Abstract: Using superposed epoch analysis methods, we analyze two sets of events: one of stormtime activations having some characteristics of sawtooth events, and another set of events defined as sawtooth events. We compare and contrast these data sets and show that the sawtooth events are associated with slightly lower than average solar wind driving but the differences are small. While the both sets of events are associated with a positive excursion of the SYM-H index, the stormtime activations show a clearer signal in the ASY-H index highlighting the role of the partial ring current in such events. In the inner magnetotail, both sets of events show qualitatively similar injection and field dipolarization characteristics. We conclude that...
This paper investigates the auroral evolution during different magnetospheric modes: substorms, stea...
Abstract. We conducted a statistical analysis of the geo-magnetic field variations during the storm ...
[1] Outstanding problems in magnetospheric substorms include what causes substorm onsets and whether...
Abstract: Using superposed epoch analysis methods, we analyze two sets of events: one of stormtime a...
comparison of solar wind conditions, geomagnetic response, and auroral boundary movement, using a si...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95189/1/jgra17938.pd
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95681/1/jgra21163.pd
dimensional physics model WINDMI is used to analyze the October 3–7, 2000 geomagnetic storm using so...
Sawtooth events are defined as quasi-periodic, large-amplitude particle flux oscillations with a per...
We have investigated a statistical relationship between sawtooth oscillations and geomagnetic storms...
We examine the 18 April 2002 sawtooth event. We find that the strong magnetic field dipolarizations ...
Sawtooth events have been identified at geosynchronous orbit as large-amplitude quasiperiodic (2–4 h...
This study describes a systematic statistical comparison of isolated non-storm substorms, steady ma...
We present here results which contrast isolated substorms with individual sawtooth events. Sawtooth...
Magnetospheric sawtooth events, first identified in the early 1990s, are named for their characteris...
This paper investigates the auroral evolution during different magnetospheric modes: substorms, stea...
Abstract. We conducted a statistical analysis of the geo-magnetic field variations during the storm ...
[1] Outstanding problems in magnetospheric substorms include what causes substorm onsets and whether...
Abstract: Using superposed epoch analysis methods, we analyze two sets of events: one of stormtime a...
comparison of solar wind conditions, geomagnetic response, and auroral boundary movement, using a si...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95189/1/jgra17938.pd
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95681/1/jgra21163.pd
dimensional physics model WINDMI is used to analyze the October 3–7, 2000 geomagnetic storm using so...
Sawtooth events are defined as quasi-periodic, large-amplitude particle flux oscillations with a per...
We have investigated a statistical relationship between sawtooth oscillations and geomagnetic storms...
We examine the 18 April 2002 sawtooth event. We find that the strong magnetic field dipolarizations ...
Sawtooth events have been identified at geosynchronous orbit as large-amplitude quasiperiodic (2–4 h...
This study describes a systematic statistical comparison of isolated non-storm substorms, steady ma...
We present here results which contrast isolated substorms with individual sawtooth events. Sawtooth...
Magnetospheric sawtooth events, first identified in the early 1990s, are named for their characteris...
This paper investigates the auroral evolution during different magnetospheric modes: substorms, stea...
Abstract. We conducted a statistical analysis of the geo-magnetic field variations during the storm ...
[1] Outstanding problems in magnetospheric substorms include what causes substorm onsets and whether...