albuminuria 发表于 2025-3-23 09:59:47
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Fine Structure of the Upper Chromosphereeded in order to answer even the simplest questions of kinematics, while the interpretation of the line spectra still poses many difficulties. The acquisition of EUV data at high spatial resolution should lead to major progress in the field, just as it already has done in showing the EUV emission to be concentrated over the network boundaries.多样 发表于 2025-3-23 21:36:41
http://reply.papertrans.cn/23/2264/226364/226364_13.pngEntropion 发表于 2025-3-24 01:15:53
Michele Averchi,Emanuele Colombohere all structures begin to merge, filling the whole corona. This variation with height compares with usual models derived from spatially resolved observations; as usual the underlying magnetic field is expected to support this channelling.提名的名单 发表于 2025-3-24 02:20:16
http://reply.papertrans.cn/23/2264/226364/226364_15.pngHla461 发表于 2025-3-24 06:39:09
Non-Static Structure of the Chromosphere-Corona Transition Regionhere all structures begin to merge, filling the whole corona. This variation with height compares with usual models derived from spatially resolved observations; as usual the underlying magnetic field is expected to support this channelling.机警 发表于 2025-3-24 11:20:20
http://reply.papertrans.cn/23/2264/226364/226364_17.png兽群 发表于 2025-3-24 16:44:04
http://reply.papertrans.cn/23/2264/226364/226364_18.pngarbovirus 发表于 2025-3-24 22:57:08
http://reply.papertrans.cn/23/2264/226364/226364_19.png沉默 发表于 2025-3-25 01:26:34
Pooling Empirical Observations,hat this pulse is a progressive acoustic wave, as suggested by the inferred flow parameters, we show that the wave loses mechanical energy in traversing the chromosphere. This implies that the bright Ca . features (K grains) are the manifestation of local heating in the chromosphere, possibly by shock waves.