The Solar Dynamics Observatory

By W. Pesnell. 2012

1,668 citations recorded by the source corpus.

Subfields: Aerospace Engineering, Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/f04ae817e8a38f29188b47bc71d15213739eb6fb

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In Aerospace Engineering

1. G. Verth
2. K. Nagashima
3. H. Hudson
4. R. Morton
5. S. Grant
6. Ioannis Giagkiozis
7. M. Temmer
8. C. Schrijver

In Astronomy and Astrophysics

1. M. Temmer
2. S. Couvidat
3. Haimin Wang
4. C. Schrijver
5. Chang Liu
6. J. Todd Hoeksema
7. H. Hudson
8. Na Deng

Citations in the corpus

• Comparison of Line-of-Sight Magnetograms Taken by the Solar Dynamics Observatory/Helioseismic and Magnetic Imager and Solar and Heliospheric Observatory/Michelson Doppler Imager (2012, background): “The enhanced Helioseismic and Magnetic Imager (HMI) (Scherrer et al., 2012; Schou et al., 2012) onboard the Solar Dynamics Observatory (SDO) (Pesnell et al., 2012) began making its routine observations on 30 April 2010.”
• Advances in Observing Various Coronal EUV Waves in the SDO Era and Their Seismological Applications (Invited Review) (2014, neutral): “…(STEREO: Kaiser et al., 2008), and the Atmospheric Imaging Assembly (AIA: Lemen et al., 2012) onboard the Solar Dynamics Observatory (SDO: Pesnell, Thompson, and Chamberlin, 2012), have each contributed to shaping our evolving understanding of EIT waves in specific and EUV waves in…”
• MAGNETIC PROPERTIES OF SOLAR ACTIVE REGIONS THAT GOVERN LARGE SOLAR FLARES AND ERUPTIONS (2016, methodology): “For this purpose, we carry out a systematic survey of observational data of flaring ARs obtained by the Solar Dynamics Observatory (SDO; Pesnell et al. 2012).”
• Multiwavelength Studies of MHD Waves in the Solar Chromosphere (2015, methodology): “…al. 2012a) instruments on the Dunn Solar Telescope, Jess et al. (2013) compared the dynamics of RPWs with magnetic field extrapolations obtained with the Helioseismic and Magnetic Imager (HMI; Schmidt et al. 2012; Schou et al. 2012) onboard the Solar Dynamics Observatory (SDO; Pesnell et al. 2012).”
• Predicting Solar Flares Using SDO/HMI Vector Magnetic Data Products and the Random Forest Algorithm (2017, background): “It is notable that since 2010 May, the Helioseismic and Magnetic Imager (HMI; Schou et al. 2012) on board the Solar Dynamics Observatory (SDO; Pesnell et al. 2012) has been producing unprecedented photospheric vector magnetograms with continuous high-cadence (normally 12 minutes), full-disk…”
• THERMAL DIAGNOSTICS WITH THE ATMOSPHERIC IMAGING ASSEMBLY ON BOARD THE SOLAR DYNAMICS OBSERVATORY: A VALIDATED METHOD FOR DIFFERENTIAL EMISSION MEASURE INVERSIONS (2015, background): “Since the launch of NASAʼs Solar Dynamics Observatory (SDO; Pesnell et al. 2012) in 2010, the Atmospheric Imaging Assembly (AIA; Boerner et al. 2012; Lemen et al. 2012) instrument on board SDO has been delivering EUV imaging observations of the solar corona with an unprecedented combination of…”
• The Interaction of Successive Coronal Mass Ejections: A Review (2016, background): “In Solar Cycle 24, high spatial and temporal resolution observations by the Solar Dynamics Observatory (SDO: Pesnell, Thompson, and Chamberlin, 2012) have returned the study of sympathetic eruptions to central stage.”