pith:CHC6NJFF
Solar active region scaling laws revisited
Solar active regions obey scaling relations linking area, pole separation and tilt to magnetic flux and latitude.
arxiv:2602.13677 v2 · 2026-02-14 · astro-ph.SR
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Claims
For the area A, pole separation d and tilt angle γ we find scalings against magnetic flux Φ and heliographic latitude λ. Residuals from these relations are also modelled. These scaling relations are recommended for use in space climate research for the modelling of future data or missing past data, as well as for the identification of candidate rogue ARs.
The ARISE active region database provides a complete and unbiased sample of bipolar active regions across cycles 23, 24, and 25, with accurate measurements of area, pole separation, tilt, flux, and latitude.
Empirical scaling relations for solar active region area, pole separation, and tilt with flux and latitude are derived from ARISE data for cycles 23-25 and recommended for space climate modeling.
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| First computed | 2026-06-19T16:10:35.332375Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
11c5e6a4a5cef71984bbe26c0b39d7bfaa823e6cff2c21bbcb240cca894d5c31
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/CHC6NJFFZ33RTBF34JWAWOOXX6 \
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Canonical record JSON
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