| タイトル | Stationarity of magnetohydrodynamic fluctuations in the solar wind |
| 本文（外部サイト） | http://hdl.handle.net/2060/19830002737 |
| 著者（英） | Goldstein, M. L.; Matthaeus, W. H. |
| 著者所属（英） | NASA Goddard Space Flight Center |
| 発行日 | 1982-06-01 |
| 言語 | eng |
| 内容記述 | Solar wind research and studies of charged particle propagation often assume that the interplanetary magnetic field represents a stationary random process. The extent to which ensemble averages of the solar wind magnetic fields follow the asymptotic behavior predicted by the ergodic theorem was investigated. Several time periods, including a span of nearly two years, are analyzed. Data intervals which span many solar rotations satisfy the conditions of weak stationarity if the effects of solar rotation are included in the asymptotic analysis. Shorter intervals which include a small integral number of interplanetary sectors also satisfy weak stationarity. The results are illustrated using magnetometer data from the ISEE-3, Voyager and IMP spacecraft. |
| NASA分類 | SOLAR PHYSICS |
| レポートNO | 83N11007
NASA-TM-83963
NAS 1.15:83963 |
| 権利 | No Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/164511 |
