Pith Number
pith:BTYBZT5K
pith:2011:BTYBZT5KCDY2433LTF7YEDVWVR
not attested
not anchored
not stored
refs pending
MRI-driven Accretion on to Magnetized stars: Global 3D MHD Simulations of Magnetospheric and Boundary Layer Regimes
arxiv:1111.3068 v1 · 2011-11-13 · astro-ph.SR
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{BTYBZT5KCDY2433LTF7YEDVWVR}
Prints a linked badge after your title and injects PDF metadata. Compiles on arXiv. Learn more · Embed verified badge
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 | 2026-05-18T01:59:39.611001Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
0cf01ccfaa10f1ae6f6b997f820eb6ac774bf96edf66dfb535e617573886f443
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/BTYBZT5KCDY2433LTF7YEDVWVR \
| 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: 0cf01ccfaa10f1ae6f6b997f820eb6ac774bf96edf66dfb535e617573886f443
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "bc9b012392d90cef15d969bf01e01e72d83ac1ce2e1cc5942d4c6cd3db97b65c",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.SR",
"submitted_at": "2011-11-13T21:39:56Z",
"title_canon_sha256": "05a6cbe50c4e68ecc088e8f79040fc5465f99df2171c4d9a1a7befa1c4e0a907"
},
"schema_version": "1.0",
"source": {
"id": "1111.3068",
"kind": "arxiv",
"version": 1
}
}