Comparing 1-year GUMICS-4 simulations of the Terrestrial Magnetosphere with Cluster Measurements

Bibliographic Details
Title: Comparing 1-year GUMICS-4 simulations of the Terrestrial Magnetosphere with Cluster Measurements
Authors: Facsko, Gabor, Sibeck, David, Honkonen, Ilja, Bor, Jozsef, Perez, German Farinas, Timar, Aniko, Shprits, Yuri, Peitso, Pyry, Degener, Laura, Tanskanen, Eija, Anekallu, Chandrasekhar Reddy, Szalai, Sandor, Kis, Arpad, Wesztergom, Viktor, Madar, Akos, Biro, Nikolett, Koban, Gergely, Illyes, Andras, Kovacs, Peter, Dalya, Zsuzsanna, Lkhagvadorj, Munkhjargal
Publication Year: 2023
Collection: Physics (Other)
Subject Terms: Physics - Space Physics
More Details: We compare the predictions of the GUMICS$-$4 global magnetohydrodynamic model for the interaction of the solar wind with the Earth's magnetosphere with Cluster~SC3 measurements for over one year, from January 29, 2002, to February 2, 2003. In particular, we compare model predictions with the north/south component of the magnetic field ($B_{z}$) seen by the magnetometer, the component of the velocity along the Sun-Earth line ($V_{x}$), and the plasma density as determined from a top hat plasma spectrometer and the spacecraft's potential from the electric field instrument. We select intervals in the solar wind, the magnetosheath, and the magnetosphere where these instruments provided good-quality data, and the model correctly predicted the region in which the spacecraft is located. We determine the location of the bow shock, the magnetopause, and the neutral sheet from the spacecraft measurements and compare these locations to those predicted by the simulation. The GUMICS$-$4 model agrees well with the measurements in the solar wind however its accuracy is worse in the magnetosheath. The simulation results are not realistic in the magnetosphere. The bow shock location is predicted well, however, the magnetopause location is less accurate. The neutral sheet positions are located quite accurately thanks to the special solar wind conditions when the $B_{y}$ component of the interplanetary magnetic field is small.
Comment: submitted to the AGU Space Weather, 51 pages, 19 figures, 8 tables
Document Type: Working Paper
DOI: 10.1002/essoar.10507311.1
Access URL: http://arxiv.org/abs/2305.03478
Accession Number: edsarx.2305.03478
Database: arXiv
More Details
DOI:10.1002/essoar.10507311.1