Abstract
The radiative lifetime of metastable N+(S25) has been measured to be 4.2±0.6 msec, a value generally in agreement with theory, by direct monitoring of the spontaneous emission from ∼ 106 N+ ions stored in a radio-frequency ion trap. Additional measurements were made of the quenching rate coefficient (2.5×109 cm3 sec1) and the production cross section (≥ 1018 cm2) of N+(S25) in N2. This work supports the interpretation of the 2145-Å feature in the spectrum of aurorae as being due to N+(S25) emission.