Small-scale solar magnetic fields
| dc.creator | de Wijn, A. G. | |
| dc.creator | Stenflo, J. O. | |
| dc.creator | Solanki, S. K. | |
| dc.creator | Tsuneta, S. | |
| dc.date | 2008-12-24 | |
| dc.date.accessioned | 2026-07-07T12:21:53Z | |
| dc.date.available | 2026-07-07T12:21:53Z | |
| dc.description | As we resolve ever smaller structures in the solar atmosphere, it has become clear that magnetism is an important component of those small structures. Small-scale magnetism holds the key to many poorly understood facets of solar magnetism on all scales, such as the existence of a local dynamo, chromospheric heating, and flux emergence, to name a few. Here, we review our knowledge of small-scale photospheric fields, with particular emphasis on quiet-sun field, and discuss the implications of several results obtained recently using new instruments, as well as future prospects in this field of research. | |
| dc.description | 43 pages, 18 figures | |
| dc.identifier | https://arxiv.org/abs/0812.4465 | |
| dc.identifier | http://arxiv.org/abs/0812.4465 | |
| dc.identifier | doi:10.1007/s11214-008-9473-6 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/213477 | |
| dc.subject | Astrophysics | |
| dc.title | Small-scale solar magnetic fields | |
| dc.type | text |