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concave f = zR SI^ unit^ :^ o^ convex^ f^ =^ -'zR
⑦ E S Mirror (^) Eq : do di =!
=> : I -^ m ( + ) : upright ; m( = ) : invert
angleof angle^
of (^) m
=dil. real^
,^ inut^ , red^ reai^ ,^ inut^ , en virt^ , upr ,^ enl.^ virt^ , (^) upr ,^ red^ di^ do^ (^ +^ ) :^ real^ ,^ in^ front^ of^ mirror reflection ~
do > f ; di > o : real , inverted do f ; di o di s dildo (t) : Virtual , behind mirror
Refraction of (^) Light : Sin-1_ (^) sin Index of Refraction (^) : n = C Vi (^) W 27 Snell's Law : nisin-1 = 12 sin-2 ·^ There is no 2 =^900
change in^ direction^ Z^ Z^ Z^ Z
air^ I
..^ I 1 C^ I 1
1 =^ C I ... a
-^ if^ there^ is^ no^ change in^ n "^1 ~ diamond · (^) The
greater the change in^ n. small^ of^ incident^ large of^ incident of^ incident is^ large enough larger incident
ninz (^) (speed v) bends toward normal the (^) greater the (^) change in (^) light enter a smaller n (n1 <^ n2) > bend > of refraction is 900 > Total internal reflection air
- propagation direction^. (^) away from normal^ Sin^ -c^ =^ n2^ ni -^ water · (^) If (^) ray change medium (^) along the n,nz (^) (speed 1) bends (^) away normal normall ) undeflected (^) (regarless n) Converging (Conrex) Lenses f O^ Diverging (Concave) Lense f^70
&^ P M · - > always
Laser beam^ will^ also^ bend^ so^ aim^ directly at^ the^ image G^ -^
I
· MV -virtu
Index of refraction : higher ifa in frequency v =^ cn real (^) , inut (^) , (^) larger virt (^) , upr , (^) larger SMI.
=> spread out in a rainbow color : dispersion do] f^ ; di < 0 do If ; di (^) largeror (^) (blue) bends towards normal *^ for^ lenses : image behind lense :^ di so - real
The (^) eye produces a real (^) , inverted (^) image on the retina = the brain (^) adjusts the (^) image to (^) appear (^) properly Ciliary muscles^ adj^ the^ shape^ of^ the^ lense^ accommodate^ near^ +^ far^ vision^ ,^ iris^ control^ #^ of^ light^ enter viewing a^ distant^ object^ Viewing a^ near^ object
distant => 0
obj relaxed^ ciliary obj^ tensed^ ciliary +^ Near^ pt :^ closest pt to^ the^ eye lens^ is^ able^ to^ focus^ (v25cm) ↑ focal (^) length
↑ (^) refractive (^) power - Far (^) pt : farthest (^) pt &which the (^) eye can focus (^) (C)
focallength-
aperture iris^ contracts^ ,^ up
Refractive (^) power : Strength of corrective lense = If^ ; SI = (^) diopter = m - Nearsighted :^ need^ far^ vision^ correction^ =)^ refractive^ power^ too^ high :^ -^ extra^ lens^ wh^ (-)^ ref^. power concave lens
stun
clear :
image formed^ in^ front^ :
& far far
Dt of^ the^ retina^ Dt
- correction : (^) image an (^) object ata^ to the (^) farpt : do =^0 , di =^ -FP (^) , ref (^) power : If^ =^ FP or f =^ -FP Farsighted :^ needs^ near^ vision^ correction^ =>^ refractive^ power too^ low^ :^ -^ extra^ lens^ w/^ (^ +^ )^ ref^. power convex lens
image formed^ behind 1 ·^ -^ ..
near O.
of the retina Dt
- correction^ : (^) image an^ object at^ normal^ near^ pt :^ do^ =^0. 25m^ ,^ di^ =^ -NP^ , ref^ power :^ 'f^ = "^0. 25 -'^ NP Magnifying glass :^ simple convex^ lens^ ,^ similar^ to^ corrective^ Telescopes^ :^ using lenses^ called^ refractors^ Compound Microscope :^2 converging lense^ ,^ I^ eyepiece
-^ no^ ·^ tobi^ teye lens (^) for (^) farsightedness do (close to (^) eye) , objective close to (^) object · , s
+ If the object move closer to the?
eye ,^ its^ angular size^ s^5 - hi-^ -^ >^ object^ placed^ nearf^ of^ objective^ lense^ :
no B
- if (^) placed at NP : - = (^) N objective eyepiece^ mobjective (^) =
- N image formed by didective
Angular magnification :^ M^ =^ -^ or^ M=^ eyepiece^ ato
> image formed atf on eyepiece image at & :
- The (^) magnification can be (^) maximized (^) by having the Total (^) magnification : the (^) product of^ m of each lens N image at^ the^ near^ pt :^ M^ total^ = "f objective^ Meyepiece^ = feyepiece
f eyepiece
relaxed (^) eye : M =^ Nf^ (image & D) > Total (^) magnification = Mtotal = Mobj Meye or M = 1 +^ N^ + N
(image @NP)^ L^ =^ fobj^ +^ feye^ =decive
eyepiece =+^ objectieyepiece
Frequency :^ f^ =^1 T^ ,^ Units^ =^ S' or^ Hz^ If^ enters^ a^ transparent material^ which^ light travels^ slower^ :^ at^ speed v^ =^ cn^ rea^ : longest I Phase (^) velocity : v =^ & T = If Vacumm (^) n = Index (^) n L i ↓ but (^) frequency stays same N vac X = Rac n superposition of^ waves^ :^ &index^ of^ ref.
I in^
- Interference^ is^ only noticeable^ if^ the^ light sources^ are^ monochromatic^ (all^ light has^ same^ 1) a^ coherent > t^ (different^ sources^ maintain^ the^ same^ phase^ relationship over^ space t^ time). · in i i^ ~ (^) interference will be constructive (2 wares (^) are in (^) phase) , destructive (^) (out of (^) phase)
~ ~^12 -^11 =^ ma^ :^ constructive^ int
Wh Wit 12-11 =^ (m-1z X : destructive int.^3 with m =^10 , 11 , 2
speed of^ sound^ =^343 m/s
frequency :^ &
a . In phase 6. Half wavelength c. Full wavelength
out of phase out^ of^ phase
(const) (destr^ C Considered^ "in^ phase" Δx =^ x^ =^0 =^3608
-x =^ xz =^1800 Bright fringes Dark fringes
Constructive Destructive ~ m-order of^ fringe from the^ centerline 2nd (^) : m =^ + (^2) Y Young's Two-Slit^ Experiment max^ (const^ .)^ (1^ =^ 2x)^ 2nd (1^ :^ =m (^) 32x)^ =^ +^2 E^ & -^ >^ to^ find^ o^ use^ tan L
- -^ min^ (destr^.^ )^ Y^ Ist : m = + 1 (1 = X 2) (1 = (^) x) 1st : m = + &distance^ bt^ slit^ &^ screen -T ~ & > Central m = (^) O ↑
sin 0 =^ -^ by
2 &^
d = L^ (1^ =^ 0)^ m^ =^ -^ then^ use^ sing^ =^ my^ to^ find^ I
m = - (1^ =^ -^ x2) thdifferent sin (^) & (1 = - x) x)
wld : distance bt the slits.
- m = - (^2) Bright (Constructive)^ :^ Using^ =^ ma^ m^ =^0.^ l^ , 12...^ (1^ =^ -^ 2x)^ nmax^ =^ d^ ~^ round^ down X Dark :^ d^ =^ sing^ =^ m- , x m^ =^11 ,^12 , 13 a =^1
of line (^) m
Diffraction (^) : When a (^) wave encounters an obstacle (^) opening , it (^) changes direction (^). Dark (^) fringes : Using = ma m =^11 , 12 , 13
- The (^) angle which (^) one find the (^) Ist min (^) : sin (^) Op = x a d : spacing of 2 slits
- Central (^) bright spot Can be narrowed (^) by (^) having a smaller W : width of (^) single slit > widening the slit. D : (^) diameter of (^) circula (^) apenture
- (^) To find (^) bright fringes > (^) aug 2 of (^) dark Resolution : (^) Ability to (^) distinguish closely spaced objects. Diffraction limits resolution Location of 1st dark (^) fringe determines the size of the central (^) spot : Sino = (^1). 22 x D > Rayleigh's criterion : if & (^) objects are (^) separate by less than the minimum & (^) , they cannot be (^) distinguised o > (^1). 22xD
- (^) To ↑ (^) separation : ↑X ↓ D (^) immerse in water ↓ 1! (^) Cred)
- (^) To see finer details (better (^) separation > (^) ↑reso) : (^) use shorter 1. & (blue) Unit : Im : 1x103mm : 1 x (^100) um : 1 x^ 10-anm