Both parties now returned to Rio, only to find that the cable was still

broken. In order to be ready for work as soon as it should be repaired,

Lieut. Com. Green proceeded to Bahia with the ship and established a

station there, Lieut. Com. Davis with his party remaining in Rio. After

waiting a month, and there still seeming to be no prospect of the

repair of the cable, the expedition finally sailed for home, arriving

at Norfolk, Va., after a pleasant and uneventful voyage of forty-five

days. Repairs to the cable were not completed until several months

afterward. In May of the next year, the party was again sent out, to

complete the measurement on the Brazilian Coast, and also to measure

from Greenwich to Lisbon, the French Bureau of Longitudes having failed

to carry out its promise to measure from Paris. There being no ship

available for the purpose the traveling was done by mail steamer. Upon

arrival in England, an interview was had with the Astronomer Royal, who

readily agreed to assist in the work. Lieut. Com. Green accordingly

established his observatory at the landing place of the cable at

Porthcurnow in Cornwall, and Lieut. Com. Davis proceeded to Lisbon and

occupied the station used there the year before. Owing to the foggy and

rainy weather prevalent in England at that season, it was found

impossible to make any astronomical observations at the Porthcurnow

observatory. The work was therefore done in this way:--Observations

were made at Greenwich and at Lisbon, and Porthcurnow and Carcavellos

were used as transmitting stations. The chronometer at Porthcurnow was

compared automatically with the clock at Greenwich, and by cable with

the chronometer at Carcavellos. The latter was compared automatically

with that at Lisbon, before and after the cable exchange. At this time

there were made at Carcavellos, some experiments with a view to making

the receipt of the time signals over the cable automatic, thus doing

away with the personal equation of the receiver. The instrument in use

for the regular business of the cable was what is known as the siphon

recorder, also the invention of Sir Wm. Thompson. In this a small coil

of fine wire is suspended by a fibre of silk, between the poles of a

powerful permanent magnet. The currents from the cable pass through

this coil and the action is to deflect it to the right or left, just as

the mirror is deflected in the instrument already described. Attached

to this coil is a siphon made of a capillary glass tube. One end of the

siphon dips into a reservoir of aniline ink, and the other hangs

immediately over the centre of a fillet of paper, which is unwound by

clock-work. If the siphon touched the paper, the feeble currents sent

through the cable would be powerless to move it, on account of the

friction, and in order to produce a mark some means must be found of

forcing the ink through the capillary tube. This is accomplished by

electrifying the ink positively and the paper negatively, by means of a

small inductive machine, driven by an electric motor. The effort of the

two electricities to unite, forces the ink through the tube and it

appears on the paper as a succession of small dots. When the paper is

in motion and the coil at rest, a straight line is formed along the

middle of the fillet by these dots, but as soon as a current is sent

through the coil the siphon moves to the right or left making an offset

to this line. These offsets on one side or the other are used as the

dots and dashes of the Morse alphabet. A time signal sent over the

cable while this instrument was in circuit, appeared as a single offset

on the paper, and it was only necessary to graduate the paper into

seconds spaces by the local chronometer, in order to have the automatic

record required. The ordinary chronometer circuit could not be put

through the coil directly, as it would then charge the cable and

interfere with the signals, and besides, the current, unless by the

introduction of a high resistance it was reduced in strength, would

infallibly give such a violent motion to the coil as to break the

siphon, if it did no other damage. The result was obtained in this way;

an ordinary telegraph relay was put in the chronometer circuit and the

armature of course moved with the beats. To this armature was fastened

one end of a fine thread. The other end was attached to a slender piece

of elastic brass which was fixed at one end to the framework supporting

the paper, in such a way that the other end touched the metallic vessel

holding the ink, except when the thread was drawn tight enough to pull

it away. This the armature of the relay did while the circuit through

the chronometer was complete, but as soon as it was broken at the

beginning of a second, the tension of the thread was relaxed and the

brass sprung back against the ink well, allowing the positive and

negative electricities to unite independently of the siphon. The ink

then ceased to flow, until the spring was drawn away, thus leaving a

small blank space in the line of dots and forming a very good

chronographic record. This was liable to a small error due to the

length of time that elapsed between the release of the spring by the

armature and its impact on the ink well. Had there been time for more

extensive experiment this difficulty might have been overcome. Or if

the same method had been adopted at both stations, the result would

have been affected by only the difference between the times of movement

of the brass spring which would have been minute. Lack of time for

experiment, and the fact that the observers were averse to introducing

untested methods into a chain of measurements most of the links of

which were already completed, prevented any use being made of this

achievement. The measurement between Greenwich and Lisbon being

satisfactorily completed, Lieut. Com. Green by order of the Navy

Department returned to the United States, and the links between Rio and

Pernambuco and between the latter place and Para, were measured by

Lieut. Com. Davis and the writer, completing the work of the

expedition, after which the party returned to Washington.

The computation of this work, showed the somewhat surprising fact that

the heretofore accepted position in longitude of Lisbon, differed from

the true one by about two miles. The longitude of Rio Janeiro had

always been more or less in doubt, various determinations had differed

by as much as nine miles, but the position finally decided upon by the

best authorities agreed very closely with that obtained by telegraph.

The next expedition was sent out by the Bureau of Navigation to China,

Japan and the East Indies, Lieut. Com. Green being still in charge. The

officers composing the party sailed from San Francisco by mail steamer

in April, 1881, for Yokohama, where they joined the U. S. Steamer

Palos. From Hong Kong north to Vladivostok in Eastern Siberia the

cables were owned by a Danish company. From Hong Kong to the south and

west they were the property of English companies. Beginning at

Vladivostok observations were made at all stations on the Asiatic coast

except Penang, as far as Madras, India. It was intended to try and make

some use of the automatic method of receiving time signals, on this

work, but on arriving in Japan it was found that the recording

instrument used by the Danish company was entirely different from that

used by the English lines. It consisted of a series of electro-magnets

acting on a single armature, which carried a siphon made of silver. The

signals consisted of long and short movements, to one side of the

middle line, instead of equal deflections on both sides as in the

Thompson recorder. An attempt was made to convert this instrument into

a relay, by causing the siphon to make and break a circuit, but it was

not successful. The movements of the siphon were not regular enough,

and the contact was not firm. Consequently the mirror method of

exchanging signals was still adhered to.

The longitude of the position occupied in Vladivostok, had been

determined telegraphically from Pulkova, by the Russians, using the

land lines across Siberia. The English had also determined the position

at Madras, using the cables through the Mediterranean and Red Seas. The

work of the United States Expedition joined these two positions,

completing a chain of measurements extending over many thousand miles,

made by observers of different nationalities in various climates. It

was to be expected that considerable discrepancy would be found in the

final result, but taking the longitude of Vladivostok as brought from

Madras, and comparing it with that determined by the Russians, the

difference was only 0^{s}.39. Taking everything into consideration,

this result was gratifyingly close. Upon the conclusion of this series

of determinations, the connection of Lieut. Commander Green with the

work was severed, he receiving his promotion to the rank of Commander.

The next work was under the charge of Lieut. Com. Davis, and consisted

in the determination in 1883-84, of positions in Mexico, Central

America and the west coast of South America. Cables had just been

completed, extending from Galveston, Texas, to Vera Cruz, thence across

Mexico to the Pacific and down that coast to Lima, Peru, where

connection was made with another system extending to Valparaiso.

Galveston was a point determined by the Coast Survey, and the

measurement thence to Vera Cruz was the first one made. It was

completed in May '83, and in the Autumn of the same year the party

proceeded to the South American coast, and stations were established

and observations made at various points from Valparaiso to Panama, and

at one point, La Libertad, in Central America. It was at first the

intention to extend the series across the Isthmus of Tehuantepec and

connect with Vera Cruz, but lack of time prevented this, and as the

station at Panama determined nearly ten years before, afforded a

convenient starting point, the idea was abandoned. From Valparaiso, a

measurement was made with the coöperation of Dr. Gould to his

observatory at Cordova, using the line across the Andes, and exchanging

signals automatically. These measurements constituted the final links

in a long chain, extending from the prime meridian Greenwich across the

Atlantic to the United States, thence via the West Indies to Panama,

down the west coast of South America to Valparaiso, across the Andes to

Cordova and Buenos Ayres, up the east coast to Pernambuco, across the

Atlantic to Lisbon, and thence to Greenwich, altogether a distance of

eighteen to twenty thousand miles. The two longitudes of Cordova, as

brought from Greenwich by the two routes, differed from each other by

only 0^{s}.048, a result which speaks well for the accuracy of the

methods employed. When preparations were being made for this

expedition, it was determined to accomplish if possible something in

the way of getting rid of the personal equation in exchanging signals.

An idea which had been suggested by work done by Major Campbell, R. E.

in the measurement between Bombay and Aden, seemed to promise well. It

was to be used with the siphon or other form of recorder. The ordinary

double current cable key with two levers, was arranged with an

additional lever in such a manner that while in ordinary use in the

telegraph office, it could also be put in circuit with the chronometer

and chronograph in the observatory, and a signal sent through the cable

would have its time of sending registered on the chronograph.

Ordinarily in speaking over a cable line, connection is made in such a

way that the current sent does not pass through the recorder at the

sending station, as a violent movement of the siphon would result. By

means of a shunt, however, it is possible to control this movement

somewhat. Suppose now, that the connections at each station are made in

such a way, by means of this key and the shunt, that a signal sent from

one, is registered on both recorders and on the sender's chronograph.

The observers leaving their assistants to take care of the

chronographs, go to the respective telegraph offices, and all being

ready, the observer A taps his key. This sends an impulse through the

cable, which appears on A's recorder, as a violent jump or kick of the

siphon. On B's recorder it is registered as a deflection like the

ordinary dot or dash, at the same instant is recorded on A's

chronograph the time of sending. As soon as B sees the signal on his

recorder, he taps his key also registering the signals on both

recorders and on his chronograph. A, seeing B's signal again taps his

key, and so on, as long as desired. The result is that each observer

has a record on his siphon fillet of all signals sent and received,

while the times of those he sent are recorded on his chronograph. By

the use of the diagonal scale and the Rule of Three, he can without

difficulty find the times of the signals received. The siphon recorders

are well made, and the paper moves with great regularity. This system

was used in the measurement between Galveston and Vera Cruz with great

success. It was intended to employ the same method throughout the

measurement on the west coast of America, but on arriving at Lima, it

was found that the company owning the lines south of that point still

used the mirror galvanometer, and it was of course necessary to return

to the old method. The improved key was used however, which eliminated

the error in sending signals.

After this work was completed and the results published in 1885,

nothing was done in this line by the Bureau of Navigation for some

years. Upon the return of the writer in the spring of 1888, from a

cruise in the South Pacific, he found that the subject of sending an

expedition to complete the measurements in Mexico and Central America

was under consideration in the Bureau of Navigation and the

Hydrographic office. It was finally decided that the work should be

done, and the writer was placed in charge. The instruments were brought

out of their retirement, and by the aid of the Hydrographic Office a

very complete outfit was furnished, and in November of last year a

start was made from New York, the expedition proceeding by mail steamer

to Vera Cruz. Here the spot occupied by Lieut. Com. Davis in '83 was

found, his transit pier, which was still standing was repaired, and

instruments mounted. Lieut. Charles Laird, U. S. N., who had been

identified with the longitude work since the China expedition in 1881,

was left in charge of the observatory at Vera Cruz, and the writer

proceeded with his party to the small town of Coatzacoalcos, at the

mouth of the river of the same name. This point is about one hundred

and twenty miles southeast of Vera Cruz, and is the landing place of

the cable. A land line extends from this point to Salina Cruz on the

Pacific coast, a distance of about two hundred miles. In exchanging

time signals between Vera Cruz and Coatzacoalcos, the automatic method

was employed, the cable being short. The old wooden observatories were

used at these points, but as they were too heavy for transportation

across the Isthmus, tents made especially for astronomical purposes

were substituted for them in the observations made on the Pacific

coast. The journey across the Isthmus was slow, about two weeks being

employed in traveling two hundred miles, though as the route was

devious, the actual distance was nearer three hundred. Some of the

instruments were heavy, and after being taken in canoes a hundred miles

up the Coatzacoalcos river, against a rapid current, they were loaded

on a train of pack mules, and carried the rest of the way by land.

While the first party was crossing the Isthmus, the other was on its

way from Vera Cruz, and being ready at about the same time, a

successful measurement was made between Coatzacoalcos and Salina Cruz,

exchanging signals automatically. The Coatzacoalcos party then crossed

to Salina Cruz, while the other proceeded to La Libertad in Salvador,

where the station established in the Spring of '84, was again occupied.

The measurement between these places being completed, the Libertad

party went on to San Juan del Sur, in Nicaragua, near the terminus of

the proposed interoceanic canal. In the measurement between this point

and Salina Cruz, as well as in the one preceding, the exchange was

effected by mirror signals. This completed the season's work, and the

two parties made the best of their way home via Panama, arriving in

Washington in April and May respectively. The computation of the

observations is not yet complete though well advanced; it was the

intention to publish preliminary results this Fall, but owing to lack

of time that can not be done.

Another piece of work is laid out for the same party for the coming

winter, which is the measurement from Santiago de Cuba, through Hayti

and San Domingo to La Guayra in Venezuela, over the cables of a French

company, which have just been completed. This work will consume about

six months, and the expedition which is to start almost immediately

will probably return in April or May next. The determination of the

longitude of La Guayra will give a point from which many other

measurements may be made along the north coast of South America,

furnishing material for extensive corrections of the charts of that

region.

* * * * *

Having presented an outline of the work done so far, as well as that

proposed for the near future, I will now mention some of the trials and

tribulations, as well as the pleasures experienced in carrying out the

object desired in an expedition of this kind. The greatest politeness

and kindness have always been experienced from the officials and

employees of the various telegraph companies over whose lines work has

been carried on. The government officials of the foreign countries

visited, have also invariably shown the utmost politeness, but

sometimes this politeness has been visibly tinged with suspicion. The

measurements in Peru and Chili were made amid the closing scenes of the

war between the countries. Upon the arrival of the expedition in Lima,

an interview was had with the Chilian Commander-in-Chief who had

possession of the city, and permission was requested and readily

granted to occupy a station in Arica. Upon arriving at the latter place

some days after, the Chilian governor in charge was found to have

instructions to facilitate the work, and readily granted permission to

establish the observatory in a convenient locality, but flatly refused

to allow a wire to be extended to the telegraph office, and also

refused to forward to his immediate superior, a request that it might

be allowed. He evidently supposed the party were emissaries of the

United States, sent to treat secretly with conquered Peru, but how he

expected this was to be done remains a secret. By a vigorous use of the

telegraph in communicating with the U. S. Ministers to both Chili and

Peru, his objections were silenced, and the wire was put up. The

observatory at Arica was erected on the side of a hill to the windward

of the town, because it afforded a clear view, and was less dirty than

other eligible sites. It also was a safe position in case of a possible

earthquake or tidal wave, by which Arica had already been twice visited

with disastrous effect. In digging for a foundation for the transit

pier, several mummies of the ancient Peruvians were unearthed at a

depth of a foot. They had evidently belonged to the poorer class of

people, as their wrappings were composed of coarse mats, instead of the

fine cloth with which the wealthier people were usually interred. One

was the body of a female with long hair, which had been turned to a

reddish yellow color by the alkali in the soil. The whole coast of Peru

is barren and desolate, except in the river valleys, it being seldom

visited by rain, while it is nearly always overhung with heavy clouds

and fog banks, which render astronomical work exceedingly difficult.

Even when partially clear in the day time, it generally becomes cloudy

at night. Many times the observer would be at his place before sunset

ready to seize the first suitable star revealed by the darkness, only

to be baffled by thick banks of cloud which would cover the entire sky

in from five to ten minutes.

In northern Peru, with a latitude of about five degrees south, is the

town of Paita. It is an assemblage of mud-colored houses, at the foot

of high, mud colored bluffs. On top of these bluffs is a perfectly

barren table land extending inland and up and down the coast for many

miles. Before visiting it the observers were informed that its one good

point was the perfect astronomical weather which always prevailed.

Clouds were unknown, and such a thing as rain had never been heard of.

The extreme dryness of the atmosphere was so favorable to health that

no one ever died, and when a consumptive invalid was imported by the

inhabitants in the hope of starting a cemetery, he blasted their

expectations by recovering. Judge then of their feeling, when upon

arriving at this delightful place, they were met with the information

that while it was true that the sky was, in general, perfectly clear

both by night and day, yet about once in seven years, rain could be

expected, and that the year then present was the rainy one. And sure

enough it did rain. The usually dusty streets became rivers and

quagmires, the rocky valleys in the vicinity were transformed into

roaring torrents, and the table land usually an arid desert became a

swamp with a rank growth of vegetation. However by using every

opportunity and snatching stars between clouds and showers the work was

finally completed.

Upon arriving in Panama shortly after this experience, the party was

met with the pleasant intelligence that yellow fever was prevalent, and

that the foreigners were dying like sheep. Nearly every day of the

party's stay, some one died of sufficient importance to have the church

bells tolled for his funeral, while of the ordinary people little

notice was taken. Every morning, the writer remembers passing a

carpenter's shop where nothing was made but coffins, and the supply was

evidently not equal to the demand, for finally the proprietor began to

import them, apparently by the ship load. The weather however was

delightful, and the nights were the most perfect, astronomically

speaking, that could be desired.

The observers who went from Japan to Vladivostok were obliged to wait

several weeks at Nagasaki, before an opportunity offered for proceeding

to their destination, and when they finally arrived, the getting away

again was a problem. Communication with the outside world by water was

only open during the summer months, and even then it was more

accidental than otherwise. The party established the observatory

however, and settled down to work, letting the future take care of

itself. In the early part of the work, rather an amusing incident

occurred. As the community was full of all sorts and conditions of men,

Koreans, Chinamen and Russian exiles, the last not political but

criminal offenders; it was thought wise to have a sentry stationed at

the observatory to guard against any possible harm to the instruments.

So the Governor of the town was asked to furnish a soldier for that

purpose, which request was readily granted, and one night the sentry

was posted with orders to let no one touch the observatory. These

orders he construed literally, and when the observers appeared to

commence their night's work, he kept them off at the point of the

bayonet. His only language being Russian with which the observers were

not familiar, it was impossible to explain the true state of affairs,

and it was only after hunting up an interpreter and communicating with

his commanding officer that an entry was finally effected. A good deal

of bad weather was experienced at this place, but at the end of six

weeks enough observations had been made for the required purpose, and

the party was fortunate enough to secure passage to Nagasaki, in a

small steamer that had brought a load of coal out from Germany.

In the expedition to the Asiatic coast one of the most interesting

experiences was the trip to Manila in the Philippine Islands. This is

quite a large town when intact, but a great portion of it is usually in

the condition of being shaken down by an earthquake or blown over by a

typhoon. The inhabitants are full of energy, however, and find time

between downfalls to build up again. The cable from Hong Kong lands at

a point about one hundred and twenty miles from Manila, and the writer

was directed to proceed thither, with a chronometer and chronograph for

the purpose of transmitting time signals. The first part of the journey

was made in a small coasting steamer uncommonly dirty, and occupied

about thirty-six hours. At the end of that time the village of Sual in

the Gulf of Lingayen was reached. This was distant from the cable

station about thirty miles, and the remainder of the journey was made

in a native boat, with mat sails, and bamboo outriggers, part of the

time through channels between numerous small islands and for some

distance in the open sea. The progress was slow, but it was a pleasant

way of traveling, except for the sleeping accommodations which were

primitive; consisting of a palm leaf mat thrown over a platform made of

split bamboo, in which all the knots had been carefully preserved.

About three days, including stoppages, were consumed in this thirty

mile voyage, and the traveler finally reached his destination to be

received with the greatest hospitality by the staff at the telegraph

station, and just in time to allay the fears of the observers at Hong

Kong and Manila who had begun to think him lost. About three weeks were

spent here, and as the work only occupied a short time at night, the

days were pleasantly passed in exploring the surrounding country,

making friends with the natives, shooting and photographing the

scenery. The return to Manila was by the same route and occupied nearly

the same length of time.

The measurement from Singapore to Madras was over one of the longest

lines of cable ever used for this purpose, the distance being about

1600 nautical miles. The Atlantic cables used by Dr. Gould in 1866 were

a little more than 1,850 miles in length. There was an intermediate

station at Penang about 400 miles from Singapore, where all the work of

the line was repeated. For the longitude measurement however the cables

were connected through to form an unbroken line. The mirror was the

only instrument that could be used and even with this the signals were

feeble and much affected by earth currents.

The National Geographic Magazine, Vol. II., No. 1, April, 1890 · 第 2 / 7 段