{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:JGK2ZH7MAFMYVCUVKTEF3H5XWP","short_pith_number":"pith:JGK2ZH7M","schema_version":"1.0","canonical_sha256":"4995ac9fec01598a8a9554c85d9fb7b3e2da56a9f8c5a0b1e764635425c6eec4","source":{"kind":"arxiv","id":"1610.03789","version":1},"attestation_state":"computed","paper":{"title":"Suprathermal electron distributions in the solar transition region","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.space-ph"],"primary_cat":"astro-ph.SR","authors_text":"C. Vocks, E. Dzifcakova, G. Mann","submitted_at":"2016-10-12T17:02:25Z","abstract_excerpt":"Suprathermal tails are a common feature of solar wind electron velocity distributions, and are expected in the solar corona. From the corona, suprathermal electrons can propagate through the steep temperature gradient of the transition region towards the chromosphere, and lead to non-Maxwellian electron velocity distribution functions (VDFs) with pronounced suprathermal tails. We calculate the evolution of a coronal electron distribution through the transition region in order to quantify the suprathermal electron population there. A kinetic model for electrons is used which is based on solving"},"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":"1610.03789","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-10-12T17:02:25Z","cross_cats_sorted":["physics.space-ph"],"title_canon_sha256":"81b5ee7da63b6d7ac2455e8c7d3bc290de27a9cc0c8e1327e99b961e41fe2803","abstract_canon_sha256":"acc3cdcb83ec8557f7463713c514151d095e6e231b422dab7f59f850c7ae5b6a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:02:29.224945Z","signature_b64":"hxAyGV2If413r1vlNtEoNzWM5HoHx9vfo0lljX+nH6gDPf54t2O2/BK7T4+thxIoItnVvjDmoFrVG4dEcwFWCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4995ac9fec01598a8a9554c85d9fb7b3e2da56a9f8c5a0b1e764635425c6eec4","last_reissued_at":"2026-05-18T01:02:29.224265Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:02:29.224265Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Suprathermal electron distributions in the solar transition region","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.space-ph"],"primary_cat":"astro-ph.SR","authors_text":"C. Vocks, E. Dzifcakova, G. Mann","submitted_at":"2016-10-12T17:02:25Z","abstract_excerpt":"Suprathermal tails are a common feature of solar wind electron velocity distributions, and are expected in the solar corona. From the corona, suprathermal electrons can propagate through the steep temperature gradient of the transition region towards the chromosphere, and lead to non-Maxwellian electron velocity distribution functions (VDFs) with pronounced suprathermal tails. We calculate the evolution of a coronal electron distribution through the transition region in order to quantify the suprathermal electron population there. A kinetic model for electrons is used which is based on solving"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1610.03789","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":"1610.03789","created_at":"2026-05-18T01:02:29.224385+00:00"},{"alias_kind":"arxiv_version","alias_value":"1610.03789v1","created_at":"2026-05-18T01:02:29.224385+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1610.03789","created_at":"2026-05-18T01:02:29.224385+00:00"},{"alias_kind":"pith_short_12","alias_value":"JGK2ZH7MAFMY","created_at":"2026-05-18T12:30:25.849896+00:00"},{"alias_kind":"pith_short_16","alias_value":"JGK2ZH7MAFMYVCUV","created_at":"2026-05-18T12:30:25.849896+00:00"},{"alias_kind":"pith_short_8","alias_value":"JGK2ZH7M","created_at":"2026-05-18T12:30:25.849896+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/JGK2ZH7MAFMYVCUVKTEF3H5XWP","json":"https://pith.science/pith/JGK2ZH7MAFMYVCUVKTEF3H5XWP.json","graph_json":"https://pith.science/api/pith-number/JGK2ZH7MAFMYVCUVKTEF3H5XWP/graph.json","events_json":"https://pith.science/api/pith-number/JGK2ZH7MAFMYVCUVKTEF3H5XWP/events.json","paper":"https://pith.science/paper/JGK2ZH7M"},"agent_actions":{"view_html":"https://pith.science/pith/JGK2ZH7MAFMYVCUVKTEF3H5XWP","download_json":"https://pith.science/pith/JGK2ZH7MAFMYVCUVKTEF3H5XWP.json","view_paper":"https://pith.science/paper/JGK2ZH7M","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1610.03789&json=true","fetch_graph":"https://pith.science/api/pith-number/JGK2ZH7MAFMYVCUVKTEF3H5XWP/graph.json","fetch_events":"https://pith.science/api/pith-number/JGK2ZH7MAFMYVCUVKTEF3H5XWP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JGK2ZH7MAFMYVCUVKTEF3H5XWP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JGK2ZH7MAFMYVCUVKTEF3H5XWP/action/storage_attestation","attest_author":"https://pith.science/pith/JGK2ZH7MAFMYVCUVKTEF3H5XWP/action/author_attestation","sign_citation":"https://pith.science/pith/JGK2ZH7MAFMYVCUVKTEF3H5XWP/action/citation_signature","submit_replication":"https://pith.science/pith/JGK2ZH7MAFMYVCUVKTEF3H5XWP/action/replication_record"}},"created_at":"2026-05-18T01:02:29.224385+00:00","updated_at":"2026-05-18T01:02:29.224385+00:00"}