356560 For wavelength of visible radiation of hydrogen spectrum Balmer gave an equation as \(\lambda = \frac{{\left( {k{m^2}} \right)}}{{\left( {{m^2} - 4} \right)}}\), where '\(m\)' is principal quantum number of energy level. The value of \(k\) in terms of Rydberg's constant \(R\) is
356560 For wavelength of visible radiation of hydrogen spectrum Balmer gave an equation as \(\lambda = \frac{{\left( {k{m^2}} \right)}}{{\left( {{m^2} - 4} \right)}}\), where '\(m\)' is principal quantum number of energy level. The value of \(k\) in terms of Rydberg's constant \(R\) is
356560 For wavelength of visible radiation of hydrogen spectrum Balmer gave an equation as \(\lambda = \frac{{\left( {k{m^2}} \right)}}{{\left( {{m^2} - 4} \right)}}\), where '\(m\)' is principal quantum number of energy level. The value of \(k\) in terms of Rydberg's constant \(R\) is
356560 For wavelength of visible radiation of hydrogen spectrum Balmer gave an equation as \(\lambda = \frac{{\left( {k{m^2}} \right)}}{{\left( {{m^2} - 4} \right)}}\), where '\(m\)' is principal quantum number of energy level. The value of \(k\) in terms of Rydberg's constant \(R\) is