Physics of the Earth and Planetary Interiors 156 (2006) 213–222 The nature of a cryptochron from a paleomagnetic study of chron C4r.2r recorded in sediments off the Antarctic Peninsula Gary Acton a,∗ , Yohan Guyodo b,1 , Stefanie Brachfeld c,2 a One Shields Avenue, Department of Geology, University of California, Davis, CA 95616, USA b Laboratoire des Sciences du Climat et de l’Environnement (LSCE), Domaine du CNRS, 12 Avenue de la Terrasse, Gif-sur-Yvette, Cedex 91198, France c Department of Earth & Environmental Studies, Montclair State University, Montclair, NJ 07043, USA Received 2 May 2005; received in revised form 9 September 2005; accepted 9 September 2005 Abstract The magnetostratigraphy from Ocean Drilling Program (ODP) Site 1095, off the Pacific margin of the Antarctic Peninsula, contains an extra normal polarity event that occurs near the base of Chron 4r.2r (8.072–8.699Ma), which we interpret to be cryptochron C4r.2r-1. Owing to the relatively high sedimentation rates (about 90m/m.y.), this event is particularly well recorded at the site, spanning 4.99 m of the stratigraphic section. This allows the characteristics of the cryptochron to be investigated in greater detail than possible from marine magnetic anomalies, where it was originally identified, or from other sedimentary sections in which it has been recorded at much lower resolution. Our observations suggest that the cryptochron is a full geomagnetic reversal, in which both the direction and paleointensity attain levels similar to that of other normal polarity chrons at the site. Based on its position within Chron 4r.2r, the cryptochron started at 8.622 Ma and terminated 56 k.y. later at 8.566 Ma. At the transition zones bounding the cryptochron, the paleointensity collapses to near zero, but recovers within a few thousand years. Our results, as well as paleomagnetic observations from other thick sedimentary units, indicate that cryptochrons are not always purely paleointensity variations. Instead they are a record of short-term geomagnetic variability that includes short geomagnetic reversals, excursions, intervals of high paleosecular variation, and paleointensity lows, all of which are part of a vector field that varies in both strength and direction over time. © 2006 Elsevier B.V. All rights reserved. Keywords: Cryptochrons; Excursions; Geomagnetic polarity timescale; Magnetostratigraphy; Geomagnetism; Relative paleointensity; Ocean Drilling Program; Site 1095; Antarctic Peninsula ∗ Corresponding author. Tel.: +1 530 752 1861; fax: +1 530 752 0951. E-mail addresses: acton@geology.ucdavis.edu (G. Acton), guyodo@lsce.cnrs-gif.fr (Y. Guyodo), brachfelds@mail.montclair.edu (S. Brachfeld). 1 Tel.: +33 1 69 82 35 62; fax: +33 1 69 82 35 68. 2 Tel.: +1 973 655 5129; fax: +1 973 655 4072. 1. Introduction Cryptochrons, a term coined by Cande and Kent (1992a), are geomagnetic events of short duration (roughly 30 k.y. or less) whose origins are debated and whose characteristics are uncertain owing to the few direct observations that have been obtained from them. Rather than being identified from paleomagnetic studies of rocks or sediments, cryptochrons have been identi- fied as small magnetic anomalies (referred to as “tiny 0031-9201/$ – see front matter © 2006 Elsevier B.V. All rights reserved. doi:10.1016/j.pepi.2005.09.015