Multiscale Variability of Solar Irradiance at Earth: Reference amplitudes from minutes to gigayears
Giulio Ruffini
Solar irradiance at Earth varies over thirteen decades of period, but the published amplitudes are not additive. They are normalized to different denominators; several of the listed periods are amplitude envelopes of other terms rather than independent oscillators; and the choice between peak-to-peak and semi-amplitude is often left unstated, an ambiguity of two in amplitude and four in variance. Summed naively, correctly quoted numbers can inflate an energy budget by an order of magnitude.
We tabulate representative periods and amplitudes from minutes to gigayears under three conventions. All amplitudes are peak-to-peak over a stated parameter range. Every local insolation entry names the diagnostic it summarizes, since 65^ N summer insolation is not a number until the summer window is fixed. Every percentage is normalized to the present-day value of its own diagnostic. Orbital and local entries are computed from the stated elements rather than quoted; the implementation reproduces the four insolation values of Huybers (2006) and recovers an eccentricity, , that the source leaves implicit. At 65^ N the fractional obliquity and precession amplitudes hold to across summer windows spanning {108}{178}{days}, while the corresponding absolute amplitudes drift by and ; the fraction is therefore the quotable quantity and the absolute value is not.
For display across thirteen decades we use the variance density per logarithmic period, , rather than a power spectral density. It weights equal decades equally, and it exposes envelope double counting, since a term carrying no independent variance contributes no area.
The forcing so defined is the one required by WP0202, which studies algorithmic regulation on a Daisyworld and records the absence of a forcing that is stochastic and partially predictable at once. Solar forcing separates physically into a deterministic orbital component, computable to the {50}{Myr} Solar-System chaos horizon, and a broadband stochastic magnetic component.
Solar irradiance data from across the literature can't be added together without first fixing a bookkeeping problem that inflates energy budgets by an order of magnitude.
The core issue is that published irradiance amplitudes look like they're measuring the same thing but aren't. A 0.1% solar-cycle variation is a fraction of total solar irradiance at Earth's mean distance. A 13% precessional variation is a fraction of a local seasonal insolation diagnostic at 65°N. These have different denominators and can't be summed. On top of that, some listed "periods" — like the 405,000-year eccentricity cycle — aren't independent oscillators at all; they modulate the amplitude of shorter cycles whose variance is already counted. Adding them as separate sinusoids double-counts the same energy. And many tables don't say whether they're quoting peak-to-peak amplitude or semi-amplitude, an ambiguity of 2× in amplitude and 4× in variance.
This paper fixes the bookkeeping. It builds a reference table spanning minutes to gigayears under explicit conventions: all amplitudes are peak-to-peak, every local insolation entry names the exact diagnostic it summarizes (because "65°N summer insolation" is undefined until you specify what counts as summer), and every percentage is normalized to the present-day value of its own diagnostic. The orbital and local entries are computed from first principles rather than copied from other tables, and the implementation is validated against Huybers (2006) — reproducing four specific insolation values and recovering an eccentricity value (~0.05) that the original source left implicit. A sensitivity sweep shows that fractional amplitudes (obliquity ~5.7%, precession ~13.8%) are stable to 3% across a wide range of summer-window definitions, while the corresponding absolute values in W/m² drift by up to 22%. The fraction is the transferable quantity; the absolute value is not.
For displaying variance across thirteen decades of period, the paper uses variance density per logarithmic period, D(P) = f·S(f), rather than a conventional power spectral density. This weights each decade equally so that area on the plot corresponds to actual variance — and it makes envelope double-counting visible, since a term with no independent variance contributes no area.
The practical payoff connects to WP0202, which studies planetary regulation on a Daisyworld and needs a forcing that is simultaneously stochastic and partially predictable. Solar forcing has exactly that structure for physical reasons: the orbital component (eccentricity, obliquity, precession) is deterministic and computable up to the ~50 Myr Solar System chaos horizon, while the magnetic component (sunspot cycles, grand minima/maxima) is broadband and stochastically driven. This paper supplies the clean forcing specification that WP0202 requires, with the energy budget correctly normalized so the regulation studies don't inherit inflated numbers.
- WP ID
- WP0205
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- completed
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- open
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- drive_legacy
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- WP0205
- 0.1.0 (draft) · auto-run-placeholder
