LECTURE I. NATURE AND DIFFERENT FORMS OF RADIATION. 1. Radiation is a form of energy, and, as such, can be produced from other forms of energy and converted into other forms of energy. The most convenient form of energy for the production of rad- iation is heat energy, and radiation when destroyed by being intercepted by an opaque body, usuaDy is converted into heat. Thus in an incandescent lamp, the heat energy produced by the electric current in the resistance of the filament, is converted into radiation. If I hold my hand near the lamp, the radiation intercepted by the hand is destroyed, that is, converted into heat, and is felt as such. On the way from the lamp to the hand, how- ever, the energy is not heat but radiation, and a body which is transparent to the radiation may be interposed between the lamp and the hand and remains perfectly cold. The terms "heat radiation " and " radiant heat," which are occasionally used, therefore are wrong: the so-called radiant heat is not heat but radiation energy, and becomes heat only when, intercepted by an opaque body, it ceases to be radiation; the same, however, applies to any radiation. If we do not feel the radiation of a mercury lamp or that of the moon as heat, while we feel that of a coal fire, it is merely because the total energy of the latter is very much greater; a sufficiently sensitive heat-measuring instrument, as a bolometer, shows the heat produced by the interception of the rays of the mercury lamp or the rays of the moon. The most conspicuous form of radiation is light, and, therefore, it was in connection with this form that the laws of radiation were first studied. 1 2 RADIATION, LIGHT, AND ILLUMINATION. 2. The first calculations of the velocity of light were made by astronomers in the middle of the eighteenth century, from the observations of the eclipses of the moons of Jupiter. A number of moons revolve around the planet Jupiter, some of them so close that seen from the earth they pass behind Jupiter and so are eclipsed at every revolution. As the orbits of Jupiter's moons were calculated from their observations by the law of gravita- tion, the time at which the moon M should disappear from sight, FIG. 1. when seen from the earth E, by passing behind Jupiter, 7 (Fig. 1), could be exactly calculated. It was found, however, that some- times the moon disappeared earlier, sometimes later than cal- culated, and the difference between earliest and latest disappear- ance amounts to about 17 min. It was also found that the disappearance of the moon behind Jupiter occurred earlier when the earth was at the same side of the sun as Jupiter, at A, while the latest disappearance occurred when the earth was on the opposite side of the sun from Jupiter, at B. Now, in the latter case, the earth is further distant from Jupiter by the diameter ASB of the orbit of the earth around the sun S, or by about 195,000,000 miles and the delay of 17J min. thus must be due to the time taken by the light to traverse the additional distance of 195,000,000 miles. Seventeen and one-third min. are 1040 sec. and 195,000,000 miles in 1040 sec. thus gives a velocity of light of » or 188,000 miles per sec. Later, the velocity of light was measured directly in a number of different ways. For instance, let, in Fig. 2, D be a disk per- forated with holes at its periphery. A lamp L sends its light through a hole H0 in the disk to a mirror M located at a con- siderable distance, for instance 5 miles; there the light is reflected NATURE AND DIFFERENT FORMS OF RADIATION. 3 and the mirror is adjusted so that the reflected beam of light passes through another hole Hl of the disk into the telescope T. If the disk is turned half the pitch of the holes the light is blotted out as a tooth stands in front of both the lamp and the telescope. Again turning the disk half the pitch of the holes in the same 5_MOE_S FIG. 2. direction the light reappears. If the disk is slowly revolved, alter- nate light and darkness will be observed, but when the speed in- creases so that more than from 10 to 20 holes pass per second, the eye is no longer able to distinguish the individual flashes of light but sees a steady and uniform light; then increasing the speed still more the light grows fainter and finally entirely disappears. This means when a hole H0 is in front of the lamp, a beam of light passes through the hole. During the time taken by the light to travel the 10 miles to the mirror and back, the disk D has moved, and the hole Hv which was in front of the telescope when the light from the lamp passed through the hole HQ, has moved away, and a tooth is now in front of the telescope and intercepts the light. Therefore, at the speed at which the light disappears, the time it takes the disk to move half the pitch of a hole is equal to the time it takes the light to travel 10 miles. Increasing still further the velocity of the disk D, the light appears again, and increases in brilliancy, reaching a maximum at twice the speed at which it had disappeared. Then the light reflected from the mirror M again passes through the center of a hole into the telescope, but not through the same hole Ht through which it would have passed with the disk stationary, but through the next hole H2, that is, the disk has moved a distance equal to the pitch of one hole while the light traveled 10 miles. Assume, for instance, that the disk D has 200 holes and makes 4 RADIATION, LIGHT, AND ILLUMINATION. 94 rev. per sec. at the moment when the light has again reached full brilliancy* In this case, 200 X 94 = 18,800 holes pass the telescope per second, and the time of motion by the pitch of one hole is sec., and as this is the time required by the light 18,800 to travel 10 miles, this gives the velocity of light as 10 •* > lo,oOU or 188,000 miles per sec. The velocity of light in air, or rather in empty space, thus is 188,000 miles or 3 X 1010 cm. per sec. For electrical radiation, the velocity has been measured by Herz, and found to be the same as the velocity of light, and there is very good evidence that all radiations travel with the same velocity through space (except perhaps the rays of radioactive substances). 3. Regarding the nature of radiation, two theories have been proposed. Newton suggested that light rays consisted of extremely minute material particles thrown off by the light- giving bodies with enormous velocities, that is, a kind of bom- bardment. This theory has been revived in recent years to explain the radiations of radium, etc. Euler explained the light as a wave motion. Which of these explanations is correct can be experimentally decided in the following manner: Assum- ing light to be a bombardment of minute particles, if we com- bine two rays of light in the same path they must add to each other, that is, two equal beams of light together give a beam of twice the intensity. If, however, we assume light is a wave motion, then two equal beams of light add to one of twice the intensity only in case the waves are in phase, as Al and B^ in Fig. 3 add to Cr If, however, the two beams A2 and B2 are not in phase, their resultant C2 is less than their sum, and if the two beams A3 and B3 in Fig. 3 happen to be in opposition (180 degrees apart), that is, one-half wave length out of phase with each other, their resultant is zero, that is, they blot each other out. Assuming now we take a plain glass plate A (Fig. 4) and a slightly curved plate B, touching each other at (7, and illuminate them by a beam of uniform light — as the yellow light given by coloring the flame of a bunsen burner with some sodium salt — a part of the light b, is then reflected from the lower surface of NATURE AND DIFFERENT FORMS OF RADIATION. 5 the curved glass plate B, a part c, passes out of it, and is reflected from the upper surface of the plain glass plate A. A beam of FIG. 3. reflected light a, thus is a combination of a beam b and a beam c. The two beams of light which combine to a single one, a, differ from each other in phase by twice the distance between the two glass plates. At those points dv dv etc. at which the distance FIG. 4. between the two glass plates is J wave length, or j, J, etc., the two component beams of a would differ by \, f , |, etc. wave lengths, and thus would blot each other out, producing darkness, 6 RADIATION, LIGHT, AND ILLUMINATION. while at those points where the distance between the glass plates is J, 1, lj, etc. wave lengths, and the two component beams a thus differ in phase by a full wave or a multiple thereof, they would add. If, therefore, light is a wave motion, such a structure would show the contact point C of the plates surrounded by alternate dark rings, d, and bright rings, y. This is actually the case, and therefore this phenomenon, called " interference" proves light to be a wave motion, and has lead to the universal acceptance of the Eulerian theory. Measuring the curvature of the plate B, and the diameter of the dark rings d, the distance between the plates B and A at the dark rings d, can be calculated and as this distance is one- quarter wave length, or an odd multiple thereof, the wave length can be determined therefrom. The wave length of light can be measured with extremely high accuracy and has been proposed as the absolute standard of length, instead of the meter, which was intended to be 10~7 of the quadrant of the earth. 4. It is found, however, that the different colors of light have different wave lengths; red light has the greatest wave length, and then in the following order: red, orange, yellow, green, blue, indigo, violet, the wave length decreases, violet light having the shortest wave length. If in experiment (Fig. 4) instead of uniform light (monochro- matic light), ordinary white light is used, which is a mixture of all colors, the dark and bright rings of the different colors appear at different distances from each other, those of the violet near- est and those of the red the furthest apart, and so superimpose upon each other, and instead of alternately black and light rings, colored rings appear, so-called interference rings. Wherever a thin film of air or anything else of unequal thickness is inter- posed between two other materials, such interference colors thus appear. They show, for instance, between sheets of mica, etc. The colors of soap bubbles are thus produced. The production of such colors by the interference of rays of light differing from each other by a fractional wave length is called iridescence. Iridescent colors, for instance, are those of mother-of-pearl, of opal, of many butterflies, etc. Light, therefore, is a wave motion. NATURE AND DIFFERENT FORMS OF RADIATION. 1 The frequency of radiation follows from the velocity of light, and the wave length. The average wave length of visible radiation, or light, is about lw = 60 microcentimeters,* that is, 60 X 10~8 cm. (or about ^ field: 15 20,000 km. = 12,500 mi. 25 12.000 km. = 7, 500 mi. 3.15 60 5, 000 km. = 3, 100 mi. 133 2,250 km. = 1,400 mi. High frequency cur- \ rents, surges and oscillations, arcing V (9.57) 31.64 grounds, lightning phenomena, etc. J Wireless telegraph ( 105 3 km. = 10,000 ft. 9.63 ) A ~, waves : ( 107 30 m. = 100 ft. 16.25 \ 6'62 Herzian waves: 107 109 30 m. = 100 ft. 30 cm. = 1 ft. 16.25 ) 22.90 I 12.3 Limit of electric waves : 6X1010 0.6 cm. = 0.25 in. 28.55 ) ) First gap : [4.25] Ultra-red rays : 10'2 4X10' 30,000x10-" =0.03 cm. 76xlO~8 cm. 3280 ) ftAQ 41.48 f b>ba Visible light rays : j 7.7X10' 76xlO-6cm. 39xlO~e cm. 41.48 i ft Q7 42.45 ] U