

we compare our midsummer twilight with that of the tropics. Even

with us the duration of twilight is very much shorter at the time

of the equinoxes, and it is probably not much more than a third

shorter than this at the equator. Travellers usually exaggerate the

shortness of the tropical twilight, it being sometimes said that if

we turn a page of the book we are reading when the sun disappears,

by the time we turn over the next page it will be too dark to see to

read. With an average book and an average reader this is certainly

not true, and it will be well to describe as correctly as we can

what really happens.

In fine weather the air appears to be somewhat more transparent near

the equator than with us, and the intensity of sunlight is usually

very great up to the moment when the solar orb touches the horizon.

As soon as it has disappeared the apparent gloom is proportionally

great, but this hardly increases perceptibly during the first ten

minutes. During the next ten minutes however it becomes rapidly

darker, and at the end of about twenty-five minutes from sunset

the complete darkness of night is almost reached. In the morning

the changes are perhaps even more striking. Up to about a quarter

past five o’clock the darkness is complete; but about that time a

few cries of birds begin to break the silence of night, perhaps

indicating that signs of dawn are perceptible in the eastern

horizon. A little later the melancholy voices of the goatsuckers

are heard, varied croakings of frogs, the plaintive whistle of

mountain thrushes, and strange cries of birds or mammals peculiar

to each locality. About half-past five the first glimmer of light

becomes perceptible; it slowly becomes lighter, and then increases so

rapidly that at about a quarter to six it seems full daylight. For

the next quarter of an hour this changes very little in character;

when, suddenly, the sun’s rim appears above the horizon, decking the

dew-laden foliage with glittering gems, sending gleams of golden

light far into the woods, and waking up all nature to life and

activity. Birds chirp and flutter about, parrots scream, monkeys

chatter, bees hum among the flowers, and gorgeous butterflies

flutter lazily along or sit with fully expanded wings exposed to

the warm and invigorating rays. The first hour of morning in the

equatorial regions possesses a charm and a beauty that can never

be forgotten. All nature seems refreshed and strengthened by the

coolness and moisture of the past night; new leaves and buds unfold

almost before the eye, and fresh shoots may often be observed to

have grown many inches since the preceding day. The temperature is

the most delicious conceivable. The slight chill of early dawn,

which was itself agreeable, is succeeded by an invigorating warmth;

and the intense sunshine lights up the glorious vegetation of the

tropics, and realises all that the magic art of the painter or

the glowing words of the poet, have pictured as their ideals of

terrestrial beauty.

Tropical nature, and other essays · 第 1 / 25 段