posted on 2025-08-04, 15:22authored byKJ Trattner, J LaBelle, O Santolik, CA Kletzing, DM Miles, SA Fuselier, JW Bonnell, SR Bounds, I Kolmasova, SM Petrinec, RP Sawyer, SK Vines, C Moser-Gauthier, IH Cairns, Timothy YeomanTimothy Yeoman
<p dir="ltr">On the morning of December 8, 2018, two sounding rockets were launched into the northern hemisphere cusp region to investigate the spatial and temporal nature of cusp structures. The two rockets, designated Twin Rockets to Investigate Cusp Electrodynamics 2 (TRICE-2), consisted of a high- and a low-flyer rocket launched two minutes apart. The TRICE-2 mission was a pathfinder for the upcoming Tandem Reconnection and Cusp Electrodynamics Reconnaissance Satellites (TRACERS) mission and carried almost identical payloads to those proposed for the twin spacecraft of the TRACERS mission. Results from the TRICE-2 mission are summarized, including observed cusp features (low energy ions in the cusp, overlapping cusp ion dispersions and cusp ion signatures) and the connection of the cusp structures to ionospheric convection cells, provided by SuperDARN radar observations, to show the advantages of coordinated space and ground-based observations. A description is provided for how these results – and those of other experiments which made measurements of particles and waves in the cusp and in the dayside magnetosphere – have guided the science objectives of the TRACERS mission.</p>
Funding
The research at LASP was supported by the TRICE-2 mission grant NNX15AL08G, the MMS prime grant NNG04EB99C and by 80NSSC19K0849, 80NSSC23K0009 and 80NSSC20K0688. Research at SWRI was funded by NASA grant NNG04EB99C. Work at Lockheed Martin was performed on Contracts 499935Q and 80NSSC18K1379. Work at Dartmouth College was supported by subaward #1002052568 to NASA award 80GSFC18C0008 to the University of Iowa. TRACERS is supported by 80GSFC18C0008. I.H.C. is supported by the Australian Research Council grant IC170100023 for the ARC Training Centre for CubeSats, UAV’s and their Applications (CUAVA)
A Consolidated Grant Proposal for Solar and Planetary Science at the University of Leicester, 2019 - 2022
The TRICE-2 data are available from the University of Iowa at the following website: https://space.physics.uiowa.edu/rockets/data/SCIENCE/TRICEII_Mission/. Data sets from the Magnetospheric Multiscale (MMS) mission are available through the MMS Science Data Center (https://lasp.colorado.edu/mms/sdc/). Interactive Data Language (IDL) routines for display of MMS and TRICE-2 data are available in the current Space Physics Environment Data Analysis Software (SPEDAS) software package, which can be found through the MMS Science Data Center and through the SPEDAS website (http://spedas.org).
Solar wind observations are provided by the Wind “Solar Wind Experiment” (Wind/SWE) (Ogilvie et al. 1995). The interplanetary magnetic field (IMF) measurements are provided by the Wind “Magnetic Field Instrument” (Wind/MFI) (Lepping et al. 1995). The solar wind data are available at the Coordinated Data Analysis Web (CDAWeb; http://cdaweb.gsfc.nasa.gov/istp_public/).
The authors acknowledge the use of SuperDARN data. SuperDARN is a collection of radars funded by the national scientific funding agencies of Australia, Canada, China, France, Italy, Japan, Norway, South Africa, the United Kingdom, and the United States of America. SuperDARN RawACF data were obtained via setting up a user account for the British Antarctic Survey Data mirror (https://www.bas.ac.uk/project/superdarn). The Radar Software Toolkit (RST) to process the SuperDARN data can be downloaded from Zenodo (https://doi.org/10.5281/zenodo.1403226). Due to the nature of the account setup, data may not be accessible immediately. This research used the SPECTRE High Performance Computing Facility at the University of Leicester.