Time Variations of the Barometric Coefficient of Cosmic Ray Neutron Component at Morioka, Tokyo and Mt. Norikura during the Period 1970-1973
スポンサーリンク
概要
- 論文の詳細を見る
In this paper, trial calculations of the barometric coefficient by various methodsare given using the neutron component observed at Morioka, Tokyo, Mt. Norikura. andDeep River during the period, January 1970 - December 1973. The results of the calculationsobtained are discussed in comparison with each other. It was found that themethod by multiple correlation is the best one among three methods used here, that is,method by deviation, method by single correlation, and the above one. The variabletendency of the barometric coefficients with solar activity as pointed out by Bachelet etal. and others was not found clearly because of the short period of analysis. It will bepossible to derive a significant conclusion about the long-term variation of the barometriccoefficients by developing this study over a longer period.
- 岩手大学教育学部の論文
著者
関連論文
- 12p-KA-4 ニユートロンモニターによる宇宙線異方性の観測
- 6p-FF-4 宇宙線のSpherical Zonal Componentsと惑星間プラズマ
- 7p-F-3 宇宙線の異方性における27日周期変化
- Observation of Cosmic Ray Neutron Intensity at Morioka Part III. Cosmic Ray Neutron Intensities Observed during August 1970 - January 1975
- 28p-C-12 宇宙線異方性の27日周期変化
- 1p-B-2 低精度における地上および山上宇宙線日変化の比較II
- 14a-C-4 宇宙線中性子計にもとずく宇宙線異方性の比較
- 30p-A-9 宇宙線中性子成分方向測定による宇宙線異方性
- 1a-SE-1 フォーブッシュ減少時における宇宙線リジィディティスペクトル
- 6a-FF-6 宇宙線中性子成分の計数記録システム
- 28a-ME-8 盛岡(岩手大)における宇宙線中性子線分の観測計画
- 9p-YE-2 盛岡(岩手大)におけるNM-64型カウンターによる宇宙線中性子成分の観測
- Correlation between Cosmic Ray Neutron Intensities in Morioka and Tokyo during a Solar Rotation
- Time Variations of the Barometric Coefficient of Cosmic Ray Neutron Component at Morioka, Tokyo and Mt. Norikura during the Period 1970-1973
- 14p-B-13 宇宙線中性子成分気圧効果係数の長期変化
- 5p-A-11 盛岡における宇宙線中性子強度変化の測定
- 11p-D-1 盛岡における宇宙線中性子強度変化
- 3a-S-1 宇宙線中性子計による気圧効果計数
- 10a-C-10 惑星間空間における宇宙線の Spherical Zonal Components
- 11p-D-2 太陽自転周期の間の宇宙線Rigidity Spectrum