{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:S3ES2NXF63AKNOBHBQWHQZBTVR","short_pith_number":"pith:S3ES2NXF","schema_version":"1.0","canonical_sha256":"96c92d36e5f6c0a6b8270c2c786433ac7d046ddd83be5fdb2f148912d1990240","source":{"kind":"arxiv","id":"1109.4558","version":1},"attestation_state":"computed","paper":{"title":"Simulating Gyrokinetic Microinstabilities in Stellarator Geometry with GS2","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"physics.plasm-ph","authors_text":"D. R. Mikkelsen, E. A. Belli, G. Rewoldt, G. W. Hammett, J. A. Baumgaertel, P. Xanthopoulos, W. Dorland, W. Guttenfelder, W. M. Tang","submitted_at":"2011-09-21T15:35:06Z","abstract_excerpt":"The nonlinear gyrokinetic code GS2 has been extended to treat non-axisymmetric stellarator geometry. Electromagnetic perturbations and multiple trapped particle regions are allowed. Here, linear, collisionless, electrostatic simulations of the quasi-axisymmetric, three-field period National Compact Stellarator Experiment (NCSX) design QAS3-C82 have been successfully benchmarked against the eigenvalue code FULL. Quantitatively, the linear stability calculations of GS2 and FULL agree to within ~10%."},"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":"1109.4558","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2011-09-21T15:35:06Z","cross_cats_sorted":[],"title_canon_sha256":"438729d805bf07e2a91c12eb04a7d0aa44691f4887b29f58962fa0c879599de8","abstract_canon_sha256":"24b64ad0831b3aa4db121963cecf9b32dec2dd544f15cbac41d7203aa2d29a53"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:42:34.079049Z","signature_b64":"zHPs5KfWj4XHS8+aPMBytEPMQCGL3FvnufBUrJE+Yv1pW7iimGRUQgOmxCLTn3JKkeOtylnSv5fNNjKmawPbCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"96c92d36e5f6c0a6b8270c2c786433ac7d046ddd83be5fdb2f148912d1990240","last_reissued_at":"2026-05-18T03:42:34.078451Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:42:34.078451Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Simulating Gyrokinetic Microinstabilities in Stellarator Geometry with GS2","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"physics.plasm-ph","authors_text":"D. R. Mikkelsen, E. A. Belli, G. Rewoldt, G. W. Hammett, J. A. Baumgaertel, P. Xanthopoulos, W. Dorland, W. Guttenfelder, W. M. Tang","submitted_at":"2011-09-21T15:35:06Z","abstract_excerpt":"The nonlinear gyrokinetic code GS2 has been extended to treat non-axisymmetric stellarator geometry. Electromagnetic perturbations and multiple trapped particle regions are allowed. Here, linear, collisionless, electrostatic simulations of the quasi-axisymmetric, three-field period National Compact Stellarator Experiment (NCSX) design QAS3-C82 have been successfully benchmarked against the eigenvalue code FULL. Quantitatively, the linear stability calculations of GS2 and FULL agree to within ~10%."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1109.4558","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":"1109.4558","created_at":"2026-05-18T03:42:34.078510+00:00"},{"alias_kind":"arxiv_version","alias_value":"1109.4558v1","created_at":"2026-05-18T03:42:34.078510+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1109.4558","created_at":"2026-05-18T03:42:34.078510+00:00"},{"alias_kind":"pith_short_12","alias_value":"S3ES2NXF63AK","created_at":"2026-05-18T12:26:41.206345+00:00"},{"alias_kind":"pith_short_16","alias_value":"S3ES2NXF63AKNOBH","created_at":"2026-05-18T12:26:41.206345+00:00"},{"alias_kind":"pith_short_8","alias_value":"S3ES2NXF","created_at":"2026-05-18T12:26:41.206345+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/S3ES2NXF63AKNOBHBQWHQZBTVR","json":"https://pith.science/pith/S3ES2NXF63AKNOBHBQWHQZBTVR.json","graph_json":"https://pith.science/api/pith-number/S3ES2NXF63AKNOBHBQWHQZBTVR/graph.json","events_json":"https://pith.science/api/pith-number/S3ES2NXF63AKNOBHBQWHQZBTVR/events.json","paper":"https://pith.science/paper/S3ES2NXF"},"agent_actions":{"view_html":"https://pith.science/pith/S3ES2NXF63AKNOBHBQWHQZBTVR","download_json":"https://pith.science/pith/S3ES2NXF63AKNOBHBQWHQZBTVR.json","view_paper":"https://pith.science/paper/S3ES2NXF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1109.4558&json=true","fetch_graph":"https://pith.science/api/pith-number/S3ES2NXF63AKNOBHBQWHQZBTVR/graph.json","fetch_events":"https://pith.science/api/pith-number/S3ES2NXF63AKNOBHBQWHQZBTVR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/S3ES2NXF63AKNOBHBQWHQZBTVR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/S3ES2NXF63AKNOBHBQWHQZBTVR/action/storage_attestation","attest_author":"https://pith.science/pith/S3ES2NXF63AKNOBHBQWHQZBTVR/action/author_attestation","sign_citation":"https://pith.science/pith/S3ES2NXF63AKNOBHBQWHQZBTVR/action/citation_signature","submit_replication":"https://pith.science/pith/S3ES2NXF63AKNOBHBQWHQZBTVR/action/replication_record"}},"created_at":"2026-05-18T03:42:34.078510+00:00","updated_at":"2026-05-18T03:42:34.078510+00:00"}