{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:SJKPKXH4CI4E7DB6QODGXCYGDH","short_pith_number":"pith:SJKPKXH4","schema_version":"1.0","canonical_sha256":"9254f55cfc12384f8c3e83866b8b0619c4f71deb681d03116372fb663969d8e2","source":{"kind":"arxiv","id":"1412.6033","version":4},"attestation_state":"computed","paper":{"title":"Observation of Rayleigh-Taylor-Instability Evolution in a Plasma with Magnetic and Viscous Effects","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"physics.plasm-ph","authors_text":"Auna L. Moser, Colin S. Adams, Scott C. Hsu","submitted_at":"2014-12-18T19:54:41Z","abstract_excerpt":"We present time-resolved observations of Rayleigh--Taylor-instability (RTI) evolution at the interface between an unmagnetized plasma jet colliding with a stagnated, magnetized plasma. The observed instability growth time ($\\sim 10$~$\\mu$s) is consistent with the estimated linear RTI growth rate calculated using experimentally inferred values of density ($\\sim 10^{14}$~cm$^{-3}$) and deceleration ($\\sim 10^9$~m/s$^2$). The observed mode wavelength ($\\gtrsim 1$~cm) nearly doubles within a linear growth time. Theoretical estimates of magnetic and viscous stabilization and idealized magnetohydrod"},"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":"1412.6033","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2014-12-18T19:54:41Z","cross_cats_sorted":[],"title_canon_sha256":"c8d6738fdd8bd1899516afa8d3b6d05916715ad5cef35b3ebe3c3abe488e6092","abstract_canon_sha256":"9842cbec89aec391bd5d1c493ebceba34f0ac6ff899e3e5edb8e2a4972ffdbca"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:26:48.999026Z","signature_b64":"eTw87ZSEfzPs8Lc1LgZlurrHc3geqtc7O2y+oD1SFxGLUUsNNh8no8c/YVHkCpGtL/NfAY5Jjjj5tPZISIEgDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9254f55cfc12384f8c3e83866b8b0619c4f71deb681d03116372fb663969d8e2","last_reissued_at":"2026-05-18T01:26:48.998278Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:26:48.998278Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Observation of Rayleigh-Taylor-Instability Evolution in a Plasma with Magnetic and Viscous Effects","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"physics.plasm-ph","authors_text":"Auna L. Moser, Colin S. Adams, Scott C. Hsu","submitted_at":"2014-12-18T19:54:41Z","abstract_excerpt":"We present time-resolved observations of Rayleigh--Taylor-instability (RTI) evolution at the interface between an unmagnetized plasma jet colliding with a stagnated, magnetized plasma. The observed instability growth time ($\\sim 10$~$\\mu$s) is consistent with the estimated linear RTI growth rate calculated using experimentally inferred values of density ($\\sim 10^{14}$~cm$^{-3}$) and deceleration ($\\sim 10^9$~m/s$^2$). The observed mode wavelength ($\\gtrsim 1$~cm) nearly doubles within a linear growth time. Theoretical estimates of magnetic and viscous stabilization and idealized magnetohydrod"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1412.6033","kind":"arxiv","version":4},"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":"1412.6033","created_at":"2026-05-18T01:26:48.998416+00:00"},{"alias_kind":"arxiv_version","alias_value":"1412.6033v4","created_at":"2026-05-18T01:26:48.998416+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1412.6033","created_at":"2026-05-18T01:26:48.998416+00:00"},{"alias_kind":"pith_short_12","alias_value":"SJKPKXH4CI4E","created_at":"2026-05-18T12:28:49.207871+00:00"},{"alias_kind":"pith_short_16","alias_value":"SJKPKXH4CI4E7DB6","created_at":"2026-05-18T12:28:49.207871+00:00"},{"alias_kind":"pith_short_8","alias_value":"SJKPKXH4","created_at":"2026-05-18T12:28:49.207871+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/SJKPKXH4CI4E7DB6QODGXCYGDH","json":"https://pith.science/pith/SJKPKXH4CI4E7DB6QODGXCYGDH.json","graph_json":"https://pith.science/api/pith-number/SJKPKXH4CI4E7DB6QODGXCYGDH/graph.json","events_json":"https://pith.science/api/pith-number/SJKPKXH4CI4E7DB6QODGXCYGDH/events.json","paper":"https://pith.science/paper/SJKPKXH4"},"agent_actions":{"view_html":"https://pith.science/pith/SJKPKXH4CI4E7DB6QODGXCYGDH","download_json":"https://pith.science/pith/SJKPKXH4CI4E7DB6QODGXCYGDH.json","view_paper":"https://pith.science/paper/SJKPKXH4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1412.6033&json=true","fetch_graph":"https://pith.science/api/pith-number/SJKPKXH4CI4E7DB6QODGXCYGDH/graph.json","fetch_events":"https://pith.science/api/pith-number/SJKPKXH4CI4E7DB6QODGXCYGDH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SJKPKXH4CI4E7DB6QODGXCYGDH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SJKPKXH4CI4E7DB6QODGXCYGDH/action/storage_attestation","attest_author":"https://pith.science/pith/SJKPKXH4CI4E7DB6QODGXCYGDH/action/author_attestation","sign_citation":"https://pith.science/pith/SJKPKXH4CI4E7DB6QODGXCYGDH/action/citation_signature","submit_replication":"https://pith.science/pith/SJKPKXH4CI4E7DB6QODGXCYGDH/action/replication_record"}},"created_at":"2026-05-18T01:26:48.998416+00:00","updated_at":"2026-05-18T01:26:48.998416+00:00"}