| タイトル | Anti-parallel Filament Flows and Bright Dots Observed in the EUV with Hi-C |
| 本文（外部サイト） | http://hdl.handle.net/2060/20140006483 |
| 著者（英） | Regnier, Stephane; Alexander, Caroline E.; Winebarger, Amy; Walsh, Robert |
| 発行日 | 2013-12-11 |
| 言語 | eng |
| 内容記述 | Hi-C obtained the highest spatial and temporal resolution observations ever taken in the solar EUV corona. Hi-C reveals dynamics and structure at the limit of its temporal and spatial resolution. Hi-C observed various fine-scale features that SDO/AIA could not pick out. For the first time in the corona, Hi-C revealed magnetic braiding and component reconnection consistent with coronal heating. Hi-C shows evidence of reconnection and heating in several different regions and magnetic configurations with plasma being heated to 0.3 - 8 x 10(exp 6) K temperatures. Surprisingly, many of the first results highlight plasma at temperatures that are not at the peak of the response functions. |
| NASA分類 | Solar Physics |
| レポートNO | M13-3131 |
| 権利 | Copyright, Distribution as joint owner in the copyright |
|
