Pith Number

pith:Q4D326G5

pith:2026:Q4D326G5WADUVAMQGYZQJDYVBJ

not attested not anchored not stored refs resolved

Energy Evolution from the Chromosphere to the Heliosphere in the 2021 October 28 Solar Eruption

Andryi Koval, Bin Chen, Christopher S. Moore, Chunming Zhu, Cynthia Cattell, Dana W. Longcope, Daniel B. Seaton, Daniel Pacheco, Domenico Trotta, Durgesh Tripathi, Federico Fraschetti, Joe Giacalone, Katharine K. Reeves, Liam David, Matthew J. West, Phillip Hess, Sijie Yu, Sophie Musset, Soumya Roy, Surajit Mondal, Tatiana Niembro, Xudong Sun, Yeimy J. Rivera

In the 2021 October 28 solar eruption the total released energy matches pre-event stored magnetic energy, with CME kinetic plus potential energy dominating the partition.

arxiv:2605.16111 v1 · 2026-05-15 · astro-ph.SR

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\usepackage{pith}
\pithnumber{Q4D326G5WADUVAMQGYZQJDYVBJ}

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Record completeness

1 Bitcoin timestamp

2 Internet Archive

3 Author claim open · sign in to claim

4 Citations open

5 Replications open

✓ 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.

Claims

C1strongest claim

We find that the total energy released during the event is consistent with estimates of the pre-event stored magnetic energy, and the CME kinetic + potential energy dominates the energy partition.

C2weakest assumption

Scaling laws derived from previous observations accurately convert remote-sensing and in-situ measurements into energy values for non-thermal particles, EUV wave dissipation, and CME energy flux in this specific event (abstract paragraph on methods).

C3one line summary

Multi-spacecraft analysis of the 2021 October 28 solar eruption shows total released energy consistent with pre-event magnetic energy, with CME kinetic plus potential energy dominating the partition.

References

111 extracted · 111 resolved · 0 Pith anchors

[1] K., & Sturrock, P 1978

[2] Atwood, W. B., Abdo, A. A., Ackermann, M., et al. 2009, ApJ, 697, 1071 2009

[3] Aschwanden, M. J. 2004, in ESA Special Publication, Vol. 575, SOHO 15 Coronal Heating, ed. R. W. Walsh, J. Ireland, D. Danesy, & B. Fleck, 97 2004

[4] J., & Alexander, D 2001

[5] J., Caspi, A., Cohen, C 2017

Formal links

2 machine-checked theorem links

Receipt and verification

First computed	2026-05-20T00:01:53.341891Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

8707bd78ddb0074a81903633048f150a5be2ba5dd488d14c4c15c0e4fa23bae2

Aliases

arxiv: 2605.16111 · arxiv_version: 2605.16111v1 · doi: 10.48550/arxiv.2605.16111 · pith_short_12: Q4D326G5WADU · pith_short_16: Q4D326G5WADUVAMQ · pith_short_8: Q4D326G5

Agent API

Resolver JSON Graph JSON Events JSON Schema Signing key

Verify this Pith Number yourself

curl -sH 'Accept: application/ld+json' https://pith.science/pith/Q4D326G5WADUVAMQGYZQJDYVBJ \
  | 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: 8707bd78ddb0074a81903633048f150a5be2ba5dd488d14c4c15c0e4fa23bae2

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "a7ee344efe2326850503f495874f3d5d370447b887795e514ab539ca2d8c7cf2",
    "cross_cats_sorted": [],
    "license": "http://creativecommons.org/licenses/by/4.0/",
    "primary_cat": "astro-ph.SR",
    "submitted_at": "2026-05-15T15:57:26Z",
    "title_canon_sha256": "86ac0e7b553c09d31ededf873a065db6c87fcf3b1dd9c6343f3c29012754cca1"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2605.16111",
    "kind": "arxiv",
    "version": 1
  }
}