IES STOP Optics Optimizer
Documentation: 🔭 STOP Optics User & Engineering Manual
📑 Table of Contents (12 User Guides) ▼
Platform User Guide

Structural, Thermal & Optical Performance (STOP) Engine

A step-by-step user guide for setting up optical parameters, defining mechanical boundary conditions, executing simulations, and exporting Zernike wavefront polynomials.

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1. Platform Capabilities & Analysis Scope

Web-Based Optomechanical Simulation & Multi-Objective Design Optimization

The STOP Optics Optimizer is an interactive web platform designed to evaluate and optimize circular and annular mirror assemblies. It couples thermo-elastic mechanical deformations directly to optical wavefront quality, allowing optical designers and mechanical engineers to iterate quickly without local software installations.

🔍 Dual-Surface Tracking

Simultaneously evaluates deformation across both the front clear aperture and the back mounting plane.

🌡️ Environmental Loads

Applies uniform temperature soak, axial gradients, radial gradients, and 3D gravity vectors.

⚖️ Wavefront Decompositions

Converts continuous surface deformation into standard or fringe Zernike coefficients ready for optical design software.

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2. Access Channels & Billing Verification

Self-Service Runs, Assisted Modes & Institutional PO Settlement

The platform provides two primary modes of access depending on your organization:

💳 Standard User Access

Self-service users can configure designs, preview run parameters, and proceed through integrated payment gateways (Razorpay for domestic UPI/NetBanking/Cards, or PayPal for international transactions). Invoices compliant with GST Rule 46 generate automatically upon completion.

🛡️ Institutional & Assisted Access

For academic, laboratory, and corporate clients with active Purchase Orders (PO), our technical support desk can provision access tokens or execute runs directly, linking orders to formal enterprise billing accounts.

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3. Optical Substrate Library & Custom Entry

Pre-Calibrated Material Presets and User-Defined Properties

Selecting a substrate defines the mechanical stiffness and thermal sensitivity of the mirror. Select a preset from the dropdown menu, or choose Custom Substrate to specify proprietary values:

Preset Name Modulus E (GPa) Poisson's Ratio ν CTE α (10⁻⁶ / K) Density ρ (kg/m³) Typical Application
Fused Silica 72.7 0.16 0.55 2200 UV/VIS laser systems, spectrometer optics
Zerodur® Glass-Ceramic 90.3 0.24 0.05 2530 Thermally stable ground and space telescope mirrors
ULE® Titanium Silicate 67.6 0.17 0.03 2210 Near-zero expansion cryogenic and satellite mirrors
Silicon Carbide (SiC) 410.0 0.14 2.40 3160 High-stiffness lightweight scanning mirrors
N-BK7 Optical Glass 82.0 0.206 7.10 2510 Standard laboratory flats, test windows
Cleartran® (ZnS Multispectral) 74.5 0.29 6.50 4090 Infrared FLIR windows and multispectral systems
Aluminum 6061-T6 68.9 0.33 23.60 2700 Diamond-turned all-aluminum athermal designs
Invar 36 148.0 0.29 1.20 8050 Athermal metering mounts and bezel rings
Titanium Ti-6Al-4V (Gr 5) 113.8 0.34 8.60 4430 Kinematic bipod flexures and mounting brackets
Configuring Custom Properties: When selecting Custom Substrate, ensure all four engineering parameters are provided in matching units: Modulus in GPa, Poisson's ratio as a dimensionless fraction, CTE in 10-6 / K, and density in kg/m3.
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4. Geometric Parameter Definitions

Aperture Sizing, Inner Hole Radius, and Thickness Specification

Input the primary physical dimensions in millimeters. The interface provides real-time validation to verify that dimensions remain within realistic manufacturing aspect ratios:

Outer Diameter (Do) [mm]:

The full mechanical diameter of the optic, including outer non-optical mounting margins and protective bevels.

Inner Hole Diameter (Di) [mm]:

Specify an inner cutout for Cassegrain, Ritchey-Chrétien, or beam-clearance configurations. Enter 0 for solid mirror disks.

Substrate Thickness (h) [mm]:

Uniform thickness of the blank. Increasing thickness reduces self-weight deflection while increasing overall mass.

Optical Clear Aperture (CA) [mm]:

The diameter over which the optical beam passes. Zernike decomposition and surface RMS figures are evaluated strictly inside this zone (CA ≤ Do).

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4.1 Mirror Structural Architecture: Solid Flat Optics vs. Lightweighted Honeycomb

The platform supports two distinct optomechanical paradigms configured via the Mirror Structural Architecture selector:

🔵 Option A: Solid Flat Optics (Continuous Annular Support)

Solid, un-machined mirror blank or optical transmission flat of uniform thickness h.

  • Stage 1 Support: Continuous circular annular cushion with mean radius amfg and radial band width ΔR.
  • Dual-Surface RMS Tracking: Both the front optical faceplate and the rear mounting face are polished continuous surfaces; optical surface figure RMS, PV, and Zernike modal expansions are computed for both surfaces.
  • Typical Applications: Optical flats, fold mirrors, laser windows, spectroscopy beamsplitters, test plates.
🔶 Option B: Lightweighted Honeycomb Mirror (Back Pockets & Joint Pads)

Lightweighted open-back mirror structure featuring pocket cavities, concentric rib rings, radial spokes, and outer rim designed for aerospace weight reduction.

  • Stage 1 Support: Supported on 3 small circular planar pads (radius rpad) positioned symmetrically at 120° rib-joint intersections (Triads T1, T2, etc.).
  • Stage 2 Operational: Retained by 3 glued perimeter blade patches at 120° around the outer rim.
  • Parametric CAD Output: Automatically generates production 3D STEP AP214 and native FreeCAD (.FCStd) models.
  • Typical Applications: Airborne telescopes, spaceborne optical instruments, scanning lidar payloads.
⚠️ Crucial Optical Figure Rule for Honeycomb Mirrors: Back-Surface RMS Omission

Why is back-surface RMS not calculated for Honeycomb Mirrors?
In lightweighted honeycomb mirrors, the rear face consists of deep pocket cavities separated by thin structural ribs. Optical wavefront metrics—such as Root-Mean-Square (RMS) surface figure error, Peak-to-Valley (PV) sag, and Zernike aberration coefficients—quantify optical phase errors across a continuous reflective surface. Because the back face is open and pocketed rather than an optical reflective boundary, calculating an optical surface figure for the back face is physically meaningless.

Therefore, when Option B: Lightweighted Honeycomb Mirror is selected, the platform designates the rear surface metrics as N/A (Pocketed Back Face). All optical wavefront evaluations, interferometric sag maps, and Zernike modal expansions are concentrated exclusively on the continuous front optical faceplate (z = −h/2).

Parameter Symbol Default Engineering Description & Role
Honeycomb Pocket Base Parameter n 3 (Min: 2, Max: 5) Centered regular hexagonal numbers N(n) = 1 + 3n(n−1) ∈ {1, 7, 19, 37, 61} pockets. Optimization engine decides final n within bounds [nmin, nmax].
Central Hub Radius rhub 0.0 mm (Min: 0.0, Max: 60.0) Central solid hub radius. Set to 0.0 mm for pure continuous hexagonal core without central hub. Math guaranteed never to fail (zero-safe).
Rib Wall Thickness wrib 3.5 mm Internal structural rib wall thickness separating adjacent hexagonal pockets. Cavity pocket arm: spocket = s − wrib/√3.
Pocket Floor Thickness tfloor 6.0 mm Uniform residual faceplate thickness forming the optical front reflective skin under all pocket cells.
Support Pad Annular Width ΔRpad 4.5 mm Annular radial wall width of the 3 hollow circular support pads. Inner blind hole radius is rhole = rpad − ΔRpad. No outer rim support is used during Stage 1.
Joint Support Pad Outer Radius rpad 12.0 mm Outer contact radius of the 3 hollow circular pads supporting the mirror during Stage 1 at 120° symmetric hexagonal rib joints. Contact area: Apad = π(rpad² − rhole²).
Imaginary Central Hub Pitch rhub 35.0 mm Purely imaginary reference guide circle passing through joint supports; does not cut away honeycomb core cells.
Symmetric Triad Selection Triad Auto (-1) Choice of canonical 120° symmetric joint vertex triplet on the hexagonal grid where the 3 planar pads are placed.
Tensile Safety Factor (σ₁) SFσ1 2.0 Factor of safety for Rankine maximum principal tensile stress criterion to prevent brittle glass fracture under Stage 1 pad reaction.
📐 Rankine Maximum Principal Tensile Stress Criterion (σ₁) for Brittle Optics

Unlike ductile metals (which yield according to von Mises shear strain energy), optical glasses and ceramics (Zerodur, Fused Silica, ULE, Silicon Carbide) are brittle materials that fail via micro-crack propagation under tensile stress. The platform automatically computes the peak tensile principal stress σ1 and evaluates the Rankine Margin of Safety:

MSσ1 = (σallowable / σ1, peak) − 1 ≥ 0,   where   σallowable = σtensile_limit / SFσ1

A positive Margin of Safety (MS ≥ 0) guarantees structural survivability under launch shocks, 1g assembly gravity, and thermal gradients.

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5. Stage 1 Inputs: Metrology & Fabrication Support

Annular Support Ring Sizing (Option A) vs. 3-Point Joint Support Pads (Option B)

Stage 1 models the optical substrate resting horizontally under 1.00g gravity during interferometric optical testing, polishing, or mount adhesive curing. The physical reaction boundary conditions automatically adapt based on your chosen Mirror Structural Architecture:

🔵 5.1 Option A: Solid Flat Optics — Continuous Annular Cushion Support Option A

For solid blanks, the rear face rests on a compliant elastomeric or knife-edge continuous circular annular band. This balances inner sag against outer cantilever overhang roll-off.

Figure 1A: Stage 1 Continuous Annular Support Ring Schematic
Figure 1A: Kinematic annular support showing mean ring radius amfg, contact band width ΔR, and optical clear aperture CA.
Support Ring Radius (amfg) [mm]:

Mean radial location of the annular ring. For minimum gravity sag on a solid disk, the optimal theoretical balance occurs near amfg ≈ 0.681 × R.

Support Ring Bandwidth (ΔR) [mm]:

Contact radial width of the annular cushion. Uniform reaction pressure is computed as qcontact = M·g / [2π amfg ΔR].

Dual-Surface RMS Tracking: Because both the front optical clear aperture and the back mounting plane are continuous surfaces, Stage 1 evaluates deflection profiles, Peak-to-Valley (PV) sag, and Zernike modal expansions for both surfaces.
🔶 5.2 Option B: Hexagonal Honeycomb Mirror — Stage 1 3-Point Symmetric Kinematic Joint Support Option B

For lightweighted mirrors with open-back pocket cavities, a continuous annular cushion cannot be used because it would span unsupported thin pocket floors, inducing severe localized bending ("oil-canning"). Instead, the mirror features a true regular hexagonal honeycomb rib architecture (derived from centered hexagonal numbers N(n) = 1 + 3n(n−1) for rings k = n−1). The mirror is supported kinematically on 3 green kinematic columns with hollow circular planar pads located strictly at 120° rotational symmetry directly beneath hexagonal rib-intersection joint vertices, extending up into 3 blind counterbore holes on the back face. No outer rim support is required during Stage 1.

Fig 1: Stage 1 Kinematic 3-Column Support Setup (Option B: Honeycomb)
Fig 1: Stage 1 Kinematic 3-Column Support Setup (Option B: Honeycomb) — (Left) Top Plan View: Continuous regular hexagonal honeycomb core, purely imaginary central hub guide circle (passes through joint supports without interrupting hex pockets), 3 hollow circular support pads (ΔRpad, rhole), and perimeter Blade Patch #0 at Top (90°); (Right) Front Sectional Elevation View: 3 green kinematic support columns extending UP into 3 blind counterbore holes in the substrate back face (depth dblind stopping safely above floor tfloor without penetrating the front optical face). Reaction pressure distributes across the 3 hollow circular areas: σpad = M·g / [3π(rpad² − rhole²)].
Figure 1B-1: Symmetrical Hexagonal Honeycomb Grid
Figure 1B-1: True Symmetrical Hexagonal Honeycomb back-face geometry (n=3, 19 regular hex pockets, stiffener ribs, and outer bounding circle).
Figure 1B-2: Honeycomb Sizing Progression (n=1 to 4)
Figure 1B-2: Honeycomb progression across Pocket Base Parameter n ∈ {1, 2, 3, 4} → N ∈ {1, 7, 19, 37} pockets with exact outer touching bounding circles.
Mathematical Hexagonal Honeycomb & Pad Reaction Formulas:
Total Hexagons: N(n) = 1 + 3n(n−1)
Hex Side / Arm: s = R / √N
Cavity Pocket Arm: spocket = max(0.1, s − wrib/√3)
Hole Radius: rhole = rpad − ΔRpad
Hollow Pad Area: Apad = π(rpad² − rhole²)
Pad Stress: σpad = M·g / (3 Apad)
Honeycomb Base Parameter (n):

Governs pocket order sequence (n=1..5 → 1, 7, 19, 37, 61 pockets). Configured with nominal value and bounds [nmin, nmax] so the multi-tier optimizer selects the best structural mass/sag trade-off.

Imaginary Hub Pitch (rhub) [mm]:

Purely imaginary reference guide circle passing through joint supports; does not cut away honeycomb core cells. Pockets remain continuous across the substrate.

Pad Outer Radius & ΔRpad [mm]:

Outer radius rpad and wall width ΔRpad defining hollow circular pads with blind hole radius rhole = rpad − ΔRpad. Reaction pressure distributes over the 3 hollow areas: σpad = M·g / [3π(rpad² − rhole²)].

Symmetric Triad Selection:

Choice of canonical 120° joint vertex triplet on the hexagonal grid where the 3 planar pads are placed. Auto (-1) selects the Airy-optimal minimum deflection node triad.

Rib Wall Thickness (wrib) [mm]:

Structural rib thickness providing bearing stiffness directly under the support pads and transferring transverse shear loads across pocket walls.

Uniform Pocket Floor (tfloor) [mm]:

Uniform faceplate thickness across all cells forming the polished front optical reflective boundary. Back blind holes stop safely above floor tfloor, keeping the front optical plane solid.

⚠️ Crucial Engineering Principle: Back Surface RMS is NOT Evaluated for Honeycomb Mirrors

Because the back face of a lightweighted honeycomb mirror contains open pocket cavities and thin rib walls, calculating an optical surface figure RMS, PV sag, or Zernike modal expansion on the back face is physically meaningless. The solver explicitly sets back surface optical metrics to N/A (Pocketed Back Face) and concentrates all wavefront optimization strictly on the continuous front optical faceplate (z = −h/2).

🔗 5.3 Assembly Sag Carry-Forward Coupling

The checkbox "Consider Stage 1 Deflection Carry Forward" is enabled by default. During mounting assembly, the mirror rests on its Stage 1 supports (the annular cushion for Option A or the 3 joint pads for Option B) under 1.00g gravity while the 3 Stage 2 perimeter blade patches cure and solidify with their positions fixed. When the temporary Stage 1 leveling supports are withdrawn post-cure, the manufacturing sag remains locked into the substrate. Carry-Forward couples this locked-in sag with all operational loads:

wnet(r, θ) = wstage1(r, θ) + wstage2(r, θ)
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6. Stage 2 Inputs: Operational Mount & Thermal Loads

Three-Point Rim Pads, Orientation Angles, and Thermal Gradients

Stage 2 models the optic installed inside its operational housing, kinematically retained by three mechanical mounting blades bonded to adhesive patches spaced at 120° around the outer cylindrical rim. The coordinate frame positions Blade Patch 0 at the Top (12 o'clock, θ = 90°), Blade Patch 1 at θ = 210° (lower-left), and Blade Patch 2 at θ = 330° (lower-right), with in-plane gravity pointing downward opposing elevation tilt:

Figure 2: Stage 2 Operational Kinematics & 3-Point Glued Rim Configuration
Figure 2: Operational assembly kinematics: (Left) Planar Mount with Blade Patch 0 at Top (90°) and downward in-plane gravity, (Center) Input-Time 3D Spatial Attitude & Kinematics Telemetry showing Elevation 60.0° [Zenith / Facing Up] with optical axis pointing upward and 1g downward gravity, and (Right) Cylindrical Rim Bond with axial offset zshift and notch stress concentration.
🪐 Stage 2: 3D Spatial Attitude & Gravity 60.0° [Zenith / Facing Up]
Elevation / Zenith: 60.0° [Facing Up]
Azimuth / Clocking: Az: 0.0° | Clk: 0.0°
Gravity Load: 1.00g (9.83 m/s²)
Patch Shift Offset: +1.00 mm (Kt=1.73)
3D attitude: Optical axis at 60.0° Elevation, 0.0° Azimuth, and 0.0° Clocking under 1.00g (9.83 m/s²) downward gravity.
Adhesive Axial Offset (zpatch = +1.00 mm):

The axial distance from the mirror neutral plane (z=0) to the bond center. For nominal blank thickness h = 25.0 mm and pad width w = 20.0 mm, offsets must stay within the physical rim boundary |zshift| ≤ (h − w)/2 = 2.50 mm. Eccentric shifts produce localized bending line moments (Mpad = Fr · zpatch) during temperature swings.

3D Gravity Pointing Angles (θel = 60.0°, β = 0.0°, γ = 0.0°):

Specify Elevation (θel = 60.0° [Zenith / Facing Up]) pointing upward into space, Azimuth (Az = 0.0°), and In-Plane Clocking Angle (γ = 0.0°) under standard 1.00g (9.83 m/s²) downward gravity.

Radial Pre-Mount Mount Forces (P0: +120N, P1: -80N, P2: +40N):

Kinematic mount blade patches positioned at 120° intervals: Blade Patch 0 at Top (90°) with +120 N inward pre-load, Patch 1 (210°) with -80 N outward tension, and Patch 2 (330°) with +40 N inward force.

Bond Fillet Radius (rfillet = 1.50 mm → Kt = 1.73):

Fillet radius of the adhesive junction used to calculate Peterson/Pilkey stress concentration factor (Kt = 1.73), verifying peak interfacial stress against allowable tensile and cleavage yield limits.

🧭 Optomechanical Coordinate & Deflection Sign Convention:

Transverse deflection w(r, θ) is defined positive downward along the optical axis, pointing from the front optical face (z = −h/2) toward the rear mounting surface (z = +h/2). Under downward gravity (1.00g) and rear reaction loads, sagging toward the rear cell produces positive displacement (w > 0). This directly quantifies physical gravitational sag and backing flexure without requiring inverted coordinate signs. When interfacing with optical design packages (Zemax OpticStudio / CODE V), exported wavefront grid sag files (.ZRN / .DAT) automatically format phase and sag to optical pupil standards.

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7. Selecting Optical Zernike Polynomial Conventions

ISO 24157 / Noll Standard vs ISO 14999-2 / Fringe 37

The platform provides two selectable Zernike representations to ensure direct compatibility with your downstream optical design or testing software:

Zernike Standard ISO 24157 / Noll

Orthonormal polynomial basis over the unit circle with explicit RMS scaling:

√(n + 1) for m = 0
√(2(n + 1)) for m ≠ 0

Configurable from 15 to 66 modes. Each coefficient directly indicates its contribution to the root-mean-square (RMS) wavefront error.

Zernike Fringe ISO 14999-2 / U. Arizona

Peak-to-edge normalized polynomials over the unit circle (Rnm(1) = 1.0):

Standard 37-term sequence
Wyant 48-term expansion

Directly maps to classical interferometry outputs (spherical, coma, astigmatism, trefoil) used in optical shop testing.

Wavefront Invariance: While coefficient numbers differ between Standard and Fringe representations, the calculated physical surface RMS across the clear aperture remains identical.
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8. Execution Workflow & Calculation Queue

Job Submission, Status Tracking, and Download Access

The platform processes simulations sequentially through an automated cloud execution queue. Here is how your job progresses from submission to deliverable retrieval:

1

Validation & Submission

Clicking Run STOP Analysis verifies geometric constraints (CA ≤ Do, Di < Do) and submits your configuration to the queue with a unique Order ID.

2

Cloud Computation

The solver calculates thermo-mechanical deflections, extracts front/rear surface sag, fits the selected Zernike polynomials, and renders 300 DPI contour plots.

3

Deliverable Package

Output files, including the summary report, high-resolution plots, CSV coefficient tables, and CAD grid sag files, are assembled into a downloadable ZIP archive.

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9. Deliverables Suite & Optical Software Integration

Summary Reports, High-Resolution Plots, and Grid Sag Export

Upon completion, download the complete package as STOP_Optics_Deliverable.zip containing:

📄 Engineering Summary PDF:

A multi-page documentation package with all input properties, boundary assumptions, resulting deformation tables, and an executive compliance summary.

📈 High-Resolution Visualizations:

Stage 1 and Stage 2 configuration diagrams, full 2D surface deflection contours, and Zernike modal spectrum bar charts.

📊 CSV Modal Coeffs & Grids:

Exported numeric tables of front and back Zernike coefficients, RMS contributions, and sampled surface displacement points.

🎯 Optical CAD Grid Sag (.ZRN):

Standard surface sag files formatted for immediate import into optical ray-tracing and design environments (e.g., Ansys Zemax OpticStudio, Synopsys CODE V).

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10. Invoicing, Institutional Procurement & Tax Compliance

GST Rule 46 Compliance, SAC 998145, and Purchase Order Integration

Tax invoices are issued in compliance with statutory Central Goods and Services Tax (GST) provisions:

  • Service Accounting Code: Designated under SAC 998145 ("Research and development originals in other fields n.e.c.").
  • Standard Referencing: Deliverables and invoices explicitly reference published international standards (ISO 24157, ISO 14999-2) for audit compliance.
  • Institutional Purchase Orders (PO): Organizations purchasing through procurement channels will have their designated PO reference numbers printed directly on the final invoice.
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11. Order Management & Technical Support

Tracking Jobs, Re-Running Iterations, and Technical Assistance

Users and organizations can manage and reference past runs via the user portal:

🔄 Re-Running Analyses Quickly reload saved parameters from previous runs to adjust geometry or thermal loads without re-entering all data.
✏️ Assisted Adjustments Our engineering support team can review parameter configurations and assist in troubleshooting convergence warnings.
💼 Billing & Invoices Access download links for historical invoices, GST documentation, and signed computation certificates.
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12. Frequently Asked Questions

Key Technical and Operational Questions for Engineers

Q1: When should I choose Zernike Standard vs Zernike Fringe?

Select Zernike Standard when your primary goal is evaluating root-mean-square (RMS) wavefront error budgets according to ISO 24157 or ANSI Z80.28. Select Zernike Fringe (37-term) when exporting to interferometer software (e.g., Zygo MetroPro) or standard optical modeling packages that default to the classic Fringe sequence.

Q2: How does the adhesive patch offset induce optical distortion?

Differential thermal expansion between the substrate and mount ring produces radial shear forces. If the bond center is shifted axially away from the neutral plane of the optic (zpatch ≠ 0), this shear force creates a localized bending moment (Mpad = Fr · zpatch) that curls the outer rim and distorts the wavefront.

Q3: Why should I keep Stage 1 Deflection Carry-Forward enabled?

During assembly, the finished optic rests on temporary supports—either a knife-edge leveling ring (annular ring amfg for Option A Solid Optics) or 3 kinematic circular column pads at 120° joint nodes (Option B Honeycomb Optics)—while structural adhesive is applied at three mechanical blade patches along the cylindrical rim. The adhesive slowly cures and solidifies under this assembly sag. Once fully cured and the temporary Stage 1 supports are removed, that initial gravitational sag remains permanently locked in place. Enabling Carry-Forward ensures this locked-in assembly sag is added to subsequent operational flight loads (thermal soak ΔT, 3D pointing tilt, and rim forces) via wnet = wstage1 + wstage2.

Q4: How do I define the 3D pointing angles?

Elevation angle θel defines inclination: 0° corresponds to horizontal pointing (where lateral gravity dominates) and 90° corresponds to zenith pointing (pure axial sag). Clocking angle β rotates the lateral gravity component around the optical axis relative to the first support pad.

Q5: Can I simulate Cassegrain primary mirrors with central holes?

Yes. Entering an Inner Hole Diameter (Di > 0) automatically switches the geometry to an annular configuration with traction-free inner boundary conditions.

Q6: How is the bond stress concentration factor utilized?

The transition between the flexible adhesive bond and the stiff mirror substrate experiences localized stress concentrations. The platform calculates stress factors based on your specified fillet radius (rfillet) to help ensure bondline safety under thermal extremes.

Q7: How do I import the .ZRN file into optical design software?

Place the exported .ZRN file into your optical software's grid sag directory (for example, the Objects/Grid Files directory in OpticStudio). Then set the optical surface type to Grid Sag or Zernike Fringe Sag and link the file directly.

Q8: Can educational and research institutions arrange institutional billing?

Yes. We support institutional Purchase Orders (PO) for universities, government laboratories, and defense contractors, providing invoicing under SAC 998145 upon job delivery.

Q9: How fast does the cloud solver complete a run?

Because the platform leverages optimized cloud solvers and pre-structured boundary templates, typical runs complete—including PDF compilation, contour rendering, and Zernike file generation—in under 10 seconds.

Q10: Are custom substrate materials saved for subsequent runs?

Yes. Custom substrate values entered during an active session remain cached in your session state and are saved alongside your Order ID for easy re-use.

Q11: Why is optical surface figure RMS not calculated for the back face of honeycomb mirrors?

Lightweighted honeycomb mirrors feature open-back pocket cavities and structural rib walls machined into the rear substrate to minimize payload mass while preserving flexural rigidity. Optical wavefront quality (RMS surface figure error, PV sag, and Zernike modal decompositions) characterizes optical phase distortion across a continuous reflective faceplate. Because the back face is open and pocketed rather than an optical boundary, computing an optical figure RMS on that face is physically meaningless. The platform marks the back surface as N/A (Pocketed Back Face) and rigorously concentrates all optical metrics on the continuous front optical faceplate.

Q12: How are the 3 planar support pads positioned in honeycomb mirrors?

Rather than resting on a continuous circular ring (as in solid optics), the honeycomb mirror is supported kinematically on 3 green support columns extending up into 3 blind counterbore holes machined on the back face of the substrate at 120° rotational symmetry beneath hexagonal rib-joint nodes. No outer rim support is used during Stage 1. The blind holes stop safely above the front faceplate floor (tfloor), keeping the polished optical front surface 100% continuous and unbroken. Each column terminates in a hollow circular planar pad of outer radius rpad and annular radial width ΔRpad (blind hole radius rhole = rpad − ΔRpad), distributing reaction pressure across the 3 hollow circular areas: σpad = M·g / [3π(rpad² − rhole²)].

Q13: Why does the platform evaluate Rankine maximum principal stress (σ₁) for honeycomb mirrors?

Standard von Mises stress is based on the distortional energy (octahedral shear) yield criterion, which applies to ductile metals (like aluminum or steel). Optical mirror materials (Zerodur, Fused Silica, ULE, Silicon Carbide) are brittle glasses and ceramics that do not yield plastically; instead, they fail catastrophically under tensile principal stress through Griffith micro-crack propagation. The platform computes the peak principal tensile stress σ1 and verifies that the Rankine Margin of Safety MSσ1 = (σallowable / σ1, peak) − 1 ≥ 0 against a user-configurable safety factor (default SF ≥ 2.0).