Power of lenses in contact: P_eff = P1 + P2 + P3 + P4
All identical with power p: P_eff = 4p
Magnification of lenses in series: m_eff = m1 x m2 x m3 x m4
All identical with magnification m: m_eff = m x m x m x m = m^4
Answer: 4p and m^4
When lenses are in contact (touching): equivalent focal length 1/f = 1/f1 + 1/f2 + ... Equivalent power P = P1 + P2 + ... Powers simply add. For n identical lenses of power p each: P_total = np. Applications: camera lenses (multiple elements to correct aberrations), microscope objectives, eyepieces.
For a system of lenses in series (not in contact but in sequence): total magnification = product of individual magnifications. m_total = m1 x m2 x m3... This is because each lens takes the image of the previous as its object. For n identical lenses: m_total = m^n. Compare with power (sum) vs magnification (product).
Lens formula: 1/v - 1/u = 1/f. Magnification: m = v/u = (f)/(f+u) for thin lens. For convex lens: can give magnified, diminished, or equal image depending on object position. Inside focal length: virtual, erect, magnified (magnifying glass). At 2f: real, inverted, equal size. Between f and 2f: real, inverted, magnified. Beyond 2f: real, inverted, diminished.
Power P = 1/f (f in metres). Unit: dioptre (D). Converging lens: positive power. Diverging lens: negative power. Combination in contact: P = P1 + P2. Example: +3D and -1D lenses in contact give +2D = converging lens of focal length 50 cm. Spectacle lenses: prescription written in dioptres. Myopia: negative power (diverging). Hyperopia: positive power (converging).
Chromatic aberration: different wavelengths refract differently, different focal lengths. Corrected by achromatic doublet (convex + concave lens of different glass). Spherical aberration: rays from edge of lens focused at different point than rays through centre. Corrected by aspheric lenses or lens combinations. Cameras use multiple lens elements (6-20) to correct various aberrations. Telescope objectives: large aperture requires careful aberration correction.
Human eye: biconvex crystalline lens of variable power (accommodation). Power range: 40-44 D (approximately). Far point: point on which unaccommodated eye focuses. Normal: infinity. Near point (least distance of distinct vision): 25 cm for normal adult eye. Accommodation: ciliary muscles change lens curvature (power). Presbyopia: loss of accommodation with age (need reading glasses). Power of eye system: cornea contributes ~43D, lens ~20D (variable).
Simple microscope (magnifying glass): single convex lens. M = 1 + D/f (D = 25 cm). Compound microscope: objective (short f, high power) + eyepiece. Total M = (L/fo)(1+D/fe) where L = tube length. Telescope (astronomical): objective (long f, large aperture) + eyepiece (short f). Magnification M = fo/fe. For viewing: final image at infinity, M = fo/fe. Resolving power of telescope: R = D/1.22lambda (larger aperture = better resolution). Camera: inverted real image on film/sensor. f-number = f/D (aperture).
When light travels from denser to rarer medium at angle greater than critical angle: total internal reflection occurs. Critical angle C: sin C = 1/n (n = refractive index of denser medium). Applications: optical fibres (light trapped by TIR, information transmitted over long distances with minimal loss), diamonds (cut to maximize TIR, giving brilliance), mirage (hot air near ground acts as rarer medium), prism binoculars (two TIR prisms fold optical path).