| Автор | Uri Feldman |
| Дата выпуска | 1993-01-01 |
| dc.description | Highly ionized atomic physics systems are used to probe processes taking place in the upper solar atmosphere, a region that, when flares are included, encompasses some three orders of magnitude in the temperature (3 × 10<sup>4</sup>−3 × 10<sup>7</sup>K). A thorough review of spectral line intensities implies that plasmas in the different parts of the upper solar atmosphere are transiently ionizing and are consistently associated with increased electron density. A possible mechanism consistent with the observations is a current driven plasma compression. |
| Формат | application.pdf |
| Издатель | Institute of Physics Publishing |
| Название | Highly ionized atoms in space; or highly ionized atoms, what are they teaching us about the solar coronal heating processes? |
| Тип | paper |
| DOI | 10.1088/0031-8949/1993/T46/004 |
| Electronic ISSN | 1402-4896 |
| Print ISSN | 0031-8949 |
| Журнал | Physica Scripta |
| Том | 1993 |
| Первая страница | 34 |
| Последняя страница | 43 |
| Аффилиация | Uri Feldman; E. O. Hulburt Center for Space Research, Naval Research Laboratory, Washington DC 20375-5000, USA |
| Выпуск | T46 |
