REPEATING WAVE-FORM INITIATED BY A 180-190-KA GEOMAGNETIC EXCURSION IN WESTERN NORTH-AMERICA - IMPLICATIONS FOR FIELD BEHAVIOR DURING POLARITY TRANSITIONS AND SUBSEQUENT SECULAR VARIATION
Rm. Negrini et al., REPEATING WAVE-FORM INITIATED BY A 180-190-KA GEOMAGNETIC EXCURSION IN WESTERN NORTH-AMERICA - IMPLICATIONS FOR FIELD BEHAVIOR DURING POLARITY TRANSITIONS AND SUBSEQUENT SECULAR VARIATION, J GEO R-SOL, 99(B12), 1994, pp. 24105-24119
New paleomagnetic, lithologic, and stratigraphic data are presented fr
om the sediments of Lake Chewaucan in the Summer Lake Basin, Oregon. T
he new data place better age constraints on the sediments and improve
the accuracy of the previously published paleomagnetic record from thi
s locality. A complex, yet distinct, waveform is observed in all three
components of the paleomagnetic vector. The waveform begins as the 18
0-190 ka Pringle Falls/Long Valley/Summer Lake II geomagnetic excursio
n and continues for two cycles after the excursion, until the record i
s interrupted by an unconformity that we correlate to the oxygen isoto
pe stage 6/5e boundary. The waveform's directional morphology in virtu
al geomagnetic pole (VGP) space is defined by two clockwise loops foll
owed by a distinctive counterclockwise, clockwise, counterclockwise lo
oping sequence. The VGP paths of the two cycles after the excursion ar
e rotated 180 degrees about Earth's spin axis with respect to the VGP
paths of the excursion cycle. The waveform also consists of a relative
paleointensity variation which repeats during the two cycles after th
e excursion. The average paleointensity of the postexcursion waveform
repetitions is high relative to the extremely low values that occur du
ring the excursion. This observation indicates that excursion-initiate
d secular variations can occur after the field fully recovers from the
low intensities which commonly typify excursions. Because of the simi
larities noted previously between this excursion and full polarity tra
nsitions (Tric et al., 1991), our new observations constrain models fo
r a wide range of field behavior including polarity transitions, excur
sions, and secular variation.