Constarium
← Search

Imaging · dataset · 2026

Ultraviolet observations of spectral variability and dynamic processes during solar flares

Listed in ZivaHub and Deakin Research Online and DMU Figshare — shown once because both records carry DOI 10.17034/32826242.v1

EUV and HXR observations of solar flares provide key constraints on energy release and transport in the flaring solar atmosphere.

Description

This thesis investigates high-cadence, spectrally resolved observations of the transition-region H I Lyman-alpha (1216 Å) and Si III (1206 Å) lines from SOLSTICE to examine their spectral variability during flares, with a further investigation into the role of erupted material in flare irradiance enhancements being made with EUV imaging data from AIA.<br><br>An initial analysis compared Lyman-alpha spectral variability to HXR emission and UV imaging during two M-class flares.

Both events exhibited enhancements across the full Lyman-alpha profile coincident with HXR emission, consistent with chromospheric heating by nonthermal electrons. One event displayed enhanced blue-wing emission that was interpreted as blueshifted emission from the eruption.<br><br>Following this, Doppler shifts in Si III were measured during 11 flares, with two showing significant velocities: a redshift of 201.36±21.94 km s⁻¹ and a blueshift of -39.75±11.00 km s⁻¹.

Read the rest (2 more)

The blueshifted event corresponded to the same eruptive flare that exhibited enhanced blue-wing emission in Lyman-alpha. The redshift during the other event was instead interpreted as a signature of chromospheric condensation.<br><br>Finally, the contribution of erupting material to flare irradiance was quantified for nine eruptive events using spatially resolved AIA observations. Eruptions were found to contribute, on average, between 9% and 24% of the total excess radiated energy in different EUV passbands.

HXR imaging showed little overlap between erupted material and HXR sources, indicating that their emission was not primarily driven by local nonthermal electron heating.<br><br>This work demonstrates that spectral variability UV lines, and dynamic motions in the chromosphere, during solar flares are driven primarily by heating of the chromosphere by nonthermal electrons, with a significant contribution also being made by emission from erupted material above in numerous events.

Links

Where it is published

Catalogue records · 1

Topics

Provenance · 3 source records, 13 field assertions
SourceKeyLast seenRaw
ZivaHuboai:figshare.com:article/328262426 d agoJSON v1
Deakin Research Onlineoai:figshare.com:article/328262426 d agoJSON v1
DMU Figshareoai:figshare.com:article/328262426 d agoJSON v1
FieldAssertionExtractorEvidence
concepts[field].local:field:chemistrymapping · figshare dmu ac ukconnector:figshare_dmu_ac_uk@1.0.0
concepts[field].local:field:chemistrymapping · dro deakin edu auconnector:dro_deakin_edu_au@1.0.0
concepts[field].local:field:chemistrymapping · zivahub uct ac zaconnector:zivahub_uct_ac_za@1.0.0
concepts[field].local:field:earth-environmentalmapping · dro deakin edu auconnector:dro_deakin_edu_au@1.0.0
concepts[field].local:field:earth-environmentalmapping · figshare dmu ac ukconnector:figshare_dmu_ac_uk@1.0.0
concepts[field].local:field:earth-environmentalmapping · zivahub uct ac zaconnector:zivahub_uct_ac_za@1.0.0
concepts[modality].local:modality:imagingmapping · figshare dmu ac ukvocabulary-mapper@1.0.0keywords['imaging']
concepts[modality].local:modality:imagingmapping · zivahub uct ac zavocabulary-mapper@1.0.0keywords['imaging']
concepts[modality].local:modality:imagingmapping · dro deakin edu auvocabulary-mapper@1.0.0keywords['imaging']
descriptionsource · zivahub uct ac zaconnector:zivahub_uct_ac_za@1.0.0/metadata/dc/description
license_textsource · zivahub uct ac zaconnector:zivahub_uct_ac_za@1.0.0
publication_datesource · zivahub uct ac zaconnector:zivahub_uct_ac_za@1.0.0
titlesource · zivahub uct ac zaconnector:zivahub_uct_ac_za@1.0.0/metadata/dc/title