惑星分光観測衛星プロジェクトチーム

カリオコスキ ミラ

Milla Kalliokoski

基本情報

所属
国立研究開発法人宇宙航空研究開発機構 宇宙科学研究所

研究者番号
40978780
ORCID ID
 https://orcid.org/0000-0002-6445-5595
J-GLOBAL ID
202301014723641186
researchmap会員ID
R000049384

研究キーワード

 1

論文

 30
  • Milla Kalliokoski, Kazushi Asamura, Iku Shinohara, Takefumi Mitani, Tomoaki Hori, Yoshizumi Miyoshi, Nana Higashio, Takeshi Takashima
    2024年3月8日  
  • Adnane Osmane, Emilia Kilpua, Harriet Elizabeth George, Oliver Allanson, Milla M H Kalliokoski
    Astrophysical Journal, Supplement Series 269(2) 2023年12月1日  
  • Milla M H Kalliokoski, Michael G. Henderson, Steven K. Morley, Emilia Kilpua, Adnane Osmane, Leonid Olifer, Drew L. Turner, Allison N. Jaynes, Harriet Elizabeth George, Sanni Hoilijoki, Lucile Turc, Minna Palmroth
    Journal of Geophysical Research 128(2) 2023年2月  
  • Milla M. H. Kalliokoski, Michael G. Henderson, Steven K. Morley, Emilia K. J. Kilpua, Adnane Osmane, Leonid Olifer, Drew L. Turner, Allison N. Jaynes, Harriet George, Sanni Hoilijoki, Lucile Turc, Minna Palmroth
    Journal of Geophysical Research: Space Physics 2023年2月  
  • Sanni Hoilijoki, Emilia Kilpua, Adnane Osmane, Milla M H Kalliokoski, Harriet George, Mikko Savola, Timo Asikainen
    Frontiers in Astronomy and Space Sciences 9 2022年10月19日  
    In this study, we use mutual information from information theory to investigate non-linear correlation between geomagnetic activity indicated by auroral electrojet (AE) index with both the global ultra low frequency (ULF) Pc5 wave power and medium energy (>= 30 keV) electron precipitation at the central outer radiation belt. To investigate the energy and magnetic local time (MLT) dependence of the non-linearity, we calculate the mutual information and Pearson correlation coefficient separately for three different energy ranges (30-100 keV, 100-300 keV and >= 300 keV) and four different MLT sectors (0-6, 6-12, 12-18, 18-24). We compare results from 2 years 2004 and 2007 representing geomagnetically more active and less active years, respectively. The correlation analysis between the AE index and electron precipitation shows a clear MLT and energy dependence in both active and quiet conditions. In the two lowest energy ranges of the medium energy electrons (30-100 keV and 100-300 keV) both non-linear correlation and Pearson correlation indicate strong dependence with the AE index in the dawn sector. The linear dependence indicated by the Pearson correlation coefficient decreases from dawn to dusk while the change in the non-linear correlation is smaller indicating an increase in the non-linearity from dawn to dusk. The non-linearity between the AE index and electron precipitation is larger at all MLT sectors except MLTs 6-12 during geomagnetically more active year when larger amount of the activity is driven by interplanetary coronal mass ejections (ICMEs) compared to lower activity year with high speed stream (HSS) and stream interaction region (SIR) driven activity. These results indicate that the processes leading to electron precipitation become more non-linear in the dusk and during geomagnetically more active times when the activity is driven by ICMEs. The non-linearity between the AE index and global ULF Pc5 activity is relatively low and seems not to be affected by the difference in the geomagnetic activity during the 2 years studied.