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Such radiation spectrum is characterized by the strength parameter $a = \\lambda_{B}} e|B|/mc^2$, where $\\lambda_{B}}$ is the length scale of the turbulent field. When $a$ is much larger than the Lorentz factor of a radiating electron $\\gamma$, synchrotron radiation is realized, while $a\\ll 1$ corresponds to the so-called jitter radiation regime. Because for $1<a<\\gamma$ we cannot use either approximations, we should have reco"},"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":"1106.2216","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2011-06-11T07:44:54Z","cross_cats_sorted":[],"title_canon_sha256":"05c21be20f46a680e40ca87189cdc3fc8a3e30d5c6e1355dc8843055be4a634c","abstract_canon_sha256":"05426e1226eed25f416a0328aa3385122ea678a7c3f8659896bc5461a4d0aca7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:01:39.726773Z","signature_b64":"oWRwHz+xBiZQ5Kd2W9J+MvVm5INAuFo+LBcKHCW1BEKy0GtMnQd+HE6hb1b4vOvu7cYixipn8jgD31LFK+V0Dw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"80cb374b8708cdc5e8de70141180a6683a64235a027a00448e63eb0d29265fe4","last_reissued_at":"2026-05-18T02:01:39.726356Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:01:39.726356Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A Novel Emission Spectrum From A Relativistic Electron Moving In A Random Magnetic Field","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Fumio Takahara, Yuto Teraki","submitted_at":"2011-06-11T07:44:54Z","abstract_excerpt":"We calculate numerically the radiation spectrum from relativistic electrons moving in small scale turbulent magnetic fields expected in high energy astrophysical sources. 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