MAIZE
发表于 2025-3-26 21:21:06
George L. Roth,Anthony J. DiBellaf two-ribbon flares, show continuous expansion motions during their eruption. Meanwhile, flare ribbons separate continuously in space from each other. Such observational phenomena are interpreted in theory by continuously rising of the magnetic reconnection site, which closely follows erupting magne
CUB
发表于 2025-3-27 02:59:29
George L. Roth,Anthony J. DiBellaf two-ribbon flares, show continuous expansion motions during their eruption. Meanwhile, flare ribbons separate continuously in space from each other. Such observational phenomena are interpreted in theory by continuously rising of the magnetic reconnection site, which closely follows erupting magne
前兆
发表于 2025-3-27 07:36:44
George L. Roth,Anthony J. DiBellauring solar flares.Includes unique new observations of stellThis volume is devoted to the dynamics and diagnostics of solar magnetic fields and plasmas in the Sun’s atmosphere. Five broad areas of current research in Solar Physics are presented: (1) New techniques for incorporating radiation transfe
dilute
发表于 2025-3-27 09:53:50
George L. Roth,Anthony J. DiBelland can only be applied to relatively small areas, ., a single active region. We apply a method for nonlinear force-free coronal magnetic field modelling of photospheric vector magnetograms in spherical geometry which allows us to study the connectivity between multi-active regions. We use Vector Spe
漫步
发表于 2025-3-27 17:40:41
George L. Roth,Anthony J. DiBellaThe second part, with the original title, was to be published by de Feiter in about one year from now. However, to the deep sorrow of all of us, Dr de Feiter died suddenly and unexpectedly when the present book was in print. Thus, unfortunately, de Feiter‘s second part may not appear. Due to the fac
inveigh
发表于 2025-3-27 20:52:12
George L. Roth,Anthony J. DiBellaThe second part, with the original title, was to be published by de Feiter in about one year from now. However, to the deep sorrow of all of us, Dr de Feiter died suddenly and unexpectedly when the present book was in print. Thus, unfortunately, de Feiter‘s second part may not appear. Due to the fac
我说不重要
发表于 2025-3-28 01:54:42
http://reply.papertrans.cn/89/8848/884712/884712_37.png
LATHE
发表于 2025-3-28 03:32:22
http://reply.papertrans.cn/89/8848/884712/884712_38.png
和平主义者
发表于 2025-3-28 09:32:39
George L. Roth,Anthony J. DiBella 2″. At flare maximum the 2....— —2.... transitions of Fe . are present, and show the location of the (approx.) 20 × 10. deg plasma with respect to the surface magnetic field and chromospheric (He .) emissions. Three examples are discussed (two only briefly)..In the small, intense disk flare of 1973
ostrish
发表于 2025-3-28 13:31:49
regular 12±2 h synoptic observation rate. The form and brightness of coronal active region structures are seen to vary on time scales ranging from seconds, for flare associated changes, to several solar rotations for long term evolution of the regions. The extrapolation of photospheric magnetic fie