361 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Goddard Space Flight CenterUS285 papers
- Catholic University of AmericaUS75 papers
- University of AmericaUS75 papers
- University of Maryland, Baltimore CountyUS51 papers
- University of Maryland, College ParkUS45 papers
- University of California, BerkeleyUS44 papers
- Centre National de la Recherche ScientifiqueFR42 papers
- Johns Hopkins University Applied Physics LaboratoryUS36 papers
- George Mason UniversityUS33 papers
- University of New HampshireUS28 papers
- Sorbonne UniversitéFR27 papers
- Southwest Research InstituteUS27 papers
21 papers · 2 filters
Energetic Proton Back-Precipitation onto the Solar Atmosphere in Relation to Long-Duration Gamma-Ray Flares
Adam Hutchinson, Silvia Dalla, Timo Laitinen +4
Gamma-ray emission during long-duration gamma-ray flare (LDGRF) events is thought to be caused mainly by 300 MeV protons interacting with the ambient plasma at or near the photo…
Magnetic Field Line Random Walk and Solar Energetic Particle Path Lengths: Stochastic Theory and PSP/ISoIS Observation
R. Chhiber, W. H. Matthaeus, C. M. S. Cohen +21
Context:In 2020 May-June, six solar energetic ion events were observed by the Parker Solar Probe/ISoIS instrument suite at 0.35 AU from the Sun. From standard velocity-dispersion a…
From Pseudostreamer Jets to CMEs: Observations of the Breakout Continuum
Pankaj Kumar, Judith T. Karpen, Spiro K. Antiochos +3
The magnetic breakout model, in which reconnection in the corona leads to destabilization of a filament channel, explains numerous features of eruptive solar events, from small-sca…
Modeling Interplanetary Expansion and Deformation of CMEs with ANTEATR-PARADE I: Relative Contribution of Different Forces
C. Kay, T. Nieves-Chinchilla
Coronal Mass Ejections (CMEs) are key drivers of space weather activity but most predictions have been limited to the expected arrival time of a CME, rather than the internal prope…
Deciphering Solar Magnetic Activity: 140 Years Of The `Extended Solar Cycle' -- Mapping the Hale Cycle
Scott W. McIntosh, Robert J. Leamon, Ricky Egeland +6
We investigate the occurrence of the "extended solar cycle" (ESC) as it occurs in a host observational data spanning 140 years. Investigating coronal, chromospheric, photospheric a…
Observations and modeling of the onset of fast reconnection in the solar transition region
L. -J. Guo, B. De Pontieu, Y. -M. Huang +2
Magnetic reconnection is a fundamental plasma process that plays a critical role not only in energy release in the solar atmosphere, but also in fusion, astrophysical, and other sp…
The Solar Orbiter Science Activity Plan: translating solar and heliospheric physics questions into action
I. Zouganelis, A. De Groof, A. P. Walsh +182
Solar Orbiter is the first space mission observing the solar plasma both in situ and remotely, from a close distance, in and out of the ecliptic. The ultimate goal is to understand…
Transition region contribution to AIA observations in the context of coronal heating
Samuel J. Schonfeld, James A. Klimchuk
We investigate the relative contributions from the transition region and corona of coronal loops observed by the Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observator…
Nanoflare Diagnostics from Magnetohydrodynamic Heating Profiles
Kalman J. Knizhnik, Will T. Barnes, Jeffrey W. Reep +1
The nanoflare paradigm of coronal heating has proven extremely promising for explaining the presence of hot, multi-million degree loops in the solar corona. In this paradigm, local…
Identifying Flux Rope Signatures Using a Deep Neural Network
Luiz F. G. dos Santos, Ayris Narock, Teresa Nieves-Chinchilla +2
Among the current challenges in Space Weather, one of the main ones is to forecast the internal magnetic configuration within Interplanetary Coronal Mass Ejections (ICMEs). Current…
Analysis of the Helical Kink Stability of Differently Twisted Magnetic Flux Ropes
Marta Florido-Llinas, Teresa Nieves-Chinchilla, Mark G. Linton
Magnetic flux ropes (MFRs) are usually considered to be the magnetic structure that dominates the transport of helicity from the Sun into the heliosphere. They entrain a confined p…
Connecting Atmospheric Properties and Synthetic Emission of Shock Waves Using 3D RMHD Simulations of Quiet Sun
Viacheslav M. Sadykov, Irina N. Kitiashvili, Alexander G. Kosovichev +1
We analyze the evolution of shock waves in high-resolution 3D radiative MHD simulations of the quiet Sun and their synthetic emission characteristics. The simulations model the dyn…
Solar Flare Arcade Modelling: Bridging the gap from 1D to 3D Simulations of Optically Thin Radiation
Graham S. Kerr, Joel C. Allred, Vanessa Polito
Solar flares are 3D phenomenon but modelling a flare in 3D, including many of the important processes in the chromosphere, is a computational challenge. Accurately modelling the ch…
Hot X-ray Onsets of Solar Flares
Hugh S. Hudson, Paulo J. A. Simoes, Lyndsay Fletcher +2
The study of the localized plasma conditions before the impulsive phase of a solar flare can help us understand the physical processes that occur leading up to the main flare energ…
Inferences About the Magnetic Field Structure of a CME with Both In Situ and Faraday Rotation Constraints
Brian E. Wood, Samuel Tun-Beltran, Jason E. Kooi +2
On 2012 August 2, two CMEs (CME-1 and CME-2) erupted from the west limb of the Sun as viewed from Earth, and were observed in images from the white light coronagraphs on the SOHO a…
Using radio triangulation to understand the origin of two subsequent type II radio bursts
Immanuel Christopher Jebaraj, Jasmina Magdalenic, Tatiana Podladchikova +7
Context: Eruptive events such as coronal mass ejections (CMEs) and flares accelerate particles and generate shock waves which can arrive at Earth and can disturb the magnetosphere.…
Prediction of Dst during solar minimum using in situ measurements at L5
R. L. Bailey, C. Möstl, M. A. Reiss +6
Geomagnetic storms resulting from high-speed streams can have significant negative impacts on modern infrastructure due to complex interactions between the solar wind and geomagnet…
Statistical Study of GOES X-ray Quasi-Periodic Pulsations in Solar Flares
Laura A. Hayes, Andrew R. Inglis, Steven Christe +2
Small amplitude quasi-periodic pulsations (QPPs) detected in soft X-ray emission are commonplace in many flares. To date, the underpinning processes resulting in the QPPs are unkno…
The Extreme Space Weather Event in 1903 October/November: An Outburst from the Quiet Sun
Hisashi Hayakawa, Paulo Ribeiro, José M. Vaquero +11
While the Sun is generally more eruptive during its maximum and declining phases, observational evidence shows certain cases of powerful solar eruptions during the quiet phase of t…
Density Fluctuations in the Solar Wind Based on Type III Radio Bursts Observed by Parker Solar Probe
Vratislav Krupar, Adam Szabo, Milan Maksimovic +20
Radio waves are strongly scattered in the solar wind, so that their apparent sources seem to be considerably larger and shifted than the actual ones. Since the scattering depends o…
Relating streamer flows to density and magnetic structures at the Parker Solar Probe
Alexis P. Rouillard, Athanasios Kouloumvakos, Angelos Vourlidas +34
The physical mechanisms that produce the slow solar wind are still highly debated. Parker Solar Probe's (PSP's) second solar encounter provided a new opportunity to relate in situ…