WEKO3
アイテム
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Special issue"}]}]}, "item_1_creator_8": {"attribute_name": "著者名(英)", "attribute_type": "creator", "attribute_value_mlt": [{"creatorNames": [{"creatorName": "Yumoto,Kiyohumi", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "1387", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Saito,Takao", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "58231", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Tsurutani,Bruce T.", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "58232", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Smith,Edward J.", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "58233", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Akasofu,Syun-Ichi", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "58234", "nameIdentifierScheme": "WEKO"}]}]}, "item_1_description_1": {"attribute_name": "ページ属性", "attribute_value_mlt": [{"subitem_description": "P(論文)", "subitem_description_type": "Other"}]}, "item_1_description_12": {"attribute_name": "抄録(英)", "attribute_value_mlt": [{"subitem_description": "Daytime Pc 3-4 pulsation activities observed at globally coordinated low-latitude stations [SGC (L=1.8,λ=118.0°W), EWA (1.15,158.1°W), ONW (1.3,141.5°E)] are evidently controlled by the cone angle θ_\u003cXB\u003e of the IMF observed at ISEE 3. Moreover, the Pc 3-4 frequencies (\u0026fnof;) at the low latitudes and high latitude (COL; L=5.6 and λ=147.9°W) on the ground and that of compressional waves at geosynchronous orbit (GOES 2; L=6.67 and λ=106.7°W) are simultaneously correlated with the IMF magnitude (B_\u003cIMF\u003e). The correlation of \u0026fnof; of the compressional Pc 3-4 waves at GOES 2 against B_\u003cIMF\u003e is higher than those of the Pc 3-4 pulsations at the globally coordinated ground stations, i. e., γ=0.70 at GOES 2,and (0.36,0.60,0.66,0.54) at (COL, SGC, EWA, ONW), respectively. The standard deviation (σ_n=±Δ\u0026fnof;mHz) of the observed frequencies from the form \u0026fnof; (mHz)=6.0×B_\u003cIMF\u003e(nT) is larger at the ground stations than at GOES 2,i. e., Δ\u0026fnof;=±6.6mHz at GOES 2,and ±(13.9,9.1,10.7,12.1) mHz at (COL, SGC, EWA, ONW), respectively. The correlations between the IMF magnitude B_\u003cIMF\u003e and Pc 3-4 frequencies at the low latitudes are higher than that at the high latitude on the ground, which can be interpreted as a \"filtering action\" of the magnetosphere for daytime Pc 3-4 magnetic pulsations. The scatter plots of pulsation frequencies observed in the magnetosphere versus the IMF magnitude show a remarkable distribution restricted within the forms of \u0026fnof;=4.5×B_\u003cIMF\u003e and \u0026fnof;=7.5×B_\u003cIMF\u003e. The observed frequency range is theoretically confirmed to be consistent with the inferred frequency range (ω_\u003csc\u003e/Ω_i=0.3-0.5) in the spacecraft frame of the magnetosonic upstream waves excited by the anomalous ion cyclotron resonance with reflected ion beams, which is observed to be V_∥=650-1150km/s in the solar wind frame by the ISEE satellite in the earth\u0027s foreshock. It is concluded that the magnetosonic right-handed waves excited by the reflected ion beams in the earth\u0027s foreshock are convected through the magnetosheath to the magnetopause, being transmitted into the magnetosphere without significant changes in spectra, and then couple with various HM waves in the Pc 3-4 frequency range at various locations in the magnetosphere.", "subitem_description_type": "Other"}]}, "item_1_source_id_13": {"attribute_name": "雑誌書誌ID", "attribute_value_mlt": [{"subitem_source_identifier": "AA00733561", "subitem_source_identifier_type": "NCID"}]}, "item_1_text_10": {"attribute_name": "著者所属(英)", "attribute_value_mlt": [{"subitem_text_language": "en", "subitem_text_value": "Onagawa Magnetic Observatory and Geophysical Institute, Tohoku University/Onagawa Magnetic Observatory and Geophysical Institute, Tohoku University/Jet Propulsion Laboratory, California Institute of Technology/Jet Propulsion Laboratory, California Institute of Technology/Geophysical Institute,University of Alaska"}]}, "item_files": {"attribute_name": "ファイル情報", "attribute_type": "file", "attribute_value_mlt": [{"accessrole": "open_date", "date": [{"dateType": "Available", "dateValue": "1985-07-01"}], "displaytype": "detail", "download_preview_message": "", "file_order": 0, "filename": "KJ00000012374.pdf", "filesize": [{"value": "2.4 MB"}], "format": "application/pdf", "future_date_message": "", "is_thumbnail": false, "licensetype": "license_6", "mimetype": "application/pdf", "size": 2400000.0, "url": {"label": "KJ00000012374", "url": "https://nipr.repo.nii.ac.jp/record/1742/files/KJ00000012374.pdf"}, "version_id": "a3aa139b-b868-4f3d-a536-6b8446cc281a"}]}, "item_language": {"attribute_name": "言語", "attribute_value_mlt": [{"subitem_language": "eng"}]}, "item_resource_type": {"attribute_name": "資源タイプ", "attribute_value_mlt": [{"resourcetype": "departmental bulletin paper", "resourceuri": "http://purl.org/coar/resource_type/c_6501"}]}, "item_title": "Effects of the interplanetary magnetic field on the characteristics of Pc 3-4 pulsations at globally coordinated stations", "item_titles": {"attribute_name": "タイトル", "attribute_value_mlt": [{"subitem_title": "Effects of the interplanetary magnetic field on the characteristics of Pc 3-4 pulsations at globally coordinated stations", "subitem_title_language": "en"}]}, "item_type_id": "1", "owner": "4", "path": ["390"], "permalink_uri": "https://nipr.repo.nii.ac.jp/records/1742", "pubdate": {"attribute_name": "公開日", "attribute_value": "1985-07-01"}, "publish_date": "1985-07-01", "publish_status": "0", "recid": "1742", "relation": {}, "relation_version_is_last": true, "title": ["Effects of the interplanetary magnetic field on the characteristics of Pc 3-4 pulsations at globally coordinated stations"], "weko_shared_id": 4}
Effects of the interplanetary magnetic field on the characteristics of Pc 3-4 pulsations at globally coordinated stations
https://nipr.repo.nii.ac.jp/records/1742
https://nipr.repo.nii.ac.jp/records/17423723a4d2-d125-4a61-b3a3-31ffc3c745b5
名前 / ファイル | ライセンス | アクション |
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KJ00000012374 (2.4 MB)
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Item type | 紀要論文(ELS) / Departmental Bulletin Paper(1) | |||||
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公開日 | 1985-07-01 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Effects of the interplanetary magnetic field on the characteristics of Pc 3-4 pulsations at globally coordinated stations | |||||
言語 | ||||||
言語 | eng | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||
資源タイプ | departmental bulletin paper | |||||
ページ属性 | ||||||
内容記述タイプ | Other | |||||
内容記述 | P(論文) | |||||
著者名(英) |
Yumoto,Kiyohumi
× Yumoto,Kiyohumi× Saito,Takao× Tsurutani,Bruce T.× Smith,Edward J.× Akasofu,Syun-Ichi |
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著者所属(英) | ||||||
en | ||||||
Onagawa Magnetic Observatory and Geophysical Institute, Tohoku University/Onagawa Magnetic Observatory and Geophysical Institute, Tohoku University/Jet Propulsion Laboratory, California Institute of Technology/Jet Propulsion Laboratory, California Institute of Technology/Geophysical Institute,University of Alaska | ||||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Daytime Pc 3-4 pulsation activities observed at globally coordinated low-latitude stations [SGC (L=1.8,λ=118.0°W), EWA (1.15,158.1°W), ONW (1.3,141.5°E)] are evidently controlled by the cone angle θ_<XB> of the IMF observed at ISEE 3. Moreover, the Pc 3-4 frequencies (ƒ) at the low latitudes and high latitude (COL; L=5.6 and λ=147.9°W) on the ground and that of compressional waves at geosynchronous orbit (GOES 2; L=6.67 and λ=106.7°W) are simultaneously correlated with the IMF magnitude (B_<IMF>). The correlation of ƒ of the compressional Pc 3-4 waves at GOES 2 against B_<IMF> is higher than those of the Pc 3-4 pulsations at the globally coordinated ground stations, i. e., γ=0.70 at GOES 2,and (0.36,0.60,0.66,0.54) at (COL, SGC, EWA, ONW), respectively. The standard deviation (σ_n=±ΔƒmHz) of the observed frequencies from the form ƒ (mHz)=6.0×B_<IMF>(nT) is larger at the ground stations than at GOES 2,i. e., Δƒ=±6.6mHz at GOES 2,and ±(13.9,9.1,10.7,12.1) mHz at (COL, SGC, EWA, ONW), respectively. The correlations between the IMF magnitude B_<IMF> and Pc 3-4 frequencies at the low latitudes are higher than that at the high latitude on the ground, which can be interpreted as a "filtering action" of the magnetosphere for daytime Pc 3-4 magnetic pulsations. The scatter plots of pulsation frequencies observed in the magnetosphere versus the IMF magnitude show a remarkable distribution restricted within the forms of ƒ=4.5×B_<IMF> and ƒ=7.5×B_<IMF>. The observed frequency range is theoretically confirmed to be consistent with the inferred frequency range (ω_<sc>/Ω_i=0.3-0.5) in the spacecraft frame of the magnetosonic upstream waves excited by the anomalous ion cyclotron resonance with reflected ion beams, which is observed to be V_∥=650-1150km/s in the solar wind frame by the ISEE satellite in the earth's foreshock. It is concluded that the magnetosonic right-handed waves excited by the reflected ion beams in the earth's foreshock are convected through the magnetosheath to the magnetopause, being transmitted into the magnetosphere without significant changes in spectra, and then couple with various HM waves in the Pc 3-4 frequency range at various locations in the magnetosphere. | |||||
雑誌書誌ID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AA00733561 | |||||
書誌情報 |
Memoirs of National Institute of Polar Research. Special issue 巻 36, p. 15-26, 発行日 1985-07 |