Search Results - "MIERLA, M"
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OBSERVATIONAL EVIDENCE OF TORUS INSTABILITY AS TRIGGER MECHANISM FOR CORONAL MASS EJECTIONS: THE 2011 AUGUST 4 FILAMENT ERUPTION
Published in The Astrophysical journal (20-04-2014)“…Solar filaments are magnetic structures often observed in the solar atmosphere and consist of plasma that is cooler and denser than their surroundings. They…”
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The Role of Streamers in the Deflection of Coronal Mass Ejections: Comparison between STEREO Three-dimensional Reconstructions and Numerical Simulations
Published in The Astrophysical journal (01-01-2012)“…On 2009 September 21, a filament eruption and the associated coronal mass ejection (CME) were observed by the Solar Terrestrial Relations Observatory (STEREO)…”
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AUTOMATED DETECTION OF CORONAL MASS EJECTIONS IN STEREO HELIOSPHERIC IMAGER DATA
Published in The Astrophysical journal (10-12-2016)“…ABSTRACT We have performed, for the first time, the successful automated detection of coronal mass ejections (CMEs) in data from the inner heliospheric imager…”
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Solar Sources of Interplanetary Coronal Mass Ejections During the Solar Cycle 23/24 Minimum
Published in Solar physics (01-10-2014)“…We examine solar sources for 20 interplanetary coronal mass ejections (ICMEs) observed in 2009 in the near-Earth solar wind. We performed a detailed analysis…”
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Comparisons of CME Morphological Characteristics Derived from Five 3D Reconstruction Methods
Published in Solar physics (2013)“…We compare different methods to reconstruct three-dimensional (3D) coronal mass ejection (CME) morphology. The explored methods include geometric localisation,…”
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The SWAP EUV Imaging Telescope. Part II: In-flight Performance and Calibration
Published in Solar physics (01-08-2013)“…The Sun Watcher with Active Pixel System detector and Image Processing (SWAP) telescope was launched on 2 November 2009 onboard the ESA PROBA2 technological…”
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TRACKING THE CME-DRIVEN SHOCK WAVE ON 2012 MARCH 5 AND RADIO TRIANGULATION OF ASSOCIATED RADIO EMISSION
Published in The Astrophysical journal (20-08-2014)“…We present a multiwavelength study of the 2012 March 5 solar eruptive event, with an emphasis on the radio triangulation of the associated radio bursts. The…”
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Typical Profiles and Distributions of Plasma and Magnetic Field Parameters in Magnetic Clouds at 1 AU
Published in Solar physics (01-08-2016)“…Magnetic clouds (MCs) are a subset of interplanetary coronal mass ejections (ICMEs). They are important because of their simple internal magnetic field…”
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Comparing the Heliospheric Cataloging, Analysis, and Techniques Service (HELCATS) Manual and Automatic Catalogues of Coronal Mass Ejections Using Solar Terrestrial Relations Observatory/Heliospheric Imager (STEREO/HI) Data
Published in Solar physics (01-02-2022)“…We present the results of a comparative study between automatic and manually compiled coronal mass ejection (CME) catalogues based on observations from the…”
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On the 3-D reconstruction of Coronal Mass Ejections using coronagraph data
Published in Annales geophysicae (1988) (01-01-2010)“…Coronal Mass ejections (CMEs) are enormous eruptions of magnetized plasma expelled from the Sun into the interplanetary space, over the course of hours to…”
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The Eruption of 22 April 2021 as Observed by Solar Orbiter: Continuous Magnetic Reconnection and Heating After the Impulsive Phase
Published in Solar physics (01-01-2023)“…We report on one of the first solar-eruptive events that was simultaneously observed by three of the remote-sensing instruments onboard Solar Orbiter during…”
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On 3D Reconstruction of Coronal Mass Ejections: I. Method Description and Application to SECCHI-COR Data
Published in Solar physics (01-10-2009)“…The data from SECCHI-COR1 and SECCHI-COR2 coronagraphs onboard the STEREO mission, which was launched in October 2006, provide us with the first-ever…”
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Study of Multiple Coronal Mass Ejections at Solar Minimum Conditions
Published in Solar physics (01-11-2012)“…The aim of this work is to provide a physical explanation for the genesis of multiple coronal mass ejections (CMEs) in an asymmetric coronal field…”
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Estimating Travel Times of Coronal Mass Ejections to 1 AU Using Multi-spacecraft Coronagraph Data
Published in Solar physics (01-08-2012)“…We study the relationship between the speeds of coronal mass ejections (CMEs) obtained close to the Sun and in the interplanetary medium during the low…”
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On the Tomographic Reconstruction of the 3D Electron Density for the Solar Corona from STEREO COR1 Data
Published in Solar physics (01-10-2009)“…We present for the first time a three-dimensional reconstruction of the electron density in the corona at distances from 1.5 R ⊙ to 4 R ⊙ using COR1 STEREO…”
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Linking Remote-Sensing and In Situ Observations of Coronal Mass Ejections Using STEREO
Published in Solar physics (01-06-2011)“…The twin STEREO spacecraft have been observing the Sun since 2006. Even though STEREO has only been active during solar minimum conditions so far, an important…”
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Study of a Prominence Eruption using PROBA2/SWAP and STEREO/EUVI Data
Published in Solar physics (01-08-2013)“…Observations of the early rise and propagation phases of solar eruptive prominences can provide clues about the forces acting on them through the behavior of…”
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Study of Coronal Jets During Solar Minimum Based on STEREO/SECCHI Observations
Published in Solar physics (01-07-2010)“…During the 2007 – 2008 minimum of solar activity, the internally occulted coronagraphs SECCHI-COR1 onboard the STEREO space mission recorded numerous jet-like…”
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A Quick Method for Estimating the Propagation Direction of Coronal Mass Ejections Using STEREO-COR1 Images
Published in Solar physics (01-11-2008)“…We describe here a method to obtain the position of a coronal moving feature in a three-dimensional coordinate system based on height – time measurements…”
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3D Reconstruction of the Leading Edge of the 20 May 2007 Partial Halo CME
Published in Solar physics (01-10-2009)“…We have reconstructed the leading edge of a coronal mass ejection (CME) observed on 20 May 2007 by COR1 and COR2 of the SECCHI suite onboard the twin STEREO…”
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