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At low frequencies (<100 MHz) radio bursts with short durations of milliseconds, such as solar S-bursts, have been identified. To date, their origin and many of their characteristics remain unclear. Aims. We report observations from the Ukrainian T-shaped Radio telescope, (UTR-2), and the LOw Frequency ARray (LOFAR) which give us new insight into their nature. Methods. Over 3000 S-bursts were observed on 9 July 2013 at frequencies of 17.4-83.1 MHz during a period of low sol"},"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":"1901.07424","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2019-01-22T15:39:28Z","cross_cats_sorted":[],"title_canon_sha256":"566c4f0f89b74db40aa7f7fe4bc61ef114ea8375659ee1a363a0e9c97d6ec59f","abstract_canon_sha256":"130b6c89cddaa58967dce373e57dc403320072dd9154498d7bc96f1f31023ee2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:45:20.338229Z","signature_b64":"46CY6zwE0NZ3kh89VWVSKxY9qnPY/ZHjrzxC0tqPS7VmbtN0loxbqTSLFguCwfGZgO32uMzcWOWSvJCfEeCdCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7755cbfea380c7dc157ec9abc19632ffff238efe8137d535053d7167f15310f3","last_reissued_at":"2026-05-17T23:45:20.337761Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:45:20.337761Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Properties and magnetic origins of solar S-bursts","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Alexander A. Konovalenko, Brendan P. Clarke, Diana E. Morosan, Eoin P. Carley, Peter T. Gallagher, Vladimir V. Dorovskyy","submitted_at":"2019-01-22T15:39:28Z","abstract_excerpt":"Context. Solar activity is often accompanied by solar radio emission, consisting of numerous types of solar radio bursts. At low frequencies (<100 MHz) radio bursts with short durations of milliseconds, such as solar S-bursts, have been identified. To date, their origin and many of their characteristics remain unclear. Aims. We report observations from the Ukrainian T-shaped Radio telescope, (UTR-2), and the LOw Frequency ARray (LOFAR) which give us new insight into their nature. Methods. 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