Formation Of The Lyman Continuum During Solar Flares Article Swipe
YOU?
·
· 2023
· Open Access
·
· DOI: https://doi.org/10.48550/arxiv.2301.01648
The Lyman Continuum (LyC; $<911.12$Å) forms at the top of the chromosphere in the quiet-Sun, making LyC a powerful tool for probing the chromospheric plasma during solar flares. To understand the effects of non-thermal energy deposition in the chromosphere during flares, we analysed LyC profiles from a grid of field-aligned radiative hydrodynamic models generated using the RADYN code as part of the F-CHROMA project. The spectral response of LyC, the temporal evolution of the departure coefficient of hydrogen, $b_1$, and the color temperature, $T_c$, in response to a range of non-thermal electron distribution functions, were investigated. The LyC intensity was seen to increase by 4-5.5 orders of magnitude during solar flares, responding most strongly to the non-thermal electron flux of the beam. Generally, $b_1$ decreased from $10^2$-$10^3$ to closer to unity during solar flares, indicating a stronger coupling to local conditions, while $T_c$ increased from $8$-$9$kK to $10$-$16$kK. $T_c$ was found to be approximately equal to the electron temperature of the plasma when $b_1$ was at a minimum. Both optically thick and optically thin components of LyC were found in agreement with the interpretation of recent observations. The optically thick layer forms deeper in the chromosphere during a flare compared to quiescent periods, whereas the optically thin layers form at higher altitudes due to chromospheric evaporation, in low-temperature, high-density regions propagating upwards. We put these results in the context of current and future missions.
Related Topics
- Type
- preprint
- Language
- en
- Landing Page
- http://arxiv.org/abs/2301.01648
- https://arxiv.org/pdf/2301.01648
- OA Status
- green
- Related Works
- 10
- OpenAlex ID
- https://openalex.org/W4313598497
Raw OpenAlex JSON
- OpenAlex ID
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https://openalex.org/W4313598497Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.48550/arxiv.2301.01648Digital Object Identifier
- Title
-
Formation Of The Lyman Continuum During Solar FlaresWork title
- Type
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preprintOpenAlex work type
- Language
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enPrimary language
- Publication year
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2023Year of publication
- Publication date
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2023-01-04Full publication date if available
- Authors
-
S. McLaughlin, Ryan O. Milligan, Graham S. Kerr, Aaron J. Monson, Paulo J. A. Simões, M. MathioudakisList of authors in order
- Landing page
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https://arxiv.org/abs/2301.01648Publisher landing page
- PDF URL
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https://arxiv.org/pdf/2301.01648Direct link to full text PDF
- Open access
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YesWhether a free full text is available
- OA status
-
greenOpen access status per OpenAlex
- OA URL
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https://arxiv.org/pdf/2301.01648Direct OA link when available
- Concepts
-
Chromosphere, Physics, Solar flare, Astrophysics, Radiative transfer, Plasma, Flare, Spectral line, Astronomy, Optics, Quantum mechanicsTop concepts (fields/topics) attached by OpenAlex
- Cited by
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0Total citation count in OpenAlex
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10Other works algorithmically related by OpenAlex
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| abstract_inverted_index.evaporation, | 215 |
| abstract_inverted_index.high-density | 218 |
| abstract_inverted_index.hydrodynamic | 51 |
| abstract_inverted_index.temperature, | 82 |
| abstract_inverted_index.$10^2$-$10^3$ | 126 |
| abstract_inverted_index.approximately | 153 |
| abstract_inverted_index.chromospheric | 23, 214 |
| abstract_inverted_index.field-aligned | 49 |
| abstract_inverted_index.investigated. | 95 |
| abstract_inverted_index.observations. | 186 |
| abstract_inverted_index.interpretation | 183 |
| abstract_inverted_index.$<911.12$Å) | 4 |
| abstract_inverted_index.low-temperature, | 217 |
| cited_by_percentile_year | |
| countries_distinct_count | 0 |
| institutions_distinct_count | 6 |
| sustainable_development_goals[0].id | https://metadata.un.org/sdg/7 |
| sustainable_development_goals[0].score | 0.8100000023841858 |
| sustainable_development_goals[0].display_name | Affordable and clean energy |
| citation_normalized_percentile.value | 0.00548021 |
| citation_normalized_percentile.is_in_top_1_percent | False |
| citation_normalized_percentile.is_in_top_10_percent | False |