Revisiting the emission behavior of the characteristic line <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mn>1</mml:mn><mml:mi>s</mml:mi><mml:mn>2</mml:mn><mml:mi>p</mml:mi><mml:mspace width="0.16em" /><mml:mmultiscripts><mml:mi>P</mml:mi><mml:mn>1</mml:mn><mml:none /><mml:mprescripts /><mml:none /><mml:mn>1</mml:mn></mml:mmultiscripts><mml:mo>→</mml:mo><mml:mn>1</mml:mn><mml:msup><mml:mi>s</mml:mi><mml:mn>2</mml:mn></mml:msup><mml:mspace width="0.16em" /><mml:mmultiscripts><mml:mi>S</mml:mi><mml:mn>0</mml:mn><mml:none /><mml:mprescripts /><mml:none /><mml:mn>1</mml:mn></mml:mmultiscripts></mml:mrow></mml:math> following electron-impact excitation of heliumlike ions-Reference-Cited by-同舟云学术

Revisiting the emission behavior of the characteristic line 1s2pP11→1s2S01 following electron-impact excitation of heliumlike ions

Author:

Wu Z. W.^ORCID,Tian Z. Q.,Dong C. Z.

Funder

National Basic Research Program of China

National Natural Science Foundation of China

Northwest Normal University

Longyuan Youth Innovation and Entrepreneurship Talent Project of Gansu Province of China

Youth Science and Technology Talent Promotion Project of Gansu Provincial Science and Technology Association of China

Publisher

American Physical Society (APS)

Link

Reference47 articles.

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