{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2011:ZHYILEO7OZW6LLHWWDLBQI3IEJ","short_pith_number":"pith:ZHYILEO7","canonical_record":{"source":{"id":"1108.5026","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-08-25T07:18:17Z","cross_cats_sorted":[],"title_canon_sha256":"af15b7938dec19b2593f1c69b9dd8ef51731cac1ee55b9cb1fc30dc384caf295","abstract_canon_sha256":"3e2e9aa68acfa7d5be45e5dead1279e5f7ff899f417c9a66ea7ebe44b3694c86"},"schema_version":"1.0"},"canonical_sha256":"c9f08591df766de5acf6b0d61823682251697a43c74ac28bb706ece4a191c3fa","source":{"kind":"arxiv","id":"1108.5026","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1108.5026","created_at":"2026-05-18T02:00:48Z"},{"alias_kind":"arxiv_version","alias_value":"1108.5026v1","created_at":"2026-05-18T02:00:48Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1108.5026","created_at":"2026-05-18T02:00:48Z"},{"alias_kind":"pith_short_12","alias_value":"ZHYILEO7OZW6","created_at":"2026-05-18T12:26:47Z"},{"alias_kind":"pith_short_16","alias_value":"ZHYILEO7OZW6LLHW","created_at":"2026-05-18T12:26:47Z"},{"alias_kind":"pith_short_8","alias_value":"ZHYILEO7","created_at":"2026-05-18T12:26:47Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2011:ZHYILEO7OZW6LLHWWDLBQI3IEJ","target":"record","payload":{"canonical_record":{"source":{"id":"1108.5026","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-08-25T07:18:17Z","cross_cats_sorted":[],"title_canon_sha256":"af15b7938dec19b2593f1c69b9dd8ef51731cac1ee55b9cb1fc30dc384caf295","abstract_canon_sha256":"3e2e9aa68acfa7d5be45e5dead1279e5f7ff899f417c9a66ea7ebe44b3694c86"},"schema_version":"1.0"},"canonical_sha256":"c9f08591df766de5acf6b0d61823682251697a43c74ac28bb706ece4a191c3fa","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:00:48.312190Z","signature_b64":"Gpl+RC6B8+ATCfs0H9y+8CngLcyzlrSYpXyFHJO3zybT6yHUYuzMbN+cM/VsQJ84vPQ+L2R9s2RvJwS53Vt+Cg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c9f08591df766de5acf6b0d61823682251697a43c74ac28bb706ece4a191c3fa","last_reissued_at":"2026-05-18T02:00:48.311545Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:00:48.311545Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1108.5026","source_version":1,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T02:00:48Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"1gFqk5oRzKzyGYJEFzdZc02A1OIrWU+7C/kL7TgE4SceBGl5jX+05g1PEPokdDhN4oOhhgELwwib6pi5IRR+Cg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-27T07:11:56.610226Z"},"content_sha256":"29e7a093862b6c2d6a317604a64b098018e2454292c57e61841b7bacaa59cf83","schema_version":"1.0","event_id":"sha256:29e7a093862b6c2d6a317604a64b098018e2454292c57e61841b7bacaa59cf83"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2011:ZHYILEO7OZW6LLHWWDLBQI3IEJ","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Magnetic Reconnection in Non-Equilibrium Ionization Plasma","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"H. Hara, I. Murakami, S. Imada, T. Shimizu, T. Watanabe","submitted_at":"2011-08-25T07:18:17Z","abstract_excerpt":"We have studied the effect of time-dependent ionization and recombination processes on magnetic reconnection in the solar corona. Petschek-type steady reconnection, in which model the magnetic energy is mainly converted at the slow-mode shocks, was assumed. We carried out the time-dependent ionization calculation in the magnetic reconnection structure. We only calculated the transient ionization of iron; the other species were assumed to be in ionization equilibrium. The intensity of line emissions at specific wavelengths were also calculated for comparison with {\\it Hinode} or other observati"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1108.5026","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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T02:00:48Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"bxK9Y5mQRCB3qOnoo81nViRi3uUmRFUUATwc3ZQsGljGQ1nxASUNJSFEgDsoUZbqOVomVVrVnUU10SXQ37uLDw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-27T07:11:56.610914Z"},"content_sha256":"37a149e320f3a8c80bba939fe95bd9c17031dc173621d3b17d586afc419a41f5","schema_version":"1.0","event_id":"sha256:37a149e320f3a8c80bba939fe95bd9c17031dc173621d3b17d586afc419a41f5"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/ZHYILEO7OZW6LLHWWDLBQI3IEJ/bundle.json","state_url":"https://pith.science/pith/ZHYILEO7OZW6LLHWWDLBQI3IEJ/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/ZHYILEO7OZW6LLHWWDLBQI3IEJ/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-05-27T07:11:56Z","links":{"resolver":"https://pith.science/pith/ZHYILEO7OZW6LLHWWDLBQI3IEJ","bundle":"https://pith.science/pith/ZHYILEO7OZW6LLHWWDLBQI3IEJ/bundle.json","state":"https://pith.science/pith/ZHYILEO7OZW6LLHWWDLBQI3IEJ/state.json","well_known_bundle":"https://pith.science/.well-known/pith/ZHYILEO7OZW6LLHWWDLBQI3IEJ/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2011:ZHYILEO7OZW6LLHWWDLBQI3IEJ","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"3e2e9aa68acfa7d5be45e5dead1279e5f7ff899f417c9a66ea7ebe44b3694c86","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-08-25T07:18:17Z","title_canon_sha256":"af15b7938dec19b2593f1c69b9dd8ef51731cac1ee55b9cb1fc30dc384caf295"},"schema_version":"1.0","source":{"id":"1108.5026","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1108.5026","created_at":"2026-05-18T02:00:48Z"},{"alias_kind":"arxiv_version","alias_value":"1108.5026v1","created_at":"2026-05-18T02:00:48Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1108.5026","created_at":"2026-05-18T02:00:48Z"},{"alias_kind":"pith_short_12","alias_value":"ZHYILEO7OZW6","created_at":"2026-05-18T12:26:47Z"},{"alias_kind":"pith_short_16","alias_value":"ZHYILEO7OZW6LLHW","created_at":"2026-05-18T12:26:47Z"},{"alias_kind":"pith_short_8","alias_value":"ZHYILEO7","created_at":"2026-05-18T12:26:47Z"}],"graph_snapshots":[{"event_id":"sha256:37a149e320f3a8c80bba939fe95bd9c17031dc173621d3b17d586afc419a41f5","target":"graph","created_at":"2026-05-18T02:00:48Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"We have studied the effect of time-dependent ionization and recombination processes on magnetic reconnection in the solar corona. Petschek-type steady reconnection, in which model the magnetic energy is mainly converted at the slow-mode shocks, was assumed. We carried out the time-dependent ionization calculation in the magnetic reconnection structure. We only calculated the transient ionization of iron; the other species were assumed to be in ionization equilibrium. The intensity of line emissions at specific wavelengths were also calculated for comparison with {\\it Hinode} or other observati","authors_text":"H. Hara, I. Murakami, S. Imada, T. Shimizu, T. Watanabe","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-08-25T07:18:17Z","title":"Magnetic Reconnection in Non-Equilibrium Ionization Plasma"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1108.5026","kind":"arxiv","version":1},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:29e7a093862b6c2d6a317604a64b098018e2454292c57e61841b7bacaa59cf83","target":"record","created_at":"2026-05-18T02:00:48Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"3e2e9aa68acfa7d5be45e5dead1279e5f7ff899f417c9a66ea7ebe44b3694c86","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-08-25T07:18:17Z","title_canon_sha256":"af15b7938dec19b2593f1c69b9dd8ef51731cac1ee55b9cb1fc30dc384caf295"},"schema_version":"1.0","source":{"id":"1108.5026","kind":"arxiv","version":1}},"canonical_sha256":"c9f08591df766de5acf6b0d61823682251697a43c74ac28bb706ece4a191c3fa","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"c9f08591df766de5acf6b0d61823682251697a43c74ac28bb706ece4a191c3fa","first_computed_at":"2026-05-18T02:00:48.311545Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T02:00:48.311545Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"Gpl+RC6B8+ATCfs0H9y+8CngLcyzlrSYpXyFHJO3zybT6yHUYuzMbN+cM/VsQJ84vPQ+L2R9s2RvJwS53Vt+Cg==","signature_status":"signed_v1","signed_at":"2026-05-18T02:00:48.312190Z","signed_message":"canonical_sha256_bytes"},"source_id":"1108.5026","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:29e7a093862b6c2d6a317604a64b098018e2454292c57e61841b7bacaa59cf83","sha256:37a149e320f3a8c80bba939fe95bd9c17031dc173621d3b17d586afc419a41f5"],"state_sha256":"9e7520e25926d7db7c79adad9379a2fc1b9a0c0059610501492d42122f7819be"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"EOn959pilr/bCRIxJMcYZ7GHDz/mAFPVSH+jR5cckVLBbN5xbLuaMyaZmWDYjhq8AjgP9i/TgTFEbi676bcSCw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-27T07:11:56.614167Z","bundle_sha256":"6833ab72132bc2a9bd5112004489eee5e3df1bb58789d767cf0c37860c24e03d"}}