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- W2760558103 abstract "Coronal fans (see Figure 1) are bright observational structures that extend to large distances above the solar surface and can easily be seen in EUV (174 angstrom) above the limb. They have a very long lifetime and can live up to several Carrington rotations (CR), remaining relatively stationary for many months. Note that they are not off-limb manifestation of similarly-named active region fans. The solar conditions required to create coronal fans are not well understood. The goal of this research was to find as many associations as possible of coronal fans with other solar features and to gain a better understanding of these structures. Therefore, we analyzed many fans and created an overview of their properties. We present the results of this statistical analysis and also a case study on the longest living fan." @default.
- W2760558103 created "2017-10-06" @default.
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- W2760558103 date "2017-09-04" @default.
- W2760558103 modified "2023-09-27" @default.
- W2760558103 title "Observational Analysis of Coronal Fans" @default.
- W2760558103 hasPublicationYear "2017" @default.
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