Figure F11. Spikes in magnetic susceptibility in carbonate ooze of Unit I, Hole 1184A. Most spikes correspond to intervals containing abundant volcanic glass shards. Similar shards are rare in the rest of Unit I. The small increases in susceptibility in the tops of Cores 192-1184A-2R and 3R may be caused by contamination. See legend in Figure F10, .

Figure F11. Spikes in magnetic susceptibility in carbonate ooze of Unit I, Hole 1184A. Most spikes correspond to intervals containing abundant volcanic glass shards. Similar shards are rare in the rest of Unit I. The small increases in susceptibility in the tops of Cores 192-1184A-2R and 3R may be caused by contamination. See legend in Figure F10.