The ground level concentrations of methane in the atmosphere have been measured to be in the range from 1.45 to 1.62 parts per million by volume (ppmv) The major hydrocarbon present in the natural atmosphere of the earth is methane, which is found in a relative concentration of =1.6 parts per million by volume (ppmv) throughout the troposphere (1-3). Most hydrogen and most carbon in the atmosphere are found in oxidized forms, and CH4 is subject to relatively rapid oxidation to other chemical forms. The major sources for the continuous replenishment of atmospheric CH4 certainly involve gaseous evolution from biological material under anaerobic conditions-e.g., rice paddies, swamps, enteric fermentation, etc.-but are not known in any precise quantitative detail. The overall biological origin of most of the atmospheric CH4 is inferred from the near-equivalence between the '4C/'2C ratio in it to that in living material that draws both 12CO2 and 14Co2 from the atmosphere (1-4). Any carbonaceous material isolated for >20,000 yr from exchange with the cosmic ray-produced atmospheric 14C reservoir will have a negligible 14C content. Hence, the contribution to atmospheric CH4 from the flaring of natural gas, or by volcanoes, earthquakes, etc. (5), cannot be major because these sources should be essentially devoid of 14C. Ehhalt (3) has placed an upper limit of 10% on the nonbiogenic sources of CH4.Methane has been known as a component of the atmosphere since 1948 (6), and several groups have reported (Table 1) higher concentrations in the northern than in the southern hemispheres (7-15, ¶). A consensus developed in the late 1970s that a concentration gradient does indeed exist between the two hemispheres. Ehhalt (10) has further demonstrated that the presence of N/S hemispheric gradients in methane concentrations provides some boundary conditions on the atmospheric residence time of CH4 and upon the N/S distribution of its sources and sinks.During 1977-1979 we carried out three series of measurements of CH4 concentrations in tropospheric samples collected in remote locations at the surface between 620N and 540S latitudes, and we have consistently observed a N/S gradient with =5-7% higher concentrations in the north than in the south. The removal of CH4 from the atmosphere is usually assumed to occur almost entirely by reaction 1 with OH radicals, OH + CH4-* H20 + CH3, [1] with most of this attack occurring in the lowest 6 km of the atmosphere. Quantitative estimates of the overall rate of this reaction are limited by the current imprecision in the knowledge of worldwide concentrations of OH in both time and space. In the absence ofbetter information concerning sources and sinks, the atmospheric residence time of CH4 has not yet been well established and further data can be very useful. Previous estimates of the atmospheric residence time for CH4 have ranged from 1.5 (16) or 2 (17) yr to much longer times of 21.5 (12) or 29 (18) yr. Ehhalt (10) has recently estimated a most probable value of about 5 yr with a r...