Bs. Singer et al., Dating transitionally magnetized lavas of the late Matuyama Chron: Toward a new Ar-40/Ar-39 timescale of reversals and events, J GEO R-SOL, 104(B1), 1999, pp. 679-693
The K-Ar based geomagnetic polarity timescale was constructed using data fr
om lavas and tuffs that bracketed, but rarely dated, the transitions betwee
n polarity intervals. Subsequent Ar-40/Ar-39 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 p
recise temporal definition remained uncertain. We have taken a different ap
proach and used incremental-heating techniques to obtain 18 new Ar-40/Ar-39
ages from basaltic lavas within flow sequences at Punaruu Valley, Tahiti,
and Haleakala volcano, Hawaii. These lavas record transitional paleomagneti
c directions corresponding to four mid-Pleistocene polarity reversals or ev
ents. Three lavas from Punaruu Valley previously thought to record the Cobb
Mountain Normal Polarity Subchron (CMNS) gave a mean age of 1.105 +/- 0.00
5 Ma, indicating that they were erupted about 76 kyr after the CMNS; this p
eriod of transitional field behavior is designated the Punaruu event. In ad
dition, seven new Ar-40/Ar-39 ages from the Punaruu Valley indicate that th
e Jaramillo Normal Polarity Subchron (JNS) lasted about 67 kyr, starting at
1.053 +/- 0.006 Ma and ending 0.986 +/- 0.005 Ma. This agrees with astrono
mical estimates but conflicts with JNS ages proposed by Spell ann McDougall
[1992] and Izett and Obradovich [1994] on the basis of Ar-40/Ar-39 dating
of rhyolite domes in the Valles Caldera. Indistinguishable Ar-40/Ar-39 ages
of seven lavas, including one from Punaruu Valley and six from Haleakala t
hat record broadly similar intermediate paleodirections, suggest that the K
amikatsura event occurred at 0.886 +/- 0.003 Ma. Moreover, these data indic
ate that the Kamikatsura event occurred 20-40 kyr after another geomagnetic
event, most probably taking place at 0.92 Ma. We designate this earlier fi
eld behavior the Santa Rosa event, adopting its name from that of a transit
ionally magnetized rhyolite dome which happened to figure prominently in th
e original definition of the end of the JNS in the 1968 study of Doell et a
l. [1968]. The discovery of these new short-lived polarity events during th
e Matuyama reversed chron suggests that the 400 kyr period between 1.18 and
0.78 Ma experienced no less than 7 and perhaps more than 11 attempts by th
e geodynamo to reverse. This newly determined higher frequency of geomagnet
ic activity illustrates vividly the importance of obtaining precise age con
trol directly from transitionally magnetized rocks.