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Latitudinal patterns for quantitative traits in insect are commonly used to investigate climatic adaptation. We compare the cold resistance of the leafminer (Liriomyza sativae) pupa among populations distributed from tropical to temperate regions, incorporating the thermal overwintering limit of the insect's range. The patterns of cold resistance for northern and southern populations differ. The southern populations significantly increased their cold resistance with latitude, showing a latitudinal pattern independent of seasons, acclimation regimes, and assay methods. In contrast, the northern populations showed no stable patterns; they were always intermediate in cold hardiness between the low-latitude and high-latitude populations within the overwintering limit. Integration of these data with those of the biologically similar congeneric leafminer, L. huidobrensis, suggests that a pattern shift in stress tolerance associated with the overwintering range limit is probably a general adaptive strategy adopted by freeze-intolerant species that have a high-latitude boundary of distribution, but can only overwinter and develop in protected greenhouses in harsh seasons. Considering the widespread availability of greenhouses for overwintering insects in northern China, we speculated that the large-scale existence of thermally-buffered microhabitats in greenhouses might eliminate the development of cold resistance of the leafminer populations. However, results suggest a strong selection for increased cold resistance for natural populations of Liriomyza species at higher latitudes that can overwinter in the field, but not for populations at latitudes above the thermal limit. Thus, habitat modification associated with greenhouses can limit gene flow and reduce cold tolerances even at latitudes above where the leafminers can overwinter in the field.

The cricket tentatively identified as Pteronemobius taprobanensis shows a stepwise pattern of latitudinal variation in ovipositor length. Abrupt elongation of ovipositor at about 28° N marks the replacement of the subtropical form by the temperate form. The latter maintains almost a constant ovipositor length up to about 35° N within the bivoltine area. Further north in the univoltine area, an ascending cline extends to about 39° N, beyond which no further increase occurs. The ovipositor length adjusted for body size shows a northeastward increase in each of the univoltine and bivoltine areas, though this tendency is less clear in the latter. The optimum length of ovipositor would vary with the relative amounts of gain (due to the protection of eggs in the soil) and loss (due to the metabolic cost and the difficulty to emerge from the soil) in fitness. If so, it may be predicted that a longer ovipositor would be selected for, when the metabolic cost and the risk at hatching are smaller, the environmental pressure in the egg stage is stronger, and the egg stage lasts longer. The last parameter seems to be mainly responsible for the observed association of the type of life cycle with the geographic pattern of variation in ovipositor length.

The standard metabolic rate (SMR) of birds correlates broadly with climate of origin. SMR tends to be higher in birds from cold climates and lower in tropical forms than would be expected from the bird's mass. SMR changes, on the average, 1% per degree change in latitude. The influence of climate on SMR is, however, subject to modification by other aspects of the bird's life history. For example, in tropical species adaptive modifications in SMR correlate with thermal microhabitat. Tropical birds which forage in the sun have SMR's averaging 25% lower than expected, while SMR of species which forage in the shade is normal. Species of penguins which undergo prolonged fasts during the breeding season do not show elevated SMR's typical of high latitude birds.

The cricket tentatively identified as Pteronemobius taprobanensis shows a saw-toothed pattern of variation in adult size along the latitudinal gradient of the Japanese Islands. A slight but abrupt increase in adult size at about 28° N indicates the replacement of the subtropical form by the temperate one. The body size of the latter slightly decreases north to about 33° N, then conspicuously increases to about 39° N and again decreases to the northern extreme. This pattern of variation seems to be related to the local adjustment of nymphal development by means of the photoperiodic response and genetic variation, since the adult size varies as a function of the duration of nymphal development. Multiple regression analysis of the variance between local populations reared at various photoperiods suggests, however, that the decrease in body size due to selection for shorter development in cooler climates is to a certain extent counteracted by selection for a higher rate of growth. The latter component of climatic selection is possibly due to greater egg production by larger-sized females within the shorter reproductive season. This hypothesis may also account for the divergence in size between the two climatic forms of this nominal species.

The survival potential of lichens in a given habitat is determined by the response of CO2 exchange to photosynthetically active radiation (PhAR), thallus temperature, and thallus relative water content (RWC). Therefore morphologically similar lichens from contrasting climatic environments 1) should differ in their CO2 exchange responses, and 2) these differences should reflect adaptations to their climatic regimes. The CO2 exchange responses of a subarctic (55°N, 67°W) Cladina stellaris (Opiz) Brodo population and a temperate (29°N, 82°W) Cladina evansii (Abb.) Hale and W. Culb, population were used to test these two related hypotheses. Infrared gas analysis with lichens collected in September–October 1975 established that the two populations differed in their responses to incident PhAR, thallus temperature, and thallus RWC. Net photosynthesis in C. stellaris had an optimum at a lower temperature and a greater relative photosynthetic capacity at low temperatures than did C. evansii. Cladina evansii maintained net photosynthesis above 35°C thallus temperature; C. stellaris did not. In both species the optimum temperature for net photosynthesis increased with increasing irradiance. The C. stellaris light saturation point was consistently lower than that of C. evansii. Both species had maximal rates of net photosynthesis at 70–80% relative water content. In C. evansii the CO2 exchange rates, expressed as percentages of the maximum rate, declined more rapidly under suboptimal conditions. The absolute CO2 exchange rates of C. evansii were greater than those of C. stellaris. At 20°C and 90–95% RWC, resaturation respiration occurred in both species and continued until 6–7 h after wetting. Contrasts in the temporal patterns of thallus condition at each collection site suggest that not all differences in the two response surfaces reflect climatic adaptation. The two populations appear well adapted to incident PhAR and thallus temperature regimes but the 70–80% RWC optimum for net photosynthesis common to both species is puzzling since their water regimes differ markedly. The overall adaptedness of the CO2 exchange responses in the two species cannot be judged without a comprehensive quantitative analysis of carbon balance under differing climatic regimes.