When an atom comes down from some higher energy level to the first energy level then emitted lines form of Lyman series. λL1=R121−n21
where R is Rydberg's constant.
When an atom comes from higher energy level to the second level, then Balmer series are obtained. λB1=R221−n21
For maximum wavelength n=2,λL1=R1−(2)21=R1−41=43R….(i) n=3,λB1=R(2)21−(3)21=R365….(ii)
Dividing Eq. (ii) by Eq. (i), we get λBλL=275