Test a wavelength calibration with an unused spectral reference
A spectrum maps detector coordinates to wavelength before physical line interpretation. Reflection, refraction or diffraction can disperse different wavelengths to different positions, but a pixel number is not itself a wavelength. Calibration needs identified reference features and a specified model of the coordinate relation.
Learning outcome: Reconstruct slope and intercept, then evaluate the unused reference before trusting the target result. Change the common pixel offset and explain why the check residual persists; propose a discriminating additional reference.
Starting recap
Keep photon energy/count, density convention, propagation, collection/resolution, calibration and source-quality assumptions distinct.
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Try
At offset o=10, anchors are pixels 110 and 410 and the fitted relation is λ=x+290 nm. A target at x=300 gives 590 nm conditionally. The unused check at x=265 predicts 555 rather than its known 550 nm, retaining a +5 nm validation residual.
Open the experimentPredict
Can a perfect fit to two calibration anchors establish that every other wavelength is correctly calibrated?
Experiment
Reconstruct slope and intercept, then evaluate the unused reference before trusting the target result. Change the common pixel offset and explain why the check residual persists; propose a discriminating additional reference.
Fit a wavelength scale and challenge it with an unused line
Worked teaching model · synthetic values · Original calibration anchors:400 nm at pixel100+offset,700 nm at400+offset. Linear scale fitted from these two only. An independent550 nm check appears at255+offset, five pixels away from the fitted prediction. Target interpolation is conditional; validation residual challenges global linearity.
Reset keeps your prediction, captures and practice history.
Two anchors determine a line, but an unused reference tests whether that line is adequate.
The persistent check residual can reflect a mistaken line identification, centroid error or nonlinearity. It must not be erased by calling the interpolation calibrated beyond its evidence. This original pixel record does not replace the actual SDSS wavelength column.
| Quantity | Value | Unit |
|---|---|---|
| Fitted dispersion | 1 | nm/pixel |
| Fitted wavelength intercept | 290 | nm |
| Conditional target wavelength | 590 | nm |
| Unused check-line fitted wavelength | 555 | nm |
| Check-line known wavelength | 550 | nm |
| Validation residual fitted minus known | 5 | nm |
Actual SDSS records are explicitly labeled; all other packets are original models. No direct solar viewing, radiation experiment or instrument operation is requested.
Two anchors determine a line, but an unused reference tests whether that line is adequate.
The persistent check residual can reflect a mistaken line identification, centroid error or nonlinearity. It must not be erased by calling the interpolation calibrated beyond its evidence. This original pixel record does not replace the actual SDSS wavelength column.
Captures preserve recipes and replay their calculated results. They are synthetic model evidence, not physical measurements.
Understand
Apply
Public practice checks a specific claim. It does not establish independent mastery.
Use offset 20 and target pixel 200. Find the fitted target wavelength and unused-reference residual.
Continue
Completion requires a saved prediction, at least one capture and a reflection. Presence checks do not grade your reasoning.
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