{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2015:GZHNRJ54KWGFJIHFY5BDTEPUCE","short_pith_number":"pith:GZHNRJ54","canonical_record":{"source":{"id":"1511.08863","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2015-11-28T02:11:47Z","cross_cats_sorted":[],"title_canon_sha256":"148c6690b1a0ffa1e67cef3b815eca005c11f011c0311dc6b593019744c754ba","abstract_canon_sha256":"9e8d471401eba367517944a23a0372c80934dcacf63474dfa970ae60ab74a3cc"},"schema_version":"1.0"},"canonical_sha256":"364ed8a7bc558c54a0e5c7423991f41111e8c5b3e60d028b74964428756f3172","source":{"kind":"arxiv","id":"1511.08863","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1511.08863","created_at":"2026-05-18T01:14:52Z"},{"alias_kind":"arxiv_version","alias_value":"1511.08863v2","created_at":"2026-05-18T01:14:52Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1511.08863","created_at":"2026-05-18T01:14:52Z"},{"alias_kind":"pith_short_12","alias_value":"GZHNRJ54KWGF","created_at":"2026-05-18T12:29:22Z"},{"alias_kind":"pith_short_16","alias_value":"GZHNRJ54KWGFJIHF","created_at":"2026-05-18T12:29:22Z"},{"alias_kind":"pith_short_8","alias_value":"GZHNRJ54","created_at":"2026-05-18T12:29:22Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2015:GZHNRJ54KWGFJIHFY5BDTEPUCE","target":"record","payload":{"canonical_record":{"source":{"id":"1511.08863","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2015-11-28T02:11:47Z","cross_cats_sorted":[],"title_canon_sha256":"148c6690b1a0ffa1e67cef3b815eca005c11f011c0311dc6b593019744c754ba","abstract_canon_sha256":"9e8d471401eba367517944a23a0372c80934dcacf63474dfa970ae60ab74a3cc"},"schema_version":"1.0"},"canonical_sha256":"364ed8a7bc558c54a0e5c7423991f41111e8c5b3e60d028b74964428756f3172","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:14:52.759457Z","signature_b64":"x0d5or7cviCi/cG0LCXBeUemmHdGsvwKl9UY7Rcynd4YkYaZBAq66OUDSMm8pD+n/6kQDqpORLN30jmhfq7ABg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"364ed8a7bc558c54a0e5c7423991f41111e8c5b3e60d028b74964428756f3172","last_reissued_at":"2026-05-18T01:14:52.758813Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:14:52.758813Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1511.08863","source_version":2,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T01:14:52Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"SphVOfLghfyr8Yr9DmLfp2FLwSO6ZEOvsXPHBgiIQCub5FzV8cMiHjzBL5d5nt+LE8womDb2W0Ibdv3nzluLBg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-04T15:11:58.952905Z"},"content_sha256":"e78fda9abb50bb22f77c80f8c3557e333cedf4258fbb9020f9db211d60bba5fb","schema_version":"1.0","event_id":"sha256:e78fda9abb50bb22f77c80f8c3557e333cedf4258fbb9020f9db211d60bba5fb"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2015:GZHNRJ54KWGFJIHFY5BDTEPUCE","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Diagnose Physical Conditions Near the Flare Energy-release Sites from Observations of Solar Microwave Type III Bursts","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Baolin Tan, Guangli Huang, Hana Meszarosova, Marian Karlicky","submitted_at":"2015-11-28T02:11:47Z","abstract_excerpt":"In the physics of solar flares, it is crucial to diagnose the physical conditions near the flare energy-release sites. However, so far it is unclear how do diagnose these physical conditions. Solar microwave type III burst is believed to be a sensitive signature of the primary energy release and electron accelerations in solar flares. This work takes into account the effect of magnetic field on the plasma density and developed s set of formulas which can be used to estimate the plasma density, temperature, magnetic field near the magnetic reconnection site and particle acceleration region, and"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1511.08863","kind":"arxiv","version":2},"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":"2026-05-18T01:14:52Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"f5a7lCEikbeu9/o9dhR5DqRWT4qrYFcaZlqLkbKqI2JRbZlbxbbD9zOGWAps29NHnqjiM96Ro5LSnfJSrnFKDw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-04T15:11:58.953242Z"},"content_sha256":"2c80a3191a16271c10c80c86ce65c3e531977f61ece6cbdfb0a8fa53b8270c8f","schema_version":"1.0","event_id":"sha256:2c80a3191a16271c10c80c86ce65c3e531977f61ece6cbdfb0a8fa53b8270c8f"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/GZHNRJ54KWGFJIHFY5BDTEPUCE/bundle.json","state_url":"https://pith.science/pith/GZHNRJ54KWGFJIHFY5BDTEPUCE/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/GZHNRJ54KWGFJIHFY5BDTEPUCE/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":"2026-06-04T15:11:58Z","links":{"resolver":"https://pith.science/pith/GZHNRJ54KWGFJIHFY5BDTEPUCE","bundle":"https://pith.science/pith/GZHNRJ54KWGFJIHFY5BDTEPUCE/bundle.json","state":"https://pith.science/pith/GZHNRJ54KWGFJIHFY5BDTEPUCE/state.json","well_known_bundle":"https://pith.science/.well-known/pith/GZHNRJ54KWGFJIHFY5BDTEPUCE/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2015:GZHNRJ54KWGFJIHFY5BDTEPUCE","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":"9e8d471401eba367517944a23a0372c80934dcacf63474dfa970ae60ab74a3cc","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2015-11-28T02:11:47Z","title_canon_sha256":"148c6690b1a0ffa1e67cef3b815eca005c11f011c0311dc6b593019744c754ba"},"schema_version":"1.0","source":{"id":"1511.08863","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1511.08863","created_at":"2026-05-18T01:14:52Z"},{"alias_kind":"arxiv_version","alias_value":"1511.08863v2","created_at":"2026-05-18T01:14:52Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1511.08863","created_at":"2026-05-18T01:14:52Z"},{"alias_kind":"pith_short_12","alias_value":"GZHNRJ54KWGF","created_at":"2026-05-18T12:29:22Z"},{"alias_kind":"pith_short_16","alias_value":"GZHNRJ54KWGFJIHF","created_at":"2026-05-18T12:29:22Z"},{"alias_kind":"pith_short_8","alias_value":"GZHNRJ54","created_at":"2026-05-18T12:29:22Z"}],"graph_snapshots":[{"event_id":"sha256:2c80a3191a16271c10c80c86ce65c3e531977f61ece6cbdfb0a8fa53b8270c8f","target":"graph","created_at":"2026-05-18T01:14:52Z","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":"In the physics of solar flares, it is crucial to diagnose the physical conditions near the flare energy-release sites. However, so far it is unclear how do diagnose these physical conditions. Solar microwave type III burst is believed to be a sensitive signature of the primary energy release and electron accelerations in solar flares. This work takes into account the effect of magnetic field on the plasma density and developed s set of formulas which can be used to estimate the plasma density, temperature, magnetic field near the magnetic reconnection site and particle acceleration region, and","authors_text":"Baolin Tan, Guangli Huang, Hana Meszarosova, Marian Karlicky","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2015-11-28T02:11:47Z","title":"Diagnose Physical Conditions Near the Flare Energy-release Sites from Observations of Solar Microwave Type III Bursts"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1511.08863","kind":"arxiv","version":2},"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:e78fda9abb50bb22f77c80f8c3557e333cedf4258fbb9020f9db211d60bba5fb","target":"record","created_at":"2026-05-18T01:14:52Z","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":"9e8d471401eba367517944a23a0372c80934dcacf63474dfa970ae60ab74a3cc","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2015-11-28T02:11:47Z","title_canon_sha256":"148c6690b1a0ffa1e67cef3b815eca005c11f011c0311dc6b593019744c754ba"},"schema_version":"1.0","source":{"id":"1511.08863","kind":"arxiv","version":2}},"canonical_sha256":"364ed8a7bc558c54a0e5c7423991f41111e8c5b3e60d028b74964428756f3172","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"364ed8a7bc558c54a0e5c7423991f41111e8c5b3e60d028b74964428756f3172","first_computed_at":"2026-05-18T01:14:52.758813Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:14:52.758813Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"x0d5or7cviCi/cG0LCXBeUemmHdGsvwKl9UY7Rcynd4YkYaZBAq66OUDSMm8pD+n/6kQDqpORLN30jmhfq7ABg==","signature_status":"signed_v1","signed_at":"2026-05-18T01:14:52.759457Z","signed_message":"canonical_sha256_bytes"},"source_id":"1511.08863","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:e78fda9abb50bb22f77c80f8c3557e333cedf4258fbb9020f9db211d60bba5fb","sha256:2c80a3191a16271c10c80c86ce65c3e531977f61ece6cbdfb0a8fa53b8270c8f"],"state_sha256":"aabfe6165b91d2c2ed9f72581b8e8c9b33b237702f2f2400bdbdc9e46ffa96c4"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"/vfh0HDJZb0eNS5PayrJtgc2AfZOFh0Uw6eY0LeFjdqqyAtRws5jbD7YKIChXS4HCxF4UHMVrO0N6+JFtUOuBA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-04T15:11:58.955134Z","bundle_sha256":"fae592911183f5535459cad0358fb125d19658e132a2cc975cfc9c3db3458249"}}