{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2017:PQYNQIKG4RKUQOUFTLZDC3B43Y","short_pith_number":"pith:PQYNQIKG","canonical_record":{"source":{"id":"1701.01822","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.space-ph","submitted_at":"2017-01-07T12:10:41Z","cross_cats_sorted":[],"title_canon_sha256":"217bdb4f78ea6d05ad61eba259d395ffbd15920fe2786fae075caee7b8c2590b","abstract_canon_sha256":"44f41a48255f46aab37e4daf71cc7451e84f0cb49e79ea26bf06ad3e4a372c0c"},"schema_version":"1.0"},"canonical_sha256":"7c30d82146e455483a859af2316c3cde2613885945d5ee771cffd644e987eadb","source":{"kind":"arxiv","id":"1701.01822","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1701.01822","created_at":"2026-05-18T00:47:48Z"},{"alias_kind":"arxiv_version","alias_value":"1701.01822v2","created_at":"2026-05-18T00:47:48Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1701.01822","created_at":"2026-05-18T00:47:48Z"},{"alias_kind":"pith_short_12","alias_value":"PQYNQIKG4RKU","created_at":"2026-05-18T12:31:37Z"},{"alias_kind":"pith_short_16","alias_value":"PQYNQIKG4RKUQOUF","created_at":"2026-05-18T12:31:37Z"},{"alias_kind":"pith_short_8","alias_value":"PQYNQIKG","created_at":"2026-05-18T12:31:37Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2017:PQYNQIKG4RKUQOUFTLZDC3B43Y","target":"record","payload":{"canonical_record":{"source":{"id":"1701.01822","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.space-ph","submitted_at":"2017-01-07T12:10:41Z","cross_cats_sorted":[],"title_canon_sha256":"217bdb4f78ea6d05ad61eba259d395ffbd15920fe2786fae075caee7b8c2590b","abstract_canon_sha256":"44f41a48255f46aab37e4daf71cc7451e84f0cb49e79ea26bf06ad3e4a372c0c"},"schema_version":"1.0"},"canonical_sha256":"7c30d82146e455483a859af2316c3cde2613885945d5ee771cffd644e987eadb","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:47:48.573817Z","signature_b64":"RPW+G+uWViBwGi9dyBN2hbrEUi2vMF+f+g1WdsiXrlg1n0R4H3Utv26K3IpewEB9QzM8r7sOKiYg1RyCI7rPDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7c30d82146e455483a859af2316c3cde2613885945d5ee771cffd644e987eadb","last_reissued_at":"2026-05-18T00:47:48.573143Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:47:48.573143Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1701.01822","source_version":2,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T00:47:48Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"J1/FshbQjAamdP8TGNWncnTejTwY4QoMlzTNCs+6RnJ+ozoHLS89XWXFyE+hxXSZuc8aMIYMUYUGJUbD3gXUCw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-25T18:03:33.945046Z"},"content_sha256":"c4fb369d97a30170e172176e15548a965353f8daa55bc60dd59d130fc77858c6","schema_version":"1.0","event_id":"sha256:c4fb369d97a30170e172176e15548a965353f8daa55bc60dd59d130fc77858c6"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2017:PQYNQIKG4RKUQOUFTLZDC3B43Y","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Observations of kinetic-size magnetic holes in the magnetosheath","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"physics.space-ph","authors_text":"A. De Spiegeleer, A. M. Tian, B. L. Giles, C. J. Xiao, C. T. Russell, H. Zhang, J. Liu, J. Vaverka, M. Hamrin, M. M. Wang, M. Nowada, Q. G. Zong, Q. Q. Shi, R. L. Guo, S. C. Bai, S. T. Yao, S. Y. Fu, S. Y. Huang, T. Pitk\\\"anen, W. J. Sun, W. Y. Li, X. F. Ji, X. G. Wang, X. Z. Zhou, Y. C. Xiao, Z. H. Yao, Z. Y. Li, Z. Y. Pu","submitted_at":"2017-01-07T12:10:41Z","abstract_excerpt":"Magnetic holes (MHs), with a scale much greater than \\r{ho}i (proton gyroradius), have been widely reported in various regions of space plasmas. On the other hand, kinetic-size magnetic holes (KSMHs), previously called small size magnetic holes (SSMHs), with a scale of the order of magnitude of or less than \\r{ho}i have only been reported in the Earth's magnetospheric plasma sheet. In this study, we report such KSMHs in the magnetosheath whereby we use measurements from the Magnetospheric Multiscale (MMS) mission, which provides three-dimensional (3D) particle distribution measurements with a "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1701.01822","kind":"arxiv","version":2},"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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T00:47:48Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"m+9X2LPHB0Kh3I7Po1J/Ufd3FyZV906usQawTN63lEV9rSHCMnfQpIe8VxDCqb+Ju+UWaYHki/bnNPDZIQmwAQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-25T18:03:33.945572Z"},"content_sha256":"61e261bba06b5c448b04dbd0ce5b4207441ff51cb9ad7c591854ad23ddcece58","schema_version":"1.0","event_id":"sha256:61e261bba06b5c448b04dbd0ce5b4207441ff51cb9ad7c591854ad23ddcece58"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/PQYNQIKG4RKUQOUFTLZDC3B43Y/bundle.json","state_url":"https://pith.science/pith/PQYNQIKG4RKUQOUFTLZDC3B43Y/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/PQYNQIKG4RKUQOUFTLZDC3B43Y/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-05-25T18:03:33Z","links":{"resolver":"https://pith.science/pith/PQYNQIKG4RKUQOUFTLZDC3B43Y","bundle":"https://pith.science/pith/PQYNQIKG4RKUQOUFTLZDC3B43Y/bundle.json","state":"https://pith.science/pith/PQYNQIKG4RKUQOUFTLZDC3B43Y/state.json","well_known_bundle":"https://pith.science/.well-known/pith/PQYNQIKG4RKUQOUFTLZDC3B43Y/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2017:PQYNQIKG4RKUQOUFTLZDC3B43Y","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"44f41a48255f46aab37e4daf71cc7451e84f0cb49e79ea26bf06ad3e4a372c0c","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.space-ph","submitted_at":"2017-01-07T12:10:41Z","title_canon_sha256":"217bdb4f78ea6d05ad61eba259d395ffbd15920fe2786fae075caee7b8c2590b"},"schema_version":"1.0","source":{"id":"1701.01822","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1701.01822","created_at":"2026-05-18T00:47:48Z"},{"alias_kind":"arxiv_version","alias_value":"1701.01822v2","created_at":"2026-05-18T00:47:48Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1701.01822","created_at":"2026-05-18T00:47:48Z"},{"alias_kind":"pith_short_12","alias_value":"PQYNQIKG4RKU","created_at":"2026-05-18T12:31:37Z"},{"alias_kind":"pith_short_16","alias_value":"PQYNQIKG4RKUQOUF","created_at":"2026-05-18T12:31:37Z"},{"alias_kind":"pith_short_8","alias_value":"PQYNQIKG","created_at":"2026-05-18T12:31:37Z"}],"graph_snapshots":[{"event_id":"sha256:61e261bba06b5c448b04dbd0ce5b4207441ff51cb9ad7c591854ad23ddcece58","target":"graph","created_at":"2026-05-18T00:47:48Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"Magnetic holes (MHs), with a scale much greater than \\r{ho}i (proton gyroradius), have been widely reported in various regions of space plasmas. On the other hand, kinetic-size magnetic holes (KSMHs), previously called small size magnetic holes (SSMHs), with a scale of the order of magnitude of or less than \\r{ho}i have only been reported in the Earth's magnetospheric plasma sheet. In this study, we report such KSMHs in the magnetosheath whereby we use measurements from the Magnetospheric Multiscale (MMS) mission, which provides three-dimensional (3D) particle distribution measurements with a ","authors_text":"A. De Spiegeleer, A. M. Tian, B. L. Giles, C. J. Xiao, C. T. Russell, H. Zhang, J. Liu, J. Vaverka, M. Hamrin, M. M. Wang, M. Nowada, Q. G. Zong, Q. Q. Shi, R. L. Guo, S. C. Bai, S. T. Yao, S. Y. Fu, S. Y. Huang, T. Pitk\\\"anen, W. J. Sun, W. Y. Li, X. F. Ji, X. G. Wang, X. Z. Zhou, Y. C. Xiao, Z. H. Yao, Z. Y. Li, Z. Y. Pu","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.space-ph","submitted_at":"2017-01-07T12:10:41Z","title":"Observations of kinetic-size magnetic holes in the magnetosheath"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1701.01822","kind":"arxiv","version":2},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:c4fb369d97a30170e172176e15548a965353f8daa55bc60dd59d130fc77858c6","target":"record","created_at":"2026-05-18T00:47:48Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"44f41a48255f46aab37e4daf71cc7451e84f0cb49e79ea26bf06ad3e4a372c0c","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.space-ph","submitted_at":"2017-01-07T12:10:41Z","title_canon_sha256":"217bdb4f78ea6d05ad61eba259d395ffbd15920fe2786fae075caee7b8c2590b"},"schema_version":"1.0","source":{"id":"1701.01822","kind":"arxiv","version":2}},"canonical_sha256":"7c30d82146e455483a859af2316c3cde2613885945d5ee771cffd644e987eadb","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"7c30d82146e455483a859af2316c3cde2613885945d5ee771cffd644e987eadb","first_computed_at":"2026-05-18T00:47:48.573143Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:47:48.573143Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"RPW+G+uWViBwGi9dyBN2hbrEUi2vMF+f+g1WdsiXrlg1n0R4H3Utv26K3IpewEB9QzM8r7sOKiYg1RyCI7rPDw==","signature_status":"signed_v1","signed_at":"2026-05-18T00:47:48.573817Z","signed_message":"canonical_sha256_bytes"},"source_id":"1701.01822","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:c4fb369d97a30170e172176e15548a965353f8daa55bc60dd59d130fc77858c6","sha256:61e261bba06b5c448b04dbd0ce5b4207441ff51cb9ad7c591854ad23ddcece58"],"state_sha256":"0264d494d058301df3e561e915553ce3858bf1a170ffc594abc678fdb43a5251"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"BO/Zyb2ACdhmyH0DKi9Kj8rbNsdEigdv3nBUfyWCUjIjVGQZjsNhFTy9ywPgtV5bHayoXaqUpz4nI4rRVE2nBw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-25T18:03:33.948773Z","bundle_sha256":"efbb35cce5a208c056e75d723d93f5f2b708cf0567be88efd76ec7471190a1e3"}}