{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:2DJVOWX4ZK3PMNWMC4SWICEEWE","short_pith_number":"pith:2DJVOWX4","schema_version":"1.0","canonical_sha256":"d0d3575afccab6f636cc1725640884b11185aa24c4e4b86b6f759dcb342ee1fc","source":{"kind":"arxiv","id":"2209.05037","version":1},"attestation_state":"computed","paper":{"title":"In-situ Observation Of Alfv'en Waves In Icme Shock-Sheath Indicates Existence Of Alfv'enic Turbulence","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["physics.space-ph"],"primary_cat":"astro-ph.SR","authors_text":"Anil Raghav, Kalpesh Ghag, Omkar Dhamane, Prathmesh Tari, Utsav Panchal, Zubair Shaikh","submitted_at":"2022-09-12T06:22:14Z","abstract_excerpt":"The dynamic evolution of coronal mass ejection (CME) in interplanetary space generates highly turbulent, compressed, and heated shock-sheath. This region furnishes a unique environment to study the turbulent fluctuations at the small scales and serve an opportunity for unfolding the physical mechanisms by which the turbulence is dissipated and plasma is heated. How does the turbulence in the magnetized plasma control the energy transport process in space and astrophysical plasmas is an attractive and challenging open problem of the 21st century. For this, the literature discusses three types o"},"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":"2209.05037","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.SR","submitted_at":"2022-09-12T06:22:14Z","cross_cats_sorted":["physics.space-ph"],"title_canon_sha256":"b3bf34c47f22bb8efc60b7a160709abff7df253180817adc371f4beaafeb0dac","abstract_canon_sha256":"b7755216fa120fe96192fb26c2b5b15e5072758a91c034d3e774670f8638bdec"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:56:26.008808Z","signature_b64":"iy0pPQiwwPmO9tK9yuDyr6qvF3b95MvmK+7uV2rsjnP3Dtne0pYfwA1kCC01zmCo2orRAhQsxOJPUUveC6VLDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d0d3575afccab6f636cc1725640884b11185aa24c4e4b86b6f759dcb342ee1fc","last_reissued_at":"2026-07-05T04:56:26.008382Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:56:26.008382Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"In-situ Observation Of Alfv'en Waves In Icme Shock-Sheath Indicates Existence Of Alfv'enic Turbulence","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["physics.space-ph"],"primary_cat":"astro-ph.SR","authors_text":"Anil Raghav, Kalpesh Ghag, Omkar Dhamane, Prathmesh Tari, Utsav Panchal, Zubair Shaikh","submitted_at":"2022-09-12T06:22:14Z","abstract_excerpt":"The dynamic evolution of coronal mass ejection (CME) in interplanetary space generates highly turbulent, compressed, and heated shock-sheath. This region furnishes a unique environment to study the turbulent fluctuations at the small scales and serve an opportunity for unfolding the physical mechanisms by which the turbulence is dissipated and plasma is heated. How does the turbulence in the magnetized plasma control the energy transport process in space and astrophysical plasmas is an attractive and challenging open problem of the 21st century. For this, the literature discusses three types o"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2209.05037","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2209.05037/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2209.05037","created_at":"2026-07-05T04:56:26.008438+00:00"},{"alias_kind":"arxiv_version","alias_value":"2209.05037v1","created_at":"2026-07-05T04:56:26.008438+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2209.05037","created_at":"2026-07-05T04:56:26.008438+00:00"},{"alias_kind":"pith_short_12","alias_value":"2DJVOWX4ZK3P","created_at":"2026-07-05T04:56:26.008438+00:00"},{"alias_kind":"pith_short_16","alias_value":"2DJVOWX4ZK3PMNWM","created_at":"2026-07-05T04:56:26.008438+00:00"},{"alias_kind":"pith_short_8","alias_value":"2DJVOWX4","created_at":"2026-07-05T04:56:26.008438+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/2DJVOWX4ZK3PMNWMC4SWICEEWE","json":"https://pith.science/pith/2DJVOWX4ZK3PMNWMC4SWICEEWE.json","graph_json":"https://pith.science/api/pith-number/2DJVOWX4ZK3PMNWMC4SWICEEWE/graph.json","events_json":"https://pith.science/api/pith-number/2DJVOWX4ZK3PMNWMC4SWICEEWE/events.json","paper":"https://pith.science/paper/2DJVOWX4"},"agent_actions":{"view_html":"https://pith.science/pith/2DJVOWX4ZK3PMNWMC4SWICEEWE","download_json":"https://pith.science/pith/2DJVOWX4ZK3PMNWMC4SWICEEWE.json","view_paper":"https://pith.science/paper/2DJVOWX4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2209.05037&json=true","fetch_graph":"https://pith.science/api/pith-number/2DJVOWX4ZK3PMNWMC4SWICEEWE/graph.json","fetch_events":"https://pith.science/api/pith-number/2DJVOWX4ZK3PMNWMC4SWICEEWE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2DJVOWX4ZK3PMNWMC4SWICEEWE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2DJVOWX4ZK3PMNWMC4SWICEEWE/action/storage_attestation","attest_author":"https://pith.science/pith/2DJVOWX4ZK3PMNWMC4SWICEEWE/action/author_attestation","sign_citation":"https://pith.science/pith/2DJVOWX4ZK3PMNWMC4SWICEEWE/action/citation_signature","submit_replication":"https://pith.science/pith/2DJVOWX4ZK3PMNWMC4SWICEEWE/action/replication_record"}},"created_at":"2026-07-05T04:56:26.008438+00:00","updated_at":"2026-07-05T04:56:26.008438+00:00"}