{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:N4LC47CMHXLF5ES4XRDBLDZUBA","short_pith_number":"pith:N4LC47CM","schema_version":"1.0","canonical_sha256":"6f162e7c4c3dd65e925cbc46158f34080ba182581d0e094ea6bae39828a6d3a2","source":{"kind":"arxiv","id":"1502.07213","version":1},"attestation_state":"computed","paper":{"title":"Non-linear propagation of kink waves to the solar chromosphere","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"F. Giannattasio, M. Stangalini, S. Jafarzadeh","submitted_at":"2015-02-25T15:45:37Z","abstract_excerpt":"Small-scale magnetic field concentrations (magnetic elements) in the quiet Sun are believed to contribute to the energy budget of the upper layers of the Sun's atmosphere, as they are observed to support a large number of MHD modes. In recent years, kink waves in magnetic elements were observed at different heights in the solar atmosphere, from the photosphere to the corona. However, the propagation of these waves has not been fully evaluated. Our aim is to investigate the propagation of kink waves in small magnetic elements in the solar atmosphere. We analysed spectropolarimetric data of high"},"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":"1502.07213","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2015-02-25T15:45:37Z","cross_cats_sorted":[],"title_canon_sha256":"22014cd66e6e4edbbb413309f06423f4dee86c5e07f7bb2608fbed44407898a8","abstract_canon_sha256":"884d23f8a093db5273c85b17239aeecbf574eac2b63955e36677f2d9091e559d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:17:35.726304Z","signature_b64":"pvzdSXSsXqTywP/KuqLPh91LC5I7LN4x0eybEZ9yeX5frQ5ppb/1JuIuD+xKEEFl1ACB2Dr0+w9zwlgFw/YfDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6f162e7c4c3dd65e925cbc46158f34080ba182581d0e094ea6bae39828a6d3a2","last_reissued_at":"2026-05-18T02:17:35.725672Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:17:35.725672Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Non-linear propagation of kink waves to the solar chromosphere","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"F. Giannattasio, M. Stangalini, S. Jafarzadeh","submitted_at":"2015-02-25T15:45:37Z","abstract_excerpt":"Small-scale magnetic field concentrations (magnetic elements) in the quiet Sun are believed to contribute to the energy budget of the upper layers of the Sun's atmosphere, as they are observed to support a large number of MHD modes. In recent years, kink waves in magnetic elements were observed at different heights in the solar atmosphere, from the photosphere to the corona. However, the propagation of these waves has not been fully evaluated. Our aim is to investigate the propagation of kink waves in small magnetic elements in the solar atmosphere. We analysed spectropolarimetric data of high"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1502.07213","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":"1502.07213","created_at":"2026-05-18T02:17:35.725779+00:00"},{"alias_kind":"arxiv_version","alias_value":"1502.07213v1","created_at":"2026-05-18T02:17:35.725779+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1502.07213","created_at":"2026-05-18T02:17:35.725779+00:00"},{"alias_kind":"pith_short_12","alias_value":"N4LC47CMHXLF","created_at":"2026-05-18T12:29:32.376354+00:00"},{"alias_kind":"pith_short_16","alias_value":"N4LC47CMHXLF5ES4","created_at":"2026-05-18T12:29:32.376354+00:00"},{"alias_kind":"pith_short_8","alias_value":"N4LC47CM","created_at":"2026-05-18T12:29:32.376354+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/N4LC47CMHXLF5ES4XRDBLDZUBA","json":"https://pith.science/pith/N4LC47CMHXLF5ES4XRDBLDZUBA.json","graph_json":"https://pith.science/api/pith-number/N4LC47CMHXLF5ES4XRDBLDZUBA/graph.json","events_json":"https://pith.science/api/pith-number/N4LC47CMHXLF5ES4XRDBLDZUBA/events.json","paper":"https://pith.science/paper/N4LC47CM"},"agent_actions":{"view_html":"https://pith.science/pith/N4LC47CMHXLF5ES4XRDBLDZUBA","download_json":"https://pith.science/pith/N4LC47CMHXLF5ES4XRDBLDZUBA.json","view_paper":"https://pith.science/paper/N4LC47CM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1502.07213&json=true","fetch_graph":"https://pith.science/api/pith-number/N4LC47CMHXLF5ES4XRDBLDZUBA/graph.json","fetch_events":"https://pith.science/api/pith-number/N4LC47CMHXLF5ES4XRDBLDZUBA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/N4LC47CMHXLF5ES4XRDBLDZUBA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/N4LC47CMHXLF5ES4XRDBLDZUBA/action/storage_attestation","attest_author":"https://pith.science/pith/N4LC47CMHXLF5ES4XRDBLDZUBA/action/author_attestation","sign_citation":"https://pith.science/pith/N4LC47CMHXLF5ES4XRDBLDZUBA/action/citation_signature","submit_replication":"https://pith.science/pith/N4LC47CMHXLF5ES4XRDBLDZUBA/action/replication_record"}},"created_at":"2026-05-18T02:17:35.725779+00:00","updated_at":"2026-05-18T02:17:35.725779+00:00"}