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 …
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 …
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 …
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 …
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 …
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 …
Measurements of magnetic fields near seismic sources during solar flares are vital for understanding the dynamics of solar activity. We used spectropolarimetric observations of …
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 …
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 …