{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2018:GEWWWHPTYC6CZFATP5RQH2OYED","short_pith_number":"pith:GEWWWHPT","canonical_record":{"source":{"id":"1802.10506","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2018-02-28T16:14:13Z","cross_cats_sorted":["physics.plasm-ph"],"title_canon_sha256":"ec1c6d74389029fce83bd1c045875a2505994a538f3f9f924c23f6ff80a83b2d","abstract_canon_sha256":"4f069d17b9f75d20664d0dc6459a6bc8768af3b24541013d4a463721a881e0b6"},"schema_version":"1.0"},"canonical_sha256":"312d6b1df3c0bc2c94137f6303e9d820f422b9545e5fc309103dc824b8d38c44","source":{"kind":"arxiv","id":"1802.10506","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1802.10506","created_at":"2026-05-18T00:04:30Z"},{"alias_kind":"arxiv_version","alias_value":"1802.10506v1","created_at":"2026-05-18T00:04:30Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1802.10506","created_at":"2026-05-18T00:04:30Z"},{"alias_kind":"pith_short_12","alias_value":"GEWWWHPTYC6C","created_at":"2026-05-18T12:32:25Z"},{"alias_kind":"pith_short_16","alias_value":"GEWWWHPTYC6CZFAT","created_at":"2026-05-18T12:32:25Z"},{"alias_kind":"pith_short_8","alias_value":"GEWWWHPT","created_at":"2026-05-18T12:32:25Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2018:GEWWWHPTYC6CZFATP5RQH2OYED","target":"record","payload":{"canonical_record":{"source":{"id":"1802.10506","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2018-02-28T16:14:13Z","cross_cats_sorted":["physics.plasm-ph"],"title_canon_sha256":"ec1c6d74389029fce83bd1c045875a2505994a538f3f9f924c23f6ff80a83b2d","abstract_canon_sha256":"4f069d17b9f75d20664d0dc6459a6bc8768af3b24541013d4a463721a881e0b6"},"schema_version":"1.0"},"canonical_sha256":"312d6b1df3c0bc2c94137f6303e9d820f422b9545e5fc309103dc824b8d38c44","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:04:30.279839Z","signature_b64":"REEkJolpr6LYOkZ1pMJBCeFS8sW1MGhSBHdHJrTmFO0c4PCzCaoQDWPTaRco/c+K4Z9xaQShrVA9oEFGSidyBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"312d6b1df3c0bc2c94137f6303e9d820f422b9545e5fc309103dc824b8d38c44","last_reissued_at":"2026-05-18T00:04:30.279423Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:04:30.279423Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1802.10506","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":"2026-05-18T00:04:30Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"mQGENc1PkOH+9eq1/Z413+65S0HVV6K65aWqL/nzLXDh9JwO4tP7WdYtzK1upFaW2FbOxMynFkcYSaTSnQjCBQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-05T08:42:30.457410Z"},"content_sha256":"3184644df6f6300722b6b13d82c3b008170379d4dbc17361145e2af6c45f5d02","schema_version":"1.0","event_id":"sha256:3184644df6f6300722b6b13d82c3b008170379d4dbc17361145e2af6c45f5d02"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2018:GEWWWHPTYC6CZFATP5RQH2OYED","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Behavior of thin disk crystalline morphology in the presence of corrections to ideal magnetohydrodynamics","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.plasm-ph"],"primary_cat":"astro-ph.SR","authors_text":"Giovanni Montani, Mariachiara Rizzo, Nakia Carlevaro","submitted_at":"2018-02-28T16:14:13Z","abstract_excerpt":"We analyze an axisymmetric magnetohydrodynamics configuration, describing the morphology of a purely differentially rotating thin plasma disk, in which linear and non-linear perturbations are triggered associated with microscopic magnetic structures. We study the evolution of the non-stationary correction in the limit in which the co-rotation condition (i.e., the dependence of the disk angular velocity on the magnetic flux function) is preserved and the poloidal velocity components are neglected. The main feature we address here is the influence of ideal (finite electron inertia) and collision"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1802.10506","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":"2026-05-18T00:04:30Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"pHZAZPEwkJBSwh5ka8DdGus7zIIBGnnTPXqw3y5Fsd+faxBIy3g3k65LzDF+zYuZmKXw/mjJYiSOYkikmlC8DQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-05T08:42:30.457760Z"},"content_sha256":"b0d92004caf155303774367cf4a6920b7b10449b0a3978bdf59312b4fcc5f974","schema_version":"1.0","event_id":"sha256:b0d92004caf155303774367cf4a6920b7b10449b0a3978bdf59312b4fcc5f974"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/GEWWWHPTYC6CZFATP5RQH2OYED/bundle.json","state_url":"https://pith.science/pith/GEWWWHPTYC6CZFATP5RQH2OYED/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/GEWWWHPTYC6CZFATP5RQH2OYED/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":"2026-06-05T08:42:30Z","links":{"resolver":"https://pith.science/pith/GEWWWHPTYC6CZFATP5RQH2OYED","bundle":"https://pith.science/pith/GEWWWHPTYC6CZFATP5RQH2OYED/bundle.json","state":"https://pith.science/pith/GEWWWHPTYC6CZFATP5RQH2OYED/state.json","well_known_bundle":"https://pith.science/.well-known/pith/GEWWWHPTYC6CZFATP5RQH2OYED/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2018:GEWWWHPTYC6CZFATP5RQH2OYED","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":"4f069d17b9f75d20664d0dc6459a6bc8768af3b24541013d4a463721a881e0b6","cross_cats_sorted":["physics.plasm-ph"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2018-02-28T16:14:13Z","title_canon_sha256":"ec1c6d74389029fce83bd1c045875a2505994a538f3f9f924c23f6ff80a83b2d"},"schema_version":"1.0","source":{"id":"1802.10506","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1802.10506","created_at":"2026-05-18T00:04:30Z"},{"alias_kind":"arxiv_version","alias_value":"1802.10506v1","created_at":"2026-05-18T00:04:30Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1802.10506","created_at":"2026-05-18T00:04:30Z"},{"alias_kind":"pith_short_12","alias_value":"GEWWWHPTYC6C","created_at":"2026-05-18T12:32:25Z"},{"alias_kind":"pith_short_16","alias_value":"GEWWWHPTYC6CZFAT","created_at":"2026-05-18T12:32:25Z"},{"alias_kind":"pith_short_8","alias_value":"GEWWWHPT","created_at":"2026-05-18T12:32:25Z"}],"graph_snapshots":[{"event_id":"sha256:b0d92004caf155303774367cf4a6920b7b10449b0a3978bdf59312b4fcc5f974","target":"graph","created_at":"2026-05-18T00:04:30Z","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 analyze an axisymmetric magnetohydrodynamics configuration, describing the morphology of a purely differentially rotating thin plasma disk, in which linear and non-linear perturbations are triggered associated with microscopic magnetic structures. We study the evolution of the non-stationary correction in the limit in which the co-rotation condition (i.e., the dependence of the disk angular velocity on the magnetic flux function) is preserved and the poloidal velocity components are neglected. The main feature we address here is the influence of ideal (finite electron inertia) and collision","authors_text":"Giovanni Montani, Mariachiara Rizzo, Nakia Carlevaro","cross_cats":["physics.plasm-ph"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2018-02-28T16:14:13Z","title":"Behavior of thin disk crystalline morphology in the presence of corrections to ideal magnetohydrodynamics"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1802.10506","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":"sha256:3184644df6f6300722b6b13d82c3b008170379d4dbc17361145e2af6c45f5d02","target":"record","created_at":"2026-05-18T00:04:30Z","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":"4f069d17b9f75d20664d0dc6459a6bc8768af3b24541013d4a463721a881e0b6","cross_cats_sorted":["physics.plasm-ph"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2018-02-28T16:14:13Z","title_canon_sha256":"ec1c6d74389029fce83bd1c045875a2505994a538f3f9f924c23f6ff80a83b2d"},"schema_version":"1.0","source":{"id":"1802.10506","kind":"arxiv","version":1}},"canonical_sha256":"312d6b1df3c0bc2c94137f6303e9d820f422b9545e5fc309103dc824b8d38c44","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"312d6b1df3c0bc2c94137f6303e9d820f422b9545e5fc309103dc824b8d38c44","first_computed_at":"2026-05-18T00:04:30.279423Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:04:30.279423Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"REEkJolpr6LYOkZ1pMJBCeFS8sW1MGhSBHdHJrTmFO0c4PCzCaoQDWPTaRco/c+K4Z9xaQShrVA9oEFGSidyBA==","signature_status":"signed_v1","signed_at":"2026-05-18T00:04:30.279839Z","signed_message":"canonical_sha256_bytes"},"source_id":"1802.10506","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:3184644df6f6300722b6b13d82c3b008170379d4dbc17361145e2af6c45f5d02","sha256:b0d92004caf155303774367cf4a6920b7b10449b0a3978bdf59312b4fcc5f974"],"state_sha256":"3234325c4c0f46ef28652aa92a1c145add3d2de237bea84d9f42da9c598008c3"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"nXMq3LBcfKPTfynjumZ7CTXlw4D2GIBLZo91tWw1g/PYY/OXzZqGQK37t12Azifts9q6wsjtKO9bVn9vh1SZDA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-05T08:42:30.459808Z","bundle_sha256":"15ec0bfcff4eb8addeb5b4b733e8e67fbbd87dbafd5de5611f0485f7bfa8b452"}}