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19942026
most citedObservation of Gravitational Waves from a Binary Black Hole Merger

14.2k citations

Showing 2018Show all

59 papers · 1 filter

astro-ph.HE2018★ 72 cited

Observatory science with eXTP

Jean J. M. in 't Zand, Enrico Bozzo, Jinlu Qu +181

In this White Paper we present the potential of the enhanced X-ray Timing and Polarimetry (eXTP) mission for studies related to Observatory Science targets. These include flaring s…

astro-ph.SR2018★ 40 cited

Evolution of A Magnetic Flux Rope toward Eruption

Wensi Wang, Chunming Zhu, Jiong Qiu +3

It is well accepted that a magnetic flux rope (MFR) is a critical component of many coronal mass ejections (CMEs), yet how it evolves toward eruption remains unclear. Here we inves…

astro-ph.HE2018★ 65 cited

The Impact of Radio AGN Bubble Composition on the Dynamics and Thermal Balance of the Intracluster Medium

H. -Y. K. Yang, M. Gaspari, C. Marlow

Feeding and feedback of active galactic nuclei (AGN) are critical for understanding the dynamics and thermodynamics of the intracluster medium (ICM) within the cores of galaxy clus…

astro-ph.SR2018★ 21 cited

Evidence of Twisting and Mixed-polarity Solar Photospheric Magnetic Field in Large Penumbral Jets: IRIS and Hinode Observations

Sanjiv K. Tiwari, Ronald L. Moore, Bart De Pontieu +4

A recent study using {\it Hinode} (SOT/FG) data of a sunspot revealed some unusually large penumbral jets that often repeatedly occurred at the same locations in the penumbra, name…

astro-ph.CO2018★ 20 cited

To be or not to be: hot WHIM absorption in the blazar PKS 2155-304 sight line?

J. Nevalainen, E. Tempel, J. Ahoranta +8

The cosmological missing baryons at z<1 most likely hide in the hot (T K) phase of the Warm Hot Intergalactic Medium (WHIM). While the hot WHIM is hard to detect d…

astro-ph.SR2018★ 25 cited

A Two-Sided-Loop X-Ray Solar Coronal Jet Driven by a Minifilament Eruption

Alphonse C. Sterling, Louise K. Harra, Ronald L. Moore +1

Most of the commonly discussed solar coronal jets are of the type consisting of a single spire extending approximately vertically from near the solar surface into the corona. Recen…

astro-ph.SR2018★ 67 cited

IRIS and SDO Observations of Solar Jetlets Resulting from Network-Edge Flux Cancelation

Navdeep K. Panesar, Alphonse C. Sterling, Ronald L. Moore +3

Recent observations show that the buildup and triggering of minifilament eruptions that drive coronal jets result from magnetic flux cancelation at the neutral line between merging…

astro-ph.GA2018★ 72 cited

Spectacular HST observations of the Coma galaxy D100 and star formation in its ram pressure stripped tail

William J. Cramer, Jeffrey D. P. Kenney, Ming Sun +5

We present new HST F275W, F475W, and F814W imaging of the region of the Coma cluster around D100, a spiral galaxy with a remarkably long and narrow ( kpc) ram pressu…

astro-ph.SR2018★ 69 cited

Magnetohydrodynamic Simulation of the X9.3 Flare on 2017 September 6: Evolving Magnetic Topology

Chaowei Jiang, Peng Zou, Xueshang Feng +7

Three-dimensional magnetic topology is crucial to understanding the explosive release of magnetic energy in the corona during solar flares. Much attention has been given to the pre…

astro-ph.GA2018★ 8 cited

Probing the dynamical state, baryon content, and multiphase nature of galaxy clusters with bright background QSOs

Chong Ge, Q. Daniel Wang, Joseph N. Burchett +5

We have initiated a programme to study the physical/dynamical state of gas in galaxy clusters and the impact of the cluster environment on gaseous halos of individual galaxies usin…

astro-ph.HE2018★ 10 cited

Probability models of chance fluctuations in spectra of astronomical sources with applications to X-ray absorption lines

Massimiliano Bonamente

The search for faint emission or absorption lines in astronomical spectra has received considerable attention in recent years, especially in the X-ray wavelength range. These featu…

astro-ph.SR2018

Modeling Inner Boundary Values at 18 Solar Radii During Solar Quiet time for Global Three-dimensional Time-Dependent Magnetohydrodynamic Numerical Simulation

Chin-Chun Wu, Kan Liou, Simon Plunkett +6

The solar wind speed plays a key role in the transport of CME out of the Sun and ultimately determines the arrival time of CME-driven shocks in the heliosphere. Here, we develop an…

astro-ph.SR2018★ 77 cited

Automated detection of small-scale magnetic flux ropes in the solar wind: First results from the Wind spacecraft measurements

Qiang Hu, Jinlei Zheng, Yu Chen +2

We have developed a new automated small-scale magnetic flux rope (SSMFR) detection algorithm based on the Grad-Shafranov (GS) reconstruction technique. We have applied this detecti…

astro-ph.GA2018★ 31 cited

A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE).V. Properties of the ionised gas filament of M87

A. Boselli, M. Fossati, A. Longobardi +22

We have observed the giant elliptical galaxy M87 during the Virgo Environmental Survey Tracing Galaxy Evolution (VESTIGE), a blind narrow-band Halpha+[NII] imaging survey of the Vi…

physics.comp-ph2018★ 4 cited

Boltzmann-Fokker-Planck Kinetic Solver with Adaptive Mesh in Phase Space

Vladimir Kolobov, Robert Arslanbekov, Dmitry Levko

We describe the implementation of kinetic solvers in 1d2v phase space using adaptive Cartesian mesh. Spherical coordinates in velocity space are used to simplify the Lorentz and Fo…

astro-ph.HE2018★ 44 cited

A Fermi Gamma-ray Burst Monitor Search for Electromagnetic Signals Coincident with Gravitational-Wave Candidates in Advanced LIGO's First Observing Run

ray Burst Monitor Team, The LIGO Scientific Collaboration, the Virgo Collaboration +1160

We present a search for prompt gamma-ray counterparts to compact binary coalescence gravitational wave (GW) candidates from Advanced LIGO's first observing run (O1). As demonstrate…

physics.ao-ph2018★ 1 cited

Performance of a simple proxy for U.S. cloud-to-ground lightning

Michael K. Tippett, Chiara Lepore, William J. Koshak +2

The product of convective available potential energy (CAPE) and precipitation rate has previously been used as a proxy for cloud-to-ground (CG) lightning flash counts in climate ch…

astro-ph.SR2018★ 55 cited

Plasma Energization in Colliding Magnetic Flux Ropes

Senbei Du, Fan Guo, Gary P. Zank +2

Magnetic flux ropes are commonly observed throughout the heliosphere, and recent studies suggest that interacting flux ropes are associated with some energetic particle events. In…

physics.plasm-ph2018★ 29 cited

New closures for more precise modeling of Landau damping in the fluid framework

P. Hunana, G. P. Zank, M. Laurenza +5

Incorporation of kinetic effects such as Landau damping into a fluid framework was pioneered by Hammett and Perkins PRL 1990, by obtaining closures of the fluid hierarchy, where th…

physics.plasm-ph2018★ 4 cited

Kinetic Solvers with Adaptive Mesh in Phase Space for Low-Temperature Plasmas

Vladimir Kolobov, Robert Arslanbekov, Dmitry Levko

We describe the implementation of 1d1v and 1d2v Vlasov and Fokker-Planck kinetic solvers with adaptive mesh refinement in phase space (AMPS) and coupling these kinetic solvers to P…

astro-ph.EP2018★ 30 cited

Saturn northern aurorae at solstice from HST observations coordinated with Cassini Grand Finale

L. Lamy, R. Prangé, C. Tao +8

Throughout 2017, the Hubble Space Telescope (HST) observed the northern far-ultraviolet aurorae of Saturn at northern solstice, during the Cassini Grand Finale. These conditions pr…

physics.flu-dyn2018★ 8 cited

Clustering of Rapidly Settling, Low-Inertia Particle Pairs in Isotropic Turbulence. II. Comparison of Theory and DNS

Sarma L. Rani, Rohit Dhariwal, Donald L. Koch

Part I of this study presented a stochastic theory for the clustering of monodisperse, rapidly settling, low-Stokes-number particle pairs in homogeneous isotropic turbulence. The t…

physics.flu-dyn2018★ 7 cited

Clustering of Rapidly Settling, Low-Inertia Particle Pairs in Isotropic Turbulence. I. Drift and Diffusion Flux Closures

Sarma L. Rani, Vijay K. Gupta, Donald L. Koch

In this two--part study, we present the development and analysis of a stochastic theory for characterizing the relative positions of monodisperse, low-inertia particle pairs that a…

astro-ph.SR2018★ 10 cited

Is the enhancement of type II radio bursts during CME interactions related to the associated solar energetic particle event?

Liu-Guan Ding, Zhi-Wei Wang, Li Feng +2

We investigated 64 pairs of interacting-CME events identified by the simultaneous observations of SOHO and STEREO spacecraft from 2010 January to 2014 August, to examine the relati…