{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2010:ERSGDALHCGLPBMAC5S3KUTKQV6","short_pith_number":"pith:ERSGDALH","canonical_record":{"source":{"id":"1006.3738","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2010-06-18T16:04:54Z","cross_cats_sorted":[],"title_canon_sha256":"a3306b00a353e6b4314e7585ecab3e9a31169ac4b3c57963849c8eb8fc588f37","abstract_canon_sha256":"23b341e6b0715a571ec3a7f94016010db5128179d4fbe62f02b7a06da86dfbe4"},"schema_version":"1.0"},"canonical_sha256":"24646181671196f0b002ecb6aa4d50af92d5ced86233fcf5a49734dbe38203a7","source":{"kind":"arxiv","id":"1006.3738","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1006.3738","created_at":"2026-05-18T02:06:44Z"},{"alias_kind":"arxiv_version","alias_value":"1006.3738v1","created_at":"2026-05-18T02:06:44Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1006.3738","created_at":"2026-05-18T02:06:44Z"},{"alias_kind":"pith_short_12","alias_value":"ERSGDALHCGLP","created_at":"2026-05-18T12:26:06Z"},{"alias_kind":"pith_short_16","alias_value":"ERSGDALHCGLPBMAC","created_at":"2026-05-18T12:26:06Z"},{"alias_kind":"pith_short_8","alias_value":"ERSGDALH","created_at":"2026-05-18T12:26:06Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2010:ERSGDALHCGLPBMAC5S3KUTKQV6","target":"record","payload":{"canonical_record":{"source":{"id":"1006.3738","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2010-06-18T16:04:54Z","cross_cats_sorted":[],"title_canon_sha256":"a3306b00a353e6b4314e7585ecab3e9a31169ac4b3c57963849c8eb8fc588f37","abstract_canon_sha256":"23b341e6b0715a571ec3a7f94016010db5128179d4fbe62f02b7a06da86dfbe4"},"schema_version":"1.0"},"canonical_sha256":"24646181671196f0b002ecb6aa4d50af92d5ced86233fcf5a49734dbe38203a7","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:06:44.480242Z","signature_b64":"6HH2GAC6KsPOdTaQpXMVw7rc4H8e+l6iqRRrrpyDsnbJiiRroeFDFKA4FJl+hxBR3sCkx77jU6zyOeirZCrbAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"24646181671196f0b002ecb6aa4d50af92d5ced86233fcf5a49734dbe38203a7","last_reissued_at":"2026-05-18T02:06:44.479878Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:06:44.479878Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1006.3738","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":"2026-05-18T02:06:44Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"IPffQf7aBBgpinbZXgK/NpnmIsPAh8ZkNXGUeOhEcgxlRG2XlaDmLCZ3+hNbhVhpG1j1ihBuiVbxEUpWLJuTCw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-25T20:22:02.854337Z"},"content_sha256":"93e0eecfda26d9b4c7700a4b402b1daececd22cb3f9cf8ad9fe2526557255f88","schema_version":"1.0","event_id":"sha256:93e0eecfda26d9b4c7700a4b402b1daececd22cb3f9cf8ad9fe2526557255f88"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2010:ERSGDALHCGLPBMAC5S3KUTKQV6","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Magnetic Structure of Rapidly Rotating FK Comae-Type Coronae","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"D. Elstner, H. Korhonen, J.J. Drake, O. Cohen, T.I. Gombosi, V.L. Kashyap","submitted_at":"2010-06-18T16:04:54Z","abstract_excerpt":"We present a three-dimensional simulation of the corona of an FK Com-type rapidly rotating G giant using a magnetohydrodynamic model that was originally developed for the solar corona in order to capture the more realistic, non-potential coronal structure. We drive the simulation with surface maps for the radial magnetic field obtained from a stellar dynamo model of the FK Com system. This enables us to obtain the coronal structure for different field topologies representing different periods of time. We find that the corona of such an FK Com-like star, including the large scale coronal loops,"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1006.3738","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":"2026-05-18T02:06:44Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"kmASNIn2xJCKI6ULQncohUj6v2DJw0XGHag/nO2n6Aa6V9CrxE94pQIFtcb2G1J+vai1628j/2z5vNfbMHf7Aw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-25T20:22:02.854897Z"},"content_sha256":"f167509725957509db86c8909df530a1243e85866f3993eae312208c7cd392da","schema_version":"1.0","event_id":"sha256:f167509725957509db86c8909df530a1243e85866f3993eae312208c7cd392da"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/ERSGDALHCGLPBMAC5S3KUTKQV6/bundle.json","state_url":"https://pith.science/pith/ERSGDALHCGLPBMAC5S3KUTKQV6/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/ERSGDALHCGLPBMAC5S3KUTKQV6/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":"2026-05-25T20:22:02Z","links":{"resolver":"https://pith.science/pith/ERSGDALHCGLPBMAC5S3KUTKQV6","bundle":"https://pith.science/pith/ERSGDALHCGLPBMAC5S3KUTKQV6/bundle.json","state":"https://pith.science/pith/ERSGDALHCGLPBMAC5S3KUTKQV6/state.json","well_known_bundle":"https://pith.science/.well-known/pith/ERSGDALHCGLPBMAC5S3KUTKQV6/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2010:ERSGDALHCGLPBMAC5S3KUTKQV6","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":"23b341e6b0715a571ec3a7f94016010db5128179d4fbe62f02b7a06da86dfbe4","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2010-06-18T16:04:54Z","title_canon_sha256":"a3306b00a353e6b4314e7585ecab3e9a31169ac4b3c57963849c8eb8fc588f37"},"schema_version":"1.0","source":{"id":"1006.3738","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1006.3738","created_at":"2026-05-18T02:06:44Z"},{"alias_kind":"arxiv_version","alias_value":"1006.3738v1","created_at":"2026-05-18T02:06:44Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1006.3738","created_at":"2026-05-18T02:06:44Z"},{"alias_kind":"pith_short_12","alias_value":"ERSGDALHCGLP","created_at":"2026-05-18T12:26:06Z"},{"alias_kind":"pith_short_16","alias_value":"ERSGDALHCGLPBMAC","created_at":"2026-05-18T12:26:06Z"},{"alias_kind":"pith_short_8","alias_value":"ERSGDALH","created_at":"2026-05-18T12:26:06Z"}],"graph_snapshots":[{"event_id":"sha256:f167509725957509db86c8909df530a1243e85866f3993eae312208c7cd392da","target":"graph","created_at":"2026-05-18T02:06:44Z","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 present a three-dimensional simulation of the corona of an FK Com-type rapidly rotating G giant using a magnetohydrodynamic model that was originally developed for the solar corona in order to capture the more realistic, non-potential coronal structure. We drive the simulation with surface maps for the radial magnetic field obtained from a stellar dynamo model of the FK Com system. This enables us to obtain the coronal structure for different field topologies representing different periods of time. We find that the corona of such an FK Com-like star, including the large scale coronal loops,","authors_text":"D. Elstner, H. Korhonen, J.J. Drake, O. Cohen, T.I. Gombosi, V.L. Kashyap","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2010-06-18T16:04:54Z","title":"Magnetic Structure of Rapidly Rotating FK Comae-Type Coronae"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1006.3738","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":"sha256:93e0eecfda26d9b4c7700a4b402b1daececd22cb3f9cf8ad9fe2526557255f88","target":"record","created_at":"2026-05-18T02:06:44Z","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":"23b341e6b0715a571ec3a7f94016010db5128179d4fbe62f02b7a06da86dfbe4","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2010-06-18T16:04:54Z","title_canon_sha256":"a3306b00a353e6b4314e7585ecab3e9a31169ac4b3c57963849c8eb8fc588f37"},"schema_version":"1.0","source":{"id":"1006.3738","kind":"arxiv","version":1}},"canonical_sha256":"24646181671196f0b002ecb6aa4d50af92d5ced86233fcf5a49734dbe38203a7","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"24646181671196f0b002ecb6aa4d50af92d5ced86233fcf5a49734dbe38203a7","first_computed_at":"2026-05-18T02:06:44.479878Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T02:06:44.479878Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"6HH2GAC6KsPOdTaQpXMVw7rc4H8e+l6iqRRrrpyDsnbJiiRroeFDFKA4FJl+hxBR3sCkx77jU6zyOeirZCrbAQ==","signature_status":"signed_v1","signed_at":"2026-05-18T02:06:44.480242Z","signed_message":"canonical_sha256_bytes"},"source_id":"1006.3738","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:93e0eecfda26d9b4c7700a4b402b1daececd22cb3f9cf8ad9fe2526557255f88","sha256:f167509725957509db86c8909df530a1243e85866f3993eae312208c7cd392da"],"state_sha256":"25047eaf40c5fe0d933a5f17f4829c20963c3f9a88b9e4ab822c702b27860720"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"EuWYdcR3qwmen7+ujVhqj842jPiEpxLhpBPhR44qw6VVKkiglm6yHkC3TOP8tstTxHs0L3Pq+Xv+mbVx+K5uBg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-25T20:22:02.858260Z","bundle_sha256":"5c39a74be5049db2e2987995dba819b9455cf20497e30824f26d5fbb67e0c132"}}