{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:EZBVIJ2PZMQHWCKTSMJKSNK76C","short_pith_number":"pith:EZBVIJ2P","schema_version":"1.0","canonical_sha256":"264354274fcb207b09539312a9355ff09e8d2bff7115366fb71972007ed3c95c","source":{"kind":"arxiv","id":"1211.7112","version":1},"attestation_state":"computed","paper":{"title":"Stochastic Particle Acceleration by Helical Turbulence in Solar Flares","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Gregory D. Fleishman, Igor N. Toptygin","submitted_at":"2012-11-29T22:43:20Z","abstract_excerpt":"Flaring release of magnetic energy in solar corona is only possible if the magnetic field deviates from a potential one. We show that the linear MHD modes excited on top of the non-potential magnetic field possess a nonzero kinetic helicity. Accordingly, this necessarily results in a noticeable kinetic helicity of the turbulence, composed of these linear modes with various scales and random phases, generated at the flare site by the primary energy release, which may be important for many applications. In particular, a nonzero turbulence helicity has a potentially strong effect on the particle "},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1211.7112","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2012-11-29T22:43:20Z","cross_cats_sorted":[],"title_canon_sha256":"62ce60f95f559df6b27cf8d6106cd16a09ba9db2c7b05408108f040152858b66","abstract_canon_sha256":"1a5eecf56e15ff771878260a0b4de16470ab88a79f894246729dc7d34da46560"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:52:53.051411Z","signature_b64":"OeRodfhfKgbbtM/5spOei1I5usGceVtacUZDSQDpzasYpy7g6YypV505bqxEK1sRvtPCF8CVfTI/YQotJ8uJCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"264354274fcb207b09539312a9355ff09e8d2bff7115366fb71972007ed3c95c","last_reissued_at":"2026-05-18T01:52:53.050797Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:52:53.050797Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Stochastic Particle Acceleration by Helical Turbulence in Solar Flares","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Gregory D. Fleishman, Igor N. Toptygin","submitted_at":"2012-11-29T22:43:20Z","abstract_excerpt":"Flaring release of magnetic energy in solar corona is only possible if the magnetic field deviates from a potential one. We show that the linear MHD modes excited on top of the non-potential magnetic field possess a nonzero kinetic helicity. Accordingly, this necessarily results in a noticeable kinetic helicity of the turbulence, composed of these linear modes with various scales and random phases, generated at the flare site by the primary energy release, which may be important for many applications. In particular, a nonzero turbulence helicity has a potentially strong effect on the particle "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1211.7112","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"1211.7112","created_at":"2026-05-18T01:52:53.050894+00:00"},{"alias_kind":"arxiv_version","alias_value":"1211.7112v1","created_at":"2026-05-18T01:52:53.050894+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1211.7112","created_at":"2026-05-18T01:52:53.050894+00:00"},{"alias_kind":"pith_short_12","alias_value":"EZBVIJ2PZMQH","created_at":"2026-05-18T12:27:04.183437+00:00"},{"alias_kind":"pith_short_16","alias_value":"EZBVIJ2PZMQHWCKT","created_at":"2026-05-18T12:27:04.183437+00:00"},{"alias_kind":"pith_short_8","alias_value":"EZBVIJ2P","created_at":"2026-05-18T12:27:04.183437+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/EZBVIJ2PZMQHWCKTSMJKSNK76C","json":"https://pith.science/pith/EZBVIJ2PZMQHWCKTSMJKSNK76C.json","graph_json":"https://pith.science/api/pith-number/EZBVIJ2PZMQHWCKTSMJKSNK76C/graph.json","events_json":"https://pith.science/api/pith-number/EZBVIJ2PZMQHWCKTSMJKSNK76C/events.json","paper":"https://pith.science/paper/EZBVIJ2P"},"agent_actions":{"view_html":"https://pith.science/pith/EZBVIJ2PZMQHWCKTSMJKSNK76C","download_json":"https://pith.science/pith/EZBVIJ2PZMQHWCKTSMJKSNK76C.json","view_paper":"https://pith.science/paper/EZBVIJ2P","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1211.7112&json=true","fetch_graph":"https://pith.science/api/pith-number/EZBVIJ2PZMQHWCKTSMJKSNK76C/graph.json","fetch_events":"https://pith.science/api/pith-number/EZBVIJ2PZMQHWCKTSMJKSNK76C/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EZBVIJ2PZMQHWCKTSMJKSNK76C/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EZBVIJ2PZMQHWCKTSMJKSNK76C/action/storage_attestation","attest_author":"https://pith.science/pith/EZBVIJ2PZMQHWCKTSMJKSNK76C/action/author_attestation","sign_citation":"https://pith.science/pith/EZBVIJ2PZMQHWCKTSMJKSNK76C/action/citation_signature","submit_replication":"https://pith.science/pith/EZBVIJ2PZMQHWCKTSMJKSNK76C/action/replication_record"}},"created_at":"2026-05-18T01:52:53.050894+00:00","updated_at":"2026-05-18T01:52:53.050894+00:00"}