pith:Z2QOKHDB
$1/f$ Noise in Synthetic and Solar Wind Data: Superposition Principles
Superposition of independent signals with distributed correlation times produces the 1/f spectrum observed in solar wind magnetic fields.
arxiv:2601.20121 v2 · 2026-01-27 · physics.space-ph
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Claims
Using synthetic time series with scale-invariant or lognormal distributions of correlation times, we examine the efficacy of several superposition approaches in generating a 1/f regime. The persistence of 1/f spectrum is further illustrated with decade-long in situ magnetic field measurements from the ACE spacecraft.
That the component signals are statistically independent and that their correlation times are drawn from scale-invariant or lognormal distributions that remain stationary over the full observation interval.
Superposition of signals with distributed correlation times generates 1/f spectral density in both synthetic time series and decade-long ACE spacecraft solar wind data.
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| First computed | 2026-05-18T03:10:11.266844Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
cea0e51c6136b36e488939bdf251c13d499c419d13e6ffaf39adb14a0e856f4c
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/Z2QOKHDBG2ZW4SEJHG67EUOBHV \
| jq -c '.canonical_record' \
| python3 -c "import sys,json,hashlib; b=json.dumps(json.loads(sys.stdin.read()), sort_keys=True, separators=(',',':'), ensure_ascii=False).encode(); print(hashlib.sha256(b).hexdigest())"
# expect: cea0e51c6136b36e488939bdf251c13d499c419d13e6ffaf39adb14a0e856f4c
Canonical record JSON
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