stsw1.stelab.nagoya-u.ac.jp

Solar Wind Group [Japanese Page]

Link to English page, click here. Ê Ê ü û q w z E z T O Ì È º H x(HTML Å). Å w @ Ä à æ è(PDF). Ú { w m ï Proceedings of the Japan Academy, Ser. B, Vol. 89 No. 2 (2013). Munetoshi TOKUMARU, Three-dimensional exploration of the solar wind using observations of interplanetary scintillation. STEL Newsletter æ è. IPS Ï ª f [ ð p z å K ÍMHD V [ V F Ø ª ê(PDF). Z Ì ä ð T é V µ d g ] z C [ W O u F Û @ (PDF). Z É å ú Ì z F Ø ª ê(PDF). F Ô ó Ô V ` [ V Ï ª Ì x F X(PDF). Ú { n f È w A j [ X [JGL æ è. Z v Y } F X(PDF).

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Solar Wind Group [Japanese Page] | stsw1.stelab.nagoya-u.ac.jp Reviews

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Link to English page, click here. Ê Ê ü û q w z E z T O Ì È º H x(HTML Å). Å w @ Ä à æ è(PDF). Ú { w m ï Proceedings of the Japan Academy, Ser. B, Vol. 89 No. 2 (2013). Munetoshi TOKUMARU, Three-dimensional exploration of the solar wind using observations of interplanetary scintillation. STEL Newsletter æ è. IPS Ï ª f [ ð p z å K ÍMHD V [ V F Ø ª ê(PDF). Z Ì ä ð T é V µ d g ] z C [ W O u F Û @ (PDF). Z É å ú Ì z F Ø ª ê(PDF). F Ô ó Ô V ` [ V Ï ª Ì x F X(PDF). Ú { n f È w A j [ X [JGL æ è. Z v Y } F X(PDF).

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Solar Wind Group [Japanese Page] | stsw1.stelab.nagoya-u.ac.jp Reviews

https://stsw1.stelab.nagoya-u.ac.jp

Link to English page, click here. Ê Ê ü û q w z E z T O Ì È º H x(HTML Å). Å w @ Ä à æ è(PDF). Ú { w m ï Proceedings of the Japan Academy, Ser. B, Vol. 89 No. 2 (2013). Munetoshi TOKUMARU, Three-dimensional exploration of the solar wind using observations of interplanetary scintillation. STEL Newsletter æ è. IPS Ï ª f [ ð p z å K ÍMHD V [ V F Ø ª ê(PDF). Z Ì ä ð T é V µ d g ] z C [ W O u F Û @ (PDF). Z É å ú Ì z F Ø ª ê(PDF). F Ô ó Ô V ` [ V Ï ª Ì x F X(PDF). Ú { n f È w A j [ X [JGL æ è. Z v Y } F X(PDF).

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stsw1.stelab.nagoya-u.ac.jp

1

ISEE IPS Array

http://stsw1.stelab.nagoya-u.ac.jp/uhf_ant.html

UHF Radio Telescope Array. UHF Radio Telescope at Fuji Station. Photos of ISEE UHF Radio Telescopes. Solar Wind Imaging Facility Telescope, Toyokawa (SWIFT). Fuji IPS Telescope (FIT). Kiso IPS Telescope (KIT). Location of Observation Sites. Geographic Locations of Observation Sites. 137 deg.E 22'09". 34 deg.N 50'05". 138 deg.E 36'42". 35 deg.N 25'36". 137 deg.E 37'49". 35 deg.N 47'34". 138 deg.E 19'16". 36 deg.N 31'12". Asymmetric Cylindrical Parabolic Reflector Antenna. 74m E-W, 27m N-S (Kiso).

2

Toyokawa IPS Workshop 2007

http://stsw1.stelab.nagoya-u.ac.jp/ips_toyokawa.html

Thank you for joining the Toyokawa IPS Workshop held on October 30-31, 2007. October 30 (Tue) and 31 (Wed), 2007. Toyokawa City Plaza (Toyokawa, Aichi, Japan). Information of Toyokawa city is available via http:/ www.city.toyokawa.lg.jp/english/index.html. Session 1: (talks and discussions). Session 2: (talks and discussions). Session 3: (talks and discussions). Session 4: (talks and discussions). Excursion to Toyokawa Observatory and "Toyokawa Inari". Check in : 3:00 PM. Access Map to Toyokawa.

3

IPS Observations of the Solar Wind

http://stsw1.stelab.nagoya-u.ac.jp/ips_data.html

CAT解析によるSynoptic Map anonymous ftp. CAT解析によるSynoptic Map http menu. 速度の時間変化電波源毎, V-plot. 惑星における太陽風データ MHD IPS Tomography解析による. Kojima, M. and T. Kakinuma. Solar cycle dependence of global distribution of the solar wind speed, Space Sci. Rev., 53. Asai, K., Y. Ishida, M. Kojima, K. Maruyama, H. Misawa, and N. Yoshimi. Multi-station system for solar wind observations using the interplanetary scintillation method, J. Geomag. Geoelectr., 47.

4

Snapshot

http://stsw1.stelab.nagoya-u.ac.jp/snapshot.html

Photo Album of Solar Wind Group. ２０１６年８月６日土７日日. ６日１５１６時に東大木曽天文台で、電波のまたたきで宇宙の風を探る徳丸という題目の講演を行いましたインターネットでも中継. ２０１５年８月８日土９日日. ２０１３年８月３日土４日日. Stanford VLFチームが観測システムを設置２０１２年１１月２６日２７日. ２０１２年８月４日土５日日. アラバマ大学ハンツビル校のTae Kim来訪 JPSPサマープログラム２０１２年６月１９日８月２１日. ２０１１年８月６日土７日日. ２０１０年８月７日土８日日. ７日午後には、東大木曽天文台で講演題目太陽と地球をつなぐ宇宙の風を行いました。９８年８月８日土９日日. 木曽観測所特別公開９７年８月９日土１０日日.

5

Information

http://stsw1.stelab.nagoya-u.ac.jp/info.html

７月１６日土、１７日日、自己推薦入試. ８月２４日水２６日金、一般選抜入試. ２０１６年８月６日(土)午後から７日日午前、木曽観測所一般公開. ２０１５年３月３１日火、プレスリリース. ２０１５年２月１８日水、プレスリリース. ２０１４年３月１１日火、プレスリリース. ２０１３年１１月２３日(土) ２４日日、国際IPSワークショップ. 豊川のアンテナがＮＨＫ教育ＴＶ高校講座地学１学期大８回太陽の中で紹介されています平成２１２３年放映。一般向け小冊子太陽太陽風５０のなぜが出版されました。

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astroarts.co.jp

電波のまたたきでとらえたアイソン彗星のイオンテイル - アストロアーツ

http://www.astroarts.co.jp/news/2015/02/23ison/index-j.shtml

星を見る宇宙を知る天文を楽しむ AstroArts. 名古屋大学と日本大学の共同研究チームが、2013年11月に太陽に最接近して消滅したアイソン彗星 C/2012 S1 の尾を、電波のまたたき現象を利用した観測でとらえることに成功した。伊集朝哉さん名古屋大学らは愛知県豊川市などに設置された専用アンテナを使って、太陽風太陽からのプラズマ粒子の流れごしに見る遠方の電波源のまたたき interplanetary scintillation IPS現象を調べている。 Icarus Plasma distribution of Comet ISON (C/2012 S1) observed using the radio scintillation method. 名古屋大学太陽風研究室 http:/ stsw1.stelab.nagoya-u.ac.jp/. 投稿画像ギャラリーアイソン彗星 C/2012 S1. The Greatest Comets in History. 2013/12/12 - 明かされゆくアイソン彗星の正体まずは大きさと組成.

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stsw1.stelab.nagoya-u.ac.jp

Solar Wind Group [Japanese Page]

Link to English page, click here. Ê Ê ü û q w z E z T O Ì È º H x(HTML Å). Å w @ Ä à æ è(PDF). Ú { w m ï Proceedings of the Japan Academy, Ser. B, Vol. 89 No. 2 (2013). Munetoshi TOKUMARU, Three-dimensional exploration of the solar wind using observations of interplanetary scintillation. STEL Newsletter æ è. IPS Ï ª f [ ð p z å K ÍMHD V [ V F Ø ª ê(PDF). Z Ì ä ð T é V µ d g ] z C [ W O u F Û @ (PDF). Z É å ú Ì z F Ø ª ê(PDF). F Ô ó Ô V ` [ V Ï ª Ì x F X(PDF). Ú { n f È w A j [ X [JGL æ è. Z v Y } F X(PDF).

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