A1 Vertaisarvioitu alkuperäisartikkeli tieteellisessä lehdessä
GUMICS-4 analysis of interplanetary coronal mass ejection impact on Earth during low and typical Mach number solar winds
Tekijät: Lakka A, Pulkkinen TI, Dimmock AP, Kilpua E, Ala-Lahti M, Honkonen I, Palmroth M, Raukunen O
Kustantaja: COPERNICUS GESELLSCHAFT MBH
Julkaisuvuosi: 2019
Journal: Annales Geophysicae
Tietokannassa oleva lehden nimi: ANNALES GEOPHYSICAE
Lehden akronyymi: ANN GEOPHYS-GERMANY
Vuosikerta: 37
Numero: 4
Aloitussivu: 561
Lopetussivu: 579
Sivujen määrä: 19
ISSN: 0992-7689
DOI: https://doi.org/10.5194/angeo-37-561-2019
Rinnakkaistallenteen osoite: https://research.utu.fi/converis/portal/detail/Publication/41781911
We study the response of the Earth's magnetosphere to fluctuating solar wind conditions during interplanetary coronal mass ejections (ICMEs) using the Grand Unified Magnetosphere-Ionosphere Coupling Simulation (GUMICS-4). The two ICME events occurred on 15-16 July 2012 and 29-30 April 2014. During the strong 2012 event, the solar wind upstream values reached up to 35 particles cm(-3), speeds of up to 694 km s(-1), and an interplanetary magnetic field of up to 22 nT, giving a Mach number of 2.3. The 2014 event was a moderate one, with the corresponding upstream values of 30 particles cm(-3), 320 km s(-1) and 10 nT, indicating a Mach number of 5.8. We examine how the Earth's space environment dynamics evolves during both ICME events from both global and local perspectives, using well-established empirical models and in situ measurements as references. We show that on the large scale, and during moderate driving, the GUMICS-4 results are in good agreement with the reference values. However, the local values, especially during high driving, show more variation: such extreme conditions do not reproduce local measurements made deep inside the magnetosphere. The same appeared to be true when the event was run with another global simulation. The cross-polar cap potential (CPCP) saturation is shown to depend on the Alfven-Mach number of the upstream solar wind. However, care must be taken in interpreting these results, as the CPCP is also sensitive to the simulation resolution.
Ladattava julkaisu This is an electronic reprint of the original article. |  |
