{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:GTRD6O32W4DVHSHT4RSD7NAMZV","short_pith_number":"pith:GTRD6O32","schema_version":"1.0","canonical_sha256":"34e23f3b7ab70753c8f3e4643fb40ccd5038d71708b23649b484aa53816ea518","source":{"kind":"arxiv","id":"1106.3417","version":1},"attestation_state":"computed","paper":{"title":"EUV jets, type III radio bursts and sunspot waves investigated using SDO/AIA observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"D. E. Innes, R. H. Cameron, S. K. Solanki","submitted_at":"2011-06-17T09:11:24Z","abstract_excerpt":"Images from the Solar Dynamics Observatory (SDO) at 211A are used to identify the solar source of the type III radio bursts seen in WIND/WAVES dynamic spectra. We analyse a 2.5 hour period during which six strong bursts are seen. The radio bursts correlate very well with the EUV jets coming from the western side of a sunspot in AR11092. The EUV jet emission also correlates well with brightening at what looks like their footpoint at the edge of the umbra. For 10-15 min after strong EUV jets are ejected, the footpoint brightens at roughly 3 min intervals. In both the EUV images and the extracted"},"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":"1106.3417","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-06-17T09:11:24Z","cross_cats_sorted":[],"title_canon_sha256":"fe71dae82e48d148a0305f9fe8023f3da783345e33086be93215453b3bfad07d","abstract_canon_sha256":"d7b3efc7f0b518114c19f8c48fb6038f3b627cedec99378234a543c7816c0390"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:01:35.836993Z","signature_b64":"otcTHyIWj777j7hRLwg3lGBOP/J3nbt4+PLHGWY4T8CKf7PnZwKVDEhQof0p59WDkr6yL/lt/dZ2wUHNh+g4Dw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"34e23f3b7ab70753c8f3e4643fb40ccd5038d71708b23649b484aa53816ea518","last_reissued_at":"2026-05-18T02:01:35.836151Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:01:35.836151Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"EUV jets, type III radio bursts and sunspot waves investigated using SDO/AIA observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"D. E. Innes, R. H. Cameron, S. K. Solanki","submitted_at":"2011-06-17T09:11:24Z","abstract_excerpt":"Images from the Solar Dynamics Observatory (SDO) at 211A are used to identify the solar source of the type III radio bursts seen in WIND/WAVES dynamic spectra. We analyse a 2.5 hour period during which six strong bursts are seen. The radio bursts correlate very well with the EUV jets coming from the western side of a sunspot in AR11092. The EUV jet emission also correlates well with brightening at what looks like their footpoint at the edge of the umbra. For 10-15 min after strong EUV jets are ejected, the footpoint brightens at roughly 3 min intervals. In both the EUV images and the extracted"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1106.3417","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":"1106.3417","created_at":"2026-05-18T02:01:35.836294+00:00"},{"alias_kind":"arxiv_version","alias_value":"1106.3417v1","created_at":"2026-05-18T02:01:35.836294+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1106.3417","created_at":"2026-05-18T02:01:35.836294+00:00"},{"alias_kind":"pith_short_12","alias_value":"GTRD6O32W4DV","created_at":"2026-05-18T12:26:30.835961+00:00"},{"alias_kind":"pith_short_16","alias_value":"GTRD6O32W4DVHSHT","created_at":"2026-05-18T12:26:30.835961+00:00"},{"alias_kind":"pith_short_8","alias_value":"GTRD6O32","created_at":"2026-05-18T12:26:30.835961+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/GTRD6O32W4DVHSHT4RSD7NAMZV","json":"https://pith.science/pith/GTRD6O32W4DVHSHT4RSD7NAMZV.json","graph_json":"https://pith.science/api/pith-number/GTRD6O32W4DVHSHT4RSD7NAMZV/graph.json","events_json":"https://pith.science/api/pith-number/GTRD6O32W4DVHSHT4RSD7NAMZV/events.json","paper":"https://pith.science/paper/GTRD6O32"},"agent_actions":{"view_html":"https://pith.science/pith/GTRD6O32W4DVHSHT4RSD7NAMZV","download_json":"https://pith.science/pith/GTRD6O32W4DVHSHT4RSD7NAMZV.json","view_paper":"https://pith.science/paper/GTRD6O32","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1106.3417&json=true","fetch_graph":"https://pith.science/api/pith-number/GTRD6O32W4DVHSHT4RSD7NAMZV/graph.json","fetch_events":"https://pith.science/api/pith-number/GTRD6O32W4DVHSHT4RSD7NAMZV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GTRD6O32W4DVHSHT4RSD7NAMZV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GTRD6O32W4DVHSHT4RSD7NAMZV/action/storage_attestation","attest_author":"https://pith.science/pith/GTRD6O32W4DVHSHT4RSD7NAMZV/action/author_attestation","sign_citation":"https://pith.science/pith/GTRD6O32W4DVHSHT4RSD7NAMZV/action/citation_signature","submit_replication":"https://pith.science/pith/GTRD6O32W4DVHSHT4RSD7NAMZV/action/replication_record"}},"created_at":"2026-05-18T02:01:35.836294+00:00","updated_at":"2026-05-18T02:01:35.836294+00:00"}