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Optics for Engineers Chapter 9 Charles A. DiMarzio Northeastern University Mar. 2014 Gaussian Beams • Applications – Many Laser Beams – Minimum–Uncertainty – Simple Equations – Good Approximation – Extensible (e.g. Hermite– Gaussian) • Equations – Solution of Helmholz Equation – Solution to Laser Cavity – Kogelnik and Li, 1966 – Spherical Gaussian Waves – “Gaussians Are Forever” Mar. 2014 • Imaginary Part of Field – Gaussian Profile – Spherical Wavefront • Focusing and Propagation – Simple Equations – Relation to ABCD Matrix c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–1 Derivation (1) • Spherical Wave and Paraxial Approximation √ √ √ 2 +y 2 +z 2 x jk Psphere e Psphere jkz jk x2+y2 2z √ Esphere = ≈ e e 4π 4πz x2 + y 2 + z 2 • Radius of Curvature = z: Substitute Complex q √ √ √ 2 +y 2 +q 2 jk x Psphere e Psphere 1 jkq jk x2+y2 2q √ e e E= ≈ 4π 4π q x2 + y 2 + q 2 • Separate Real and Imaginary Parts of q in Exponents √ E≈ Mar. 2014 Psphere 1 jkq jk(x2+y2)< 1 −k(x2+y 2)= 1 2q e 2q e e 4π q c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–2 Derivation (2) • Curvature and Gaussian Profile jk e ( x2+y 2 ) 1 < 2q = x2 +y 2 jk 2ρ e −k e ( x2+y 2 ) 1 = 2q =e 2 2 −k x +y 0 2b • Definitions q = z + jb z 2 + b2 ρ= z Mar. 2014 1 1 j = − 0 q ρ b z 2 + b2 0 b = b c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–3 Gaussian Beam Parameters • Gouy Phase • Beam Radius, w w2 = 2b0 b0 = k ( e −k x2+y ) 2 1 = 2q = πw2 λ = πd2 4λ 2 2 − x +y e w2 • Curvature (Prev. Pg.) ( e jk x2 +y ) 2 1 < 2q = 2 +y 2 jk x 2ρ e z 1 1 1 −j arctan b = =√ e q z + jb z 2 + b2 z λ 1 − arctan b = e−jψ e = √ b πw2 • Linear Phase ejkq = ejk(z+jb) = ejkz e−kb • Normalized Complete Equation √ E≈ Mar. 2014 2 +y 2 x2 +y 2 − 2ρ e w2 2P − arctan z jkz jk x be e e 2 πw c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–4 Physical Meaning of Parameters √ E≈ 2P jkz jk x2 +y2 − x2 +y2 2 −jψ e e 2ρ e w e 2 πw • Radius of Curvature, ρ Dashed Black Line 1 1 =< ρ q • Distance from Waist, z z = <q • Rayleigh Range, b → d0 b = =q Mar. 2014 b= πw02 λ = πd20 4λ • Beam Diameter, d Black Diamonds 1 1 = −= b0 q πw2 πd2 b = = λ 4λ 0 c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–5 Gouy Phase • Phase Term z ψ = arctan b • See White Circle • Plot is =E Mar. 2014 c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–6 The Really Useful Equations • Beam Diameter, d √ z2 1+ 2 b b2 ρ=z+ z 5 5 4.5 4 4 3 ρ/b, Scaled Radius of Curvature d/d0, Scaled Beam Diameter d = d0 • Radius of Curvature, ρ 3.5 3 2.5 2 1.5 1 0.5 0 −5 1 0 −1 −2 −3 −4 0 z/b, Scaled Axial Distance • Near Field dg ≈ d0 • Far Field dd ≈ π4 dλ z 0 Mar. 2014 2 5 −5 −5 0 z/b, Scaled Axial Distance • Near Field ρ ≈ b2/z → ∞ • Far Field ρ ≈ z → ∞ c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–7 5 Six Questions • Four Parameters for q – z, Distance from Waist – b or d0, Waist Diameter – ρ, Radius of Curvature – b0 or d Local Diameter (at z) • Two Independent Numbers for Complex q • Pick Any Pair • Solve for the Rest • Practical Problems for Each Pair Mar. 2014 z ρ z ρ z b and and and and and and b known b0 b0 b ρ b0 c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–8 Question 1: Known z and b • Sample Application: Starting with a collimated (plane–wave) Gaussian, what are d and ρ at distance, z? • Example: Green Laser Pointer: λ = 532nm. • Solution πd2 0 = 5.91m b= 4λ ρ=z+ b2 z √ z2 d = d0 1 + 2 b ( z = 3m: z = 30m: z = 376, 000km: Mar. 2014 ρ = 14.6m ρ = 31.2m ρ = 376, 000km d = 2.2mm d = 10.4mm d = 127km 4λz π d0 ) (1mm) (10.2mm) (127km) c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–9 Question 2: Known ρ and b0 • Sample Application: What is the waist location for a focused beam? • Example: Laser Radar, λ = 10.59µm, d = 30cm, b0 = 6.6km • Solution ρ = −f 1 1 j = − 0 q ρ b z = <q = − Mar. 2014 f ( 1 j 1 = − 0 q ρ b b0 = πd2/ (4λ) ) 4λf 2 1 + πd2 1 ρ j b0 q= 1 + 1 1 1 + + 2 02 2 ρ b ρ b02 b = =q = b0 b0 + 1 f2 d2 0= c C. DiMarzio (Based on Optics for Engineers, CRC Press) d2 ( πd2 )2 1 + 4λf slides9r1–10 Question 2 Results 4 30 3.5 d0, Waist Diameter, cm −z, Distance to Waist, km 35 3 2.5 2 1.5 25 20 15 10 1 5 0.5 0 0 5 10 15 20 25 30 35 0 0 40 f, Focal Length, km A. Waist Location 5 10 15 20 f, Focal Length, km 25 30 35 B. Waist Diameter 50 45 4 10 35 30 I0/P, m−2 d, Beam Diameter, cm 40 25 20 15 2 10 0 10 10 5 −2 0 0 0.5 1 1.5 z, Distance, km 2 2.5 C. Beam Diameter (f = 1km) Mar. 2014 10 −2 10 −1 10 10 0 10 1 z, Distance, km Axial Irradiance c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–11 Question 2 Summary • Maximum Distance to Waist: (−z)max = b/2 at f = b • Two Ways to Make a Waist at any (−z) < b/2 • Near Field of d0; Strong Focusing: – (−z) ≈ −ρ = f – d0 = π4 λd • Depth of Focus: Quadratic in f 8f 2λ 1 zc = 2b1 = ( )2 2 4λf πd +1 πd2 • Collimated Beam as f → ∞ Mar. 2014 c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–12 Geometric and Diffraction Diameters • Geometric Optics • Diameter at Any Distance 2 + d d2 = d2 g d • Simple Calculation • Intuitive • Valid for Gaussians Mar. 2014 |z − f | dg = d f • Diffraction Limit 4λ dd = z πd • Fraunhofer Zone 4λ d0 ≈ dd = z πd c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–13 Question 3: Known z and b0 • Sample Application: What lens to make a waist at −z for Negative z? How big is the waist? • Example: Endoscope: λ = 1.06µm, waist at −z = 1mm with d never > 100µm • Solution: b0 = πd2/(4λ) b2 + z 2 0 b = Solve for b only if b b= b0 ± √ b02 − 4z 2 2 (z < b0/2) b2 ρ=z+ z • Typically 2 Solutions Mar. 2014 c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–14 Endoscope Focusing • Fixed Diameter at Source d = 100µm, z = 1mm πd2 0 b = = 7.4mm 4λ b= b0 ± √ b02 − 4z 2 2 z = −1mm b = 3.7047mm ± 3.5672mm • Options b = 137µm d0 = 13.6µm or b = 7.27mm d0 = 99µm • Probably Choose the First – High Irradiance – Small Depth of Field Mar. 2014 c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–15 Question 4: Known ρ and b • Sample Application: How long must the laser be to get a given d0 with a mirror of curvature ρ? • Example: Later • Solution: Solve for z if d0 Small Enough z 2 + b2 ρ= z z= ρ± √ (2b < ρ) ρ2 − 4b2 2 √ z2 d = d0 1 + 2 b Mar. 2014 c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–16 Question 5: Known z and ρ • Sample Application: How large is the beam from a laser cavity? • Example: Later • Solution: Solve for b z 2 + b2 ρ= z √ √ b= ρz − z 2 b=z √ d0 = Mar. 2014 (ρ > z) ρ −1 z or q = z + jb √ 4λb π z2 d = d0 1 + 2 b c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–17 Question 6: Known b and b0 • Sample Application: How do we launch a beam of diameter, d, into a fiber with diameter, d0? • Example: Beam diameter, d = 15µm and desired diameter, d0 = 5µm • Solution: Solve for z z 2 + b2 0 b = (b0 > b of course: d > d0) b √ z=± Mar. 2014 bb0 − b2 b2 ρ=z+ z c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–18 Fiber Launch • Equations √ z=± bb0 − b2 b2 ρ=z+ z • Inputs for d = 15µm and d0 = 5µm πd2 0 = 13µm b= 4λ πd2 0 b = = 118µm 4λ • Results √ z=− bb0 − b2 = −37µm b2 = −41.7µm ρ=z+ z • Lens: f = −ρ = 41.7µm, with Dlens > 15µm, (<f/3) • Distance: −z = 37µm (A Little Shorter than f ) Mar. 2014 c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–19 Gaussian Beam Characteristics • The complex radius of curvature can be manipulated to solve problems of Gaussian beam propagation. • The complex radius of curvature and its inverse contain four terms, which are related in such a way that only two of them are independent. • Given two parameters it is possible to characterize the Gaussian beam completely. Six examples have been discussed. • Solutions are at worst quadratic, producing zero, one, or two solutions. • Other, more complicated problems can also be posed and solved using this formulation. Mar. 2014 c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–20 Gaussian Beam Propagation • Propagation through Free Space (q = z + jb) q (z 2 ) = q (z 1 ) + z 2 − z 1 • Propagation through a Lens ( 1q = 1ρ − bj0 ) 1 1 1 + 0= s s f 1 1 1 − = 0 q q f Mar. 2014 1 1 1 + = 0 ρ −ρ f or 1 1 1 = − 0 ρ ρ f 1 1 −P = 0 q q c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–21 Matrix Optics Again • General qout = Aqin + B Cqin + D • Translation q + z12 q2 = 1 = q1 + z12 0+1 • Lens q0 = q+0 − nP0 q + nn0 1 n P = − 0 0 0 q qn n – In Air 1 1 1 1 − P = − = 0 q q q f Mar. 2014 c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–22 Refraction at a Surface • General q0 = q+0 n−n0 q + n n0 R n0 n − n0 n 1 = + q0 n0R qn0 • Planar Surface n0 0 q =q n • Rayleigh Range in a Medium πd2 0 b= 4λ/n Mar. 2014 c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–23 Propagation Example with a Lens: F to F 0 • Waist at Front Focal Plane, F q0 = jb0 πd2 0 b0 = 4λ • Three Steps q 1 = q 0 + f1 1 1 1 = − q10 q1 f 1 q2 = q10 + f1 • Result: <z2 = 0 (Waist) q1 = jb0 + f1 4λ d2 = f1 π d0 Mar. 2014 f12 0 q1 = −f1 + j b0 jf12 q2 = b0 (Fourier Transform) c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–24 Propagation Example Continued: A Second Lens (f3) • Relay Telescope d4 = 4λ f f3 = 3 d0 π d2 f1 • Matrix Optics: First Lens ( M02 = T12L1T01 = 1 0 f1 1 )( 1 − f1 1 0 1 )( 1 0 0+f f2 Aq0 + B = 1 q2 = =− Cq0 + q0 q0 − f q0 + 0 f1 1 ) ( = 0 − f1 1 4λ d2 = f1 π d0 • Both Lenses (f3 = f1): Inverting 1:1 Telecentric System ( M04 = M24M02 = 0 − f1 3 f3 0 )( 0 − f1 1 f1 0 ) f1 0 ) ( = −1 0 0 −1 ) −q0 + 0 Aq0 + B = = q0 q4 = Cq0 + D 0−1 Mar. 2014 c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–25 Two 1:1 Relays • Telecentric (Previous Page) M04 = M24M02 = ( 0 − f1 3 f3 0 ( )( 0 − f1 −1 0 1 0 −1 f1 0 ) • Afocal q4 = q0 = jb0 – Plane Wave – No Field Curvature – ρ→∞ Mar. 2014 • Single Lens (4–f Configuration) ) Mac = TbcLbTab = = ( 1 0 2f 1 )( ( 1 −1 f −1 −1 f qc = 0 1 0 −1 )( 1 0 2f 1 ) Aqa + B = Cqa + D −1qa + 0 1 = 1+ 1 −1 q − 1 a f f qa – ρ=f c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–26 ) = Summary of Gaussian Beam Propagation • Once two parameters of a Gaussian beam are known, then it’s propagation can be analyzed using simple equations for translation, refraction, and focusing. • Translation changes the beam size and curvature. It is represented by adding the distance to q. • Refraction through a lens changes the curvature, but keeps the beam diameter constant. It is represented by subtracting the optical power of the lens from the inverse of q. • Refraction through a dielectric interface changes the curvature and scale factor of q. • These equations can be generalized using the ABCD matrices developed for geometric optics. Mar. 2014 c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–27 The Collins Chart Confocal Parameter Lines of Constant z (vertical) and Constant b (horizontal) Curves of Constant b0 (circles) and Constant ρ (semicircles) Now Mostly a Visualization Aid 2 1.5 1 0.5 0 −2 −0.5 0 0.5 1 1.5 2 z, Axial Distance • Focusing (Along Circles) • Translation (Horizontal) • ρ Changes, d & b0 Don’t • z Changes, b Doesn’t Mar. 2014 −1.5 −1 c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–28 5 5 4 4 Confocal Parameter Confocal Parameter Two 1:1 Relays on Collins Chart 3 2 1 0 −3 3 2 1 −2 −1 0 1 z, Axial Distance A. Afocal Telescope Mar. 2014 2 3 0 −3 −2 −1 0 1 z, Axial Distance 2 3 B. Single Lens c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–29 Minimum Beam Diameter for Distance z12 Confocal Parameter 2 1.5 1 0.5 0 −1.5 Mar. 2014 −1 −0.5 0 0.5 z, Axial Distance 1 c C. DiMarzio (Based on Optics for Engineers, CRC Press) 1.5 slides9r1–30 Waist at −z for diameter, d 1 0.5 0 −1.5 −1 −0.5 0 0.5 1 2 2 1.5 1.5 Confocal Parameter 1.5 Confocal Parameter b, Confocal Parameter 2 1 0.5 0 −1.5 1.5 z, Axial Distance B. No Solution |z| > b0/2 −1 −0.5 0 0.5 z, Axial Distance 1 C. One Solution |z| = b0/2 1.5 1 0.5 0 −1.5 −1 −0.5 0 0.5 z, Axial Distance 1 D. Two Solutions |z| < b0/2 • Question 3 b2 + z 2 0 b = Solve for b only if b b= Mar. 2014 b0 ± √ b02 − 4z 2 2 (z < b0/2) b2 ρ=z+ z c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–31 1.5 Stable Laser Cavity Design A. Flat Output Coupler B. Flat Rear Mirror C. Confocal Resonator Mar. 2014 c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–32 Steady State in Laser Cavity • The amplitude after a round trip is unchanged. This means that any loss (including power released as output) must be offset by corresponding gain. (Gain Saturation) • The phase after a round trip must be unchanged. We discussed, in our study of interference, how this requirement on the axial phase change, ejkz , affects the laser frequency. • The beam shape must be unchanged, so that the phase and amplitude is the same for all x and y. This is the subject to be considered in this section. Mar. 2014 c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–33 Design Problem • Carbon Dioxide Laser: P(20), λ = 10.59µm • Beam Output: Collimated, 5mm Diameter • Cavity Length: 1m (Probably because of Gain) • Solution – Collimated Output: Flat Output Coupler – Rear Mirror to Match Curvature at z = −1m b = 1.85m ρ = −4.44m d = 5.7mm – Rear Mirror Concave, ρ = −4.44m – Diameter Larger than d = 5.7mm (Typically 1.5X) Mar. 2014 c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–34 Stable Cavity Examples Output toward Bottom Mar. 2014 A. Flat Output Coupler B. Flat Rear Mirror C. Confocal Resonator D. Focusing Cavity c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–35 Laser Cavity on the Collins Chart Given ρ1 ρ2 and z12 b, Confocal Parameter 3 2.5 2 1.5 1 0.5 0 −2 −1.5 −1 −0.5 0 0.5 1 1.5 2 z, Axial Distance Mar. 2014 c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–36 More Complicated Cavities • Ring Laser with Focusing Lens • Intracavity Lens (Potential Loss) • Many Other Configurations Mar. 2014 c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–37 Matrix Optics for Stable Cavities • Round–Trip Equation qout = qin • Need to Solve This: Aq + B q= Cq + D Cq 2 + (D − A)q − B = 0 • Result (Need Imaginary Solutions) q= A−D± √ (A − D)2 + 4CB 2C (A − D)2 + 4CB < 0 Mar. 2014 c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–38 Stability Condition • Argument of Square Root Must be Negative (A − D)2 + 4CB < 0 • Determinant Condition (n = n0 on Round Trip) AD − CB = 1 • Result (D − A)2 + 4DA < 4 Mar. 2014 (D + A)2 < 4 c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–39 Summary of Stable Cavity Design • Stable cavities or stable optical resonators have mirrors and possibly other optical elements that cause a Gaussian beam to replicate itself upon one round trip. • Resonator design can be accomplished using Gaussian beam propagation equations. • Most cavities will support only one Gaussian beam, and the beam parameters are determined by the curvature of the mirrors and their spacing along with the behavior of any intervening optics. • Matrix optics can be used to determine the round–trip matrix, which can be used to find the Gaussian beam parameters. • The Collins chart can help to evaluate the stability of a laser cavity. Mar. 2014 c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–40 Hermite–Gaussian Modes • Mode Definitions (Solutions of Helmholz Equation) hmn (x, y, z ) = hm (x, z ) hn (y, z ) • One–Dimensional Functions with Hermite Polynomials, H hm (x, z ) = ( )1/4 √ 2 π • Hermite Polynomials ( ) 2 x2 jkx 1 x w2 e 2ρ ejψm H e m 2mm!w w H1 (x) = 1 H2 (x) = 2x Hm+1 (x) = 2xHm (x) − 2 (m − 1) Hm−1 (x) • Gouy Phase for Hermite–Gaussian Modes ( ) 1 z ψm = + m arctan 2 b Mar. 2014 c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–41 Some Hermite–Gaussian Modes 0:0 (0:1) + i (1:0) = Donut 0:1 1:0 Mar. 2014 1:1 1:3 2:0 2:1 2:3 5:0 5:1 5:3 c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–42 Expansion in Hermite–Gaussian Modes • Expand Field in Hermite–Gaussian Modes • Ortho–Normal Basis Set E (x, y, z ) = ∞ ∑ ∞ ∑ Cmnhmn (x, y, z ) m=0 n=0 • May Take a Lot of Terms (but choose w wisely) • Power in Each Mode (and Phase) ∗ Pmn = CmnCmn Mar. 2014 φ = 6 Cmn c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–43 Finding the Coefficients, C for Given E(x, y, z) ∫ ∫ ∞ −∞ ∫ −∞ ∫ ∞ ∞ E (x, y, z) h∗m0 n0 (x, y, z) dx dy = ∞ ∗ E (x, y, z) h (x, y, z) dx dy = −∞ −∞ ∫ ∞ −∞ ∫ ∫ ∞ ∫ −∞ ∞ ∑ ∞ ∑ m=0 n=0 ∞ −∞ ∞ ∑ ∞ ∑ −∞ m=0 n=0 ∫ Cmn ∞ −∞ hmn (x, y, z) h∗m0 n0 (x, y, z) dx dy = δm,m0 δn,n0 ∫ Cm0n0 = Mar. 2014 ∞ ∫ −∞ ∞ ∫ Cmn hmn (x, y, z) h∗m0 n0 (x, y, z) dx dy ∞ −∞ hmn (x, y, z) h∗m0 n0 (x, y, z) dx dy Ortho–Normality E (x, y, z ) h∗m0n0 (x, y, z ) dx dy. c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–44 Picking the Best Waist Size • H–G Expansion Works for Any w • But it Might Not Converge Nicely • Pick the Best w to Maximize Power in T EM00 Term C00 = min [C00 (w)] ∫ C00 (w) = Mar. 2014 ∫ −∞ ∞ E (x, y, z ) h∗00 (x, y, z ) dx dy c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–45 −3 x 10 6 −5 4 0 2 5 −5 0 0 5 C00, Coefficient Expanding Uniform Circular Wave in H–G Modes 0.26 0 0.25 −10 10 −20 0.24 −30 15 0.23 1 −40 1.5 2 2.5 w, Gaussian radius B. A. 5 20 5 10 15 20 −50 C. 7 6 5 0 4 3 2 1 5 −5 0 D. Mar. 2014 5 0 −20 −40 −60 −5 0 5 x, Radial Distance E. Irradiance, dB x 10 8 −5 Irradiance, dB −3 0 −20 −40 −60 −10 0 10 x, Radial Distance F. c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–46 Coupling Equations and Mode Losses for Finite Apertures • Integration over Finite Aperture ∫ ∫ Kmnm0n0 = hmn (x, y, z ) h∗m0n0 (x, y, z ) dx dy = δm,m0 δn,n0 aperture 0 C00 K0000 0 C01 = K0100 0 C10 K1000 ... Mar. 2014 ... K0001 K0101 K1001 ... K0010 K0110 K1010 ... ... C00 C01 ... . . . C10 ... ... c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–47 Transverse Mode Beating: Mode Frequencies • Round Trip (Additional Phase Shift beyond Chapter 7) ( z1 z2 − arctan 2k` + 2 (1 + m + n) arctan b b ) = 2πN ( f (m, n, N ) 1 z z 2 ` + (1 + m + n) arctan 2 − arctan 1 c π b b ) =N arctan zb2 − arctan zb1 c c − f (m, n, N ) = N (1 + m + n) 2` 2` π Mar. 2014 c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–48 Transverse Mode Beating: Mode Control • Transverse Mode Beat Frequency z z c arctan b2 − arctan b1 f (1, n, N ) − f (0, n, N ) = 2` π • Carbon Dioxide Laser b = 1.85m, z = 1m ( 1m − arctan 0m arctan 1.85m 1.85m c 2m π • Solution: Include Appropriate Aperture – Suppress Higher Order Transverse Modes – K0000gρ1ρ2 > 1 – Kmnmngρ1ρ2 < 1 for m 6= 0, n 6= 0 f (1, n, N )−f (0, n, N ) = Mar. 2014 c C. DiMarzio (Based on Optics for Engineers, CRC Press) ) = 24MHz slides9r1–49 Summary of H–G Modes • Hermite–Gaussian modes (Equation ) form an orthogonal basis set of functions which can be used to describe arbitrary beams. • The beam can be expanded in a series. • Coefficients of the expansion can be calculated. • Each mode maintains its own profile with a size w and radius of curvature, ρ given by the usual Gaussian–beam equations. • The choice of w in Equation is arbitrary, but a value chosen badly can lead to poor convergence of the series expansion. • Higher order modes have increased Gouy phase shifts as shown in Equation . • Beam propagation problems can be solved by manipulating the coefficients with appropriate Gouy phase shifts. • Apertures can be treated using coupling coefficients which can be computed. • Higher–order transverse modes in a laser can mix with each other to produce unwanted mixing, or beat, signals. • The higher–order modes can be eliminated by placing an appropriate aperture inside the laser cavity. Mar. 2014 c C. DiMarzio (Based on Optics for Engineers, CRC Press) slides9r1–50