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Connecting speeds, directions and arrival times of 22 coronal mass ejections from the Sun to 1 AU


Möstl, Christian; Amla, K.; Hall, J.R.; Liewer, P.C.; De Jong, E.M.; Colaninno, R.C.; Veronig, A.M.; Rollett, T.; Temmer, M.; Peinhart, V. et al.
Connecting speeds, directions and arrival times of 22 coronal mass ejections from the Sun to 1 AU // The Astrophysical journal, 787 (2014), 2; 119-136 doi:10.1088/0004-637X/787/2/119 (međunarodna recenzija, članak, znanstveni)


Naslov
Connecting speeds, directions and arrival times of 22 coronal mass ejections from the Sun to 1 AU

Autori
Möstl, Christian ; Amla, K. ; Hall, J.R. ; Liewer, P.C. ; De Jong, E.M. ; Colaninno, R.C. ; Veronig, A.M. ; Rollett, T. ; Temmer, M. ; Peinhart, V. ; Davies, J.A. ; Lugaz, N. ; Liu, Y.D. ; Farrugia, C.J. ; Luhmann, J.G. ; Vršnak, Bojan ; Harrison, R.A. ; Galvin, A.B.

Izvornik
The Astrophysical journal (0004-637X) 787 (2014), 2; 119-136

Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni

Ključne riječi
solar–terrestrial relations – Sun: coronal mass ejections (CMEs) – Sun: heliosphere

Sažetak
Forecasting the in situ properties of coronal mass ejections (CMEs) from remote images is expected to strongly enhance predictions of space weather and is of general interest for studying the interaction of CMEs with planetary environments. We study the feasibility of using a single heliospheric imager (HI) instrument, imaging the solar wind density from the Sun to 1 AU, for connecting remote images to in situ observations of CMEs. We compare the predictions of speed and arrival time for 22 CMEs (in 2008–2012) to the corresponding interplanetary coronal mass ejection (ICME) parameters at in situ observatories (STEREO PLASTIC/IMPACT, Wind SWE/MFI). The list consists of front- and backsided, slow and fast CMEs (up to 2700 km s−1).We track the CMEs to 34.9±7.1 deg elongation from the Sun with J maps constructed using the SATPLOT tool, resulting in prediction lead times of −26.4 ± 15.3 hr. The geometrical models we use assume different CME front shapes (fixed-Φ, harmonic mean, self-similar expansion) and constant CME speed and direction. We find no significant superiority in the predictive capability of any of the three methods. The absolute difference between predicted and observed ICME arrival times is 8.1 ± 6.3 hr (rms value of 10.9 hr). Speeds are consistent to within 284 ± 288 km s−1. Empirical corrections to the predictions enhance their performance for the arrival times to 6.1 ± 5.0 hr (rms value of 7.9 hr), and for the speeds to 53 ± 50 km s−1. These results are important for Solar Orbiter and a space weather mission positioned away from the Sun–Earth line.

Izvorni jezik
Engleski

Znanstvena područja
Fizika



POVEZANOST RADA


Projekt / tema
007-0000000-1362 - Eruptivni procesi u Sunčevoj atmosferi (Bojan Vršnak, )

Ustanove
Geodetski fakultet, Zagreb

Profili:

Avatar Url Bojan Vršnak (autor)

Citiraj ovu publikaciju

Möstl, Christian; Amla, K.; Hall, J.R.; Liewer, P.C.; De Jong, E.M.; Colaninno, R.C.; Veronig, A.M.; Rollett, T.; Temmer, M.; Peinhart, V. et al.
Connecting speeds, directions and arrival times of 22 coronal mass ejections from the Sun to 1 AU // The Astrophysical journal, 787 (2014), 2; 119-136 doi:10.1088/0004-637X/787/2/119 (međunarodna recenzija, članak, znanstveni)
Möstl, C., Amla, K., Hall, J., Liewer, P., De Jong, E., Colaninno, R., Veronig, A., Rollett, T., Temmer, M. & Peinhart, V. (2014) Connecting speeds, directions and arrival times of 22 coronal mass ejections from the Sun to 1 AU. The Astrophysical journal, 787 (2), 119-136 doi:10.1088/0004-637X/787/2/119.
@article{article, year = {2014}, pages = {119-136}, DOI = {10.1088/0004-637X/787/2/119}, keywords = {solar–terrestrial relations – Sun: coronal mass ejections (CMEs) – Sun: heliosphere}, journal = {The Astrophysical journal}, doi = {10.1088/0004-637X/787/2/119}, volume = {787}, number = {2}, issn = {0004-637X}, title = {Connecting speeds, directions and arrival times of 22 coronal mass ejections from the Sun to 1 AU}, keyword = {solar–terrestrial relations – Sun: coronal mass ejections (CMEs) – Sun: heliosphere} }

Časopis indeksira:


  • Current Contents Connect (CCC)
  • Web of Science Core Collection (WoSCC)
    • Science Citation Index Expanded (SCI-EXP)
    • SCI-EXP, SSCI i/ili A&HCI
  • Scopus


Uključenost u ostale bibliografske baze podataka:


  • NASA ADS


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