307582 Balmer gave an equation for wavelength of visible region of H-spectrum as \({\rm{\lambda = }}\frac{{{\rm{K}}{{\rm{n}}^{\rm{2}}}}}{{{{\rm{n}}^{\rm{2}}}{\rm{ - 4}}}}\). Where \({\rm{n = }}\) principal quantum number of energy level, \({\rm{K = }}\) constant in terms of R (Rudberg constant). The value of K in terms of R is:
307582 Balmer gave an equation for wavelength of visible region of H-spectrum as \({\rm{\lambda = }}\frac{{{\rm{K}}{{\rm{n}}^{\rm{2}}}}}{{{{\rm{n}}^{\rm{2}}}{\rm{ - 4}}}}\). Where \({\rm{n = }}\) principal quantum number of energy level, \({\rm{K = }}\) constant in terms of R (Rudberg constant). The value of K in terms of R is:
307582 Balmer gave an equation for wavelength of visible region of H-spectrum as \({\rm{\lambda = }}\frac{{{\rm{K}}{{\rm{n}}^{\rm{2}}}}}{{{{\rm{n}}^{\rm{2}}}{\rm{ - 4}}}}\). Where \({\rm{n = }}\) principal quantum number of energy level, \({\rm{K = }}\) constant in terms of R (Rudberg constant). The value of K in terms of R is:
307582 Balmer gave an equation for wavelength of visible region of H-spectrum as \({\rm{\lambda = }}\frac{{{\rm{K}}{{\rm{n}}^{\rm{2}}}}}{{{{\rm{n}}^{\rm{2}}}{\rm{ - 4}}}}\). Where \({\rm{n = }}\) principal quantum number of energy level, \({\rm{K = }}\) constant in terms of R (Rudberg constant). The value of K in terms of R is:
307582 Balmer gave an equation for wavelength of visible region of H-spectrum as \({\rm{\lambda = }}\frac{{{\rm{K}}{{\rm{n}}^{\rm{2}}}}}{{{{\rm{n}}^{\rm{2}}}{\rm{ - 4}}}}\). Where \({\rm{n = }}\) principal quantum number of energy level, \({\rm{K = }}\) constant in terms of R (Rudberg constant). The value of K in terms of R is: