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Pregled bibliografske jedinice broj: 1141294

CME evolution and the corresponding Forbush decrease: modelling vs multi-spacecraft observation


Dumbovic, Mateja; Moestl, Christian; Podladchikova, Tatiana; Guo, Jingnan; Heber, Bernd; Vrsnak, Bojan; Dissauer, Karin; Veronig, Astrid; Amerstorfer, Tanja; Temmer, Manuela et al.
CME evolution and the corresponding Forbush decrease: modelling vs multi-spacecraft observation // 43rd COSPAR Scientific Assembly
online, 2021. str. 1-1 (predavanje, međunarodna recenzija, sažetak, znanstveni)


CROSBI ID: 1141294 Za ispravke kontaktirajte CROSBI podršku putem web obrasca

Naslov
CME evolution and the corresponding Forbush decrease: modelling vs multi-spacecraft observation

Autori
Dumbovic, Mateja ; Moestl, Christian ; Podladchikova, Tatiana ; Guo, Jingnan ; Heber, Bernd ; Vrsnak, Bojan ; Dissauer, Karin ; Veronig, Astrid ; Amerstorfer, Tanja ; Temmer, Manuela ; Carcaboso, Fernando ; Kirin, Anamarija

Vrsta, podvrsta i kategorija rada
Sažeci sa skupova, sažetak, znanstveni

Skup
43rd COSPAR Scientific Assembly

Mjesto i datum
Online, 28.1.-4.2.2021

Vrsta sudjelovanja
Predavanje

Vrsta recenzije
Međunarodna recenzija

Ključne riječi
coronal mass ejections, flux ropes, forbush decreases, multi-spacecraft observations

Sažetak
One of the very common in-situ signatures of interplanetary coronal mass ejections (ICMEs), as well as other interplanetary transients are Forbush decreases (FDs), i.e. short-term reductions in the galactic cosmic ray (GCR) flux. FD phenomena are caused by the interaction of GCRs with a magnetic structure, therefore it is expected that different types of interplanetary substructures cause different types of GCR time profiles, allowing us to distinguish between shock/sheath, flux rope and SIR-type of FDs. Moreover, since the interaction of GCRs and CME magnetic structure (i.e. flux rope) occurs all the way from Sun to Earth, FDs reflect the evolutionary properties of CMEs. We apply modelling to different ICME regions in order to obtain a generic FD profile. We model the shock/sheath- related FD using the propagating diffusive barrier (PDB) model, the flux-rope-related FD using the diffusion model for the expanding flux rope (ForbMod), and the exponential time profile approximates the recovery after the event. The modeled generic FD profile qualitatively agrees with our current observation-based understanding of FDs. In addition, we test ForbMod against a set of multi-spacecraft observations of the same ICME. We find a reasonable agreement of the ForbMod model with multi-spacecraft measurements, indicating that modelled FDs reflect well the flux rope evolution.

Izvorni jezik
Engleski

Znanstvena područja
Fizika



POVEZANOST RADA


Ustanove:
Geodetski fakultet, Zagreb

Profili:

Avatar Url Anamarija Kirin (autor)

Avatar Url Bojan Vršnak (autor)

Avatar Url Mateja Dumbović (autor)

Citiraj ovu publikaciju

Dumbovic, Mateja; Moestl, Christian; Podladchikova, Tatiana; Guo, Jingnan; Heber, Bernd; Vrsnak, Bojan; Dissauer, Karin; Veronig, Astrid; Amerstorfer, Tanja; Temmer, Manuela et al.
CME evolution and the corresponding Forbush decrease: modelling vs multi-spacecraft observation // 43rd COSPAR Scientific Assembly
online, 2021. str. 1-1 (predavanje, međunarodna recenzija, sažetak, znanstveni)
Dumbovic, M., Moestl, C., Podladchikova, T., Guo, J., Heber, B., Vrsnak, B., Dissauer, K., Veronig, A., Amerstorfer, T. & Temmer, M. (2021) CME evolution and the corresponding Forbush decrease: modelling vs multi-spacecraft observation. U: 43rd COSPAR Scientific Assembly.
@article{article, year = {2021}, pages = {1-1}, keywords = {coronal mass ejections, flux ropes, forbush decreases, multi-spacecraft observations}, title = {CME evolution and the corresponding Forbush decrease: modelling vs multi-spacecraft observation}, keyword = {coronal mass ejections, flux ropes, forbush decreases, multi-spacecraft observations}, publisherplace = {online} }
@article{article, year = {2021}, pages = {1-1}, keywords = {coronal mass ejections, flux ropes, forbush decreases, multi-spacecraft observations}, title = {CME evolution and the corresponding Forbush decrease: modelling vs multi-spacecraft observation}, keyword = {coronal mass ejections, flux ropes, forbush decreases, multi-spacecraft observations}, publisherplace = {online} }




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