THE 2011 FEBRUARY 15 X2 FLARE, RIBBONS, CORONAL FRONT, AND MASS EJECTION: INTERPRETING THE THREE-DIMENSIONAL VIEWS FROM THE SOLAR DYNAMICS OBSERVATORY AND STEREO GUIDED BY MAGNETOHYDRODYNAMIC…

By C. Schrijver, G. Aulanier, A. Title, Etienne Pariat, C. Delannée. 2011

159 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/ce61d5a4591656376b22ffc9936cbf685623164c

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In Astronomy and Astrophysics

Citations in the corpus

THERMAL DIAGNOSTICS WITH THE ATMOSPHERIC IMAGING ASSEMBLY ON BOARD THE SOLAR DYNAMICS OBSERVATORY: A VALIDATED METHOD FOR DIFFERENTIAL EMISSION MEASURE INVERSIONS (2015, background): “2 flare (see, e.g., Schrijver et al. 2011; Sun et al. 2012), two M-class flares and more than a dozen C-class flares.”
RESPONSE OF THE PHOTOSPHERIC MAGNETIC FIELD TO THE X2.2 FLARE ON 2011 FEBRUARY 15 (2011, background): “…illustrate in Figure 3, where the flare could be triggered by the tether-cutting reconnection (Moore et al. 1995, 2001) between the two sets of sigmoidal loops FP3–FP2 and FP4–FP1 as clearly discernible in EUV images, which results in the J-shaped flare ribbons (also see Schrijver et al. 2011).”
The standard flare model in three dimensions II: upper limit on solar flare energy (2012, background): “Firstly, sunspot groups incorporate several big sunspots, ranging from a few spots (see e.g. Schrijver et al. 2011, for February 2011) to half a dozen (see e.g. Carrington 1859; Schrijver et al. 2006, for September 1859 and October 2003 respectively) and up to more than ten (see e.g. Wang et al.…”
The Interaction of Successive Coronal Mass Ejections: A Review (2016, background): “A well studied case is AR 11158 based on the SDO/HMI vector magnetograms (see, e.g., Schrijver et al., 2011, Sun et al., 2012, SOLA: Review_v4.tex; 16 March 2017; 5:40; p. 5 Wang et al., 2012, Vemareddy, Ambastha, and Maurya, 2012).”
Solar filament eruptions and their physical role in triggering Coronal Mass Ejections (2012, background): “The long-lived ARs all had strong magnetic activity with flares, filament eruptions and CMEs (Schrijver et al., 2011; Liu et al., 2012c).”
The standard flare model in three dimensions - I. Strong-to-weak shear transition in post-flare loops (2012, background): “Their frequent association with coronal mass ejections (CMEs, see e.g. Schrijver et al. 2011) and with solar energetic particles (SEPs, see e.g. Masson et al. 2009) makes them among the most intense drivers of space weather.”
Advances in Observing Various Coronal EUV Waves in the SDO Era and Their Seismological Applications (Invited Review) (2014, unknown): “2 flare (Schrijver et al., 2011).”
The standard flare model in three dimensions - III. Slip-running reconnection properties (2013, methodology): “The present simulation shows the evolution in time of 3D magnetic fields formerly associated with a sigmoidal pre-eruptive phase similarly as Savcheva et al. (2012), and as depicted in the Figure 21 of Schrijver et al. (2011).”
ELECTRIC CURRENTS IN FLARE RIBBONS: OBSERVATIONS AND THREE-DIMENSIONAL STANDARD MODEL (2014, background): “The comparison with other filters can be seen in Movie 3 of Schrijver et al. (2011).”
MAGNETIC PROPERTIES OF SOLAR ACTIVE REGIONS THAT GOVERN LARGE SOLAR FLARES AND ERUPTIONS (2016, background): “2) flare in solar cycle 24 (e.g., Schrijver et al. 2011), AR 11429 produced the largest (X5.”
EVOLUTION OF MAGNETIC FIELD AND ENERGY IN A MAJOR ERUPTIVE ACTIVE REGION BASED ON SDO/HMI OBSERVATION (2011, methodology): “Expansion of the coronal structure and faint circular propagating fronts are visible starting around 01:48 UT, probably linked to CME initiation (Schrijver et al. 2011).”