Observations of substorm fine structure

• Main Authors: L. L. Lazutin, R. Rasinkangas, T. V. Kozelova, A. Korth, H. Singer, G. Reeves, W. Riedler, K. Torkar, B. B. Gvozdevsky
• Format: Article
• Language: English
• Published: Copernicus Publications 1998-07-01
• Series: Annales Geophysicae
• Online Access: https://www.ann-geophys.net/16/775/1998/angeo-16-775-1998.pdf
• ISSN: 0992-7689; 1432-0576

Particle and magnetic field measurements on the CRRES satellite were used, together with geosynchronous satellites and ground-based observations, to investigate the fine structure of a magnetospheric substorm on February 9, 1991. Using the variations in the electron fluxes, the substorm activity was divided into several intensifications lasting about 3–15 minutes each. The two main features of the data were: (1) the intensifications showed internal fine structure in the time scale of about 2 minutes or less. We call these shorter periods activations. Energetic electrons and protons at the closest geosynchronous spacecraft (1990 095) were found to have comparable activation structure. (2) The energetic (&gt;69 keV) proton injections were delayed with respect to electron injections, and actually coincided in time with the end of the intensifications and partial returns to locally more stretched field line configuration. We propose that the energetic protons could be able to control the dynamics of the system locally be quenching the ongoing intensification and possibly preparing the final large-scale poleward movement of the activity. It was also shown that these protons originated from the same intensification as the preceeding electrons. Therefore, the substorm instability responsible for the intensifications could introduce a negative feedback loop into the system, creating the observed fine structure with the intensification time scales.<br><br><b>Key words.</b> Magnetospheric Physics (Storms and substorms).