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関研究室（宇宙環境・惑星圏科学分野／Seki Lab）
Showing the original Japanese · View translation
オーロラや大気散逸から、惑星をとりまく宇宙環境を探る研究室。
AboutAbout the lab
宇宙天気を知り、住める惑星の条件を探る。
関研究室は、
地表から
科学衛星に
宇宙天気現象の
Key terms
- 宇宙天気
- 太陽
表面や 宇宙空間、 惑星圏の 状態の 変動。 オーロラや宇宙放射線の 変化を ふく む - プラズマ
- 原子が
電子と イオンに 分かれた 状態の 気体。 宇宙 空間の 物質の 多くは この 状態に ある - 大気散逸
- 惑星の
大気が 宇宙空間へ 逃げていく こと。 惑星の 表層の 環境の 移り 変わりを 左右する
NewsLab news
巨大磁気嵐の
発達の カギが 地球起源の 重イオンと 判明 博士課程の
学生が、 日本地球惑星科学連合2025年大会 学生優秀発表賞を 受賞 学生が、
SGEPSS第156回講演会 最優秀発表賞 （オーロラメダル）を 受賞 2024年5月に
日本に 現れた オーロラの 色の 謎を 解明 関教授が
COSPAR William Nordberg Medalを 受賞
ResearchResearch themes
宇宙天気現象の
*Illustrative imageジオスペース環境変動
太陽から
*Illustrative image火星の宇宙放射線とオーロラ
火星は
*Illustrative image火星の大気散逸と気候変動
約40億年前の
*Illustrative image固有磁場と大気散逸
惑星の
MembersFaculty
関研究室の
- Professor関 華奈子Publications ↗
- Associate Professor原 拓也
- Assistant Professor坂田 遼弥Publications ↗
- Associate Professor (Collaborative Faculty)片岡 龍峰
- Assistant Professor (Affiliated Faculty)桂華 邦裕
VoicesStudent voices
Compiled from answers by students who were in the lab. Ratings and reviews reflect individual students' experiences, not the lab's official views.
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On a 4-point scale, ● marks where students' answers fall
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RelatedLabs similar to 関研究室（宇宙環境・惑星圏科学分野／Seki Lab）
The information on this page is compiled by the LabLog team from the lab's public information and interviews. For corrections or removal requests, please contact LabLog, not the lab.
Report an errorAbout the images
The top and research theme images are illustrative and were not taken at the lab. They are cropped from Wikimedia Commons images. Cropped CC BY-SA images are provided under the same CC BY-SA license as the original (version shown on each line).
- Top image: “Aurora Australis From ISS” ISS Expedition 23 crew / Public domain (cropped)
- ジオスペース環境
変動: “Aurora Seen From Space by NASA” NASA / Public domain (cropped) - 火星の
宇宙放射線と オーロラ: “Solar Storm Excites Martian Magnetosphere (SVS5502 - marsMagnetosphere VelTracersExtended 9-6-2024a jmag normal flightA noAnnotation 4k 00420 print)” NASA's Scientific Visualization Studio / Public domain (cropped) - 火星の
大気散逸と 気候 変動: “Mars Valles Marineris EDIT” NASA （バイキング1号オービター） / Public domain (cropped) - 固有磁場と
大気散逸: “Simulation of Mercury’s magnetic environment ESA501859” European Space Agency / CC BY-SA 3.0 igo (cropped) - Related lab (天野研究室): “Supernova Remnant SN 1006” X-ray: NASA/CXC/Rutgers/G.Cassam-Chenaï, J.Hughes et al.; Radio: NRAO/AUI/NSF/GBT/VLA/Dyer, Maddalena & Cornwell; Optical: Middlebury College/F.Winkler, NOAO/AURA/NSF/CTIO Schmidt & DSS / CC BY 4.0 (cropped)
- Related lab (齋藤・篠原研究室
（宇宙プラズマ研究系） ): “Aurora borealis over Eielson Air Force Base, Alaska” United States Air Force photo by Senior Airman Joshua Strang / Public domain (cropped) - Related lab
(清水(敏文)研究室): “SOLAR-B artists concept” NASA/GSFC/C. Meaney / Public domain (cropped) - Related lab (今田研究室): “February 16, 2024 X2 5 Solar Flare (SVS14531 - SDO )” NASA's Scientific Visualization Studio - A. J. Christensen, Scott Wiessinger / Public domain (cropped)
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