The Properties of Small Magnetic Flux Ropes inside the Solar Wind Come from Coronal Holes, Active Regions, and Quiet Sun
The origination and generation mechanisms of small magnetic flux ropes (SMFRs), which are important structures in solar wind, are not clearly known. In the present study, 1993 SMFRs immersed in coronal holes, active regions, and quiet-Sun solar wind are analyzed and compared. We find that the proper...
| Egile Nagusiak: | , , , , |
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| Formatua: | Artikulua |
| Hizkuntza: | English |
| Argitaratua: |
IOP Publishing
2023-01-01
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| Saila: | The Astrophysical Journal |
| Gaiak: | |
| Sarrera elektronikoa: | https://doi.org/10.3847/1538-4357/accf9a |