A1 Vertaisarvioitu alkuperäisartikkeli tieteellisessä lehdessä

Heavy-ion acceleration and self-generated waves in coronal shocks



Tekijät: Battarbee M, Laitinen T, Vainio R

Kustantaja: EDP SCIENCES S A

Julkaisuvuosi: 2011

Journal: Astronomy and Astrophysics

Tietokannassa oleva lehden nimi: ASTRONOMY & ASTROPHYSICS

Lehden akronyymi: ASTRON ASTROPHYS

Artikkelin numero: ARTN A34

Vuosikerta: 535

Sivujen määrä: 6

ISSN: 0004-6361

DOI: https://doi.org/10.1051/0004-6361/201117507


Tiivistelmä

Conclusions. We suggest that understanding the acceleration of minor ions at coronal shocks requires simulations which allow us to explore trapping dynamics and acceleration timescales in detail, including evolution of the turbulent trapping boundary. We conclude that steady-state models do not adequately describe the acceleration of heavy ions in coronal shocks.



Ladattava julkaisu

This is an electronic reprint of the original article.
This reprint may differ from the original in pagination and typographic detail. Please cite the original version.


Last updated on 2024-26-11 at 21:37