Pith Number

pith:QCST7KMV

pith:2026:QCST7KMVR3T4VZNBOPH5SVW75H

not attested not anchored not stored refs resolved

Spectropolarimetric analysis of waves linked to FIP

M. Murabito, M. Stangalini

Stokes V amplitude asymmetries diagnose Alfvénic waves relevant to FIP bias.

arxiv:2605.13523 v1 · 2026-05-13 · astro-ph.SR

Open paper page JSON Open Graph Bundle Merged state Verified badge What is a Pith Number?

Add to your LaTeX paper

\usepackage{pith}
\pithnumber{QCST7KMVR3T4VZNBOPH5SVW75H}

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 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

The present work explores the diagnostic potential of Stokes V amplitude asymmetries as an alternative diagnostic tool for investigating wave behavior relevant to compositional fractionation processes.

C2weakest assumption

That observed Stokes V amplitude asymmetries are primarily caused by the same Alfvénic wave perturbations previously linked to FIP bias, rather than by other gradients or instrumental effects.

C3one line summary

Stokes V amplitude asymmetries are proposed as an alternative diagnostic for wave activity linked to FIP bias in the solar corona.

References

18 extracted · 18 resolved · 0 Pith anchors

[1] Widing, K. G. & Feldman, U. 1989 Abundance Variations in the Outer Solar Atmosphere Observed in SKYLAB Spectroheliograms.Astrophys. J.,344, 1046. (doi:10.1086/167871) 1989 · doi:10.1086/167871

[2] Sheeley, N. R. 1995 A Volcanic Origin for High-FIP Material in the Solar Atmosphere. Astrophys. J.,440, 884. (doi:10.1086/175326) 1995 · doi:10.1086/175326

[3] Sheeley, N. R. 1996 Elemental Abundance Variations in the Solar Atmosphere.Astrophys. J., 469, 423. (doi:10.1086/177792) 1996 · doi:10.1086/177792

[4] Laming, J. M. 2004 A Unified Picture of the First Ionization Potential and Inverse First Ionization Potential Effects.Astrophys. J.,614, 2, 1063. (doi:10.1086/423780) 2004 · doi:10.1086/423780

[5] 2015 The FIP and Inverse FIP Effects in Solar and Stellar Coronae.Living Reviews in Solar Physics12, 2 2015 · doi:10.1007/lrsp-2015-2

Receipt and verification

First computed	2026-05-18T02:44:24.345605Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

80a53fa9958ee7cae5a173cfd956dfe9c4a539508f3840f2c1e9cb0cdb0cdddd

Aliases

arxiv: 2605.13523 · arxiv_version: 2605.13523v1 · doi: 10.48550/arxiv.2605.13523 · pith_short_12: QCST7KMVR3T4 · pith_short_16: QCST7KMVR3T4VZNB · pith_short_8: QCST7KMV

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/QCST7KMVR3T4VZNBOPH5SVW75H \
  | 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: 80a53fa9958ee7cae5a173cfd956dfe9c4a539508f3840f2c1e9cb0cdb0cdddd

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "be71457fbc57767c64655761316d6061d6a1a4c43363d005af00b2270d391695",
    "cross_cats_sorted": [],
    "license": "http://creativecommons.org/licenses/by/4.0/",
    "primary_cat": "astro-ph.SR",
    "submitted_at": "2026-05-13T13:38:11Z",
    "title_canon_sha256": "ef07d3c9b1e0c448e8a1b59296619bef48f0ef925dece110fbcfea8831d3a589"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2605.13523",
    "kind": "arxiv",
    "version": 1
  }
}