The STEREO Mission: An Introduction

By M. Kaiser, T. Kucera, J. Davila, O. C. Cyr, M. Guhathakurta, E. Christian. 2008

1,542 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/8010e867aa7cf27f2a7550b9a9ece0bdee192a24

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. M. Temmer
2. N. Lugaz
3. A. Vourlidas
4. B. Vršnak
5. A. Thernisien
6. W. Manchester IV
7. R. Howard
8. J. Davies

In Molecular Biology

1. A. Thernisien
2. M. Temmer
3. N. Lugaz
4. A. Vourlidas
5. J. Davies
6. T. Sakurai
7. S. Patsourakos
8. Ilia I. Roussev

Citations in the corpus

• ACTIVITY IN GEMINID PARENT (3200) PHAETHON (2010, background): “Asteroid 1999 YC may also be dynamically related to Phaethon but its surface appears more nearly neutral with respect to the color of the Sun (Kasuga and Jewitt 2008).”
• The Physical Processes of CME/ICME Evolution (2017, background): “2015; Kay and Opher 2015) showing that slow, wide and low-mass CMEs deflect most as shown in Fig. 5. The rate of CME deflection is clearly fastest close to the Sun where magnetic forces dominate. The analysis of 14 CMEs by Isavnin et al. (2014) showed that about 60% of the total evolution from the S”
• The magnetic field in the solar atmosphere (2014, neutral): “STEREO Solar-TErrestrial RElations Observatory (Kaiser et al. 2008)”
• GEOMETRIC TRIANGULATION OF IMAGING OBSERVATIONS TO TRACK CORONAL MASS EJECTIONS CONTINUOUSLY OUT TO 1 AU (2010, methodology): “Accurate determination of the propagation direction is feasible with multiple views of the Sun-Earth space from the Solar Terrestrial Relations Observatory (STEREO; Kaiser et al. 2008).”
• Solar Orbiter (2012, background): “…et al., 1992), SOHO (Domingo, Fleck, and Poland, 1995), TRACE (Handy et al., 1999), RHESSI (Lin et al., 2002), Hinode (Kosugi et al., 2007), STEREO (Kaiser et al., 2008) and SDO (Pesnell, Thompson, and Chamberlin, 2012) have formed the foundation of our understanding of the solar corona, the…”
• CONNECTING SPEEDS, DIRECTIONS AND ARRIVAL TIMES OF 22 CORONAL MASS EJECTIONS FROM THE SUN TO 1 AU (2014, methodology): “The Solar TErrestrial RElations Observatory (STEREO, Kaiser et al. 2008), launched in late 2006, consists of two spacecraft, one ahead (STEREOA) and one behind the Earth (STEREO-B) in orbits around the Sun.”
• ON SUN-TO-EARTH PROPAGATION OF CORONAL MASS EJECTIONS (2013, methodology): “Accurate determination of CME Sun-to-Earth kinematics is feasible with the launch of the Solar Terrestrial Relations Observatory (STEREO; Kaiser et al. 2008).”
• THREE-DIMENSIONAL MODELING OF QUASI-HOMOLOGOUS SOLAR JETS (2010, background): “Recently, the ground-breaking stereoscopic capabilities of the STEREO mission (Kaiser et al. 2008) enabled direct insights into the helical structure of jets (Kamio et al. 2010).”
• The Interaction of Successive Coronal Mass Ejections: A Review (2016, methodology): “…coronagraphs such as the Large Angle and Spectrometric Coronagraph Experiment on board the Solar and Heliospheric Observatory (SOHO/LASCO: Domingo, Fleck, and Poland, 1995, Brueckner et al., 1995) and the Solar-Terrestrial Relations Observatory coronagraphs (STEREO/COR: Kaiser et al., 2008).”
• A multi-block-matching approach for stereo (2015, background): “D sensing with a wide application range in robotics [1], [2], [3], intelligent vehicles [4], [5], [6], [7] and also space science [8], [9].”
• NUMERICAL SIMULATION OF AN EUV CORONAL WAVE BASED ON THE 2009 FEBRUARY 13 CME EVENT OBSERVED BY STEREO (2009, methodology): “Following the launch of the Solar Terrestrial Relations Observatory (STEREO; Kaiser et al. 2008), coronal waves are now observed with increased temporal and spatial resolution, and have now been seen from two perspectives using the Extreme Ultra-Violet Imagers (EUVI; Wuelser et al. 2004).”
• ON A CORONAL BLOWOUT JET: THE FIRST OBSERVATION OF A SIMULTANEOUSLY PRODUCED BUBBLE-LIKE CME AND A JET-LIKE CME IN A SOLAR EVENT (2011, methodology): “In this paper, for the first time, we present a coronal blowout jet that was associated a simultaneous bubble-like and a jet-like CMEs observed by the inner coronagraph (COR1, Thompson, et al. (2003)) on board Solar Terrestrial Relations Observatory Ahead (STEREO, Kaiser et al. (2008)).”
• SIMULTANEOUS OBSERVATION OF RECONNECTION INFLOW AND OUTFLOW ASSOCIATED WITH THE 2010 AUGUST 18 SOLAR FLARE (2011, methodology): “…EUV images of this flare were obtained by the Extreme Ultraviolet Imager (EUVI; Howard et al. 2008; Wüelser et al. 2004) on the Solar Terrestrial Relation Observatory spacecraft Ahead (STEREO-A; Kaiser et al. 2008) and the Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO).”
• THE DEFLECTION OF THE TWO INTERACTING CORONAL MASS EJECTIONS OF 2010 MAY 23–24 AS REVEALED BY COMBINED IN SITU MEASUREMENTS AND HELIOSPHERIC IMAGING (2012, methodology): “Until the launch of the Solar-Terrestrial Relations Observatory (STEREO, see: Kaiser et al. 2008) in 2006, there was very limited data available beyond the field-of-view (FOV) of coronagraphs (∼ 0.15 AU).”