Interactions between reversed granulation, p-modes, and magnetism?
| dc.creator | de Wijn, Alfred G. | |
| dc.creator | McIntosh, Scott W. | |
| dc.creator | De Pontieu, Bart | |
| dc.date | 2009-02-11 | |
| dc.date.accessioned | 2026-07-07T12:40:41Z | |
| dc.date.available | 2026-07-07T12:40:41Z | |
| dc.description | We investigate features that are observed in Ca ii H sequences from Hinode in places where reversed granulation seems to interact with p-modes. These features appear ubiquitously in the quiet sun. They are co-spatial with reversed granulation, and display similar general properties, but have sharper edges and show fast brightness changes. They also appear predominantly above wide intergranular lanes, indicating a potential connection with magnetism. We report on the appearance and dynamics of these features using high-resolution, high-cadence observations from Hinode, and we discuss their possible origin. | |
| dc.description | 4 pages, 1 figure, proceedings of the Second Hinode Science Meeting, held in Boulder, CO, Sept 30 - Oct 3, 2008 | |
| dc.identifier | https://arxiv.org/abs/0902.1966 | |
| dc.identifier | http://arxiv.org/abs/0902.1966 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/219518 | |
| dc.subject | Solar and Stellar Astrophysics | |
| dc.title | Interactions between reversed granulation, p-modes, and magnetism? | |
| dc.type | text |