Journal articles
First Detection of Solar Flare Emission in Mid-ultraviolet Balmer Continuum
Abstract : We present the first detection of solar flare emission at middle-ultraviolet wavelengths around 2000Å by the channel 2 of the Large-Yield RAdiometer (LYRA) onboard the PROBA2 mission. The flare (SOL20170906) was also observed in the channel 1 of LYRA centered at the H I Lyman-α line at 1216Å, showing a clear non-thermal profile in both channels. The flare radiation in channel 2 is consistent with the hydrogen Balmer continuum emission produced by an optically thin chromospheric slab heated up to 10000 K. Simultaneous observations in channels 1 and 2 allow the separation of the line emission (primarily from the Lyman-α line) from the Balmer continuum emission. Together with the recent detection of the Balmer continuum emission in the near-ultraviolet by IRIS, the LYRA observations strengthen the interpretation of broadband flare emission as the hydrogen recombination continua originating in the chromosphere.
Cited literature [50 references]
https://hal-insu.archives-ouvertes.fr/insu-02940873
Contributor : Nathalie Pothier Connect in order to contact the contributor
Submitted on : Thursday, November 12, 2020 - 3:46:18 PM
Last modification on : Tuesday, October 12, 2021 - 5:20:36 PM
Long-term archiving on: : Saturday, February 13, 2021 - 7:53:34 PM
Contributor : Nathalie Pothier Connect in order to contact the contributor
Submitted on : Thursday, November 12, 2020 - 3:46:18 PM
Last modification on : Tuesday, October 12, 2021 - 5:20:36 PM
Long-term archiving on: : Saturday, February 13, 2021 - 7:53:34 PM
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1810.09835.pdf
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