Reducing optical aberrations with graded-index optics
View Patent ↗An aberration corrector and a method to reducing a spherical aberration are disclosed. The aberration corrector has a radial, rotationally symmetric variation of refractive index including a term varying in proportion to a fourth degree of a distance from the optical axis. Since the spherical aberration causes a wavefront deviation proportional to the fourth degree of distance from the optical axis, the spherical aberration can be reduced by the aberration corrector when its thickness causes the exact amount of the phase delay corresponding to the wavefront deviation, but with an opposite sign.
1. An optical apparatus comprising:
a first element having optical power when an optical beam propagates therethrough, for collimating the optical beam to produce a collimated optical beam having a wavefront, the first element comprising an absorbing or gain medium comprising a lens thermally induced therein by the optical beam, wherein the wavefront has a spherical aberration introduced by the first element upon collimating the optical beam; and
an aberration corrector optically coupled to the first element for receiving the collimated optical beam, the aberration corrector having an optical axis disposed generally along the collimated optical beam, and a refractive index n varying with a distance r from the optical axis, as defined by a formula
n ( r )= n 0 +a·r 2 +b·r 4 ;
wherein n 0 is a constant, a·r 2 is a radially varying second-degree refractive index component, and b·r 4 is a radially varying fourth-degree refractive index component for lessening the spherical aberration of the collimated optical beam;
wherein a magnitude of a is less than 10 −2 mm −2 at a wavelength of 1 micrometer, and a magnitude of b has a pre-defined magnitude of at least 10 −6 mm −4 at the wavelength of 1 micrometer.
2. The optical apparatus of claim 1 , wherein the magnitude of a is less than 2·10 −4 mm −2 at the wavelength of 1 micrometer.
3. The optical apparatus of claim 2 , wherein the aberration corrector has a flat optical face for receiving or outputting the collimated optical beam.
4. The optical apparatus of claim 1 , wherein a thickness of the aberration corrector is no greater than 3 mm, the apparatus further comprising a glass rod affixed to the aberration corrector, for holding the aberration corrector in a polishing station for polishing a flat optical face of the aberration corrector.
5. The optical apparatus of claim 1 , wherein the first element comprises a spherical lens.
6. The optical apparatus of claim 1 , wherein the aberration corrector has a thickness of substantially integer multiple of a half-pitch length defined by the parameter a.
7. An optical apparatus comprising:
a first element having optical power when an optical beam propagates therethrough, for collimating the optical beam to produce a collimated beam having a wavefront, wherein the wavefront has a spherical aberration introduced by the first element upon collimating the optical beam; and
an aberration corrector optically coupled to the first element for receiving the collimated optical beam, the aberration corrector having an optical axis disposed generally along the collimated optical beam, and a refractive index n varying with a distance r from the optical axis, as defined by a formula
n ( r )= n 0 +a·r 2 +b·r 4 ;
wherein n 0 is a constant, a·r 2 is a radially varying second-degree refractive index component, and b·r 4 is a radially varying fourth-degree refractive index component for lessening the spherical aberration of the collimated optical beam, wherein the aberration corrector includes a gradient-index rod having a diameter of no greater than 20 mm, wherein |b|≧10 −6 mm −4 and |a|<10 −2 mm −2 at a wavelength of 1 micrometer.
8. An optical apparatus comprising:
a first element having optical power when an optical beam propagates therethrough, for collimating the optical beam to produce a collimated beam having a wavefront, wherein the wavefront has a spherical aberration introduced by the first element upon collimating the optical beam; and
an aberration corrector optically coupled to the first element for receiving the collimated optical beam, the aberration corrector having an optical axis disposed generally along the collimated optical beam, and a refractive index n varying with a distance r from the optical axis, as defined by a formula
n ( r )= n 0 +a·r 2 +b·r 4 ;
wherein n 0 is a constant, a·r 2 is a radially varying second-degree refractive index component, and b·r 4 is a radially varying fourth-degree refractive index component for lessening the spherical aberration of the collimated optical beam, wherein the aberration corrector includes a gradient-index optical fiber having a diameter of no greater than 0.5 mm, wherein |b|≧10 −6 mm −4 and |a|<2·10 −4 mm −2 at a wavelength of 1 micrometer.
9. The optical apparatus of claim 8 , wherein the aberration corrector has a thickness along the optical axis, the thickness not exceeding 3 mm, the apparatus further comprising a thickness of coreless optical fiber fused to the gradient-index optical fiber.
10. A method for lessening a spherical aberration of a collimated optical beam propagating through an absorbing or gain medium comprising a lens thermally induced therein by the optical beam, the method comprising
(a) providing an aberration corrector having an optical axis and a refractive index n varying with a distance r from the optical axis, as defined by a formula
n ( r )= n 0 +a·r 2 +b·r 4 ;
wherein n 0 is a constant, a·r 2 is a radially varying second-degree refractive index component, and b·r 4 is a radially varying fourth-degree refractive index component for lessening the spherical aberration of the collimated optical beam, wherein a magnitude of a is less than 10 −2 mm −2 at a wavelength of 1 micrometer, and wherein b has a pre-defined magnitude of at least 10 −6 mm −4 at the wavelength of 1 micrometer; and
(b) disposing the aberration corrector of step (a) in an optical path of the collimated optical beam, so that the optical axis is disposed generally along the optical beam.
11. The method of claim 10 , wherein the aberration corrector is selected from the group consisting of a gradient-index rod and a gradient-index fiber, the method further comprising
(c) upon completing step (b), measuring a first parameter characteristic of the spherical aberration;
(d) upon completing step (c), affixing the aberration corrector in a holder of a polishing station, and polishing off a length of the aberration corrector along the optical axis thereof;
(e) re-measuring the first parameter by repeating steps (b) and (c); and
(f) repeating steps (d) and (e) to further lessen the spherical aberration.
12. The method of claim 11 , wherein step (a) includes fusing the aberration corrector to a glass rod, and wherein step (d) includes affixing the glass rod in the holder of the polishing station.
13. The method of claim 11 , wherein step (c) includes
(i) focusing the collimated beam using an optical element having a focusing power, so as to obtain a focal spot; and
(ii) measuring a diameter of the focal spot of step (i),
wherein in step (c), the first parameter is the diameter of the focal spot.
14. A method of tuning a laser by lessening a spherical aberration according to the method of claim 11 , the laser having therein the thermally induced lens generating the spherical aberration of a laser beam of the laser, wherein the collimated optical beam comprises the laser beam,
the method including lessening the spherical aberration of the laser beam by performing steps (a) through (f), wherein in step (c), measuring the first parameter comprises measuring an M 2 value of the laser beam.