{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:UZ2FS5KSZVQ2XSVBUKNV2J4UV5","short_pith_number":"pith:UZ2FS5KS","schema_version":"1.0","canonical_sha256":"a674597552cd61abcaa1a29b5d2794af55bb46a3f88304b7cf4ccde6c1a7e274","source":{"kind":"arxiv","id":"1810.01559","version":1},"attestation_state":"computed","paper":{"title":"A new method for probing magnetic field strengths from striations in the interstellar medium","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Aris Tritsis, Christoph Federrath, Konstantinos Tassis, Nicola Schneider","submitted_at":"2018-10-03T01:25:41Z","abstract_excerpt":"Recent studies of the diffuse parts of molecular clouds have revealed the presence of parallel, ordered low-density filaments termed striations. Flows along magnetic field lines, Kelvin-Helmholtz instabilities and hydromagnetic waves are amongst the various formation mechanisms proposed. Through a synergy of observational, numerical and theoretical analysis, previous studies singled out the hydromagnetic waves model as the only one that can account for the observed properties of striations. Based on the predictions of that model, we develop here a method for measuring the temporal evolution of"},"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":"1810.01559","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2018-10-03T01:25:41Z","cross_cats_sorted":[],"title_canon_sha256":"cf2c0208c4a418991f9dd6d4f855cd41ff4a5453eb30a4cee0a34853ee2a6728","abstract_canon_sha256":"a5ba2e9b12718767d178ada28dd924e95aedbac892fa17ab84c0e4c1dfbc5d18"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:03:14.599920Z","signature_b64":"54WUgBNcseNKQDsrao0GJw0V82W8WQPbRN/cqgU4tik7jutibyT6kYScurYmm6VOOBCnYB5mcW0yYilEEuS/Bw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a674597552cd61abcaa1a29b5d2794af55bb46a3f88304b7cf4ccde6c1a7e274","last_reissued_at":"2026-05-18T00:03:14.599223Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:03:14.599223Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A new method for probing magnetic field strengths from striations in the interstellar medium","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Aris Tritsis, Christoph Federrath, Konstantinos Tassis, Nicola Schneider","submitted_at":"2018-10-03T01:25:41Z","abstract_excerpt":"Recent studies of the diffuse parts of molecular clouds have revealed the presence of parallel, ordered low-density filaments termed striations. Flows along magnetic field lines, Kelvin-Helmholtz instabilities and hydromagnetic waves are amongst the various formation mechanisms proposed. Through a synergy of observational, numerical and theoretical analysis, previous studies singled out the hydromagnetic waves model as the only one that can account for the observed properties of striations. Based on the predictions of that model, we develop here a method for measuring the temporal evolution of"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1810.01559","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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1810.01559","created_at":"2026-05-18T00:03:14.599332+00:00"},{"alias_kind":"arxiv_version","alias_value":"1810.01559v1","created_at":"2026-05-18T00:03:14.599332+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1810.01559","created_at":"2026-05-18T00:03:14.599332+00:00"},{"alias_kind":"pith_short_12","alias_value":"UZ2FS5KSZVQ2","created_at":"2026-05-18T12:32:56.356000+00:00"},{"alias_kind":"pith_short_16","alias_value":"UZ2FS5KSZVQ2XSVB","created_at":"2026-05-18T12:32:56.356000+00:00"},{"alias_kind":"pith_short_8","alias_value":"UZ2FS5KS","created_at":"2026-05-18T12:32:56.356000+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/UZ2FS5KSZVQ2XSVBUKNV2J4UV5","json":"https://pith.science/pith/UZ2FS5KSZVQ2XSVBUKNV2J4UV5.json","graph_json":"https://pith.science/api/pith-number/UZ2FS5KSZVQ2XSVBUKNV2J4UV5/graph.json","events_json":"https://pith.science/api/pith-number/UZ2FS5KSZVQ2XSVBUKNV2J4UV5/events.json","paper":"https://pith.science/paper/UZ2FS5KS"},"agent_actions":{"view_html":"https://pith.science/pith/UZ2FS5KSZVQ2XSVBUKNV2J4UV5","download_json":"https://pith.science/pith/UZ2FS5KSZVQ2XSVBUKNV2J4UV5.json","view_paper":"https://pith.science/paper/UZ2FS5KS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1810.01559&json=true","fetch_graph":"https://pith.science/api/pith-number/UZ2FS5KSZVQ2XSVBUKNV2J4UV5/graph.json","fetch_events":"https://pith.science/api/pith-number/UZ2FS5KSZVQ2XSVBUKNV2J4UV5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UZ2FS5KSZVQ2XSVBUKNV2J4UV5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UZ2FS5KSZVQ2XSVBUKNV2J4UV5/action/storage_attestation","attest_author":"https://pith.science/pith/UZ2FS5KSZVQ2XSVBUKNV2J4UV5/action/author_attestation","sign_citation":"https://pith.science/pith/UZ2FS5KSZVQ2XSVBUKNV2J4UV5/action/citation_signature","submit_replication":"https://pith.science/pith/UZ2FS5KSZVQ2XSVBUKNV2J4UV5/action/replication_record"}},"created_at":"2026-05-18T00:03:14.599332+00:00","updated_at":"2026-05-18T00:03:14.599332+00:00"}