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Abstract.Topographically, the Puna plateau of northwestern Argentina is the southern continuation of the Bolivian Altiplano. Its thickening and consecutive uplift result from the Andean orogeny. To better constrain the structural style and its progressive development, we have studied field data, topographic and satellite imagery, balanced cross sections, seismic reflection data, kinematic analysis of fault slip data, anisotropy of magnetic susceptibility (AMS), paleomagnetic data, and apatite fission track (AFF) data.

Abstract. The K-Ar based geomagnetic polarity timescale was constructed using data from lavas and tuffs that bracketed, but rarely dated, the transitions between polarity intervals. Subsequent 4øAr/39Ar dating indicated that the ages of some polarity transitions had been underestimated by about 6%. Although the accepted ages of the polarity chron boundaries have increased, their precise temporal definition remained uncertain. We have taken a different approach and used incremental-heating techniques to obtain 18 new 4øAr/39Ar ages from basaltic lavas within flow sequences at Punaruu Valley, Tahiti, and

A volcanic sequence almost 700 meters thick has been sampled in the Punaruu valley on the island of Tahiti, southern central Pacific Ocean. Detailed paleomagnetic results have been obtained from 123 sites. Three reversals are recorded in this sequence. Age determinations (K-Ar) indicate that the youngest reversal corresponds to the Matuyama-Brunhes transition while the two other transitions limit the Jaramillo normal polarity subchron. An apparent R-T-R excursion has been identified lower in the volcanic sequence and K-Ar age determinations around 1.1 Ma suggest that it corresponds to the Cobb Mountain subchron, but no normal paleomagnetic directions were discovered. The Matuyama-Brunhes and the lower Jaramillo transition are defined by only a few intermediate directions while many intermediate directions are observed for the upper Jaramillo transition and the Cobb Mountain excursion. We attribute these differences to variations in the rate of eruption of the volcanic rocks. The lower Jaramillo record is characterized by a steepening of the inclination at the beginning of the reversal suggesting a possible axisymmetric control of the field at this stage. However, the transition path for the most detailed record (upper Jaramillo) is characterized by large loops; this prevents simple modeling of the transition by low order zonal harmonics at all stages of a reversal. Paleointensity determinations were attempted on 48 samples with reliable results obtained for 26 of them. Paleointensities for the transitional field range from 3 to 8 gT. Such very low field strengths were first suggested by the low intensity of the natural remanent magnetization associated with intermediate directions. An analysis of the variation of the intensity of magnetization with the angular departure from the central axial field, including all other available data from Polynesia, indicates that (1) a paleomagnetic direction should be considered as intermediate when it is more than 30 ø from the expected axial dipole direction, and (2) the average transitional geomagnetic field intensity is about 1/5 of its value during stable polarity states. Comparison of these results observed in Polynesia with previous studies from Iceland suggests an increase of the average intensity of the intermediate field with latitude.