The Overview of the Balmer series

Overview of Balmer Series n = 3 410 nm 400 Energy n = 2 Balmer series of the hydrogen spectrum n = 1 Balmer series Hydrogen visible spectrum 434 nm 486 nm Balmer series Energy levels 656 nm ℗ @kameswariservices Electron transitions Hydrogen electron transitions from the higher energy levels to n = 2 give spectral lines in the visible & UV regions of the electromagnetic spectrum . n = 6 n = 5 n = 4 n = 3 n = 2 500 Wavelength expressed in nanometers 2p - orbital 2s - orbital n = 1 Hydrogen alpha spectral line Hydrogen alpha transition Balmer series in visible region 1s - orbital Low resolution spectrometer view UV Ground state of the electron The Hydrogen - alpha doublet sse Visible Visible UV 600 Hydrogen - alpha spectral line The spectral emissions in the visible and ultraviolet regions of the hydrogen spectrum . _j = 1 / 2 j = 3/2 Y - rays view X - rays 10-16 10 - ¹4 10-12 10:10 High resolution spectrometer 700 750 400 The hydrogen alpha doublet Visible spectrum Hydrogen emission spectrum The visual representation of hydrogen emission and hydrogen absorption spectra The ultraviolet and visible spectral lines chart for the Balmer series of the hydrogen spectrum . IR - rays Microwave 10⁰ 104 104 10³ FM Radio waves Electromagnetic spectrum 10 ° 10 ORION NEBULAS THE ORION NEBULA IS A DIFFUSE NEBULA SITUATED N THE MILKY WAY , BEING SOUTH OF ORION'S BELT IN THE CONSTELLATION OF ORION . 10⁰ UV Balmer spectrum Balmer break Long radio waves Hydrogen absorption spectrum 10 O @ chemistrylearners The hydrogen alpha emissions in the ionized hydrogen electron clouds or in the Orion Nebula The Balmer formula 700 Orion Nebula in the galaxy 108 2 - ₁ ( ² - ² ) - ^ ( - ²² ) = h h -22 For more information on the Balmer series , please visit this blog post ; https://jayamchemistrylearners.blog spot.com/2022/03/balmer-series chemistry - learners.html