Global morphology of substorm growth phases observed by the IMAGE-SI12 imager

Details Global morphology of substorm growth phases observed by the IMAGE-SI12 imager Global morphology of substorm growth phases observed by the IMAGE-SI12 imager

Nov 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007jgra..11211211c&link_type=abstract

Journal of Geophysical Research, Volume 112, Issue A11, CiteID A11211

Physics

5

Magnetospheric Physics: Auroral Phenomena (2407), Magnetospheric Physics: Instruments And Techniques, Magnetospheric Physics: Solar Wind/Magnetosphere Interactions, Magnetospheric Physics: Magnetotail

Scientific paper

We present case studies and a statistical summary of optical observations of proton precipitation made during substorm growth phases. Our analysis is based on observations of the Doppler-shifted Lyman-α auroral emission obtained with the SI12 Spectrographic Imager on board the IMAGE satellite. These images are used to determine the morphology and dynamics of the auroral oval and of the polar cap boundary on a global scale, as well as the total open magnetic flux and its time evolution. We also investigate the relationship with the solar wind and the interplanetary magnetic field (IMF) characteristics measured by the ACE satellite and with the magnetic elevation angle measured by GOES-8. The statistical study shows that the sector of maximum proton precipitation during the growth phase is on average centered around 2200 MLT and rapidly shifts in local time by about 1.2 h toward midnight at the time of the onset. The open magnetic flux increases by 33% on average during the growth phase. The mean value of the open flux immediately before the substorm onset is about 0.66 GWb for substorms triggered by a northward turning of Bz and 0.74 GWb for nontriggered substorms. The averaged open flux at the substorm onset is smallest when the substorm is triggered by a sudden reversal of B z , suggesting that the accumulation of energy by the magnetosphere is perturbed by changes in B z . The open magnetic flux continues to increase during the 20 min following the onset, for a large number of events. The rate of equatorward displacement of the auroral oval boundaries during growth phase is typically ~3 deg/h. It is statistically correlated (r = 0.40) with the magnitude of the Bz component of the IMF measured by the ACE satellite. It is also correlated, with higher coefficient (r = 0.54), with functions describing the efficiency of solar wind energy transfer involving the transverse electric field carried by the solar wind. The equatorward motion may be global, restricted to local time sectors or a combination of both. At no nightside local time sector does the motion of the equatorial boundary appear more pronounced than at others, but the maximum displacement of the polar boundary is statistically located around midnight MLT.

Affiliated with

Also associated with

No associations

Rating

Global morphology of substorm growth phases observed by the IMAGE-SI12 imager does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Global morphology of substorm growth phases observed by the IMAGE-SI12 imager, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Global morphology of substorm growth phases observed by the IMAGE-SI12 imager will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-742391