by Eric Flint
Guides to Navigation
For down-timers, the leading English practical textbooks are William Bourne's Regiment for the Sea (1573, 1631), which was based on Martin Cortes' Arte de Navigar (1551);Thomas Blundeville's Exercises (1594, 1597, 1606, 1613); John Davis' Seamans Secrets (1594); Edward Wright's Certain Errors in Navigation (1599); Richard Polter's The Pathway to Perfect Sailing (1605, 1613); and Thomas Addison's Arithmetical Navigation (1625). For those more mathematically inclined, there was Robert Tanner's Brief Treatise of the Use of the Globe Celestrial and Terrestrial (1620), in eight volumes. And if you were more interested in navigational instruments, you could consult Anthony Ashley's Mariner's Mirrour (1588), William Barlow's The Navigator's Supply (1597), and various books by Edmund Gunter (1632, 1624, 1630 and 1636). (Swanick 57-67).
There are also various astronomical almanacs, but those will be discussed in the second article.
Grantville being far from the sea, it is not a likely repository for nautical texts. However, the consensus of the Editorial Board is that there will be at least a couple of editions of Bowditch's American Practical Navigator around (several having been found at a used bookstore in Parkersburg, West Virginia, and the Up-timer's Grid listing both Jack Clements, a retired Coast Guard boat pilot, and of course the aviator Jesse Wood). Even if we ignore APN, there are a surprisingly large number of useful entries in the 1911 Encyclopedia Britannica, and there are books on astronomy and mathematics in the school libraries. And the atlases and National Geographics maps will no doubt come in handy.
Navigation by Terrestrial Signs
Landmarks . The simplest form of navigation is to take note of prominent landscape features, and their bearings. Ideally, you take cross-bearings (simultaneous bearings of two different landmarks, lying in different directions), because that fixes your position. Lighthouses and buoys, of course, can be considered artificial landmarks.
Knowledge of landmarks was initially confined to local sailors. However, it became customary for long-distance mariners to draw "profiles" of the coasts they visited in their logbooks (Taylor 168). These sketches could be passed on to allied captains.
The "knowhow" of sailors was distilled into guidebooks known in ancient times as periplous, and, later as portolans, rutters and waggoners. They could include charts, profiles, and logbook summaries. The most famous of them all was Lucas Wagenaer's Mariner's Mirror (1584). Sailing directions are primarily directed to coastal navigation.
Soundings . In shallow waters, including the North Sea and Baltic Sea, it was common to navigate by soundings. This involved dropping a sounding line, a knotted rope with a lead weight, to the bottom. The number of knots passing over the side gave the depth. The weight could be "armed" with tallow to pick up sediment from the sea floor. Sailing instructions would tell mariners what to expect. For example, it might say that you have reached the shallow region between Cape Clear and the Isles of Scilly, when "at 72 fathoms [you] find fair gray sand" (Aczel, 12-3, 134-5).
The modern lead line is distinctively marked so that the leadsman can recognized the marks by feel even in the dark: two strips of leather at two fathoms, three at three, a white cotton rag at five, red woolen bunting at seven, and so on. The standard lines are twenty and one hundred fathoms long. (Mixter 11).
A sounding machine was invented by Lord Kelvin in the nineteenth century, and such machines are described in 1911EB. Soundings can be taken day or night, under harsh sea and wind conditions, and up to depths of several thousand fathoms, using galvanized steel wires which are reeled back in by an engine.
A twentieth century alternative to the sounding line is the fathometer, a SONAR-based echo sounder (Togholt 37). Unfortunately, I don't know enough about electronics to venture a guess as to when these can be built, post-RoF.
Several up-time fishing fathometers made it through the RoF. The first reference in canon is in 1633 chapter 38: "At least I could send them out ahead with Al's fishing fathometer to look for the really shallow spots." In chapter 46, Eddie, in the powerboat Outlaw, says, "'We ought to have enough water, and we'll keep an eye on the fathometer.' He tapped the digital depth display, and Larry nodded again." 1634: The Baltic War, Chap. 34 reveals the existence of at least six fishing fathometers, two on the "up-time power boats leading the ponderous line of gunboats," and the remainder on Simpson's four ironclads.
The immediate contribution which the up-timers can make to navigation by soundings is to provide copies of up-time maps with depth markings. There is typically some sounding information on National Geographic maps. Of course, it is unlikely that anyone in landlocked Grantville has the detailed marine charts of coastal waters and, even if they did, they probably don't correspond too well to seventeenth century reality; coasts and bottoms change over time.
Other signs . Those who live on the sea (and die there if they are unobservant) tend to notice subtle cues as to where they are. These include the color of the sea, the typical currents and winds, bird and fish movements, and clouds which hover over islands and perhaps even reflect the color of the land below. (Taylor, 59-60, Calahan 82).
One modern contribution might be the use of the thermometer. By sampling water temperature, you can map out currents.
Terrestial Latitude and Longitude
While we may not have thought so in high school, one of the great intellectual inventions of mankind is the coordinate system. For example, if a city is laid out as a grid, we can send someone to the intersection of, say, North Tenth Street and East Third Avenue.
Latitude and longitude are the dimensions of a gridded spherical surface coordinate system first devised by the ancient Greeks. The earth is not a perfect sphere, but for our present purposes, it is close enough. Imagine the Earth as a hollow, see-through globe, with you hovering somehow at the center. If your body were aligned with the earth's axis, you could identify any point on the earth's surface by two angles, one measuring "up-and-down" relative to "level" (latitude) and the other "left-and-right" relative to "front" (longitude).
For each of these angles, we need a reference, a "zero." For latitude, it is the earth's equator, the intersection of the earth's surface with an imaginary plane perpendicular to the axis. Any point on the equator is zero degrees latitude. Angles are traditionally measured in degrees; by ancient convention, a circle is divided into 360 degrees (each degree, symbol d*, is divided into sixty arc minutes, symbol ', and each minute into sixty arc seconds, symbol "). Above your head would be the north pole, defined as 90 degrees north latitude. Below your feet, the south pole, at 90 degrees south latitude, sometimes represented as -90 degrees.
Except at the poles, the points on the earth's surface which have a particular value of the latitude form a circle on the earth's surface; the circles are parallel to each other (that is, they maintain a constant distance), and hence are also known as "parallels" (e.g., the 49th parallel, part of the border between Canada and the western United States).
The "lines" (really, half-circles) of constant longitude are called meridians. For longitude, we have to pick an arbitrary zero. Hipparchus proposed using a meridian which passed through the city of Rhodes. Currently, the zero longitude (prime) meridian is one established by an 1884 international treaty, and passes through the Royal Observatory at Greenwich, England. Longitude is measured as being so many degrees (up to 180) east or west of the prime meridian.
On a globe, the "lines" (circles) of latitude will always cross the "lines" (circles) of longitude at right angles. (A map may distort this relationship.)
If two points are on the same meridian (constant longitude), but one degree of latitude apart, that's a distance of about 69 miles. It would be the same distance, regardless of where you were, if the earth was a perfect sphere. So an error of one degree latitude corresponds to 69 miles. An error of one arc-minute ('), 1.15 miles. An error of one arc-second ("), 100 feet.
If two points are on the same parallel (constant latitude), but one degree of longitude apart, the distance bet
ween them would be a maximum of 69 miles (at the equator). The further away they are from the equator, the shorter the distance would be.
In 1632, the down-timers did not know the true length of a degree of latitude. However, it was measured with high precision (error <1%) in 1637 (EB11/Navigation). They did know the relative length of a degree of longitude, given the latitude, having published (1599) tables of "meridional parts."
Thanks to land observations, the down-timers know the latitudes of many ports. Even those given in the Regiment of the Astrolabe (1509) are accurate to 30', sometimes even 10' (Taylor 166).
Globes and Maps
Globes, like the earth, are spherical. Maps are flat. As you can verify by trying to flatten out the skin of an orange while keeping it as a single piece, some creativity is required to flatten out a spherical surface.
The technical term for the mathematical manipulation by which points on a spherical surface are converted to points on a flat surface is "projection." Any map projection is going to distort certain properties of the earth's surface, and, hopefully, preserve others. Projections can preserve direction from a central point (azimuthal projection), distance from a central point (equidistant), local shape (conformal), area (equiareal), etc. You need to use the right map projection for a particular purpose.
It should be noted that the down-time mathematicians know quite a bit about map projections. For example, Oronce Fine (1494-1555) invented a heart-shaped projection. The empirically developed Mercator (1512-1594) projection, given proper mathematical form by Wright (1599), is still used for navigation.
Great Circles and Rhumb Lines
A great circle (orthodrome) is a circle on a sphere which has the same diameter of the sphere, and thus divides the sphere into two hemispheres. The equator (zero latitude) is a great circle, and the meridians are portions of great circles (with constant longitude). However, these are special cases, and great circles can connect points which differ in both latitude and longitude.
If a map uses a gnomonic map projection, great circles are shown as straight lines. On a mercator projection, they are curves.
The shortest distance between any two points on the surface of a sphere is a portion of the great circle which connects the two points. Unfortunately, traveling on a great circle path requires continual correction of one's compass heading. Great circle sailing can also carry one to a higher latitude than is desirable (too much ice and fog).
A rhumb line (loxodrome) is a path on the spherical earth which corresponds to following a constant true compass bearing (azimuth), or, to put it another way, to crossing every meridian at the same angle. If a map uses a mercator projection, rhumb lines are straight lines. Parallel sailing is a special case of rhumb line sailing in which one sails along a parallel (line of latitude), thereby crossing every meridian at right angles.
As a compromise between minimizing the distance (great circle route) and facilitating steering (rhumb line), a great circle route may be approximated by a series of short rhumb lines connecting waypoints which lie on the great circle.
Composite sailing is a combination of great circle sailing to and from some limiting parallel, and parallel sailing in-between.
Dead Reckoning
In dead reckoning, the navigator plots the last known location on a chart, and extrapolates the present location based on the ship's subsequent heading(s), speed(s), and time elapsed.
The Spanish called dead reckoning, navegacion de fantasia (Gurney 19), and Edward Wright (1599) referred to the estimated position as "the point of imagination." (Williams) DR estimates of longitude were sometimes over 400 miles astray (Wakefield 165).
Surface currents usually exceed ten miles per day (mpd) and in many places are 40-50 mpd. If currents are ignored, the dead reckoning will accumulate error at a rate of 10-50 mpd. Even in the late eighteenth century, long-distance journeys typically accrued longitude errors of 5-15d* (Parr 68-9).
The Traverse Board was a device used to keep track of the courses steered. Every half-hour, a peg would be placed in one of 32 holes, each representing one point of the compass. There were eight such concentric circles of holes, thus recording an entire four hour watch. (Phillip-Birt 191).
Of course, steering a particular course didn't mean that the ship necessarily moved in the expected direction. The helmsman could be lax, the ship's steering arrangement could be inaccurate, and the ship could be forced off course by powerful winds and currents.
The prudent navigator attempted to estimate "leeway" (the extent to which the ship was forced off course) by looking at the angle between the wake and the heading. (Williams 22)
Moreover, even if the ship was placed on the desired compass bearing, that bearing might not be the desired true bearing, by reason of errors in correcting for magnetic variation and deviation, or of determining true north from the sky.
Logging Speed . For measuring speed, the sailor used a log. The common log was a piece of wood tied to a knotted line. The log was thrown out behind the ship, and the line allowed to run out. One sailor counted the knots as they passed over the rail, while another watched a sand glass. The count continued until the sand glass emptied. The first written description of this method was in William Bourne's A Regiment for the Sea (1574)(Williams 39 n. 3), and the log was in general use, at least by the English and Dutch, in the 1620s (Swanick 100).
The sailing term "knots" refers to the fact that sailors estimated their speed, in nautical miles per hour, as the number of knots run out per "glass." A knot is one nautical mile (6,076 feet, about one arc-minute of latitude.) per hour. Earlier schemes overestimated speed (perhaps deliberately), but the late eighteenth century, sailors used a knot spacing of 47.25 feet and a 28 second glass. (Gurney 25; Phillip-Birt 196)
There are some other obvious problems with this method. The log might be caught in the ship's wake, and the line not pay out properly. There might be little delays in calling out the end of the time interval. The knot counter might miscount, or have trouble estimating an intermediate value. The speed of the ship might change, after the fact, as a result of shifts in wind and current.
An alternative form of the common log was the "Dutchman's log": throw a chip off the bow and time how long it takes to reach it. (Mixter 12)
The common log was ultimately replaced by the patent log. This was a towed rotator, with spiral fins (Togholt 36). The passing water caused it to spin, and the rotations were mechanically communicated to a mechanical counting device. The patent log had to be calibrated by testing it on a run of a known length. Preferably you carried out two runs in opposite directions, so as to reduce the effect of any local current.
A steamship engineer could construct a power curve relating ship speed to engine speed (RPM) by carrying out similar runs at each of several engine speeds. Then the engine tachometer could be used as a log. (Mixter 13-15).
To get the distance run, the navigator multiplied the speed (presumed constant) by the time elapsed. Measuring shipboard time in the early seventeenth century was a rather chancy proposition, typically involving sandglasses.
Plotting. When dead reckoning is figured as if the earth is flat, that is called "plane sailing." For a DR plot to be accurate over long distances, you need to use a Mercator projection chart, or correct your eastings and westings for the changing length of a degree of longitude. The corrections are carried out with a table of meridional parts, which were first published in Wright's Certaine Errors in Navigation (1599). But in the late seventeenth century, Sir John Narborough said, "I could wish all seamen would give over sailing by the false plane charts and sail by the Mercator's chart . . . but it is a hard matter to convince any of the old navigators." (Williams 43-6).
Navigational Use of the Compass
The compass has two purposes: determining which course is being steered, and providing a reference point for the measurement of azimuth (horizontal direction) in celestial navigation. An error of 3d* in setting the course of the ship results in a positi
onal error of one mile for every twenty miles run (Mixter 48).
Magnetic Compass . The standard magnetic compass has a magnetized needle which only swings horizontally. However, there are also "dip" compasses which can pivot vertically, too.
The marine compass typically has a rotatable compass card, marked with the compass directions. At least one magnetized needle is attached to the underside of the card. (Unlike the boy scout compass, in which the needle turns, and the card is stationary.) The earth's magnetic field causes the needle, and with it the compass card, to turn on its axis until the needle is properly aligned with the local magnetic field.
Needles were magnetized by stroking them with an artificial or natural magnet (lodestone). The up-timers can teach how to magnetize steel rods by inserting them into a current carrying coil.
Increasing the number of needles makes the compass more sensitive, and it thus performs better when the sea is quiet, but then it oscillates too much when the waters are rough (Walker 72).
