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吉越研究室(宇宙線研究所 高エネルギー宇宙線研究部門)
Showing the original Japanese · View translation
超高エネルギーのガンマ線で、宇宙で最もエネルギーの大きな天体活動を観測する研究室。
AboutAbout the lab
ガンマ線で、宇宙線の起源に迫る。
吉越研究室は、
解像型大気チェレンコフ望遠鏡アレイと
超新星残骸や
Key terms
- ガンマ線
- 光
（電磁波）の 仲間の うち、 いちばん エネルギーが 高い もの - 大気チェレンコフ望遠鏡
- ガンマ線が
大気に 飛び込んだ ときに 出るかすかな 青白い 光を とらえ、 ガンマ線を 観測する 地上の 望遠鏡 - 超新星残骸
- 重い星が
一生の 最後に 大爆発した あと、 飛び散った ガスが 広がって 光っている 天体
ResearchResearch themes
解像型大気チェレンコフ望遠鏡アレイと
MembersFaculty
- Associate Professor吉越 貴紀Publications ↗
VoicesStudent voices
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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: “VERITAS array” VERITAS / Public domain (cropped)
- 超
高エネルギーガンマ線天体の 観測: “Cherenkov Telescope Array LST-1” Whyistheskyblue1 / CC BY-SA 4.0 (cropped)
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