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Asgari-Targhi研究室
Showing the original Japanese · View translation
太陽の磁場と乱流が大気を温めるしくみを解き明かす研究室。
AboutAbout the lab
太陽の大気を温めるのは、磁場と乱流。
Asgari-Targhi研究室は、
磁場と
そこから、
同じ
Key terms
- コロナ
- 太陽の
表面の 外側に 広がる、うすくて 非常に 高温の ガスの 層 - 太陽風
- 太陽から
絶えず 吹き出し、 太陽系の 中を 流れていく プラズマの 流れ - 磁気リコネクション
- 磁力線の
つながり方が 組み 変わり、 たくわえられていた 磁場の エネルギーが 解き放たれる 現象
ResearchResearch themes
磁場と
*Illustrative image太陽大気の磁場と乱流
光球から
*Illustrative imageコロナ加熱と太陽風
太陽大気で
*Illustrative image恒星と銀河の磁場
太陽の
MembersFaculty
- ProfessorASGARI-TARGHI Mahboubeh
VoicesStudent voices
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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.
- Top image: “Traceimage” NASA / Public domain (cropped)
- 太陽大気の
磁場と 乱流: “Solar granulation” PetrusQ / CC BY 4.0 (cropped) - コロナ加熱と
太陽風: “05 Coronal Mass Ejection ( )” NASA/SOHO / Public domain (cropped) - 恒星と
銀河の 磁場: “Messier83 - Heic1403a” Credit: NASA, ESA, and the Hubble Heritage Team (STScI/AURA) Acknowledgement: William Blair (Johns Hopkins University) / 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 (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 (関研究室
（宇宙環境・惑星圏科学分野／Seki Lab） ): “Aurora Australis From ISS” ISS Expedition 23 crew / Public domain (cropped)
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