{"as_of":"2026-08-16T18:35:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:6e2357e17ec8c3b0537dd2e428f7a1da2384a7599c70c6191541c95bc9123050","coverage":[{"denominator":55,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":55,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T16:24:08.545771Z","state":"measured"},{"denominator":55,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":55,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2507.13856/citation-record","integrity":"/paper/2507.13856/integrity","json":"/paper/2507.13856/citation-record.json","paper":"/paper/2507.13856"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1063/1.859063","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"1989, Physics of Fluids B, 1, 1998, doi: 10.1063/1.859063","venue":"Physics of Fluids B Plasma Physics","work_id":"f77413e0-8b19-4ae3-9da8-8efa0f496b22","year":1989},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:03.810621Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:8a12d26e6115ffdef399cf6b586c56bf19278d153d5a92c4963d8233c69ce6e4","observation_id":"aa736fd1-787b-43f0-a92e-da25b0847e1a","resolution":{"observed_at":"2026-08-06T16:24:11.179444Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ac90c2","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"T., Carley, E., Ca˜ nizares, L","venue":"The Astrophysical Journal","work_id":"e8d6a89e-8fc5-435b-b080-8ab7b64b251c","year":2022},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:03.883847Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:05bcf16e95efb751c02912829f0b17f444dc7349f8f5c74c5389bba484b9cd5b","observation_id":"1f0af871-2e8c-46a1-b3fc-3723f675cf42","resolution":{"observed_at":"2026-08-06T16:24:11.170965Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1029/95gl03595","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"D., Burgess, D., Kellogg, P","venue":"Geophysical Research Letters","work_id":"ef6d0dec-1556-4031-8092-2c9df692db89","year":1996},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:03.962891Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:cac83ae05db9133b4562cd7713a77414bf198bd795bd11aa0395e4debdc775c2","observation_id":"2ad15aee-655b-46f7-9d8a-80e7d78dd229","resolution":{"observed_at":"2026-08-06T16:24:11.160973Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1063/1.5037300","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"H., & Layden, A","venue":"Physics of Plasmas","work_id":"dc7ee427-425b-4ed1-adc2-96ed4e358a56","year":2018},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:04.064763Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:c846f3c9aeabbd46e71ea95e60527566f7ab57182859f1cfafa76b4d1b091aaa","observation_id":"f9b221e0-6cd4-4518-8394-1c23c5c47d74","resolution":{"observed_at":"2026-08-06T16:24:11.151588Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1063/1.1889123","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"H., & Willes, A","venue":"Physics of Plasmas","work_id":"3455753b-615b-4345-99f0-b75477e2e3ae","year":2005},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:04.160485Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:6395503a1680f7bd23723b8a15421c1eb59b1237ca9491190b01ef31dea17f8a","observation_id":"17f8c36c-cf95-423e-b02d-9c9574b92494","resolution":{"observed_at":"2026-08-06T16:24:11.141811Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T16:24:04.253535Z","title":"2021, ApJL, 915, L22, doi: 10.3847/2041-8213/ac0b43","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:04.253535Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:9bf067c48d441eb2a7f39cd0020792607efdd657ac3765ced4040f50d4d34020","observation_id":"df0f7e5d-addf-45cb-9ece-827454f0591a","resolution":{"observed_at":"2026-08-06T16:24:04.253535Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"0185.00112","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T16:24:11.267940Z","title":null,"venue":null,"work_id":"e598244a-a8c5-420b-9fd5-8fdda0646622","year":1985},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:04.353205Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:21aa360097dc715301c29f169f948cc26bb714f15719fc544f213bdb34459fb3","observation_id":"be9b181d-1bbb-4f49-bd10-f15705fbbedc","resolution":{"observed_at":"2026-08-06T16:24:11.272363Z","resolver_source":"raw_fallback","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1063/1.870636","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"T., & Nishikawa, K","venue":"Physics of Plasmas","work_id":"fba63c46-80d4-42ef-a8e4-0f64f5372c94","year":1994},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:04.425617Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:2f253f075956db6229ac378df79352227d5751301415f2f5591e401625262008","observation_id":"0d1efa69-3601-43b2-857c-34d87d08fca0","resolution":{"observed_at":"2026-08-06T16:24:11.127260Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1063/1.873644","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"D., & Robinson, P","venue":"Physics of Plasmas","work_id":"92c15216-d662-45d4-816a-092092bccfc3","year":1999},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:04.540554Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:a51d9528f073839c461e3a17260a7050fdcb6d44580900fba5f34cacab33f2a9","observation_id":"73786f0d-5080-4b05-8064-d3c9a7db299f","resolution":{"observed_at":"2026-08-06T16:24:11.118685Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T16:24:04.605926Z","title":"J., Velli, M","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:04.605926Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:3ff0c1173ddf846cc4bfe03a47efb11db5435c1e074b4aa22e64a624d0950f94","observation_id":"f2c8fc38-af86-4b8a-8c23-1c2d498f5741","resolution":{"observed_at":"2026-08-06T16:24:04.605926Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T16:24:04.717898Z","title":"L., & Zhelezniakov, V","venue":null,"work_id":null,"year":1958},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:04.717898Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:73ae1d0160f3e554c355c1a8577bfc3ec162bc5d9b9b225a90e8b27d2c5dc76b","observation_id":"88c7ba81-a9d0-40dc-adf7-218a2fbeca36","resolution":{"observed_at":"2026-08-06T16:24:04.717898Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T16:24:11.296938Z","title":"S., & Ryzhik, I","venue":null,"work_id":"8321c5ea-df5e-4c26-848e-79a9be12f170","year":2007},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:04.832124Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:2041178d672ed6f7bcfa7b773bf89c087ed5e7c65cb6ff03f95ac283c8bcd9fa","observation_id":"a33a69fc-b8af-4e6a-b03e-49d87dada66f","resolution":{"observed_at":"2026-08-06T16:24:11.299623Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1002/jgra.50402","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"B., & Cairns, I","venue":"Journal of Geophysical Research Space Physics","work_id":"2a741721-1d94-4b40-9f61-edfc2b1a7c84","year":2013},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:04.925614Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:87ce4f21abe5b32f93078b75abba4afddeb928720fe0a8bac9c993dccb21ab7e","observation_id":"30faffdb-aeb1-4871-9eeb-587c142f347c","resolution":{"observed_at":"2026-08-06T16:24:11.105285Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrevlett.62.2680","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"E., Fried, B","venue":"Physical Review Letters","work_id":"7f3185c4-6828-466b-80ea-7ab06c2b3c25","year":1989},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:05.011480Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:2b6faaf1dfd2d9ed0e0234e60e10672416784ae6692122688492007c7b8e7929","observation_id":"34ff8ca9-62a2-4c86-87f2-2be07c72d4e9","resolution":{"observed_at":"2026-08-06T16:24:11.097000Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/2041-8213/acf857","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"C., Krasnoselskikh, V., Pulupa, M., Magdalenic, J., & Bale, S","venue":"The Astrophysical Journal Letters","work_id":"01f30045-d0bc-47fb-8ab3-04b046b625b3","year":2023},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:05.105678Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:49ec84afcc7714767ed54cdc1f27cb52ef2d414594b3b2b1083d2c44ed2e0ccc","observation_id":"6a520e12-3f15-4d63-b5ca-32bb1e0a8cc6","resolution":{"observed_at":"2026-08-06T16:24:11.089534Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1002/jgra.50443","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"J., Goetz, K., Monson, S","venue":"Journal of Geophysical Research Space Physics","work_id":"d5439a11-9aeb-4fcb-bedb-f35dfd366c56","year":2013},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:05.177677Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:584ae10cfed572fe450d2a1818e9e2d58a341f602a6db47dda12de6a397b25c9","observation_id":"68f69c34-c141-4804-9f32-b954a1e2ddbd","resolution":{"observed_at":"2026-08-06T16:24:11.080579Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrevlett.99.015003","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"H., & Robinson, P","venue":"Physical Review Letters","work_id":"5d40d5d5-b803-4986-8b08-24294b64be11","year":2007},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:05.247833Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:458e2f3dfb4a0ae480af4521353add9cd5d9d1ec1fa033af11075614f4853cfc","observation_id":"9a99b18a-f62d-4923-a3ac-70a15dca9401","resolution":{"observed_at":"2026-08-06T16:24:11.072470Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/2041-8213/ac46a7","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"2022, ApJL, 924, L24, doi: 10.3847/2041-8213/ac46a7 —","venue":"The Astrophysical Journal Letters","work_id":"d78deddf-ba0d-4435-8220-c6e7a555e9f5","year":2022},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:05.342318Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:7a0e6876aa6213c6f2594821931c44c5e11229e493b7cc9168bfab276d7fb87b","observation_id":"f97ff94f-4df2-4d3a-875a-da5939899021","resolution":{"observed_at":"2026-08-06T16:24:11.064420Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/2041-8213/ad47b5","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":null,"venue":"The Astrophysical Journal Letters","work_id":"4153997d-8acc-4b31-bc63-90af7b1fcd3a","year":2024},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:05.409475Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:5b8de7826323708ed8278dc2a69e19800816531dc1a587ed88c76b7af1c6cf17","observation_id":"f9d1fea3-3eb3-41c4-b41d-ab90b4de9b00","resolution":{"observed_at":"2026-08-06T16:24:11.055565Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ac2153","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":null,"venue":"The Astrophysical Journal","work_id":"e757621d-0db0-4f98-a01c-ffa119058638","year":2021},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:05.510525Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:a7efffa140c545b2aba52018a80ab65e0166038d957b04e66e970547c7920f50","observation_id":"795fe60c-12d6-4e3f-8cb0-c319cbb4158b","resolution":{"observed_at":"2026-08-06T16:24:11.047678Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3390/fluids4020069","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"S., & Gauthier, G","venue":"Fluids","work_id":"e57f05f1-3aa9-4417-8b0b-61ef529b295c","year":2019},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:05.587128Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:2a2cf1d4cf7d151698bb4753bedc4f94dce95a82710d02c24b5f96914cdcd4d5","observation_id":"3cdb7a33-965c-47cd-9707-c47d8bb0c176","resolution":{"observed_at":"2026-08-06T16:24:11.039770Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2506.16816","last_updated":"2025-06-20T08:11:10Z","snapshot_observed_at":"2026-08-15T19:15:42.089703Z","submitted_at":"2025-06-20T08:11:10Z","title":"Electromagnetic radiation by turbulent, magnetized and randomly inhomogeneous solar radio sources generated by electron beams","version":1},"cited_work":{"arxiv_id":"2506.16816","doi":null,"metadata_source":"pith","pith_arxiv_id":"2506.16816","snapshot_observed_at":"2026-08-06T16:24:11.187844Z","title":"Electromagnetic radiation by turbulent, magnetized and randomly inhomogeneous solar radio sources generated by electron beams","venue":"astro-ph.SR","work_id":"9b4f2e7d-c7d9-4106-b284-4b4303844144","year":2025},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:05.683880Z"},"links":{"cited_paper":"/paper/2506.16816","citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:da7af22d6321522228473cdc10cdfd8d5497e8dabc6f5a69fd5c89a94eafa443","observation_id":"b2944a4c-c772-4f45-a938-081912884f8b","resolution":{"observed_at":"2026-08-06T16:24:11.191501Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ab22bf","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"2019, ApJ, 879, 51, doi: 10.3847/1538-4357/ab22bf","venue":"The Astrophysical Journal","work_id":"642cef8f-1fe9-4e62-bd4c-0eca55af4730","year":2019},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:05.771049Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:df9896dd6f65dfa1588db285e8840ff7a1639b3126483807e2063887449eb7c2","observation_id":"3b76f0fa-c2eb-4135-bc3c-364c72269ba5","resolution":{"observed_at":"2026-08-06T16:24:11.031547Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T16:24:11.287745Z","title":"V., & Sotnikov, V","venue":null,"work_id":"8895bcf8-9222-44b1-b101-a0e51ce76415","year":1977},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:05.840478Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:78af49cc120fb68e56cf9945a51751c5e0bdc793cbe6007471321d364bd66314","observation_id":"c178a995-3b5b-460b-a9f1-90b1313fdd78","resolution":{"observed_at":"2026-08-06T16:24:11.290775Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/201425308","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"P., Soucek, J., et al","venue":"Astronomy and Astrophysics","work_id":"04e49b53-1867-4e75-bfef-8105ed27232a","year":2015},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:05.928094Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:c2880c8230c0a52f484b58744f47be3f7c7d663fa90f07c53ad4cc8b0356bb04","observation_id":"e140b997-897f-47a8-933c-6ce9a64bf8af","resolution":{"observed_at":"2026-08-06T16:24:11.023566Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T16:24:05.992237Z","title":"2020, ApJS, 246, 57, doi: 10.3847/1538-4365/ab65bd","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:05.992237Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:b603ad87190491563366ddad82c4004c0df1a07d05c25943c5ea27da79aaffba","observation_id":"f7234a48-a7c3-45a1-b3bb-f41ad983578c","resolution":{"observed_at":"2026-08-06T16:24:05.992237Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ad12ba","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"2024a, ApJ, 961, 88, doi: 10.3847/1538-4357/ad12ba —","venue":"The Astrophysical Journal","work_id":"2cb0f126-b925-49d6-8bda-afbad1b74a94","year":null},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:06.065205Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:53fdc42b4c9b06cbd62c8aa33e0f3a99c096da8375177492db92dfe5cb0cfa05","observation_id":"94a42dc8-6453-463a-9862-36c739efeab6","resolution":{"observed_at":"2026-08-06T16:24:11.008494Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrevlett.110.185001","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"H., Li, B., & Robinson, P","venue":"Physical Review Letters","work_id":"4e41bdf0-4b5e-4ab1-8c3f-9c2a3d4b3980","year":2013},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:06.128327Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:b0aa202caf42078e369fd8aa54b084b6d82cc49ad6b9eb06081ec1c5fe7b1419","observation_id":"b7ac6ed6-809a-40e5-940a-8947a5297382","resolution":{"observed_at":"2026-08-06T16:24:10.999309Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ac32bb","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"H., Lee, E., & Tu, W","venue":"The Astrophysical Journal","work_id":"973cc8bf-e064-4769-af9f-d41e0b619eba","year":2022},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:06.227473Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:e2a122bbdf107afa4ff0c4f7da3e9dee773f6374fb1217fd6af979de0dd0b6ff","observation_id":"a70eacdf-258f-4356-8606-3c9d5be989a6","resolution":{"observed_at":"2026-08-06T16:24:10.989053Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T16:24:06.319456Z","title":"F., Yoon, P","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:06.319456Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:bd9c82155ddd1e4394aea55b9a2778b4973ce39d037d9ef38e78e2e567956f6b","observation_id":"d7b06262-fbd5-4d69-a829-6dbe09db6f90","resolution":{"observed_at":"2026-08-06T16:24:06.319456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1029/2007ja012958","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"H., & Robinson, P","venue":"Journal of Geophysical Research Atmospheres","work_id":"ee8dce3d-a8d7-450a-9cba-6e7a1ddb61b3","year":null},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:06.419797Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:668230ecc65099948f63aa815d4010f833d2a4b07f7928e7603d42cc0fa573b2","observation_id":"33767dc3-151b-4166-aa87-83152b558a59","resolution":{"observed_at":"2026-08-06T16:24:10.972877Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1029/2008ja013255","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"A., & Cairns, I","venue":"Journal of Geophysical Research Atmospheres","work_id":"643a9de5-49fd-4049-b42a-55969e567df2","year":null},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:06.509675Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:0fbd3c8474d11fa73c346914f80dd94b5712e08d9e46c500b9cf1f11d98c0962","observation_id":"2d613260-741e-4128-a3c9-c34ea49af935","resolution":{"observed_at":"2026-08-06T16:24:10.963251Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1063/1.1906214","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"J., Robinson, P","venue":"Physics of Plasmas","work_id":"5ab1f9a6-5ff0-4181-80c8-0fa5f213ecc5","year":2005},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:06.608011Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:a8ddbbd4fa47759a56426579a43d22fb05410cdab9d385a2280c8865447a4d25","observation_id":"0682bb2d-b62e-4b3a-9fd2-b1282f680062","resolution":{"observed_at":"2026-08-06T16:24:10.954670Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T16:24:06.686046Z","title":"Y., Reid, H","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:06.686046Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:6f6cacf2a75ee6c191fe2d97fb49eed97a34ffc7f117e8a043b10609c89ce311","observation_id":"dd5ca57e-5cda-4868-a513-c7b44b1e8bc8","resolution":{"observed_at":"2026-08-06T16:24:06.686046Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-637x/755/1/45","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"M., Cairns, I","venue":"The Astrophysical Journal","work_id":"2f704465-b02b-492d-bc10-55f87f4a1d64","year":2012},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:06.775662Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:4a810a715d687affeffd6b1b000d06c254c45922ffb7b427ee65227354d86e27","observation_id":"71efaf36-2a5b-47eb-84c2-4c9adc5fdca2","resolution":{"observed_at":"2026-08-06T16:24:10.940571Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1007/bf00212597","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T00:03:45.533247Z","title":null,"venue":"Space Science Reviews","work_id":"08ade002-fe59-4873-9cd5-b4c6b24934aa","year":1980},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:06.867844Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:730d61d04bd424a61686ba10330b9bc79d280354d6a29e7ac962678f43218df1","observation_id":"60dc4425-146e-4006-af78-5d2b875b5eba","resolution":{"observed_at":"2026-08-06T16:24:10.931797Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T16:24:06.942550Z","title":"B., & Sy, W","venue":null,"work_id":null,"year":1972},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:06.942550Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:05c5c069045d54d93f81a531160be9a7fb13fe75923902effba561aaf19e0cbe","observation_id":"05acb38d-4853-4c2e-aadb-649bffcb0e4b","resolution":{"observed_at":"2026-08-06T16:24:06.942550Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1007/bf00239800","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T00:03:45.533247Z","title":"V., & Newman, D","venue":"Solar Physics","work_id":"871631be-99af-4fbd-a922-c5046bc22045","year":1985},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:07.031347Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:ca850b2b7bdd7d323883c7eb12702eefb4089d96f09f6f94188784a8421b9d78","observation_id":"6bdcd659-b015-41ec-a602-1b7174d66d01","resolution":{"observed_at":"2026-08-06T16:24:10.916502Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1143/jpsj.41.1757","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":null,"venue":"Journal of the Physical Society of Japan","work_id":"d4f9f92d-5377-42db-a598-c133542502b2","year":1976},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:07.128207Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:378f7029eab08acb6375ad3884a613fab26ed5bbae14d1589276d60a1f01ab05","observation_id":"ecec2119-abd2-4960-b5dd-1884277c4ddb","resolution":{"observed_at":"2026-08-06T16:24:10.906704Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/152862","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"L., & Smith, R","venue":"The Astrophysical Journal","work_id":"56d7c240-9e05-4810-8c22-96534b5e375e","year":1974},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:07.196452Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:7770537b7c80788f529f57b7871959c4e5aa1ef14c1d9c0c3657904b2d445e5b","observation_id":"07818275-60a3-4140-bfc9-cced30a12021","resolution":{"observed_at":"2026-08-06T16:24:10.758178Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/201423731","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"P., & Reid, H","venue":"Astronomy and Astrophysics","work_id":"3ab057c5-e971-4402-b3c2-dc40ff2cdbd6","year":2014},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:07.293185Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:20550c19730bc0614b1a1d46f0c36148bcdec481cab972aa4499ca3f9377a272","observation_id":"f7808bb7-f359-40e7-bdc5-928c2970f377","resolution":{"observed_at":"2026-08-06T16:24:10.526411Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T16:24:07.375456Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:07.375456Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:0f6cff6a763ba7d88ed69e2445e8d2198ef4a45be31bfa98edb844a94e62086d","observation_id":"98b8786d-ef1f-4b4f-9ba8-e5961b1cf2c8","resolution":{"observed_at":"2026-08-06T16:24:07.375456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T16:24:07.483529Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:07.483529Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:8c59ccfbc0d413404129af78e93f7bf04f84d0e1e8c858db4792bafc8f390458","observation_id":"01fbb884-f5f2-4c31-9266-e08951ec86ac","resolution":{"observed_at":"2026-08-06T16:24:07.483529Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-637x/694/1/618","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"2009, ApJ, 694, 618, doi: 10.1088/0004-637X/694/1/618","venue":"The Astrophysical Journal","work_id":"908b1a70-a432-4a56-a59a-e00f1b134e17","year":2009},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:07.542377Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:bce3ca9995d5d07734fdb1c4a9757666ee400e12e22337cf1f689b87f6a99e36","observation_id":"a0648483-d1a2-4b10-a893-bae86d15240f","resolution":{"observed_at":"2026-08-06T16:24:10.319412Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1063/1.4793726","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"H., & Kim, E","venue":"Physics of Plasmas","work_id":"bdc8a3b7-2c9a-4054-b66a-9d44aceb5e76","year":2013},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:07.659233Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:c79b3c812aaa17d82105d41bc47de3298815a1a9a5b6a0f88aa346950db1d72a","observation_id":"1bbf3c17-3772-4c20-9e58-911b7111f997","resolution":{"observed_at":"2026-08-06T16:24:10.205385Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1002/2013ja019364","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T00:03:56.115653Z","title":"H., & Kim, E.-H","venue":"Journal of Geophysical Research Space Physics","work_id":"37acf05f-cde5-42ac-a3dd-e41b6894abd7","year":2014},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:07.742145Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:bc66a9e064ff6d9159d81c61967212a2f4680c3d4aa420ba3f9bd796188cf42c","observation_id":"fb6173c9-f44d-43b3-aa19-57e922d27206","resolution":{"observed_at":"2026-08-06T16:24:09.975624Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1007/978-1-4615-7799-7","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T00:03:56.115653Z","title":null,"venue":null,"work_id":"a3672e86-ba12-4b03-b7dd-d8e08f1b4a98","year":1967},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:07.830912Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:dca60b068b3ba017073b2b0fa2e5da3497f7e8a48097760bf7287ecde2e16861","observation_id":"41d0dd3a-4dc6-4be0-b8f9-e72f71d6f034","resolution":{"observed_at":"2026-08-06T16:24:09.722753Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/abee74","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":null,"venue":"The Astrophysical Journal","work_id":"0a9aa4f4-e89c-4f01-96b3-fbf6bc347670","year":2021},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:07.924585Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:c3e8cddb96da98daf269def87564a0c1c9baa5b55837de95fb0dce55006d08e4","observation_id":"0a94613f-9995-4af9-b276-605185e6fadd","resolution":{"observed_at":"2026-08-06T16:24:09.647888Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T16:24:08.012482Z","title":null,"venue":null,"work_id":null,"year":1970},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:08.012482Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:0111c58d1044b57338a8a4919e5f6dbe13f5014c9650c1a05692c7d10cd008ea","observation_id":"e413c42c-99ae-45ce-9bff-e2f2d7aea1f9","resolution":{"observed_at":"2026-08-06T16:24:08.012482Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/aae7cc","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"S., & Krafft, C","venue":"The Astrophysical Journal","work_id":"3e2f941d-c61e-4383-90f5-85127b481e6a","year":2018},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:08.103269Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:bf538b5cfab46bc014cb7a4327ab89225188685574f01d998dc9da4c3b096ab1","observation_id":"1e0ee8fb-16b0-4292-b774-81ea9e32f0db","resolution":{"observed_at":"2026-08-06T16:24:09.472239Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1063/1.874180","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"J., & Cairns, I","venue":"Physics of Plasmas","work_id":"27715119-1959-448f-9c4d-ccccb73da661","year":2000},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:08.211522Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:5339cdadc689ea13b010fa0e8e11cfd3f420e46c9312598644cbcf07eb0d9319","observation_id":"a97a642c-8a7f-4471-92a9-0732b5adbb31","resolution":{"observed_at":"2026-08-06T16:24:09.280027Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1029/98gl01989","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"M., & Bougeret, J","venue":"Geophysical Research Letters","work_id":"1da13eec-2374-4523-8a1c-0631524eaa87","year":1998},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:08.276514Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:4ccf665dc91ae6c658dbb988cd99e2cf29f93f44fe0fa13b2d1779086e82bb42","observation_id":"496396ba-19a9-458a-ad0a-1470f1bf7d7e","resolution":{"observed_at":"2026-08-06T16:24:09.066869Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ab6a0d","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"A., B¨ uchner, J., & Liu, S","venue":"The Astrophysical Journal","work_id":"d21a3728-9738-4f17-ad86-b36f5990cd63","year":2020},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:08.356803Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:d3d19ea4989bd9d90cf9c5105919d908409ca17788e7c2e80c4756648d6d554d","observation_id":"80e010be-ef83-4348-88e0-2641e6f79364","resolution":{"observed_at":"2026-08-06T16:24:08.897860Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-637x/806/2/237","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"F., Yoon, P","venue":"The Astrophysical Journal","work_id":"cf68c19e-5b2b-47c3-b382-e6a737b0513a","year":2015},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:08.476885Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:416a7f2dd912d646f58b1aa41d73b8148fff4d5efe6d60a8573a9307104f4693","observation_id":"20d9ad09-0282-4809-be8c-9540b1bde1d1","resolution":{"observed_at":"2026-08-06T16:24:08.705341Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T16:24:11.278655Z","title":null,"venue":null,"work_id":"521db85c-d953-41da-b7c2-84a48f073fd0","year":1981},"citing_paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-06T16:24:08.545771Z"},"links":{"citing_paper":"/paper/2507.13856"},"observation_digest":"sha256:0b6fca7fb7be76b3fabcc7415afdf4347a4a2c1dd749fc32ca9e2db2b44a2417","observation_id":"c822b4e3-0992-4bc1-989e-599d440abf14","resolution":{"observed_at":"2026-08-06T16:24:11.281551Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2507.13856","last_updated":"2025-07-18T12:23:26Z","latest_version":1,"primary_category":"physics.plasm-ph","snapshot_observed_at":"2026-08-06T16:12:33.567171Z","submitted_at":"2025-07-18T12:23:26Z","title":"Linear mode conversion theory of radio emission from turbulent solar wind plasmas"},"reference_resolution":{"displayed":55,"state_counts":{"malformed_identifier":0,"metadata_mismatch":2,"parse_uncertain":0,"unresolved":11,"verified_exact":40,"verified_fuzzy":2},"total_outbound_references":55},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 16 August 2026, this Paper Citation Record lists 55 of 55 outbound references and 0 inbound Pith citation observations for arXiv:2507.13856."}