{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:2N7SQDB2754V43ZRFLYYOKF6AD","short_pith_number":"pith:2N7SQDB2","schema_version":"1.0","canonical_sha256":"d37f280c3aff795e6f312af18728be00cfa6e34e9646d846b9c5d4957f52ea92","source":{"kind":"arxiv","id":"1404.1772","version":1},"attestation_state":"computed","paper":{"title":"Turbulent magnetic energy spectrum and the cancellation function of solar photospheric magnetic fields","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"G. Marschalk\\'o, K. Petrovay","submitted_at":"2014-04-07T12:52:57Z","abstract_excerpt":"A simple analytical relation of form {\\alpha} = 2 {\\kappa} -1 between the magnetic energy spectral exponent {\\alpha} of the turbulent magnetic field in the solar photosphere and its magnetic flux cancellation exponent {\\kappa}, valid under certain restrictive assumptions, is tested and extended outside its range of validity in a series of Monte Carlo simulations. In these numerical tests artificial \"magnetograms\" are constructed in 1D and 2D by superposing a discrete set of Fourier modes of the magnetic field distribution with amplitudes following a power law spectrum and measuring the cancell"},"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":"1404.1772","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-04-07T12:52:57Z","cross_cats_sorted":[],"title_canon_sha256":"787ec950037c65152e1644867d0827ad533091fe17dfc1dd654ecabfb20578e1","abstract_canon_sha256":"8dd4c0f3e0f7b67eebcf85618ca5bd2039aed750845b74a037aa24fa5658f282"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:54:40.212733Z","signature_b64":"y76ouoz13nxj8dkgKOOOa34JALsIdpKvBjSFJ2h1IFbhti2T497lmi6K3kDj+uXLfXXYUlVkQiobOfsvlY7kBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d37f280c3aff795e6f312af18728be00cfa6e34e9646d846b9c5d4957f52ea92","last_reissued_at":"2026-05-18T02:54:40.212298Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:54:40.212298Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Turbulent magnetic energy spectrum and the cancellation function of solar photospheric magnetic fields","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"G. Marschalk\\'o, K. Petrovay","submitted_at":"2014-04-07T12:52:57Z","abstract_excerpt":"A simple analytical relation of form {\\alpha} = 2 {\\kappa} -1 between the magnetic energy spectral exponent {\\alpha} of the turbulent magnetic field in the solar photosphere and its magnetic flux cancellation exponent {\\kappa}, valid under certain restrictive assumptions, is tested and extended outside its range of validity in a series of Monte Carlo simulations. In these numerical tests artificial \"magnetograms\" are constructed in 1D and 2D by superposing a discrete set of Fourier modes of the magnetic field distribution with amplitudes following a power law spectrum and measuring the cancell"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1404.1772","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":"1404.1772","created_at":"2026-05-18T02:54:40.212367+00:00"},{"alias_kind":"arxiv_version","alias_value":"1404.1772v1","created_at":"2026-05-18T02:54:40.212367+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1404.1772","created_at":"2026-05-18T02:54:40.212367+00:00"},{"alias_kind":"pith_short_12","alias_value":"2N7SQDB2754V","created_at":"2026-05-18T12:28:11.866339+00:00"},{"alias_kind":"pith_short_16","alias_value":"2N7SQDB2754V43ZR","created_at":"2026-05-18T12:28:11.866339+00:00"},{"alias_kind":"pith_short_8","alias_value":"2N7SQDB2","created_at":"2026-05-18T12:28:11.866339+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/2N7SQDB2754V43ZRFLYYOKF6AD","json":"https://pith.science/pith/2N7SQDB2754V43ZRFLYYOKF6AD.json","graph_json":"https://pith.science/api/pith-number/2N7SQDB2754V43ZRFLYYOKF6AD/graph.json","events_json":"https://pith.science/api/pith-number/2N7SQDB2754V43ZRFLYYOKF6AD/events.json","paper":"https://pith.science/paper/2N7SQDB2"},"agent_actions":{"view_html":"https://pith.science/pith/2N7SQDB2754V43ZRFLYYOKF6AD","download_json":"https://pith.science/pith/2N7SQDB2754V43ZRFLYYOKF6AD.json","view_paper":"https://pith.science/paper/2N7SQDB2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1404.1772&json=true","fetch_graph":"https://pith.science/api/pith-number/2N7SQDB2754V43ZRFLYYOKF6AD/graph.json","fetch_events":"https://pith.science/api/pith-number/2N7SQDB2754V43ZRFLYYOKF6AD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2N7SQDB2754V43ZRFLYYOKF6AD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2N7SQDB2754V43ZRFLYYOKF6AD/action/storage_attestation","attest_author":"https://pith.science/pith/2N7SQDB2754V43ZRFLYYOKF6AD/action/author_attestation","sign_citation":"https://pith.science/pith/2N7SQDB2754V43ZRFLYYOKF6AD/action/citation_signature","submit_replication":"https://pith.science/pith/2N7SQDB2754V43ZRFLYYOKF6AD/action/replication_record"}},"created_at":"2026-05-18T02:54:40.212367+00:00","updated_at":"2026-05-18T02:54:40.212367+00:00"}