85 citations · 412 across the 22 of their papers we have counts for
22 papers
PRICM3: A novel Polarization Ratio framework for three-dimensional CME reconstruction
Yara De Leo, Manuela Temmer, Fernando M. López +15
Coronal mass ejections (CMEs) are inherently three-dimensional (3D), but traditional white-light coronagraphs provide only two-dimensional (2D) projections. While the Polarization…
A view of the evolution of a CME and the associated wave-trains at high spatial and temporal resolution
G. Russano, Y. De Leo, F. Frassati +13
Context. Studying the kinematic and dynamic evolution of fast eruptive events from the middle to high solar corona is a primary objective of the Metis coronagraph on Solar Orbiter.…
On the dynamics, thermodynamics and fine structure of virtual erupting filaments
Dion Donné, Yuhao Zhou, Hebe Cremades +1
It is not fully understood why some solar filaments erupt while others do not. Those that do typically undergo a slow rise followed by an acceleration phase, though this transition…
Automatic detection of CMEs using synthetically-trained Mask R-CNN
Francisco A. Iglesias, Diego G. Lloveras, Florencia L. Cisterna +6
Coronal mass ejections (CMEs) are a major driver of space weather. To assess CME geoeffectiveness, among other scientific goals, it is necessary to reliably identify and characteri…
Catastrophic disruption of asteroid 2023 CX1 and implications for planetary defense
Auriane Egal, Denis Vida, François Colas +94
Mitigation of the threat from airbursting asteroids requires an understanding of the potential risk they pose for the ground. How asteroids release their kinetic energy in the atmo…
Current status of the Extension of the FRIPON network in Chile
Felipe Gutiérrez Rojas, Sébastien Bouquillon, Rene A. Mendez +17
FRIPON is an efficient ground-based network for the detection and characterization of fireballs, which was initiated in France in 2016 with over one hundred cameras and which has b…
Kilometric type II radio emissions in Wind/WAVES TNR data and association with interplanetary structures near Earth
Franco Manini, Hebe Cremades, Fernando M. López +1
Type II radio bursts arise as a consequence of shocks typically driven by coronal mass ejections (CMEs). When these shocks propagate outward from the Sun, their associated radio em…
Quantifying errors in 3D CME parameters derived from synthetic data using white-light reconstruction techniques
Christine Verbeke, M. Leila Mays, Christina Kay +10
(Shortened version) Current efforts in space weather forecasting of CMEs have been focused on predicting their arrival time and magnetic structure. To make predictions, methods hav…
Distorted-Toroidal Flux Rope model for Heliospheric Flux Ropes
Teresa Nieves-Chinchilla, Miguel Angel Hidalgo, Hebe Cremades
The three-dimensional characterization of magnetic flux-ropes observed in the heliosphere has been a challenging task for decades. This is mainly due to the limitation to infer the…
Analysis of the Evolution of a Multi-Ribbon Flare and Failed Filament Eruption
Reetika Joshi, Cristina H. Mandrini, Ramesh Chandra +5
How filaments form and erupt are topics about which solar researchers have wondered since more than a century and that are still open to debate. We present observations of a filame…
Pseudostreamer influence on flux rope evolution
A. Sahade, M. Cécere, M. V. Sieyra +3
A critical aspect of solar activity is the coupling between eruptions and the surrounding coronal magnetic field, which determines the trajectory and morphology of the eruptive eve…
Direct First PSP Observation of the Interaction of Two Successive Interplanetary Coronal Mass Ejections in November 2020
Teresa Nieves-Chinchilla, Nathalia Alzate, Hebe Cremades +18
We investigate the effects of the evolutionary processes in the internal magnetic structure of two interplanetary coronal mass ejections (ICMEs) detected in situ between 2020 Novem…
Polarity relevance in flux rope deflections triggered by coronal holes
Abril Sahade, Mariana Cécere, Andrea Costa +1
Many observations show that coronal holes (CHs) deviate coronal mass ejections (CMEs) away from them. However, there are some peculiar events reported where the opposite occurs. To…
Analysis of large deflections of prominence-CME events during the rising phase of solar cycle 24
M. V. Sieyra, M. Cécere, H. Cremades +7
Motivated by the need to improve the ability to forecast whether a certain coronal mass ejection (CME) is to impact Earth, and by the insufficiency of statistical studies that anal…
Asymmetric expansion of coronal mass ejections in the low corona
Hebe Cremades, Francisco A. Iglesias, Luciano A. Merenda
Aims. The study of the morphology of coronal mass ejections (CMEs) is an auspicious approach to understanding how magnetic fields are structured within CMEs. Although earlier studi…
Analysis of a long-duration AR throughout five solar rotations: Magnetic properties and ejective events
Francisco A. Iglesias, Hebe Cremades, Luciano A. Merenda +4
Coronal mass ejections (CMEs), which are among the most magnificent solar eruptions, are a major driver of space weather and can thus affect diverse human technologies. Different p…
Moreton and EUV Waves Associated with an X1.0 Flare and CME Ejection
Carlos Francile, Fernando M. López, Hebe Cremades +3
A Moreton wave was detected in active region (AR) 12017 on 29 March 2014 with very high cadence with the Halpha Solar Telescope for Argentina (HASTA) in association with an X1.0 fl…
Blowout Jets and Impulsive Eruptive Flare in a Bald-Patch Topology
R. Chandra, C. H. Mandrini, B. Schmieder +7
Context: A subclass of broad EUV and X-ray jets, called blowout jets, have become a topic of research since they could be the link between standard collimated jets and CMEs.} Aim:…
First Simultaneous Views of the Axial and Lateral Perspectives of a Coronal Mass Ejection
I. Cabello, H. Cremades, L. Balmaceda +1
The different appearances exhibited by coronal mass ejections (CMEs) are believed to be in part the result of different orientations of their main axis of symmetry, consistent with…
Low-frequency type II radio detections and coronagraph data to describe and forecast the propagation of 71 CMEs/shocks
H. Cremades, F. A. Iglesias, O. C. St. Cyr +3
The vulnerability of technology on which present society relies demands that a solar event, its time of arrival at Earth, and its degree of geoeffectiveness be promptly forecasted.…
Coronal mass ejections from the same active region cluster: Two different perspectives
H. Cremades, C. H. Mandrini, B. Schmieder +1
The cluster formed by active regions (ARs) NOAA 11121 and 11123, approximately located on the solar central meridian on 11 November 2010, is of great scientific interest. This comp…
Linking two consecutive nonmerging magnetic clouds with their solar sources
S. Dasso, C. H. Mandrini, B. Schmieder +10
On 15 May 2005, a huge interplanetary coronal mass ejection (ICME) was observed near Earth. It triggered one of the most intense geomagnetic storms of solar cycle 23 (Dst peak = -2…