Pith Number
pith:5KT2CJ3L
pith:2021:5KT2CJ3LO3ILLJ6R4OHCOGPIZJ
not attested
not anchored
not stored
refs pending
Can small-scale magnetic fields be the major cause for the near-surface effect of the solar p-mode frequencies?
arxiv:2106.03294 v1 · 2021-06-07 · astro-ph.SR
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{5KT2CJ3LO3ILLJ6R4OHCOGPIZJ}
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Record completeness
1
Bitcoin timestamp
2
Internet Archive
3
Author claim
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claim
4
Citations
5
Replications
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Portable graph bundle live · download bundle · merged
state
The bundle contains the canonical record plus signed events. A mirror can host it anywhere and recompute the same
current state with the deterministic merge algorithm.
Receipt and verification
| First computed | 2026-07-05T03:04:25.973227Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
eaa7a1276b76d0b5a7d1e38e2719e8ca7dc1cfdcea035cf3ef35bb0a2ded7ed0
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/5KT2CJ3LO3ILLJ6R4OHCOGPIZJ \
| 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: eaa7a1276b76d0b5a7d1e38e2719e8ca7dc1cfdcea035cf3ef35bb0a2ded7ed0
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "f958ad8b1ff3b64574e1a3aedc4bad83f3fe644d3cc3ca73fb4e75869e9502b8",
"cross_cats_sorted": [],
"license": "http://creativecommons.org/licenses/by/4.0/",
"primary_cat": "astro-ph.SR",
"submitted_at": "2021-06-07T01:49:07Z",
"title_canon_sha256": "1bcb8519d804750e5dbef140c95883319e06f1fe5673b196aaf798c48f10d696"
},
"schema_version": "1.0",
"source": {
"id": "2106.03294",
"kind": "arxiv",
"version": 1
}
}