Time-resolved properties and global trends in dMe flares from simultaneous photometry and spectra

AF Kowalski, SL Hawley, JP Wisniewski… - The Astrophysical …, 2013 - iopscience.iop.org
We present a homogeneous analysis of line and continuum emission from simultaneous
high-cadence spectra and photometry covering near-ultraviolet and optical wavelengths for …

The Sun as a star: observations of white-light flares

M Kretzschmar - Astronomy & Astrophysics, 2011 - aanda.org
Context. Solar flares radiate energy at all wavelengths, but the spectral distribution of this
energy is still poorly known. White-light continuum emission is sometimes observed, and …

[HTML][HTML] On extreme geomagnetic storms

C Cid, J Palacios, E Saiz, A Guerrero… - Journal of Space …, 2014 - swsc-journal.org
Extreme geomagnetic storms are considered as one of the major natural hazards for
technology-dependent society. Geomagnetic field disturbances can disrupt the operation of …

Eruptive–Impulsive Homologous M-class Flares Associated with Double-decker Flux Rope Configuration in Minisigmoid of NOAA 12673

PK Mitra, B Joshi, AM Veronig, R Chandra… - The Astrophysical …, 2020 - iopscience.iop.org
We present a multiwavelength analysis of two homologous, short-lived, impulsive flares of
GOES class M1. 4 and M7. 3 that occurred from a very localized minisigmoid region within …

On the injection of helicity by the shearing motion of fluxes in relation to flares and coronal mass ejections

P Vemareddy, A Ambastha, RA Maurya… - The Astrophysical …, 2012 - iopscience.iop.org
An investigation of helicity injection by photospheric shear motions is carried out for two
active regions (ARs), NOAA 11158 and 11166, using line-of-sight magnetic field …

Velocity and magnetic transients driven by the X2. 2 white-light flare of 2011 February 15 in NOAA 11158

RA Maurya, P Vemareddy… - The Astrophysical …, 2012 - iopscience.iop.org
The first X-class flare of the current solar cycle 24 occurred in Active Region NOAA 11158
during its central meridian passage on 2011 February 15. This two-ribbon white-light flare …

Non-LTE calculations of the Fe I 6173 Å line in a flaring atmosphere

J Hong, MD Ding, Y Li, M Carlsson - The Astrophysical Journal …, 2018 - iopscience.iop.org
The Fe i 6173 Å line is widely used in the measurements of vector magnetic fields by
instruments including the Helioseismic and Magnetic Imager (HMI). We perform non-local …

Altitude Heterogeneity of Magnetic Fields and Doppler Velocities in the Area of Seismic Source of a Strong Solar Flare from Data in Helium, Sodium, and Nickel Lines

II Yakovkin, NI Lozitska, VG Lozitsky - Universe, 2024 - mdpi.com
Measurements of magnetic fields near seismic sources during solar flares are vital for
understanding the dynamics of solar activity. We used spectropolarimetric observations of …

Chromospheric Sunspot Oscillations in Hα and Ca ii 8542 Å

RA Maurya, J Chae, H Park, H Yang, D Song… - Initial Results from the …, 2015 - Springer
We study chromospheric oscillations including umbral flashes and running penumbral
waves in a sunspot of active region NOAA 11242 using scanning spectroscopy in Hα and …

Case study of a magnetic transient in NOAA 11429 observed by SDO/HMI during the M7. 9 flare on 2012 March 13

BJ Harker, AA Pevtsov - The Astrophysical Journal, 2013 - iopscience.iop.org
ABSTRACT NOAA 11429 was the source of an M7. 9 X-ray flare at the western solar limb
(N18 W63) on 2012 March 13 at 17: 12 UT. Observations of the line-of-sight magnetic flux …