{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:4JUFDPFSCBUZIYY63TPOQ4JN2V","short_pith_number":"pith:4JUFDPFS","schema_version":"1.0","canonical_sha256":"e26851bcb2106994631edcdee8712dd55d882cf2256a69641926fe171a36b728","source":{"kind":"arxiv","id":"2006.03285","version":1},"attestation_state":"computed","paper":{"title":"On the Scaling Properties of Magnetic Field Fluctuations Through the Inner Heliosphere","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["physics.plasm-ph"],"primary_cat":"physics.space-ph","authors_text":"Anna Milillo, Giuseppe Consolini, Maria Federica Marcucci, Monica Laurenza, Stuart D. Bale, Tommaso Alberti, Vincenzo Carbone","submitted_at":"2020-06-05T08:07:55Z","abstract_excerpt":"Although the interplanetary magnetic field variability has been extensively investigated in situ by means of data coming from several space missions, the newly launched missions providing high-resolution measures and approaching the Sun, offer the possibility to study the multiscale variability in the innermost solar system. Here by means of the Parker Solar Probe measurements we investigate the scaling properties of solar wind magnetic field fluctuations at different heliocentric distances. The results show a clear transition at distances close to say 0.4 au. Closer to the Sun fluctuations sh"},"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":"2006.03285","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"physics.space-ph","submitted_at":"2020-06-05T08:07:55Z","cross_cats_sorted":["physics.plasm-ph"],"title_canon_sha256":"0ad2a4e05f793d72c3e5e55d09813014fec92323bb1b3918479373cbaf76bd17","abstract_canon_sha256":"f925171b24d1580f52b605f2b041658c6fcf07224fa2792fe45e5e77065805c8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:44:13.357012Z","signature_b64":"zI1i4BXKP2ki3TYgTOlWZmvaGKRozGfg5K+bJ41iL/qWZG4SWErrGm7zms5DwzEeTgIsVXi5RRTuB2VupQZSDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e26851bcb2106994631edcdee8712dd55d882cf2256a69641926fe171a36b728","last_reissued_at":"2026-07-05T01:44:13.356540Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:44:13.356540Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On the Scaling Properties of Magnetic Field Fluctuations Through the Inner Heliosphere","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["physics.plasm-ph"],"primary_cat":"physics.space-ph","authors_text":"Anna Milillo, Giuseppe Consolini, Maria Federica Marcucci, Monica Laurenza, Stuart D. Bale, Tommaso Alberti, Vincenzo Carbone","submitted_at":"2020-06-05T08:07:55Z","abstract_excerpt":"Although the interplanetary magnetic field variability has been extensively investigated in situ by means of data coming from several space missions, the newly launched missions providing high-resolution measures and approaching the Sun, offer the possibility to study the multiscale variability in the innermost solar system. Here by means of the Parker Solar Probe measurements we investigate the scaling properties of solar wind magnetic field fluctuations at different heliocentric distances. The results show a clear transition at distances close to say 0.4 au. Closer to the Sun fluctuations sh"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2006.03285","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/2006.03285/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":"2006.03285","created_at":"2026-07-05T01:44:13.356599+00:00"},{"alias_kind":"arxiv_version","alias_value":"2006.03285v1","created_at":"2026-07-05T01:44:13.356599+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2006.03285","created_at":"2026-07-05T01:44:13.356599+00:00"},{"alias_kind":"pith_short_12","alias_value":"4JUFDPFSCBUZ","created_at":"2026-07-05T01:44:13.356599+00:00"},{"alias_kind":"pith_short_16","alias_value":"4JUFDPFSCBUZIYY6","created_at":"2026-07-05T01:44:13.356599+00:00"},{"alias_kind":"pith_short_8","alias_value":"4JUFDPFS","created_at":"2026-07-05T01:44:13.356599+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/4JUFDPFSCBUZIYY63TPOQ4JN2V","json":"https://pith.science/pith/4JUFDPFSCBUZIYY63TPOQ4JN2V.json","graph_json":"https://pith.science/api/pith-number/4JUFDPFSCBUZIYY63TPOQ4JN2V/graph.json","events_json":"https://pith.science/api/pith-number/4JUFDPFSCBUZIYY63TPOQ4JN2V/events.json","paper":"https://pith.science/paper/4JUFDPFS"},"agent_actions":{"view_html":"https://pith.science/pith/4JUFDPFSCBUZIYY63TPOQ4JN2V","download_json":"https://pith.science/pith/4JUFDPFSCBUZIYY63TPOQ4JN2V.json","view_paper":"https://pith.science/paper/4JUFDPFS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2006.03285&json=true","fetch_graph":"https://pith.science/api/pith-number/4JUFDPFSCBUZIYY63TPOQ4JN2V/graph.json","fetch_events":"https://pith.science/api/pith-number/4JUFDPFSCBUZIYY63TPOQ4JN2V/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4JUFDPFSCBUZIYY63TPOQ4JN2V/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4JUFDPFSCBUZIYY63TPOQ4JN2V/action/storage_attestation","attest_author":"https://pith.science/pith/4JUFDPFSCBUZIYY63TPOQ4JN2V/action/author_attestation","sign_citation":"https://pith.science/pith/4JUFDPFSCBUZIYY63TPOQ4JN2V/action/citation_signature","submit_replication":"https://pith.science/pith/4JUFDPFSCBUZIYY63TPOQ4JN2V/action/replication_record"}},"created_at":"2026-07-05T01:44:13.356599+00:00","updated_at":"2026-07-05T01:44:13.356599+00:00"}