After a brief review of magnetospheric and interplanetary phenomena for intervals with
enhanced solar wind‐magnetosphere interaction, an attempt is made to define a geomagnetic …

Solar wind fast streams emanating from solar coronal holes cause recurrent, moderate
intensity geomagnetic activity at Earth. Intense magnetic field regions called Corotating …

… Although this empirical relationship was determined for a limited data interval during solar
maxima, it appears to hold during solar minimum as well (Tsurutani and Gonzalez, 1995a). …

Ten intense magnetic storms (D st < −100 nT) occurred during the 500 days from 16 August
1978 to 28 December 1979. From our analysis of ISEE-3 field and plasma data, it is found …

The recruitment of monocytes via the endothelial expression of vascular cell adhesion molecule-1
(VCAM-1) is a key step in the formation of the initial lesion in atherosclerosis. Because …

… A complementary summary is provided by Gonzalez et al. in EOS, 1996. The full set of
review articles will be published in an AGU monograph and many of the contributed articles will …

… There is a very slight (< 50 km/s) rise in V•w and decreases in helium and proton densities
across the discontinuity. However, the sharpness of these changes cannot be determined …

… Thus the correct reconnection line W2 is poleward of W•, and hence it lies more … W• (see
Figure 5). For this reason, the potential cb2 along W• is greater than the potential cb• along W•, …

We demonstrate extreme ionospheric response to the large interplanetary electric fields
during the “Halloween” storms that occurred on October 29 and 30, 2003. Within a few (2–5) …

… Tsurutani, BT, and WD Gonzalez, The cause of high intensity longduration continuous AE …
Tsurutani, BT and WD Gonzalez The future of geomagnetic storm predictions: Implications …