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*** START OF THE PROJECT GUTENBERG EBOOK 75114 ***
TRANSCRIBER’S NOTE
Italic text is denoted by _underscores_.
Bold text is denoted by =equal signs=.
Footnote anchors are denoted by [number], and the footnotes have been
placed at the end of the book.
The tables in this book are best viewed using a monospace font.
Some minor changes to the text are noted at the end of the book.
THE NEW AIR WORLD
[Illustration: FIG. 4.—INSTRUMENT SHELTER. Frontispiece.
(_Page 66_)]
THE
NEW AIR WORLD
_The Science of Meteorology
Simplified_
BY
WILLIS LUTHER MOORE, SC.D., LL.D.
PROFESSOR METEOROLOGY GEORGE WASHINGTON
UNIVERSITY, EIGHTEEN YEARS CHIEF
UNITED STATES WEATHER BUREAU
[Illustration: (colophon)]
BOSTON
LITTLE, BROWN, AND COMPANY
1922
_Copyright, 1922_,
BY LITTLE, BROWN, AND COMPANY.
_All rights reserved_
Published October, 1922
PRINTED IN THE UNITED STATES OF AMERICA
AFFECTIONATELY DEDICATED
TO
A FRIEND OF MANY AND PLEASANT YEARS
A BELOVED TEACHER AND A
GREAT CHEMIST
DR. CHARLES E. MUNROE, PH.D.
INTRODUCTION
The author’s “Descriptive Meteorology” (Appleton, 1914) is designed
for the teaching of those who intend to make Meteorology a
profession. This book is planned for the reading of those who desire
to know something of the wonders of the New Air World into which man
is just now entering, for those who desire to become weatherwise and
make forecasts for themselves, and to apply their knowledge to their
business, their health, and their happiness; and for the reading of
the more advanced pupils of the public schools.
So far as possible technical terms are avoided and an effort made to
tell a simple story that will awaken curiosity and lead the reader
to wish to know more and more of the mysteries of the atmosphere, of
which practically nothing was known at the time of the landing of
the Pilgrims, Torricelli not having discovered the barometer until
twenty-three years later. It will be made plain how atmospheric
air was formed, how long it will remain, whither it will go, how it
is heated, cooled, and lighted; where and how storms, cold waves,
clouds, frosts, and fair-weather conditions originate and how move;
how the cyclone, the tornado, and the thunderstorm may be recognized
on the Daily Weather Map of the Government and their future
activities forecast; how a fund of simple yet wonderful information
that will be of inestimable value may be acquired by any intelligent
person.
The author acknowledges courtesies extended to him by Prof. Charles
F. Marvin, present chief of the Weather Bureau, and by R. H.
Weightman, chief clerk of the Bureau, in the matter of securing
several important illustrations; and like favors extended to him by
D. Appleton and Company, John Wiley & Sons, and the Taylor Instrument
Company, of Rochester, N. Y.
W. L. M.
AUGUST, 1922
CONTENTS
CHAPTER PAGE
INTRODUCTION vii
I ATMOSPHERES OF THE EARTH, THE SUN, AND THE PLANETS 1
II A SYNOPTIC PICTURE OF THE AIR 7
III EXPLORATIONS OF THE ATMOSPHERE 18
IV EARTH’S FOUR ATMOSPHERES 29
V LIGHT, HEAT, AND TEMPERATURE 48
VI THE ADVANTAGE OF TAKING WEATHER OBSERVATIONS AND
APPLYING THEM TO ONE’S PERSONAL NEEDS 64
VII FROST 85
VIII WIND AND PRESSURE OF THE GLOBE 98
IX HOW TO FORECAST FROM THE DAILY WEATHER MAP 112
X CLIMATE 161
XI HOW CLIMATE IS MODIFIED AND CONTROLLED 188
XII CIVILIZATION FOLLOWS THE STORM TRACKS 213
XIII HAS OUR CLIMATE CHANGED? 225
XIV CLIMATES FOR HEALTH AND PLEASURE 245
XV CONDENSATION 282
XVI DEVELOPMENT OF THE AMERICAN WEATHER SERVICE 291
INDEX 307
LIST OF FIGURES
Instrument Shelter (Figure 4) _Frontispiece_
FIGURE PAGE
1. Winter and Summer Vertical Temperature Gradients, in
degrees Centigrade and Fahrenheit 12
2. Showing light from lamp a passing into dust-free air
at _b_, and passing out at _c_ without illuminating
the interior 46
3. Standard Weather Bureau Kite 64
5. Comparison of the Thermometer Scales 67
6. Dry and Wet Bulb Thermometers 68
7. Mercurial Barometer 78
8. Continuous records of the temperature from 4 P.M.
to 9 A.M. 87
9. Continuous records of the temperature 5 feet and 35
feet above ground on a tower in a pear orchard 95
10. Average dates of last killing frost in Spring 96
11. Average dates of first killing frost in Fall 97
12. Trade wind circulation 99
13. Average surface winds and pressure of the globe 102
14. How winds would blow into a cyclone on a non-rotating
earth 108
15. Deflection of wind due to earth’s rotation 109
16. Annual, summer, and winter wind velocities with
altitude 110
17. Tornado Cloud 145
18. The St. Louis Tornado of May 27, 1896, Shot a Pine
Scantling through the Iron Side of the Eads Bridge 147
19. The St. Louis Tornado of May 27, 1896, Shot a Shovel
Six Inches into the Body of a Tree 147
20. The St. Louis Tornado Drove Straws One half Inch
into Wood 149
21. Equinoxes, March 21 and September 22 163
22. Summer Solstice, June 21 164
23. Winter Solstice, December 21 164
24. Winter and Summer Solstices, and the Equinoxes 165
25. As angle of incidence decreases from 90° to 10° the
heat received on upper end of blocks is spread
over greater area at bottom, and its temperature
diminished 165
26. Altitude attained by Sun at midday and length of its
track above the horizon at the Summer and Winter
Solstices and at the two Equinoxes 167
27. Summer day and Summer night temperatures in the same
narrow valley 204
28. Average Monthly Temperature and Rainfall of Typical
Places in North America 207
29. Average Monthly Temperature and Rainfall of Typical
Places in the Old World 208
30. Changes in Climate in California during the Christian
Era 237
31. Snow Crystals 286
LIST OF CHARTS
CHART PAGE
1. High and Low Centers of Action and Prevailing Winds
of the Globe for July 99
2. High and Low Centers of Action and Prevailing Winds
of the Globe for January 100
3. Winter Storm, December 15, 1893, 8 A.M. 114
4. Winter Storm, December 15, 1893, 8 P.M. 116
5. Winter Storm, December 16, 1893, 8 A.M. 118
6. Cold Wave Zones, March to November. Amount of Fall
and Verifying Limit 127
7. Cold Wave Zones, December, January, and February.
Amount of Fall and Verifying Limit 128
8. Lowest Temperatures in the United States, 1871-1913 129
9. Number of Cold Waves, 1904-1914, Inclusive 130
10. Storm Tracks for August for Ten Years 132
11. Storm Tracks for February for Ten Years 134
12. Average Maximum Temperature for July 195
13. Ocean Currents 196
14. Mean Annual Isotherms 200
15. Normal Wind Direction and Velocity for January and
February 202
16. Normal Wind Direction and Velocity for July and
August 204
17. Map of Climatic Energy 221
18. Density of Population in the United States, 1910 222
THE NEW AIR WORLD
CHAPTER I
ATMOSPHERES OF THE EARTH, THE SUN, AND THE PLANETS
=How Atmospheres Are Formed.= Once there were no such things on the
earth as hills and mountains, singing brooks, roaring rivers and vast
oceans; and the delicately hued landscape, with its winding roads,
hedges, flowers, green fields, and golden grain, had not evolved from
the atmosphere. The earth had not yet cooled down to the condition of
a solid crust, everything that the eye now sees existed in the form
of invisible gases, or as clouds incandescent with white heat. Fiery
blasts swirled over the face of the earth. Storms a million times
more powerful than the most destructive West Indian hurricane of the
present day moved through the indescribably hot atmosphere, throwing
down not rain as we understand it, but liquid earth and metal, as
their rising clouds ascended and cooled. It is difficult for the
human mind to grasp the wonders of this.
Small planets cool quicker than large ones and sooner come to
the conditions of a crust and to a temperature suitable for the
development of the various forms of life.
=Atmosphere of the Sun.= To the unaided eye it appears as a smooth,
bright, quiescent sphere, but the telescope reveals millions of
agitations and hundreds of red flames that shoot outward to distances
of hundreds of thousands of miles. One can form no adequate picture
of the convulsions of the atmosphere of the sun. During eclipses,
when the intense glare of its center is obscured, hydrogen flames may
be seen darting outward for as much as a million miles.
=Lifeless Planets.= The larger a planet the longer is the time that
must elapse before the hot vapors of rock and metal, which largely
compose its early atmosphere, cool and congeal into a crust, leaving
as a residual an atmosphere of such heat, density, and composition as
to permit of the beginnings of the forms of life that have inhabited
the world. Before the sun can reach this condition, an indescribable
period will have elapsed, its light will have gone out, its heat
will have ceased to reach the earth and the other planets in
quantities sufficient to maintain life, the earth will have been dead
millions of years, and the sun itself will only receive heat and
light from the feeble rays of the stars that, unlike itself, have not
yet ceased to shine. But even then the sun ever must remain dead, for
there is no external source whence it may receive heat. No vegetation
can adorn it, no water flow upon its surface, neither can the foot of
any man press its soil.
Jupiter, and perhaps Neptune, Uranus, and Saturn, have hot
atmospheres still in violent agitation,—molten surfaces composed
of all kinds of matter, from which bubble and boil off hot clouds
of vapor that surge about in huge eddies or cyclonic storms, and
that here and there are shot outward in tongues of fire. The earth
millions of years ago had a similar atmosphere. But when the heat
energy of these vaporous planets wanes, and they cool down, as the
earth did many years ago, the simplest forms of life cannot be
evolved upon them, for they are too far away from the sun to receive
life-giving heat. Mars receives less than half the intensity of the
solar rays that come to the earth, Jupiter only 0.037, Saturn 0.011,
Uranus 0.003, and Neptune 0.001.
In due time—some hundreds of millions of years—the cooling of the
sun will leave the earth to freeze and all life to become extinct,
unless, perchance, the oxygen of the air is so far absorbed by its
rocks, or filtered away into space, as to destroy life before that
time. No matter what may be the achievements of the human mind, what
wonderful civilizations may be developed, what powerful empires
created, or what wonderful secrets of creation discovered, it seems
certain that these all will pass away, and finally the surface of
the earth be as if man never lived. The dust of ages will wipe out
and obliterate every trace and vestige of the operations of life.
Silence, cold, and darkness will then reign supreme. But the time of
this is indescribably far off in the future, and man will have ample
opportunity to develop to the highest mental and spiritual estates of
which he has inherent possibilities.
The moon already is dead. If it is formed of matter abandoned by the
earth, as we believe, it once must have had an atmosphere, a portion
of which was absorbed by its rocks as it cooled, and the remainder
lost as the result of the low power of attraction of so small a
body, which is insufficient to prevent the darting molecules of the
gases of its air from shooting off into space. The absence of an
atmospheric covering allows the heat from the sun to escape almost
as rapidly as it is received; and the long nights of the moon (each
as long as fourteen of our days) during which the sun’s rays are
entirely cut off, permit the temperature of the dark side to fall to
something like -400° F.
=How Atmospheres Are Maintained and How Lost.= The processes of
nature are always adding to the various gases of the atmosphere in
some ways, and transforming or taking from them in other ways. On the
earth the loss and the gain are so nearly equal as to maintain at
present a nearly constant condition. Marked changes have taken place,
however, in long geologic periods. Our early atmosphere probably
contained large quantities of carbon dioxide which were absorbed by
the rank vegetable growth that now forms the coal beds of the earth,
and the slowly cooling rocks that constitute the crust took in large
quantities of oxygen; in fact, nearly one half of the weight of the
crust of the earth is composed of the latter element.
In consequence it may be said that our present atmosphere is what
remained after the earth had absorbed its gases nearly to depletion,
and after the lighter gases, like hydrogen and helium, which seem to
have too great molecular velocity to be imprisoned by the earth’s
attraction of gravitation, had been lost in space. Gases that cannot
be held by the moon may be imprisoned by the earth and those that can
escape from the earth may be held by the larger planets.
=Height of the Earth’s Atmosphere.= Exact computation has shown that
if the air were the same density at all elevations, which it is not,
it would extend upward a distance of only five miles. From laws that
are well understood it is known that at a height of thirty miles
the atmosphere is only about one hundredth as dense as it is at the
surface of the earth, and that at fifty miles it is too light to
manifest a measurable pressure. The oxygen ceases at about thirty
miles and the nitrogen at about fifty miles, the water vapor being
restricted below the five-mile level. The appearance of meteors,
which are rendered luminous by rushing into the earth’s atmosphere,
and whose altitudes have been determined by simultaneous observations
at several stations, reveals the presence of hydrogen and helium at a
height of nearly two hundred miles.
CHAPTER II
A SYNOPTIC PICTURE OF THE AIR
How much do you know of the great aërial ocean on the bottom of which
you live and in which human beings are just beginning to fly? Its
variations of heat, cold, sunshine, cloud, and tempest materially
affect not only the health and happiness of man but his commercial
and industrial welfare, and yet few know more than little of the
wonders of the life-giving medium that so intimately concerns them.
=At the Height of Two Hundred Miles.= Here is only the invisible,
the intangible ether which, while too tenuous to be detected or
measured by any appliances of man, is supposed to transmit the rays
of the sun. These rays, coming in the form of many different wave
lengths, and with widely differing velocities of vibration, produce
a multitude of phenomena as they are absorbed by or pass through
the air, or as they reach the surface of the earth. The longer and
slower waves are converted into heat, the shorter and more rapid ones
into light, and the minutest movements probably into electricity.
Oxygen and nitrogen, which form the greater part of the atmospheric
gases, absorb comparatively little of the solar rays, while water
vapor, which constitutes a little more than one per cent. of the
atmosphere and which remains close to the earth, absorbs large
quantities. From the fact that one half of the atmosphere, including
nearly all of its water vapor, lies below an elevation of three and
one half miles, it becomes evident that the greater part of the
absorption of the sun’s rays must take place in the lower strata. On
clear days the atmosphere absorbs nearly one half of the sun’s heat
rays; the remainder reaches the surface of the earth, warms it and
in turn is radiated back into the air,—with this difference: that
as earth radiation the wave motion of the rays is longer and slower
than it was when the rays entered our atmosphere as solar radiation.
In this slower form the rays are the more readily absorbed. The
atmosphere is thus warmed largely from the bottom upwards, which
accounts for the perpetual freezing temperatures of high mountain
peaks, although they are nearer the sun than are the bases from which
they rise.
=At the Height of One Hundred Miles.= The temperature at this
altitude must be that of outside space, probably 459° F.[1] below
zero. Air liquefies at 312° below, and therefore it cannot exist in
the gaseous state in a region having a lower temperature. When it
liquefies it has the color and general appearance of water, and about
the same specific gravity.
When a piece of steel and a lighted taper are brought together inside
of a vessel filled with liquid air, the dense supply of oxygen makes
combustion so rapid that the hard metal burns like tinder.
=At the Height of Fifty Miles.= There is enough air here to refract
light slightly, as at twilight, and to render luminous the meteors
that rush with fearful velocity against its widely scattered
molecules. At this distance from the earth there probably is no more
air than would be found under the receiver of the best air pump,
and, the reader will be surprised to learn, darkness is practically
complete, although the hour may be midday, for there are no dust
motes to scatter and diffuse and render visible the light rays of the
sun. (See Chapter III.)
=The Darkness of Outer Space.= It may be proven by taking an inclosed
volume of air, freeing it of dust motes, of which there are millions
per cubic centimeter, and then trying to illuminate it; it will
be found that no matter how powerful the light directed into it,
it remains wholly dark. When one looks upward on a clear day, he
apparently sees the whole universe illuminated; but in point of
fact only the thin stratum of the earth’s air in which he lives is
illuminated. Outer space is practically without temperature or light.
The rays of the sun do not become either light or heat or electricity
until they encounter the molecules of the air, or the invisible dust
motes, or the cloud particles near the earth and through interference
are transmuted from etheric vibrations into other forms of energy.
=The Bacteria of Disease and of Putrefaction.= These rapidly diminish
in number with elevation, and on the tops of the highest mountain
peaks practically none are found. Mid-ocean also shows but few.
=At the Height of Twenty-five Miles.= Air, light as it is, has still
sufficient density to obstruct the passage of the minutest wave
lengths of light, and here probably begins to be appreciable the
blue tint of the heavenly vault. At this short distance from the
earth there must be a deathlike stillness, for there is no medium
sufficiently dense to transmit sound. Two persons could not hear
each other speak, even if they could live in this rare atmosphere,
which they could not. Here is eternal peace and no apparent motion,
for storms and ascending and descending currents cease long before
this level is reached. The cold is intense and daylight but a feeble
illumination. There are no clouds.
=Isothermal Stratum Entered at the Height of Seven Miles.= We know
that the temperature decreases rapidly with ascent—about one degree
for each three hundred feet—until the top of the storm level is
reached, at about seven miles, when a most wonderful discovery is
made: the thermometer no longer falls as the aviator rises, or
as balloons float to great altitudes carrying self-registering
instruments. The temperature remains practically stationary, so far
as exploration has been made, which is to the height of over nineteen
miles. Major R. W. Schroeder, U. S. A., flew in an aëroplane to
36,000 feet and recorded a temperature of 69° below zero.
We have named this region above storms the _Isothermal_ stratum.
(See Figure 1.) Its temperature everywhere is about 70° below zero
and it changes only about six degrees between winter and summer. Of
course we must assume that ultimately the temperature shades away to
practically nothing as outer space is reached.
[Illustration: FIG. 1.—Winter and Summer Vertical Temperature
Gradients, in degrees Centigrade and Fahrenheit.]
Scientific and inventive genius is becoming so skillful in harnessing
the forces of nature to man’s desires that it is reasonable to
anticipate that within a quarter of a century or less human beings
will be nearly as numerous in the air as insects, they will remain
aloft longer, and sail to vastly greater distances and to higher
altitudes. In time dirigible ships may sail for days and possibly for
weeks in the pure air aloft, carrying millions of passengers.
=At a Height of One and One Half Miles.= There is little difference
in the temperatures of day and night, except that the coolest time of
the twenty-four hours is during daytime and not at night, as would be
most naturally supposed. This is important information to an aviator
or to the pilot of a balloon.
=At an Altitude of One Thousand Feet.= In free air at the hottest
time in midsummer’s heat, the air is found to be as much as fifteen
degrees lower than that at the ground. Almost within arm’s length
of the streets of great inland cities there is a cool and healthful
atmosphere when humanity is sweltering and dying from heat below.
Some youth who is reading this may develop the genius that will lift
up whole city blocks into this cool and healthful region. Open steel
work below, the first level at one or two thousand feet above the
hot streets, express elevators to carry passengers, and the climate
of the cool mountain air is accessible to those who now live in
discomfort at low populous centers. Man is just beginning to disport
himself in the hitherto trackless wilderness of the air. Certain
it is that the hanging gardens of Babylon will be outdone in the
Twentieth Century and the eyrie of the eagle left far below by those
who will live a part of their time in elevated structures having
bases resting upon the earth; or who will fly to great distances
aloft and remain at whatever altitude furnishes them the most
pleasant and beneficial conditions, and that they may thus remain not
only for days but for weeks without returning to the surface of the
earth.
Only during recent years have we realized how thin is the stratum of
air next to the earth which has sufficient heat and moisture for the
inception, growth, and maturity of animal and vegetable life. The
raising of the instrument shelter at the New York station of the U.
S. Weather Bureau from an elevation of one hundred and fifty feet
above the street to an altitude of three hundred feet has caused an
apparent lowering of the mean annual temperature of two and one half
degrees.
Air is so elastic and its density diminishes so rapidly with
elevation that nearly one half of the weight of the entire mass of
the atmosphere lies below the level of the top of Pike’s Peak, which
has a height of a little less than three miles above sea level. It
presses with a weight of about fifteen pounds per square inch of
surface, and its pressure is exerted in all directions, upward as
well as downward. An ordinary man sustains a pressure of over one
ton on each square foot of his surface, but as the air penetrates
all portions of his body and exercises a pressure outward as well as
inward he feels no inconvenience. If his body could be so tightly
sealed that no air could enter and if then the air of the interior
should be removed with a pump, his body instantly would be crushed to
a shapeless pulp.
A cubic foot of atmospheric air weighs one and one third ounces.
Water is 773 times, and mercury ten thousand times, as dense as
air. But air is a more ponderable substance than many suppose; an
ordinary lecture hall forty by fifty feet and thirty feet from
floor to ceiling contains two and one half tons of air at freezing
temperature. It would contain less at a higher temperature,
because heat expands its volume; it would contain more at a lower
temperature, because cold contracts its volume.
=Everything Evolved from the Air.= Air is so common that we seldom
stop to consider the magnitude of the force it exerts or the grandeur
wrought by this invisible architect of nature. In the great cycle
of world building—birth from the nebulæ, growth, maturity, decay,
disintegration, death, and then possibly back again to the nebulæ—the
atmosphere, be it light and tenuous as at present, or be it filled
with the hot vapors of earth and metal, is the vehicle and the medium
of the builder, transporting and transmuting, in mysterious ways and
to wondrous forms, the materials of planets. Its work as a builder
may be further illustrated by showing that the body of man itself
returns not to the earth earthy, as we have been taught, but largely
to the air whence it came. Decomposition is but the liberation of
the aëriform gases of which it is mainly composed; the residue is
but a handful that goes back to mother earth. Let us take the dried
corn plant; weigh it, then burn it in a closed vessel so that none
of the ashes can blow away. Continue the burning until the ashes are
perfectly white and it will be found that the weight of the ashes is
only about one twentieth of the weight of the great stalk, ear, and
foliage we began with. What has become of all the rest? The fire has
destroyed it, you say. No, we can destroy nothing. Remember that;
we can destroy nothing that the Creator has made, neither matter
nor force. The fire has simply changed the form of the plant; the
nineteen twentieths that have disappeared have gone back to the air
whence they came.
Thus we see that the body of man, the cereal and fruit that furnish
him food, the structure that gives him shelter, aye, the many things
that please the eye: the landscape, the beautiful flowers, the green
fields, the babbling brooks, even the rose blush on the maiden’s
cheek,[2]—really come from this wonderful fluid surrounding the
earth, and well may it be said that the queen of life rides upon the
crest of the wind.
CHAPTER III
EXPLORATION OF THE ATMOSPHERE
DISCOVERIES AS VALUABLE TO THE FUTURE AS THOSE MADE BY COLUMBUS
An entire new world is coming within the range of man’s vision. Its
possibilities for adding to the health and happiness of mankind are
almost limitless. The geographic poles have been conquered and the
jungles of Africa traversed; and deep borings have been made into the
bowels of the earth until heat has arrested further progress. The
further exploration of both regions is of the utmost importance to
the coming age. It is not at all visionary to assume that the heat of
the earth’s interior in near time will furnish the power necessary to
do the drudgery of mankind, give warmth and light to habitations, and
operate transportation systems; and the New World Above offers pure,
electrified, and highly stimulating air into which helium-inflated
dirigible balloons will sail, and in which they will remain not only
days but weeks or longer, with their multitudes of people.
While the use of kites and balloons in sending automatic
meteorological instruments far aloft has revealed more of the wonders
of this hitherto uncharted wilderness of cold and partial or total
darkness than the general public is aware of, only the outer fringes
of the mysterious regions above the clouds and the storms have been
penetrated.
When the manufacture of helium, a noncombustible gas almost as light
as hydrogen, becomes more general, as seems imminent in the United
States, the dirigible balloon may successfully compete with the
railroads in the carrying of long-distance passengers. The recent
loss of over forty lives in England by the collapse of the dirigible
ZR2 probably was largely if not entirely due to the explosion and
fire of the hydrogen gas with which the ship was inflated.
A decade ago, in a number of Chautauqua lectures, the writer
invariably was greeted with looks of incredulity when he prophesied
that within ten years travelers of the air would take breakfast at
the Waldorf-Astoria in New York and afternoon tea on the banks
of the Thames. And yet the ocean already has been crossed by an
aëroplane in continuous flight, and in the near future it is highly
probable that aërial navigation will be safer than travel by rail
or automobile. The hitherto inaccessible parts of the earth will
be sailed over and closely scrutinized, while travelers enjoy the
comforts that heretofore have been associated with Pullman service.
In 1862 the English meteorologist Glashier ascended in a balloon to
about the same height as that attained by Major R. W. Schroeder,
U. S. A., who achieved a more difficult feat when he flew in an
aëroplane to over 36,000 feet. And at Dayton, Ohio, celebrated as the
home of the Wright brothers, on September 28, 1921, Lieutenant John
A. Macready, U. S. A., reached the unprecedented height of 40,800
feet. These are the extreme altitudes to which human beings ever have
attained, but they are only the beginning of explorations into a vast
and largely unknown and extremely cold region,—one in which darkness
increases with elevation until at the outer limits of the atmosphere
no illumination whatever exists.
The high eastward wind and 69° below zero encountered by Schroeder
are conditions that already had been revealed by the work done
at the research station of the Weather Bureau, at Mount Weather,
Virginia, and at other stations in this country and in Europe, by
the sending up of instruments unaccompanied by observers. Under
the direction of the writer the Weather Bureau liberated numerous
small hydrogen gas balloons in the Rocky Mountain region, to which
were attached automatic instruments registering the temperature,
pressure, and the hygrometric conditions. As they came eastward
in the atmospheric drift that always prevails above the storms in
the middle latitudes they attained to great altitudes, one balloon
reaching 19.1 miles, the greatest altitude ever reached at that time
by the appliances of man. Ultimately the balloons would explode as
they expanded under the influence of decreasing air pressure and the
case of instruments would descend slowly under a parachute designed
to open at the right moment. The barometer traced a line on a paper
cylinder revolving by clock works, as did the thermometer. The
thermogram gave the temperature that corresponded with the varying
elevation shown by the tracing of the barogram.
In 1898, twelve hundred observations were made with kites by the
observers of the Weather Bureau at seventeen stations selected
by the writer, during the six warm months from May to October. It
was surprising to find the temperature often losing as much as
fifteen degrees with the first thousand feet ascent during middays
of extremely hot periods. The average decrease in temperature per
thousand feet elevation for all stations for all times, and at all
elevations up to 5280, was 4°.
For over five years kites were used nearly every day in the year at
Mount Weather to carry instruments aloft to heights ranging from
two to four and one half miles, and at times to keep the apparatus
up during all hours of the day, so that a comparison could be made
of the difference between day and night temperatures. There is but
little difference between midday and midnight at only a few thousand
feet above the earth.
Few are aware that the rectangular kite of the weather man was the
forerunner of the aëroplane of the aviator. In 1903, while directing
wireless experiments in the sending of messages at Roanoke Island,
North Carolina, the writer saw the Wright brothers, or their
representatives, lying flat upon the lower planes of what appeared
to be Weather Bureau kites and gliding in the air from the top of
the sand dunes. This was the beginning of real flight by man.
The ingenuity of the Wrights transformed the weather man’s kite,
strengthened it, took out the ends, hitched on a rudder, and when the
petrol engine had developed sufficient power with a given weight,
installed it, and flew.
In the future the meteorologist and the aviator will be closely
associated. With a sufficient number of weather observations made by
aviators simultaneously and well distributed over the United States
it will be possible to construct a daily weather map on some high
level—say the three-mile level—similar to the map now based upon
sea level. The pressure, temperature, wind direction, clouds, and
rainfall would be recorded and charted for the upper region clear
across the continent. Three miles is about halfway to the top of
cyclonic storms and probably in the region of greatest activity. More
accurate forecasts would be possible by the study of this additional
weather chart. This coöperation of the bird man and the weather man
in studying the geography of the new air world will mark an epoch in
meteorological science as far-reaching in its consequences as were
the discovery of the barometer by Torricelli and the uncovering of
the principles of the thermometer by Galileo, the former of which
was not known until more than twenty-three years after the landing
of the Pilgrims at Plymouth Rock. Thus swiftly does the mind of man
to-day explore the hidden recesses of nature’s mysteries, and with
each conquest carry itself to a higher realm of existence.
In the not distant future, more storm warnings may be issued by the
Weather Bureau for ships of the air than for those of the sea, for
the navigation of the air must play an increasing and important part
in the coming activities of the world. Science is becoming so skilled
in the harnessing of the forces of nature to man’s desires and in
the development of mechanical appliances, that it is reasonable to
anticipate the possibility that long-distance travel over land or
ocean ultimately will be almost entirely confined to the air.
As the result of the explorations of the atmosphere made by the
institution at Mount Weather there was ready for our fighting air men
at the front, immediately on our entry into the World War, a fund of
useful information concerning a region that but a short time before
was entirely uncharted. The instruments carried by the exploring
kites and balloons had keen scientific eyes and they recorded on
clock-timed cylinders what they saw. Thus did the air pilot know
much about the direction and the force of the wind that he would
encounter as he rose, the altitude where he would pass above clouds,
the degree of cold that he would encounter, etc. He was told that the
temperature would fall about one degree for each three hundred feet
of his ascent until he reached the top of the storm stratum at six
or seven miles, and that if he could reach that altitude he would
observe a most wonderful phenomenon: the temperature no longer would
fall with gain in altitude; he would enter a cold but an equally
heated stratum, without finding any temperatures lower than were
encountered upon entering the region, which is always about seventy
degrees below zero.
If the aërial explorer could stop his ship and keep it at an altitude
of about one and one half miles for twenty-four hours he would be
startled to find that the coolest time of the period was during the
daytime, not during the night, as he had expected to find it.
In the future the traveler in the upper reaches of the atmosphere
will carry oxygen and make the kind of air that he wishes to breathe,
and he will properly protect himself against the cold of his new
world, which he will find deficient in dust motes and doubtless
entirely wanting in the bacteria of putrefaction and of disease.
There will be no clouds to obscure his vision; no rain or snow. He
will not often ascend above the region where there are not some dust
motes to scatter and diffuse a part of the solar rays and give him at
least a partial illumination.
Few persons are familiar with the simple problems of the air which
have such important bearing on the distribution of man into realms
above those he has been accustomed to occupy. They do not know
that the northwest wind brings physical energy and mental buoyancy
because it has a downward component of motion that draws air from
above, where it is free of impurities, and where high electrification
has changed a considerable quantity of its oxygen into ozone, in
which condition it remains but a short time after reaching the
lower potential near the earth’s surface. More people die under the
influence of the south wind than under the influence of the north
wind, because the south winds hug the surface of the earth and become
laden with impurities and are lacking in electrical stimulation. When
inventive man becomes more familiar with the ocean on the bottom of
which he has heretofore lived, he will not wait for the north wind to
bring down to him the beneficial conditions that always exist higher
up; he will go after them and remain aloft as long as he desires to
do so.
The further development of the dirigible balloon and the aëroplane
are among the most important duties that the engineer of the future
owes to civilization; and the meteorologist must establish the
climatology of the vast untracked regions above the highest mountain
peaks, for here man will largely disport himself in the time to come.
The writer agrees with the opinion of Major William R. Blair,
formerly of his staff when he was the head of the U. S. Weather
Bureau, but since the beginning of the World War the chief
meteorological assistant of the Chief Signal Officer of the U. S.
Army when he says:
“With reference to air travel in the future: the present stage
of aircraft development seems to indicate that long non-stop
traffic, both freight and passenger, in the air will be by means
of lighter-than-air craft (balloons). These craft have much
larger carrying capacity than any airplanes now designed and
will travel across the continent over several prepared routes,
stopping only at important centers on these routes to discharge
and take up passengers and freight. It is believed that airplanes
(heavier-than-air craft) will ply between these important centers
and the outlying country about them, thus acting as feeders to
the main route, over which the monstrous dirigibles will operate.
Most transoceanic as well as transcontinental air traffic will
probably be carried on in these large dirigible balloons.”
Lieutenant Colonel Henry B. Hersey, who served through the World War
in the Aëronautical Service of the Signal Corps, U. S. A., and who
also was associated with the writer in the management of the Weather
Bureau, says:
“The fields of the dirigible and the air plane are separate and
there is no conflict between the two. For light loads, great
speed, and quick manœuvering, the airplane is supreme. For heavy
loads, long distance, ability to remain in the air for great
periods of time, the dirigible is the only air craft that can
fulfill the requirements. Dirigibles will soon be in use which
can start from Europe, sail over New York, and drop enough
poison gas to kill thousands and make practically the whole city
uninhabitable.”
CHAPTER IV
EARTH’S FOUR ATMOSPHERES
The earth has four important atmospheres and others of less
importance. The principal ones are oxygen, nitrogen, vapor of water,
and carbon dioxide, each comporting itself as it would do if the
others were not present. There is space between the molecules of
each gas, and therefore it is easily compressed. A doubling of its
pressure reduces its volume one half.
=Composition of Atmospheric Air.= It is difficult for the mind to
form a picture of the infinitely small molecules of the air. Let
us therefore use terms and comparisons that will the more directly
appeal to the human senses. First let us imagine each molecule
enlarged to the size of a small grain of sand. Then with the
molecules from one cubic inch of air transformed into grains of sand
we could build a roadway ten feet deep and one hundred feet wide
extending from New York to San Francisco. May one still further grasp
the idea of the atom, many of which are required to make up the
molecules? If so, the imagination has been stretched to its limits to
enable the human mind to comprehend some of the simplest facts with
regard to the wonderful fluid in which we live.
Sir William Thomson, afterwards Lord Kelvin, in endeavoring to give
relative values that would appeal to the imagination, said that if a
drop of water were enlarged to the size of the earth, the molecules
of which it is composed would be no larger than cricket balls, and
the smallest about the size of small peas.
More than a thousand years before the birth of Christ a great
Phœnician philosopher believed that all matter—solids, liquids, and
gases—was built up from infinitely small aggregations of atoms. The
learned men of Greece enlarged upon his views but this philosophy
passed into oblivion with the destruction of Rome and the coming of
the Dark Ages, and it was not revived until about one hundred and
fifty years ago. The ancients could not prove their theory, while
we to-day can count the atoms and determine their size and motions;
and, exceedingly small though they be, we no longer believe them
to be indivisible in structure. On the contrary, we know that each
atom consists of particles of positive and negative electricity.
The negative electrons arrange themselves about a positive electron
for a nucleus and, rotating about it as if it were a central sun
with planets, constitute an atom. All matter reduced to the ultimate
electron is precisely alike. The difference in matter is determined
by the number of negative electrons that are attracted and held in
place by the positive nucleus that is at the center of each atom of
which a particular kind of matter is composed. Each of the ninety-two
elements which we believe constitute the ninety-two different forms
of simple matter has an atom with its own peculiar type of nucleus,
which nucleus differs from those of the others only in the amount of
positive electricity it contains. Thus hydrogen, the lightest of all
gases, whose weight is taken as unity in measuring the magnitude of
other gases, has a nucleus whose positive charge of electricity is
only sufficient to attract one negative electron. The next element,
helium, has a nucleus with a double positive charge and consequently
holds two electrons or planets to pay it homage. In like manner
the carbon atom contains six electrons; oxygen, eight; aluminum,
thirteen; nitrogen, fourteen; sulphur, sixteen; iron, twenty-six;
copper, twenty-nine; silver, forty-seven; gold, seventy-nine;
mercury, eighty; lead, eighty-two; bismuth, eighty-three; radium,
eighty-eight; thorium, ninety; and uranium, ninety-two. The chemical
union of these elementary forms of matter creates other forms. For
instance, the union of two atoms of hydrogen and one of oxygen
constitutes a molecule of water. But the gases of the atmosphere
are not in chemical union; they exist in the form of a mechanical
mixture, each acting as though the others were not present.
It is important that this mixture of gases that constitutes our air
be maintained in the right proportion. Only a slight difference in
relative amounts might be disastrous to life. An increase in the
oxygen would stimulate mental and physical activities and hold the
human faculties at a higher tension. Man would accomplish more in a
given time, but his span of life would be shortened; and too great an
increase in the proportion of this stimulating element would quickly
terminate life. Conversely an increase in the nitrogen would render
all life more lethargic and man would be slower to act and to think;
and too great an increase would smother every living thing.
In addition to the gases named, the air contains small amounts of
many other substances,—argon, nitric acid, ammonia, ozone, xenon,
krypton, and neon; as well as organic matter, germs, and dust in
suspension. Over the land it contains sulphates in minute quantities,
and over the sea and near the seashore salt left from the evaporated
spray.
The proportion of each component of the atmosphere by volume of the
total atmosphere is different from its proportion by weight. The
percentages for the more abundant gases are as follows:
===============+=============+===========
| BY VOLUME | BY WEIGHT
---------------+-------------+-----------
Nitrogen | 78.04 | 75.46
Oxygen | 20.99 | 23.19
Argon | 0.94 | 1.30
Carbon dioxide | 0.03 | 0.05
+-------------+-----------
| 100.00 | 100.00
===============+=============+===========
=Nitrogen.= Its principal functions are to dilute the oxygen and to
furnish food to vegetation. It is inert and does not manifest many
marked chemical affinities. Its lack of activity is shown by the fact
that it will neither support combustion nor burn.
=Oxygen.= Oxygen, unlike nitrogen, is an active element that readily
enters into chemical combination with many other elements, and it
is second in quantity to nitrogen. With hydrogen it constitutes
eight ninths, by weight, of water; combined with other elements it
constitutes forty to fifty per cent. of the crust of the earth. It
burns so readily that were it not greatly diluted by an inert gas
like nitrogen it would be difficult if not impossible to stop a
conflagration when once started. It is the vitalizing principle in
all forms of life. By its chemical union with carbon in the tissues
of plants and animals it develops the energy manifested in their
movements.