Zobrazeno 1 - 10
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pro vyhledávání: '"Lin, Yuanzhang"'
Automated unit test generation has been widely studied, with Large Language Models (LLMs) recently showing significant potential. Moreover, in the context of unit test generation, these tools prioritize high code coverage, often at the expense of pra
Externí odkaz:
http://arxiv.org/abs/2410.13542
Akademický článek
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Publikováno v:
Solar Physics. 168:135-143
A solar flare with both Hβ and Fe i 5324 emissions was observed in AR 7529 (S13, E65) on 24 June, 1993 at the Bejing Astronomical Observatory. Our calculations show that the Fe i 5324 emission region of the flare was located in the low photosphere a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::17a7a563d0a351132aee5a5e5605da7b
https://doi.org/10.1007/bf00145830
https://doi.org/10.1007/bf00145830
Autor:
Lin Yuanzhang, V. Gaizauskas
Publikováno v:
Chinese Astronomy and Astrophysics. 18:455-461
Based mainly on filtergrams ofHα line center and various offbands and supplemented with measurements of the CIV 1548 line, we analyzed the evolution of a filament during a period of 15 minutes prior to the eruption of the flare of 1980 June 25 in th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c33bc0adf74fe98758d6368bbff61c3a
https://doi.org/10.1016/0275-1062(94)90014-0
https://doi.org/10.1016/0275-1062(94)90014-0
Autor:
Wang Huaning, Lin Yuanzhang
Publikováno v:
Chinese Astronomy and Astrophysics. 17:423-430
The analyses have been made with the emphasis on four existing criteria for calibrating the azimuth of the photospheric transverse magnetic field measured with a heliomagnetograph. The results indicate that the potential criterion, Krall's criterion,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::180ba8237990204649f4ba7acfeadd87
https://doi.org/10.1016/0275-1062(93)90009-e
https://doi.org/10.1016/0275-1062(93)90009-e
Publikováno v:
International Astronomical Union Colloquium. 141:446-449
It is well accepted that the source of energy for flares arises in the non-potential magnetic field from the dynamic evolution of active regions above the photosphere. So far, however, contradictory results have been suggested for the question of whe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1537da95c6b5cd4d5f817aec1b977808
https://doi.org/10.1017/s0252921100029596
https://doi.org/10.1017/s0252921100029596
Autor:
Wang Huaning, Lin Yuanzhang
Publikováno v:
International Astronomical Union Colloquium. 141:461-464
The 180° ambiguity of the transverse magnetic field measured by a heliomagnetograph is an intrinsic problem due to the linear polarization in Zeeman effect(Harvey, 1969). Thus we have to make use of some criteria for calibrating the transverse magne
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6dd51de09cbb1015f080e3d8977409a5
https://doi.org/10.1017/s0252921100029638
https://doi.org/10.1017/s0252921100029638
Publikováno v:
Magnetodynamic Phenomena in the Solar Atmosphere ISBN: 9789401066273
The solar telescope magnetograph of the Beijing Astronomical Observatory uses two wavelengths, FeI 5324 and H β for the observations of the photosphere and the chromosphere (Ai and Hu, 1986). Among hundreds of H β flares observed since 1987, only a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::bf275ec485219a45f9bcc1ce79a1652e
https://doi.org/10.1007/978-94-009-0315-9_134
https://doi.org/10.1007/978-94-009-0315-9_134
Publikováno v:
Solar Physics; Nov1993, Vol. 148 Issue 1, p133-138, 6p