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Solar Flare Spectroscopy
L Fletcher - Annual Review of Astronomy and Astrophysics, 2024 - annualreviews.org
This review covers the techniques, observations, and inferences of solar flare spectroscopy.
It is not a spectroscopist's view of solar flares but rather a solar flare physicist's view of …
It is not a spectroscopist's view of solar flares but rather a solar flare physicist's view of …
A New View of the Solar Interface Region from the Interface Region Imaging Spectrograph (IRIS)
Abstract The Interface Region Imaging Spectrograph (IRIS) has been obtaining near-and far-
ultraviolet images and spectra of the solar atmosphere since July 2013. IRIS is the highest …
ultraviolet images and spectra of the solar atmosphere since July 2013. IRIS is the highest …
The F-CHROMA grid of 1D RADYN flare models
Context. Solar flares are the result of the sudden release of magnetic energy in the corona.
Much of this energy goes into accelerating charged particles to high velocity. These particles …
Much of this energy goes into accelerating charged particles to high velocity. These particles …
Probing the physics of the solar atmosphere with the multi-slit solar explorer (MUSE). II. flares and eruptions
Current state-of-the-art spectrographs cannot resolve the fundamental spatial
(subarcseconds) and temporal (less than a few tens of seconds) scales of the coronal …
(subarcseconds) and temporal (less than a few tens of seconds) scales of the coronal …
Magnetohydrodynamic turbulence formation in solar flares: 3D simulation and synthetic observations
Turbulent plasma motion is common in the universe and invoked in solar flares to drive
effective acceleration leading to high-energy electrons. Unresolved mass motions are …
effective acceleration leading to high-energy electrons. Unresolved mass motions are …
The existence of hot X-ray onsets in solar flares
Context. It is well known among the scientific community that solar flare activity often begins
well before the main impulsive energy release. However, a consistent explanation for this …
well before the main impulsive energy release. However, a consistent explanation for this …
Solar flare ribbon fronts. I. Constraining flare energy deposition with IRIS spectroscopy
Spectral lines formed at lower atmospheric layers show peculiar profiles at the" leading
edge" of ribbons during solar flares. In particular, increased absorption of the BBSO/GST He …
edge" of ribbons during solar flares. In particular, increased absorption of the BBSO/GST He …
He I 10830 Å dimming during solar flares. I. The crucial role of nonthermal collisional ionizations
While solar flares are predominantly characterized by an intense broadband enhancement
to the solar radiative output, certain spectral lines and continua will, in theory, exhibit flare …
to the solar radiative output, certain spectral lines and continua will, in theory, exhibit flare …
An observationally constrained model of strong magnetic reconnection in the solar chromosphere-Atmospheric stratification and estimates of heating rates
Context. The evolution of the photospheric magnetic field plays a key role in the energy
transport into the chromosphere and the corona. In active regions, newly emerging magnetic …
transport into the chromosphere and the corona. In active regions, newly emerging magnetic …
Solar Flare Ribbon Fronts. II. Evolution of heating rates in individual flare footpoints
Solar flare ribbon fronts appear ahead of the bright structures that normally characterize
solar flares, and can persist for an extended period of time in spatially localized patches …
solar flares, and can persist for an extended period of time in spatially localized patches …