1 Introduction
Large ultra-precision aspheric optical elements are highly demanded for the development of laser nuclear fusion devices [
1], large-aperture astronomical telescopes [
2,
3], high-resolution earth observation systems [
4,
5], and lithography machines [
5]. However, their diameter and accuracy restrict the performance of related equipment. For example, the primary mirrors of the Thirty Meter Telescope [
6] and the 42-m European Extremely Large Telescope (E-ELT) [
2] consist of 492 and 798 quasi-hexagonal mirror segments, respectively, with a diagonal length of 1.45 m. The National Ignition Facility [
1] in the USA and the Megajoule Laser [
7] in France require 7360 and 4200 large-aperture optical elements, respectively. The typical manufacturing process of aspheric optics comprises grinding [
8], polishing [
9,
10], and focused ion beam figuring [
11]. The material removal rates of the polishing and figuring processes are extremely low. Therefore, the form error and subsurface damage depth [
12] induced by the grinding process should be reduced to minimize the required material removal depth in the subsequent processes.
Hence, considerable technological advancements pertaining to ultra-precision grinding of large-aperture mirrors have been achieved. The Steward Laboratory at the University of Arizona developed the large optical generator to grind and polish 8 m mirrors [
13]. It was successfully used to machine the 6.5-m primary mirror of the Magellan telescope [
14] and 8.4-m primary mirrors of the Large Binocular Telescope [
14,
15]. The form error of these mirrors can be reduced to less than 10 μm RMS after grinding. Researchers at the Cranfield University developed a large ultra-precision grinding machine, OAGM2500 [
16‐
18], for the manufacturing of large mirrors used in telescopes. Its maximum machinable aperture and achievable relative form error are Φ2500 mm and 1/10
6 PV, respectively. Subsequently, another large ultra-precision grinding machine, Big OptiX [
17,
18], was developed to achieve high-efficiency and low-damage grinding of hard and brittle materials. By employing a novel
R-theta grinding mode with an inclined toroidal shape diamond wheel, a high material removal rate of 187.5 mm
3/s was achieved when grinding the 1.45-m Zerodur mirror [
18] used for the E-ELT telescope. The form error and subsurface damage depth were reduced to less than 1 μm RMS and 8 μm, respectively, within a manufacturing cycle of < 20 h. The ULTRASONIC100-5 machining center developed by DMG MORI Company Ltd. integrates ultrasonic vibration with traditional grinding to improve the machining efficiency of hard and brittle materials. Using this machine, the form error of a 700 mm × 700 mm SiC high-order off-axis aspheric mirror was efficiently reduced to 2.13 μm RMS [
19]. Other companies, such as Blohm, Satisloh, Schneider, and Optotech, provide large aspheric grinding machines with a machinable diameter of Φ500‒2000 mm.
China has conducted comprehensive studies pertaining to the ultra-precision grinding of large-aperture optics in recent years. For example, researchers at Tsinghua University developed a six-axis, large-scale precision grinding machine. Grinding tests of a Ф770 mm K9 glass show that the form error was less than 10 μm, and the surface roughness can reach the submicron level. The AOCMT ultra-precision grinding machine [
20] developed by the National University of Defense Technology can machine optical elements up to a diameter of 650 mm. It has been successfully used to grind a Ф116 mm parabolic SiC workpiece to a form error of 8.9 μm. The Changchun Institute of Optics and Fine Mechanics developed a series of four-axis aspheric machine tools, namely, the 800-mm FSGJ-1 [
21], 1.2-m FSGJ-2 [
22], and 2-m FSGJ-3. These machines integrated the functions of rough grinding, fine grinding, polishing, and online measurement. Using the computer-controlled optical surfacing technique, a form precision of 12 nm RMS for a 1-m mirrors was achieved. In recent years, Jiang et al. at Xi’an Jiaotong University developed two ultra-precision aspheric grinding machines with maximum machinable diameters of Ф900 mm [
23,
24] and Ф1500 mm [
25,
26]. The achievable form error for a 400-mm mirror was smaller than 5 μm PV using the arc envelope grinding method.
The studies above indicate that it is challenging to efficiently achieve an extremely high form accuracy by grinding, e.g., 5 μm/m PV, for large aspheric optics. During the grinding of such optics, the tool setting error is one of the main error sources of the workpiece form error. For a specified geometry of the machined surface, the grinding path is determined by the geometry of the grinding wheel and the spatial locations of the wheel and workpiece. Therefore, the tool position in the X-, Y-, and Z-directions must be adjusted during the grinding process. The tool setting in the X- and Y-directions ensures the lowest point of the grinding wheel coincides with the axis of the turntable. The tool setting in the Z-direction determines the height of the grinding wheel relative to the workpiece.
The outer cylindrical surface and upper plane of the workpiece can be used as reference surfaces during the rough setting of the wheel. When the wheel is set in the X-direction, it approaches the outer cylindrical surface from both the positive and negative directions of the X-axis. The X-coordinates of the machine tool in the contact state are recorded as x1 and x2. The middle point between x1 and x2, i.e., x0 = (x1 + x2)/2, is the zero point of the workpiece in the X-direction. However, the accuracy of the wheel setting method mentioned above is limited by the form error of the cylindrical surface. In addition, the contact state between the wheel and workpiece is difficult to be determined accurately. Therefore, other methods should be developed by clarifying the evolution of the workpiece form error with the wheel setting errors.
The tool setting problem has been intensively investigated [
27,
28] to improve machining precision. Typical contact-type tool setting methods include on-machine touch probes [
28] and force sensors [
29,
30], whereas examples of non-contact methods include acoustic emission sensors [
31], digital microscopes [
32], and digital holography [
33]. However, studies pertaining to wheel setting for the grinding of aspheric optics are rare. Chen et al. [
34] discovered that inward and outward offsets generated V-shaped and Λ-shaped profiles, respectively. However, the relationship between wheel setting error and workpiece form error has not been analytically modeled. Kang et al. [
35] modeled and analyzed the form error of aspheric surfaces subjected to grinding with a cup wheel. The key error sources were discovered to be the tool setting error and radius error of the grinding wheel. Nevertheless, elaborate numerical computations were required to obtain the form error. Wei et al. [
26] and Xi et al. [
24] developed analytical tool setting error models that encompassed both the radial and lateral directions. However, these models did not account for the variation in the grinding point during arc envelope grinding; as such, the prediction accuracy was limited, especially for steep aspheric surfaces.
To overcome these challenges, the relationship between the form error of aspheric optics and the setting error of an arc grinding wheel was modeled analytically and numerically by considering the variation in the grinding point on the wheel. A grinding example is presented herein to verify the form error model and a newly proposed compensation method.