| タイトル | Methods and software for cosmic ray scintillation studies |
| 本文（外部サイト） | http://hdl.handle.net/2060/19850026819 |
| 著者（英） | Prilutsky, R. E.; Dorman, L. I.; Gulinsky, O. V. |
| 著者所属（英） | Academy of Sciences (USSR) |
| 発行日 | 1985-08-01 |
| 言語 | eng |
| 内容記述 | The principal instrument used in cosmic ray scintillation studies is the spectra constructed from intensive observation. This method has its drawbacks in that the statistical characteristics of the process undergo essential reconstruction, i.e., the process becomes nonstationary from the viewpoint of such phenomena as Forbush decrease and during solar flares. The software used to process the above includes the direct Fourier transform and its modifications, autoregressive processes, and instantaneous spectrum methods. Used in various combinations, they prove helpful in handling the time series. |
| NASA分類 | SPACE RADIATION |
| レポートNO | 85N35132
SH-9.1-17 |
| 権利 | No Copyright |
|
