期刊
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN
卷 59, 期 -, 页码 S699-S706出版社
OXFORD UNIV PRESS
DOI: 10.1093/pasj/59.sp3.S699
关键词
Sun : chromosphere; Sun : corona; Sun : flux emergence; Sun : transition region; Sun : UV radiation
资金
- STFC [PP/D002907/1, PP/E001173/1] Funding Source: UKRI
- Science and Technology Facilities Council [PP/E001173/1, PP/D002907/1] Funding Source: researchfish
We use coordinated Hinode SOT/EIS observations that include high-resolution magnetograms, chromospheric, and transition region (TR) imaging, and TR/coronal spectra in a first test to study how the dynamics of the TR are driven by the highly dynamic photospheric magnetic fields and the ubiquitous chromospheric waves. Initial analysis shows that these connections are quite subtle and require a combination of techniques including magnetic field extrapolations, frequency-filtered time-series, and comparisons with synthetic chromospheric and TR images from advanced 3D numerical simulations. As a first result, we find signatures of magnetic flux emergence as well as 3 and 5 mHz wave power above regions of enhanced photospheric magnetic field in both chromospheric, transition region, and coronal emission.
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