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Bibliographic Record
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- Material Type
- 文書・図像類
- Author/Editor
- 松元, 亮治
- Author Heading
- Text Language Code
- eng
- Subject Heading
- NDC
- Target Audience
- 一般
- Note (General)
- type:textRapid fluctuation with a frequency dependence of 1/f (with ' 1-2) is characteristic of radiationfrom black-hole objects. Its origin remains poorly understood. We examine the three-dimensional mag-netohydrodynamical (MHD) simulation data, finding that a magnetized accretion disk exhibits both 1/ffluctuation (with '2) and a fractal magnetic structure (with the fractal dimension of D1.9). The frac-tal field configuration leads reconnection events with a variety of released energy and of duration, therebyproducing 1/f fluctuations.
- Access Restrictions
- 限定公開