{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:P3VOS7J2R4T2AZRSMALMVSZ2BZ","short_pith_number":"pith:P3VOS7J2","schema_version":"1.0","canonical_sha256":"7eeae97d3a8f27a066326016cacb3a0e4c9864fa4dc102996f6b00a22e3f61ff","source":{"kind":"arxiv","id":"1504.02940","version":3},"attestation_state":"computed","paper":{"title":"Evolution of Kinetic and Magnetic Energy in Intra Cluster Media","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"physics.plasm-ph","authors_text":"Dongho Park, Kiwan Park","submitted_at":"2015-04-12T07:23:59Z","abstract_excerpt":"Intra Cluster Media (ICMs) located at galaxy clusters is in the state of hot, tenuous, magnetized, and highly ionized X-ray emitting plasmas. This overall collisionless, viscous, and conductive magnetohydrodynamic (MHD) turbulence in ICM is simulated using hyper and physical magnetic diffusivity. The results show that fluctuating random plasma motion amplifies the magnetic field, which cascades toward the diffusivity scale passing through the viscous scale. The kinetic eddies in the subviscous scale are driven and constrained by the magnetic tension which finally gets balanced with the highly "},"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":"1504.02940","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2015-04-12T07:23:59Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"9a182c51ae5f8bb89b40ebd3160dd4395f09d20121e18ef71b0b70c4308faaab","abstract_canon_sha256":"e5c0e6ce705c977cdb5c79163a0767a038f3cb122ab48bc143dbf96c6a595f97"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:37:01.562074Z","signature_b64":"1WorMYPH+mkxAHMQq7h20nqGB6EQwvDUGYKahphEvqQgHnxrfDIMiDf2XdDeSBv+O5xRCRl8Ru39wz6LW+oPCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7eeae97d3a8f27a066326016cacb3a0e4c9864fa4dc102996f6b00a22e3f61ff","last_reissued_at":"2026-05-18T01:37:01.561501Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:37:01.561501Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Evolution of Kinetic and Magnetic Energy in Intra Cluster Media","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"physics.plasm-ph","authors_text":"Dongho Park, Kiwan Park","submitted_at":"2015-04-12T07:23:59Z","abstract_excerpt":"Intra Cluster Media (ICMs) located at galaxy clusters is in the state of hot, tenuous, magnetized, and highly ionized X-ray emitting plasmas. This overall collisionless, viscous, and conductive magnetohydrodynamic (MHD) turbulence in ICM is simulated using hyper and physical magnetic diffusivity. The results show that fluctuating random plasma motion amplifies the magnetic field, which cascades toward the diffusivity scale passing through the viscous scale. The kinetic eddies in the subviscous scale are driven and constrained by the magnetic tension which finally gets balanced with the highly "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1504.02940","kind":"arxiv","version":3},"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":"1504.02940","created_at":"2026-05-18T01:37:01.561584+00:00"},{"alias_kind":"arxiv_version","alias_value":"1504.02940v3","created_at":"2026-05-18T01:37:01.561584+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1504.02940","created_at":"2026-05-18T01:37:01.561584+00:00"},{"alias_kind":"pith_short_12","alias_value":"P3VOS7J2R4T2","created_at":"2026-05-18T12:29:34.919912+00:00"},{"alias_kind":"pith_short_16","alias_value":"P3VOS7J2R4T2AZRS","created_at":"2026-05-18T12:29:34.919912+00:00"},{"alias_kind":"pith_short_8","alias_value":"P3VOS7J2","created_at":"2026-05-18T12:29:34.919912+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/P3VOS7J2R4T2AZRSMALMVSZ2BZ","json":"https://pith.science/pith/P3VOS7J2R4T2AZRSMALMVSZ2BZ.json","graph_json":"https://pith.science/api/pith-number/P3VOS7J2R4T2AZRSMALMVSZ2BZ/graph.json","events_json":"https://pith.science/api/pith-number/P3VOS7J2R4T2AZRSMALMVSZ2BZ/events.json","paper":"https://pith.science/paper/P3VOS7J2"},"agent_actions":{"view_html":"https://pith.science/pith/P3VOS7J2R4T2AZRSMALMVSZ2BZ","download_json":"https://pith.science/pith/P3VOS7J2R4T2AZRSMALMVSZ2BZ.json","view_paper":"https://pith.science/paper/P3VOS7J2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1504.02940&json=true","fetch_graph":"https://pith.science/api/pith-number/P3VOS7J2R4T2AZRSMALMVSZ2BZ/graph.json","fetch_events":"https://pith.science/api/pith-number/P3VOS7J2R4T2AZRSMALMVSZ2BZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/P3VOS7J2R4T2AZRSMALMVSZ2BZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/P3VOS7J2R4T2AZRSMALMVSZ2BZ/action/storage_attestation","attest_author":"https://pith.science/pith/P3VOS7J2R4T2AZRSMALMVSZ2BZ/action/author_attestation","sign_citation":"https://pith.science/pith/P3VOS7J2R4T2AZRSMALMVSZ2BZ/action/citation_signature","submit_replication":"https://pith.science/pith/P3VOS7J2R4T2AZRSMALMVSZ2BZ/action/replication_record"}},"created_at":"2026-05-18T01:37:01.561584+00:00","updated_at":"2026-05-18T01:37:01.561584+00:00"}