[摘要] The chemistry of peroxynitric acid (HO
2NO
2) and methylperoxynitrate (CH
3O
2NO
2)is predicted to be particularlyimportant in the upper troposphere where temperatures are frequently lowenough that these compounds do not rapidly decompose. At temperatures below240K, we calculate that about 20% of NO
y in the mid- andhigh-latitude upper troposphere is HO
2NO
2. Under these conditions,the reaction of OH with HO
2NO
2 is estimated to account for as muchas one third of the permanent loss of hydrogen radicals. During theTropospheric Ozone Production about the Spring Equinox (TOPSE) campaign, weused thermal dissociation laser-induced fluorescence (TD-LIF) to measure thesum of peroxynitrates (
PNs
HO
2NO
2+CH
3O
2NO
2+PAN+PPN+...) aboard the NCAR C-130research aircraft. We infer the sum of HO
2NO
2 andCH
3O
2NO
2 as the difference between
PN measurementsand gas chromatographic measurements of the two major peroxy acyl nitrates,peroxy acetyl nitrate (PAN) and peroxy propionyl nitrate (PPN). Comparisonwith NO
y and other nitrogen oxide measurements confirms the importanceof HO
2NO
2 and CH
3O
2NO
2 to the reactive nitrogenbudget and shows that current thinking about the chemistry of these speciesis approximately correct. During the spring high latitude conditions sampledduring the TOPSE experiment, the model predictions of the contribution of(HO
2NO
2+CH
3O
2NO
2) to NO
y are highlytemperature dependent: on average 30% of NO
y at 230K, 15% ofNO
y at 240K, and
5% of NO
y above 250K. The temperaturedependence of the inferred concentrations corroborates the contribution ofovertone photolysis to the photochemistry of peroxynitric acid. A model thatincludes IR photolysis (J=1x10
-5s
-1) agreed with the observed sum ofHO
2NO
2+CH
3O
2NO
2 to better than 35% below 240K where the concentration of these species is largest.