| タイトル | A study of coronal bright points at 20 cm wavelength |
| 著者（英） | Nitta, N.; Kundu, M. R. |
| 著者所属（英） | Maryland Univ. |
| 発行日 | 1988-01-01 |
| 言語 | eng |
| 内容記述 | The paper presents the results of a study of coronal bright points observed at 20 cm with the VLA on a day when the sun was exceptionally quiet. Microwave maps of bright points were obtained using data for the entire observing period of 5 hours, as well as for shorter periods of a few minutes. Most bright points, especially those appearing in the full-period maps, appear to be associated with small bipolar structures on the photospheric magnetogram. Overlays of bright point (BP) maps on the Ca(+) K picture, show that the brightest part of BP tends to lie on the boundary of a supergranulation network. |
| NASA分類 | SOLAR PHYSICS |
| レポートNO | 89A19062 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/366469 |
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