Observations of Flare Induced Doppler Shifts in the Si~\textsc{iii} $1206\,\textrm{Å}$ line
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arXiv
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| Format: | Preprint |
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2025
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| _version_ | 1866916936098512896 |
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| author | Majury, Luke H. Milligan, Ryan O. |
| author_facet | Majury, Luke H. Milligan, Ryan O. |
| contents | Doppler shifts in chromospheric and transition-region lines during solar flares are often interpreted as chromospheric condensation or evaporation. However, alternative sources of Doppler-shifted emission have been suggested, such as filament eruptions, jets or chromospheric bubbles. We analyse high-cadence scans from SORCE/SOLSTICE, which provide one-minute resolution profiles of the transition-region Si~\textsc{iii} ($1206\,\textrm{Å}$, $\textrm{T} = 10^{4.6}\,\textrm{K}$) line. 11 X-, M-, and C-class events observed during these scans with clear impulsive phase Si~\textsc{iii} enhancements were identified. By subtracting a quiet-Sun profile and fitting Gaussian profiles to the Si~\textsc{iii} line, measurements of flare-induced Doppler shifts were made. After correcting for a systematic trend in these shifts with solar longitude, two of the 11 events were found to exhibit a significant Doppler shift, \comment{}one with a $201.36\pm21.94\;\textrm{km\,s}^{-1}$ redshift and the other with a $-39.75\pm11.00\;\textrm{km\,s}^{-1}$ blueshift\commentend{}. Intriguingly, SDO/AIA $304\,\textrm{Å}$ and $1600\,\textrm{Å}$ imaging revealed a bright eruption coincident with the event that exhibited a blueshift, suggesting the shift may have resulted from the eruption rather than evaporation alone. Our results highlight Si~\textsc{iii} as a useful diagnostic of flaring dynamics at a temperature that has received limited attention to date. Future comparisons of these observations with radiative hydrodynamic simulations, along with new observations from state-of-the-art spectrometers such as SOLAR-C/EUVST and MUSE, should clarify the mechanisms behind the observed shifts in this study. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2509_05223 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Observations of Flare Induced Doppler Shifts in the Si~\textsc{iii} $1206\,\textrm{Å}$ line Majury, Luke H. Milligan, Ryan O. Solar and Stellar Astrophysics Doppler shifts in chromospheric and transition-region lines during solar flares are often interpreted as chromospheric condensation or evaporation. However, alternative sources of Doppler-shifted emission have been suggested, such as filament eruptions, jets or chromospheric bubbles. We analyse high-cadence scans from SORCE/SOLSTICE, which provide one-minute resolution profiles of the transition-region Si~\textsc{iii} ($1206\,\textrm{Å}$, $\textrm{T} = 10^{4.6}\,\textrm{K}$) line. 11 X-, M-, and C-class events observed during these scans with clear impulsive phase Si~\textsc{iii} enhancements were identified. By subtracting a quiet-Sun profile and fitting Gaussian profiles to the Si~\textsc{iii} line, measurements of flare-induced Doppler shifts were made. After correcting for a systematic trend in these shifts with solar longitude, two of the 11 events were found to exhibit a significant Doppler shift, \comment{}one with a $201.36\pm21.94\;\textrm{km\,s}^{-1}$ redshift and the other with a $-39.75\pm11.00\;\textrm{km\,s}^{-1}$ blueshift\commentend{}. Intriguingly, SDO/AIA $304\,\textrm{Å}$ and $1600\,\textrm{Å}$ imaging revealed a bright eruption coincident with the event that exhibited a blueshift, suggesting the shift may have resulted from the eruption rather than evaporation alone. Our results highlight Si~\textsc{iii} as a useful diagnostic of flaring dynamics at a temperature that has received limited attention to date. Future comparisons of these observations with radiative hydrodynamic simulations, along with new observations from state-of-the-art spectrometers such as SOLAR-C/EUVST and MUSE, should clarify the mechanisms behind the observed shifts in this study. |
| title | Observations of Flare Induced Doppler Shifts in the Si~\textsc{iii} $1206\,\textrm{Å}$ line |
| topic | Solar and Stellar Astrophysics |
| url | https://arxiv.org/abs/2509.05223 |