التفاصيل البيبلوغرافية
العنوان: |
TRICE‐2/SuperDARN Observations and Comparison With the Associated MMS Magnetopause Crossing. |
المؤلفون: |
Trattner, K. J., Fuselier, S. A., Kletzing, C. A., Bonnell, J. W., Bounds, S. R., Petrinec, S. M., Sawyer, R. P., Yeoman, T. K., Ergun, R. E., Burch, J. L. |
المصدر: |
Journal of Geophysical Research. Space Physics; May2024, Vol. 129 Issue 5, p1-15, 15p |
مصطلحات موضوعية: |
MAGNETOPAUSE, SOLAR cycle, ROCKETS (Aeronautics), BOUNDARY layer (Aerodynamics), ION beams, ION energy, ION bombardment |
مستخلص: |
Two sounding rockets, designated TRICE‐2, were launched on 8 December 2018 into the northern cusp region. The two rockets were designated the high‐ and low‐flyers, respectively, and launched 2 min apart to investigate cusp structures, specifically their spatial or temporal nature. 2 hr prior to the cusp encounter by the TRICE‐2 rockets, the MMS satellites, located in the magnetopause boundary layer, observed switching ion beams under very similar IMF conditions as later observed by TRICE‐2. The observed ion beam switch in the boundary layer defined the location of the primary dayside X‐line. Both, TRICE‐2 and MMS, also observed the signatures of multiple X‐lines at the magnetopause, overlapping ion‐energy dispersions in the cusp and counterstreaming ion beams in the magnetopause boundary layer, respectively. In addition to the TRICE‐2 cusp observations, ionospheric convection patterns from the SuperDARN radar are used to explain the vastly different cusp ion signatures observed by the TRICE‐2 rockets. While the high‐flyer rocket progressed north through the center of the cusp, the low‐flyer rocket drifted off to the east and crossed into the dusk convection cell, traveling perpendicular to the ionospheric convection direction before reaching the poleward oriented section of the convection cell also observed by the high‐flyer counterpart. Key Points: TRICE‐2 cusp ion dispersions are explained using the different magnetic foot points of the rockets through the ionospheric convection cellsTRICE‐2 cusp crossing occurred 2 hr after an MMS magnetopause crossing during similar IMF conditionsOverlapping cusp ion energy dispersions result from multiple magnetopause reconnection locations in agreement with MMS observations [ABSTRACT FROM AUTHOR] |
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