Hydrogenic Line Widths Produced By EnergyFluctuations In Stellar Atmospheres

机译：恒星大气中的能量流动产生的氢线宽

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A new method for obtaining the widths of spectral lines generated by energy fluctuations is presented. The energy changes of the atomic states are equated with the fractional fluctuations in energy to yield a formula for the line widths. Comparing the formula for the line widths with some published experimental and theoretical values show good agreement.

机译：提出了一种用于获得能量波动产生的谱线宽度的新方法。原子态的能量变化等同于能量的分数波动，以产生线宽的公式。将线宽的公式与一些公布的实验和理论值进行比较，表现出良好的一致性。

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《International Conference on Recent Directions in Astrophysical Quantitative Spectroscopy and Radiation Hydrodynamics》|2009年||共4页
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Octavio Cardona;
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中图分类 P141.5-532;
关键词
experimental; Comparing; fractional;

机译：实验;比较;小;

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1. SYNTHESIZED SPECTRA OF OPTICALLY THIN EMISSION LINES PRODUCED BY THE BIFROST STELLAR ATMOSPHERE CODE, INCLUDING NONEQUILIBRIUM IONIZATION EFFECTS: A STUDY OF THE INTENSITY, NONTHERMAL LINE WIDTHS, AND DOPPLER SHIFTS [J] . K. Olluri1, B. V. Gudiksen1, V. H. Hansteen1, The Astrophysical journal . 2015,第1期

机译：双峰星体大气代码产生的光学薄发射线的合成光谱，包括非平衡电离效应：强度，非热线宽度和多普勒位移的研究
2. ATOMIC LINE WIDTHS BY THERMAL ENERGY FLUCTUATIONS IN STELLAR ATMOSPHERES [J] . O. Cardona Revista Mexicana de Astronomia y Astrofisica . 2011,第Conf期

机译：恒星大气中热能波动引起的原子线宽度
3. Erratum: “The Escape of the Hydrogen-rich Atmosphere of Exoplanets: Mass-loss Rates and the Absorptions of Stellar Lyα” (2019, ApJ, 880, 90) [J] . Dongdong Yan, Jianheng Guo The Astrophysical journal . 2019,第2期

机译：勘误表：“系外行星富氢气氛的逃逸：质量损失率和恒星Lyα的吸收”（2019，ApJ，880，90）
4. Hydrogenic Line Widths Produced By EnergyFluctuations In Stellar Atmospheres [C] . Octavio Cardona International Conference on Recent Directions in Astrophysical Quantitative Spectroscopy and Radiation Hydrodynamics . 2009

机译：恒星大气中的能量流动产生的氢线宽
5. A calculation of the energy spectrum of cosmic ray-produced hydrogen isotopes in the atmosphere [D] . Cooke, Richard Henry -1

机译：大气中宇宙射线产生的氢同位素的能谱计算
6. On the Contours of Stellar Absorption Lines and the Composition of Stellar Atmospheres [O] . Cecilia H. Payne 1928

机译：恒星吸收线的轮廓和恒星大气的组成
7. ATOMIC LINE WIDTHS BY THERMAL ENERGY FLUCTUATIONS IN STELLAR ATMOSPHERES [O] . O. Cardona 2011

机译：由于大气中热能波动的原子线宽度
8. Hydrogen Line Blanketed Model Stellar Atmospheres [R] . Klinglesmith, D. A. 1971

机译：氢线覆盖模型恒星大气

Hydrogenic Line Widths Produced By EnergyFluctuations In Stellar Atmospheres

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