Use LEFT and RIGHT arrow keys to navigate between flashcards;
Use UP and DOWN arrow keys to flip the card;
H to show hint;
A reads text to speech;
41 Cards in this Set
- Front
- Back
Electromagnetic wave
|
traveling oscillation of an electric and a magnetic field
fields are perpendicular to each other and directions of propagation is perpendicular to both fields it is a transverse wave generated by acceleration of electric charge |
|
Speed of electromagnetic wave (c)
|
constant speed and always equal to ratio of magnitudes of electric field and magnetic field
c = E/B energies of 2 fields are equal |
|
Poynting vector (S)
|
describeds the rate and direction in which an electromagnetic wave is transporting energy per unit area
always perpendicular to both E and B has a magnitude of EBsin0 |
|
Light
|
tiny sliver from the electromagnetic spectrum
|
|
visible light
|
includes wavelengths from 390 to 700 nm
shorter wavelengths correspond to violet light and longer wavelengths to red light |
|
ultraviolet light
|
just beyond visible spectrum on smaller wavelength side
|
|
infrared
|
just beyond visible spectrum on longer wavelength side
|
|
colors of visible spectrum
|
Roy G. Biv
Red, orange, yellow, green, blue, indigo, violet wavelengths toward violet have more energy |
|
index of refraction (n)
|
constant for the medium light propagates through
n = c/v n: index of refraction c: speed of light in vacuum v: speed of light in medium since nothing exceeds the speed of light in a vacuum, all media have an index of refraction greater than 1 the greater the index of refraction, the slower light moves through that medium n for water = 1.3 n for glass = 1.5 |
|
plane-polarized light
|
light with electric fields in one particular direction as a result of screening out photons not have an electric field in one particular direction (filter)
|
|
isotropic light
|
unpolarized light, white light
electric fields point in all directions when polarized, it loses 1/2 of its intensity |
|
dual nature
|
acts both as a wave and a particle
propagation properties can be described with wave theory energy transformation properties are best described by particle theory |
|
angle of incidence
|
angle at which light ray strikes the interface as measured from a line normal to the interface
equals angle of reflection |
|
angle of reflection
|
angle at which light ray reflects off of interface as measured from a line normal to the interface
equals angle of incidence |
|
angle of refraction
|
angle at which light ray refracts through the interface as measured from a line normal to the interface
given by Snell's law: n1sin01 = n2sin02 |
|
Snell's law
|
gives you angle of refraction
n1sin01 = n2sin02 |
|
Energy of a single photon
|
E = hf
E: energy of single photon h: planck's constant f: frequency when light crosses into a new medium, frequency remains the same and wavelength changes |
|
total internal reflection
|
occurs when light coming from a medium with higher index of refraction, causes angle of incidence to be so large that entire amount of photons will be reflected at the angle of reflection and none will refract
this angle of reflection is the critical angle |
|
critical angle
|
angle at which light reflects when there is total internal reflection (no refraction)
0critical = sin^-1(n2/n1) 0critical: critical angle n: index of refraction |
|
refraction of different waves at interface
|
longer wavelengths (lower frequencies) move faster through a medium and therefore bend less at interface
shorter wavelengths (higher frequencies) move slower through medium and therefore bend more at interface |
|
diffraction
|
another type of wave-bending phenomenon
when wave moves through a small opening, it bends around the corners of that opening the smaller the opening and the larger the wavelength, the greater the diffraction smaller the hole the greater the spreading of light results in an image of light and dark bands or in dispersion and the creation of colors (depend upon destructive and constructive interference) |
|
virtual image
|
does not actually exist outside the mind of the observer
no light rays emanate from virtual image if a sheet of white paper is placed at the position of a virtual image, no image will appear on the paper ex: reflection in a flat mirror, a mirage, image under water |
|
real image
|
exists separately from the observer
rays of light actually intersect and then emanate from the point of intersection to form a real image if a sheet of white paper is placed at the position of a real image, the image will appear on the paper |
|
two types of mirrors
|
1. convex
2. concave |
|
two types of lenses
|
1. diverging (concave), acts like convex mirror
2. converging (convex), acts like concave mirror (3Cs: a thiCk Center Converges light) |
|
radius of curvature
|
for small section of curve is radius of extended circle
smaller radius of curvature indicates a sharper curve |
|
focal point
|
where light from horizontal rays is reflected by concave mirrors (or refracted by converging lenses) to focus on a single point
varies with frequencies |
|
focal length
|
length of separation between mirror or lens and the focal point
it is related to radius of curvature fmirror = 1/2r fmirror: focal length r: radius of curvature focal point for a lens (flens) is affected by the refractive indices of the lens and the medium that the lens is in flens is also affected by radii of curvature of both sides of the lens |
|
lens maker's equation
|
1/flens = [(n1/n2)-1][(1/r1)-(1/r2)]
when n1=n2, lens will not refract light |
|
power
|
measured in diopters, which has equivalent units of m^-1
the inverse of the focal length P = 1/f P: power f: focal length of lens |
|
lateral magnification (m)
|
ratio of size of image to size of object (compare heights)
equal to negative of ratio of distance of image and distance of object from mirror or lens negative sign indicates that if both distances are positive, than the image is inverted m = -(di/do) = (hi/ho) m: magnification di: distance of image do: distance of object hi: height of image ho: height of object |
|
thin lens equation
|
for any mirror or lens, distance of image is related to focal length and distance of object
(1/f) = (1/do) + (1/di) f: focal length do: distance of object di: distance of image applies to mirrors as well all measurements are given positive or negative values based upon their position relative to the mirror or lens |
|
1st rule of mirrors and lenses
|
draw an eye where observer will stand, and label side: positive, real and inverted (PRI)
"I (eye) am positive that real is inverted" images on side opposite the eye, are: negative, virtual and upright (NVU) |
|
2nd rule of mirrors and lenses
|
front of mirror is side that I (eye) am on
back of lens is side that I (eye) am on (stand behind camera to view object) objects are always positive when they are in front of a lens or mirror and always negative when they are behind a lens or mirror |
|
3rd rule of mirrors and lenses
|
if object is in front:
convex mirrors and diverging lenses make negative, virtual and upright images (NVU) concave mirrors and converging lenses make positive, real and inverted images (PRI), except when object is within the focal distance, in which case, they make a negative, virtual and upright image (NVU) |
|
concave mirror and converging lens
|
f is always positive
|
|
convex mirror and divergent lens
|
f is always negative
|
|
lateral magnification of a 2 lens system
|
product of lateral magnification of each lens
M = m1m2 |
|
Effective power of 2 lenses in contact with each other
|
equal to sum of their individual powers
Peff = P1 + P2 |
|
Electromagnetic radiation equations
|
c = f (wavelength)
c: speed of light f: frequency n = c/v n: refractive index c: speed of light in vacuum v: speed of light in medium E = hf E: energy of one photon h: planck's constant f: frequency n1sin01 = n2sin02 n: refractive index |
|
Mirrors and lenses equations
|
fmirror = (1/2)r
fmirror: focal length of mirror r: radius of curvature P = 1/f P: power f: focal length (1/f) = (1/di) + (1/do) f: focal length di: distance of image do: distance of object m = -(di/do) = hi/ho m: magnification di: distance of image do: distance of object hi: height of image ho: height of object |