We investigate how substorms with and without growth-phase pseudobreakups are affected by solar wind and ionospheric conditions. The study is based on 874 events identified with Polar UVI.
An AE index analysis shows that substorms with growth-phase pseudobreakups are typically weak and appear as isolated events after hours of low geomagnetic activity. During the hours before onset the average solar wind merging field Em is weaker, and the length of time with enhanced values shorter than for regular substorms. Integrating Em over the last southward IMF period before onset shows an upper limit above which these substorms do not occur.
To estimate how much Em reaches the ionosphere, polar cap potential drop and unified PC indices are examined. It is found that substorms with growth-phase pseudobreakups have on average lower polar cap values than regular substorms. The temporal evolution of the PC indices is similar for both substorm groups; the summer index correlates better with Em, the winter index with AE. Also the average polar cap potential drop curves for both types of substorms resemble one other; the dayside and nightside curves are mainly influenced by Em and AE, respectively.
Comparing growth-phase, isolated and recovery pseudobreakups shows that solar wind and ionospheric conditions around the first substorm after a pseudobreakup are similar, independent of whether the last pseudobreakup appeared hours (recovery and isolated pseudobreakups) or minutes before substorm onset (growth-phase pseudobreakups). Substorms preceded by pseudobreakups are less often associated with a northward rotation of the IMF than regular substorms.