| タイトル | Mass and energy flow in prominences |
| 著者（英） | Poland, Arthur I. |
| 著者所属（英） | NASA Goddard Space Flight Center |
| 発行日 | 1990-01-01 |
| 言語 | eng |
| 内容記述 | Mass and energy flow in quiescent prominences is considered based on the hypothesis that active region prominences have a different structure and thus different mass and energy flow characteristics. Several important physical parameters have been plotted using the computational model, representing the evolutionary process after the prominence formation. The temperature, velocity, conductive flux, and enthalpy flux are plotted against distance from the highest point in the loop to the coolest part of the prominence. It is shown that the maximum velocity is only about 5 km/s. The model calculations indicate that the transition region of prominences is dominated by complex processes. It is necessary to take into account mass flow at temperatures below 200,000 K, and both mass flow and optical depth effects in hydrogen at temperatures below 30,000 K. Both of these effects lead to a less steep temperature gradient through the prominence corona interface than can be obtained from the conduction alone. |
| NASA分類 | SOLAR PHYSICS |
| レポートNO | 91A46207 |
| 権利 | Copyright |
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