Relationship between the geomagnetic Dst(min) and the interplanetary Bz(min) during cycle 23

Details Relationship between the geomagnetic Dst(min) and the interplanetary Bz(min) during cycle 23 Relationship between the geomagnetic Dst(min) and the interplanetary Bz(min) during cycle 23

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010p%26ss...58..392k&link_type=abstract

Planetary and Space Science, Volume 58, Issue 3, p. 392-400.

Physics

4

Scientific paper

In cycle 23 for geomagnetic storms of -Dst(min) >50 nT, the plot of -Dst(min) versus -Bz(min) for the low -Bz(min) range 0-10 nT showed erratic variation in Dst(min), (correlation 0.19). Even for -Bz(min) range 10-20 nT, -Dst(min) values had considerable scatter (correlation 0.57). For -Bz(min).>20 nT, the relationship was good (correlation 0.82). For the whole range -Bz(min) 0-50 nT, the correlation was high (0.88). Thus, if -Bz(min) is very large (˜20 nT), large -Dst(min) occurs but in a wide range of 100-500 nT.

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