Počet záznamov: 1  

Spectral diagnostics of cool flare loops observed by the SST. I. Inversion of the Ca II 8542 A and H-beta lines

  1. NázovSpectral diagnostics of cool flare loops observed by the SST. I. Inversion of the Ca II 8542 A and H-beta lines
    Autor Koza Július 1970- SAVASTRO - Astronomický ústav SAV    SCOPUS    RID    ORCID
    Spoluautori Kuridze David

    Heinzel Petr

    Jejčič Sonja

    Morgan Huw

    Zapiór M.

    Zdroj.dok. The Astrophysical Journal. Vol. 885, no. 2 (2019), article no. 154, p. 1-13
    Jazyk dok.eng - angličtina
    KrajinaUS - Spojené štáty
    URLURL link
    Druh dok.rozpis článkov z periodík (rbx)
    OhlasyJING, Zhichen - PAN, Wuqi - YANG, Yukun - SONG, Dechao - TIAN, Jun - LI, Y. - CHENG, X. - HONG, Jie - DING, M. D. The Ly alpha emission in solar flares. I. A statistical study on its relationship with the 1-8 A soft X-ray emission. In ASTROPHYSICAL JOURNAL. ISSN 0004-637X, 2020, vol. 904, no. 1, article no. 41, p. 1-13.
    YAKOVKIN, I. I. - VERONIG, A. M. - LOZITSKY, V. G. Magnetic field measurements in a limb solar flare by hydrogen helium and ionized calcium lines. In ADVANCES IN SPACE RESEARCH. ISSN 0273-1177, 2021, vol. 68, no. 3, p. 1507-1518. Dostupné na: https://doi.org/10.1016/j.asr.2021.03.036.
    ANTOLIN, Patrick - FROMENT, Clara. Multi-scale variability of coronal loops set by thermal non-equilibrium and instability as a probe for coronal heating. In FRONTIERS IN ASTRONOMY AND SPACE SCIENCES, 2022, vol. 9, article no. 820116, p. 1-40. ISSN 2296-987X. Dostupné na: https://doi.org/10.3389/fspas.2022.820116.
    YAKOVKIN, I. I. - HROMOV, M. A. - LOZITSKY, V. G. Spectral manifestations of strong and especially strong magnetic fields in the active prominence on July 24, 1999. In KINEMATICS AND PHYSICS OF CELESTIAL BODIES, 2023, vol. 39, no. 5, p. 287-293. ISSN 0884-5913. Dostupné na: https://doi.org/10.3103/S0884591323050070.
    TIAN, Zheng-Yuan - FENG, Li - LU, Lei - XIA, Fan-Xiaoyu - SU, Yang - GAN, Wei-Qun - LI, Hui - ZHOU, Yue. Lyiα/i emission enhancement associated with soft X-ray microflares. In RESEARCH IN ASTRONOMY AND ASTROPHYSICS, 2023, vol. 23, no. 6, article no. 065011, p. 1-18. ISSN 1674-4527. Dostupné na: https://doi.org/10.1088/1674-4527/accc75.
    KERR, Graham S. Interrogating solar flare loop models with IRIS observations 2: Plasma properties, energy transport, and future directions. In FRONTIERS IN ASTRONOMY AND SPACE SCIENCES, 2023, vol. 9, article no. 1060862, p. 1-31. ISSN 2296-987X. Dostupné na: https://doi.org/10.3389/fspas.2022.1060862.
    PIETROW, A. G. M. - CRETIGNIER, M. - DRUETT, M. K. - ALVARADO-GOMEZ, J. D. - HOFMEISTER, S. J. - VERMA, M. - KAMLAH, R. - BARATELLA, M. - AMAZO-GOMEZ, E. M. - KONTOGIANNIS, I. - DINEVA, E. - WARMUTH, A. - DENKER, C. - POPPENHAEGER, K. - ANDRIIENKO, O. - DUMUSQUE, X. - LOFDAHL, M. G. A comparative study of two X2.2 and X9.3 solar flares observed with HARPS-N Reconciling Sun-as-a-star spectroscopy and high-spatial resolution solar observations in the context of the solar-stellar connection. In ASTRONOMY AND ASTROPHYSICS, 2024, vol. 682, article no. A46, p. 1-20. ISSN 0004-6361. Dostupné na: https://doi.org/10.1051/0004-6361/202347895.
    KategóriaADCA - Vedecké práce v zahraničných karentovaných časopisoch impaktovaných
    Kategória (od 2022)V3 - Vedecký výstup publikačnej činnosti z časopisu
    Typ výstupučlánok
    Rok vykazovania2019
    Registrované vWOS
    Registrované vSCOPUS
    Registrované vCCC
    DOI 10.3847/1538-4357/ab4426
    článok

    článok

    Názov súboruPrístupVeľkosťStiahnutéTypLicence
    Spectral diagnostics of cool flare loops observed by the SST. I. Inversion of the Ca II 8542 A and H-beta lines.pdfPrístupný3.8 MB3Vydavateľská verzia
    Spectral diagnostics of cool flare loops observed by the SST. I. Inversion of the Ca II 8542 A and H-beta lines.pdfPrístupný z IP adries SAV8.3 MB2Autorský preprint
    rokCCIFIF Q (best)JCR Av Jour IF PercSJRSJR Q (best)CiteScore
    A
    rok vydaniarok metrikyIFIF Q (best)SJRSJR Q (best)
    201920185.580Q12.741Q1
Počet záznamov: 1  

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