{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:Y5YL45GX4NJKXYEGJ3WQ7RKULX","short_pith_number":"pith:Y5YL45GX","schema_version":"1.0","canonical_sha256":"c770be74d7e352abe0864eed0fc5545dd93807f43503b88c375701ae817e8009","source":{"kind":"arxiv","id":"2505.02733","version":1},"attestation_state":"computed","paper":{"title":"Merging plasmoids and nanojet-like ejections in a coronal current sheet","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["physics.plasm-ph"],"primary_cat":"astro-ph.SR","authors_text":"F. Moreno-Insertis, Samrat Sen","submitted_at":"2025-05-05T15:33:13Z","abstract_excerpt":"Forced magnetic reconnection is triggered by external perturbations, which are ubiquitous in the solar corona. This process plays a crucial role in the energy release during solar transient events, which are often associated with electric current sheets (CSs). The CSs can often disintegrate through the development of the tearing instability, which may lead to the formation of plasmoids in the non-linear phase of evolution. However, the complexity of the dynamics, and the magnetic and thermodynamic evolution due to the coalescence of the plasmoids are not fully understood. We used a resistive m"},"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":"2505.02733","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.SR","submitted_at":"2025-05-05T15:33:13Z","cross_cats_sorted":["physics.plasm-ph"],"title_canon_sha256":"0460558448e701eac7cc6e19ba5abcf9e07946ee5b717241a17cd5c63e1b9a82","abstract_canon_sha256":"406c792e4844c27ff18af583ad835fbf2f9dfb26c0bf8a87b311048eec033afb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:29:59.079475Z","signature_b64":"MXNIBEjHny3oB1xmxwTzK5atABVgfKM7BokSgFnCxvv1T4YXmScQA3Qmwl0bc7oLZtJVJfiCAp9M3OVWoSXCBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c770be74d7e352abe0864eed0fc5545dd93807f43503b88c375701ae817e8009","last_reissued_at":"2026-07-05T11:29:59.078981Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:29:59.078981Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Merging plasmoids and nanojet-like ejections in a coronal current sheet","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["physics.plasm-ph"],"primary_cat":"astro-ph.SR","authors_text":"F. Moreno-Insertis, Samrat Sen","submitted_at":"2025-05-05T15:33:13Z","abstract_excerpt":"Forced magnetic reconnection is triggered by external perturbations, which are ubiquitous in the solar corona. This process plays a crucial role in the energy release during solar transient events, which are often associated with electric current sheets (CSs). The CSs can often disintegrate through the development of the tearing instability, which may lead to the formation of plasmoids in the non-linear phase of evolution. However, the complexity of the dynamics, and the magnetic and thermodynamic evolution due to the coalescence of the plasmoids are not fully understood. We used a resistive m"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2505.02733","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2505.02733/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2505.02733","created_at":"2026-07-05T11:29:59.079037+00:00"},{"alias_kind":"arxiv_version","alias_value":"2505.02733v1","created_at":"2026-07-05T11:29:59.079037+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2505.02733","created_at":"2026-07-05T11:29:59.079037+00:00"},{"alias_kind":"pith_short_12","alias_value":"Y5YL45GX4NJK","created_at":"2026-07-05T11:29:59.079037+00:00"},{"alias_kind":"pith_short_16","alias_value":"Y5YL45GX4NJKXYEG","created_at":"2026-07-05T11:29:59.079037+00:00"},{"alias_kind":"pith_short_8","alias_value":"Y5YL45GX","created_at":"2026-07-05T11:29:59.079037+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.03055","citing_title":"On the cool nature of coronal nanojets","ref_index":20,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/Y5YL45GX4NJKXYEGJ3WQ7RKULX","json":"https://pith.science/pith/Y5YL45GX4NJKXYEGJ3WQ7RKULX.json","graph_json":"https://pith.science/api/pith-number/Y5YL45GX4NJKXYEGJ3WQ7RKULX/graph.json","events_json":"https://pith.science/api/pith-number/Y5YL45GX4NJKXYEGJ3WQ7RKULX/events.json","paper":"https://pith.science/paper/Y5YL45GX"},"agent_actions":{"view_html":"https://pith.science/pith/Y5YL45GX4NJKXYEGJ3WQ7RKULX","download_json":"https://pith.science/pith/Y5YL45GX4NJKXYEGJ3WQ7RKULX.json","view_paper":"https://pith.science/paper/Y5YL45GX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2505.02733&json=true","fetch_graph":"https://pith.science/api/pith-number/Y5YL45GX4NJKXYEGJ3WQ7RKULX/graph.json","fetch_events":"https://pith.science/api/pith-number/Y5YL45GX4NJKXYEGJ3WQ7RKULX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/Y5YL45GX4NJKXYEGJ3WQ7RKULX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/Y5YL45GX4NJKXYEGJ3WQ7RKULX/action/storage_attestation","attest_author":"https://pith.science/pith/Y5YL45GX4NJKXYEGJ3WQ7RKULX/action/author_attestation","sign_citation":"https://pith.science/pith/Y5YL45GX4NJKXYEGJ3WQ7RKULX/action/citation_signature","submit_replication":"https://pith.science/pith/Y5YL45GX4NJKXYEGJ3WQ7RKULX/action/replication_record"}},"created_at":"2026-07-05T11:29:59.079037+00:00","updated_at":"2026-07-05T11:29:59.079037+00:00"}