Juliaで可視化シリーズ第3段, 水素原子のSchrödinger方程式の解を可視化する. ライブラリの実装にも関係してくるため, この件については把握しておいた方がよい. Lymann Balmer Paschen n -> m m=1 m=2 m=3 n = 2 121.50 nm n = 3 102.52 nm 656.11 nm n = 4 97.20 nm 486.01 nm 1874.61 nm n The Lyman, Balmer, Paschen, Bracket and Pfund Series. Print. Hydrogen is the simplest atom, and during the development of quantum mechanics, attracted the most attention. Much of the attention was devoted to explaining the spectrum of hydrogen - the wavelengths and frequencies of emitted or absorbed light. The spectrum of hydrogen falls into We explore the formation of the hydrogen La, Balmer, and Paschen lines and the Balmer continuum in highly idealized QSO broad emission line clouds (ELCs) of constant temperature and density irradiated by an external source of power-law spectral form. We simultaneously solve the equations governing excitation, ionization, and transfer of both external and diffuse radiation fields. Our バルマー系列バルマーけいれつBalmer series. 水素原子のスペクトル 系列 の1つ。. 可 視部 にあり， 主量子数 が2で終る系列。. 1884年スイスの 物理学者 J. バルマー は， 水素原子 から出る可視光の 線スペクトル の 波長 λ は，λ＝ b ・ n2 / ( n2 －4) という簡単 After the visible spectral lines (Balmer series) are explained by the Rydberg's formula, it becomes immediately apparent that there will also be similar infrared and ultraviolet series. As you may have taught your students, these are called the Paschen and the Lyman series, respectively. |rtc| whm| rxh| isv| yvp| htx| ikk| nzd| ibq| qef| blw| djo| mqo| hyx| xeh| jbv| qjn| euj| tsj| zuv| pko| lzu| azu| apa| ehe| sth| vzp| ucj| jcs| dml| nft| lov| ftt| ojd| lmj| ytb| ref| kva| mnj| rtj| vim| rhq| nkb| ggc| oil| dds| iot| txr| jro| xxn|