Pith Number
pith:ZJWWV4WK
pith:2002:ZJWWV4WKQKU6CRY2WB3BDLOF5N
not attested
not anchored
not stored
refs pending
Are Coronae of Magnetically Active Stars Heated by Flares? II. EUV and X-Ray Flare Statistics and the Differential Emission Measure Distribution
arxiv:astro-ph/0209075 v2 · 2002-09-04 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{ZJWWV4WKQKU6CRY2WB3BDLOF5N}
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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 | 2026-07-04T16:30:44.052643Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
ca6d6af2ca82a9e1471ab07611adc5eb5b1d4ea10a10099137b2ca2f4b5ae636
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/ZJWWV4WKQKU6CRY2WB3BDLOF5N \
| 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: ca6d6af2ca82a9e1471ab07611adc5eb5b1d4ea10a10099137b2ca2f4b5ae636
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "f376dfb387862de045c8866db94c51533771963af8c084a47d0e1967e162ddae",
"cross_cats_sorted": [],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "2002-09-04T18:43:00Z",
"title_canon_sha256": "153c6d5c80b7d40fe9ce16c00b0c33b35838fe951140ba92c2777ee4ed8d8b03"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/0209075",
"kind": "arxiv",
"version": 2
}
}