{"paper":{"title":"X-ray Flare Spectra from the DIOGENESS Spectrometer and its concept applied to ChemiX on the Interhelioprobe spacecraft","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Stepanov, B. Sylwester, E. Stanczyk, F Farnik, J. Sylwester, K. J. H. Phillips, M. Kowalinski, M. Siarkowski, M. Steslinski, R. Zawerbny, S. Nowak, S. Plocieniak, W. Trzebinski, Z. Kordywski, Z. Szaforz","submitted_at":"2014-11-04T10:28:15Z","abstract_excerpt":"The {\\em DIOGENESS} X-ray crystal spectrometer on the {\\em CORONAS-F} spacecraft operated for a single month (25~August to 17~September) in 2001 but in its short lifetime obtained one hundred and forty high-resolution spectra from some eight solar flares with {\\em GOES} importance ranging from C9 to X5. The instrument included four scanning flat crystals with wavelength ranges covering the regions of \\sixiii\\ (6.65~\\AA), \\sxv\\ (5.04~\\AA), and \\caxix\\ (3.18~\\AA) X-ray lines and associated dielectronic satellites. Two crystals covering the \\caxix\\ lines were oriented in a ``Dopplerometer'' manne"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1411.0850","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}