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- 藤岡 慎介
- 大阪大学 レーザーエネルギー学研究センター
書誌事項
- タイトル別名
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- Laboratory X-ray Astronomy with High Power Laser
- パワーレーザー デ ヒラク ジッケンシツXセン テンモンガク ノ カノウセイ
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説明
Laser produced plasma is one of the brilliant x-ray source that has unique capabilities for use in a wide range of science. Here, we introduce that laser-produced x-ray source is very useful to simulate x-ray astronomical phenomena in the laboratory. A 0.5-keV Planckian x-ray source was created with laser driven implosion for producing non-local-thermodynamical-equilibrium (non-LTE) photoionized plasmas, which is a key to understand astronomical compact objects. Laboratory experiment of non- LTE photoionized plasma offers novel test bed for validation and verification of computational codes used in x-ray astronomy. Recently, it is demonstrated that kilo-tesla magnetic field can be generated by using capacitor-coil targets driven by high power laser beam. This strong magnetic field will offer new controll parameter to the laboratory x-ray astrophysics.
収録刊行物
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- レーザー研究
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レーザー研究 44 (9), 589-, 2016
一般社団法人 レーザー学会
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詳細情報 詳細情報について
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- CRID
- 1390568456337191936
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- NII論文ID
- 130007957323
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- NII書誌ID
- AN00255326
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- ISSN
- 13496603
- 03870200
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- NDL書誌ID
- 027671396
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- 本文言語コード
- ja
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- データソース種別
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- JaLC
- NDL
- Crossref
- CiNii Articles
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- 抄録ライセンスフラグ
- 使用不可