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• W3100334795 endingPage "143" @default.
• W3100334795 startingPage "143" @default.
• W3100334795 abstract "For the first time, the kinematic evolution of a coronal wave over the entire solar surface is studied. Full Sun maps can be made by combining images from the Solar Terrestrial Relations Observatory satellites, Ahead and Behind, and the Solar Dynamics Observatory, thanks to the wide angular separation between them. We study the propagation of a coronal wave, also known as EIT wave, and its interaction with a coronal hole resulting in secondary waves and/or reflection and transmission. We explore the possibility of the wave obeying the law of reflection of waves. In a detailed example we find that a loop arcade at the coronal hole boundary cascades and oscillates as a result of the EUV wave passage and triggers a wave directed eastwards that appears to have reflected. We find that the speed of this wave decelerates to an asymptotic value, which is less than half of the primary EUV wave speed. Thanks to the full Sun coverage we are able to determine that part of the primary wave is transmitted through the coronal hole. This is the first observation of its kind. The kinematic measurements of the reflected and transmitted wave tracks are consistent with a fast-mode MHD wave interpretation. Eventually, all wave tracks decelerate and disappear at a distance. A possible scenario of the whole process is that the wave is initially driven by the expanding coronal mass ejection and subsequently decouples from the driver and then propagates at the local fast-mode speed." @default.
• W3100334795 created "2020-11-23" @default.
• W3100334795 creator A5000460407 @default.
• W3100334795 creator A5016535842 @default.
• W3100334795 creator A5068760885 @default.
• W3100334795 creator A5073501391 @default.
• W3100334795 date "2012-08-23" @default.
• W3100334795 modified "2023-10-02" @default.
• W3100334795 title "SECONDARY WAVES AND/OR THE “REFLECTION” FROM AND “TRANSMISSION” THROUGH A CORONAL HOLE OF AN EXTREME ULTRAVIOLET WAVE ASSOCIATED WITH THE 2011 FEBRUARY 15 X2.2 FLARE OBSERVED WITH<i>SDO</i>/AIA AND<i>STEREO</i>/EUVI" @default.
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• W3100334795 doi "https://doi.org/10.1088/0004-637x/756/2/143" @default.
• W3100334795 hasPublicationYear "2012" @default.
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