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- W2014266082 abstract "We present evidences that emergence of new flux in the lower atmosphere leads to magnetic reconnection of field lines. In a first phase the phenomenon is observed in the chromosphere by the formation of dark filaments (arch filament system) which are overlaid by bright loops visible in soft X-rays. Different types of event appear according to the magnetic field configuration and the amount of energy involved. 3-D modelling of the photospheric magnetic field provides a new tool for understanding reconnection in real configurations. The observed chromospheric and coronal loops are good diagnostics for the modelling. We document our statement by examples obtained during coordinated campaigns with the Hα Multichannel Subtractive Double Pass spectrographs-MSDP (Pic du Midi and Tenerife) and the Yohkoh instruments." @default.
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- W2014266082 date "1962-10-01" @default.
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- W2014266082 title "Space spectroscopy at U.S. naval research laboratory—photographic technique" @default.
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- W2014266082 doi "https://doi.org/10.1016/0022-4073(62)90043-2" @default.
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