Results 101 to 110 of about 15,824 (251)

An ambitious new mission seeks the origin of the moons of Mars. [PDF]

Proc Natl Acad Sci U S A, 2023
Croswell K.
europepmc   +1 more source

Perturbative QCD Calculations of Elliptic Flow and Shear Viscosity in Au+Au Collisions at $\sqrt{s_{NN}}=200$ GeV

, 2008
The elliptic flow $v_2$ and the ratio of the shear viscosity over the entropy density, $\eta/s$, of gluon matter are calculated from the perturbative QCD (pQCD) based parton cascade Boltzmann approach of multiparton scatterings. For Au+Au collisions at $\
Greiner, Carsten, Stoecker, Horst, Xu, Zhe   +2 more
core   +1 more source

Phobos

, 2020
This music score was submitted for the Kaleidoscope 2020 Call for Scores, an open access collaboration with the UCLA Music Library.
openaire   +1 more source

Elliptic Flow and Initial Eccentricity in Cu+Cu and Au+Au Collisions at RHIC

, 2007
We present a systematic study of elliptic flow as a function of centrality, pseudorapidity, transverse momentum and energy for Cu+Cu and Au+Au collisions from the PHOBOS experiment.
Alver B, Heinz U W, Hirano T, Rachid Nouicer, the PHOBOS Collaboration   +4 more
core   +1 more source

Calibration of the MEGANE gamma-ray and neutron spectrometer for JAXA’s Mars Moon eXplorer (MMX) mission to Phobos

Progress in Earth and Planetary Science
JAXA’s Mars Moon eXploration (MMX) spacecraft carries a NASA-provided γ-ray and neutron spectrometer called MEGANE. MEGANE’s measurements will be used to characterize the elemental composition of Mars’ largest and innermost moon, Phobos, with the goal of
Patrick N. Peplowski, Samuel Fix, Morgan T. Burks, John O. Goldsten, David J. Lawrence, Kathryn Marcotte, Brian Schratz, Zachary W. Yokley, Sarah Bucior, Erik Ramseth, Jack T. Wilson   +10 more
doaj   +1 more source

Longitudinal heterogeneity of Phobos’ crater size-frequency distribution: coevolution of resurfacing and orbital dynamics

Progress in Earth and Planetary Science
Phobos always keeps the same side facing its host planet like Earth’s Moon, making it a key comparative target for studying the coevolution of planet–satellite systems.
Yuki Uchida, Kosei Toyokawa, Tomohiro Usui, Yudai Suzuki, Haruhisa Tabata   +4 more
doaj   +1 more source

Surface science on Phobos with the navigation cameras of the MMX IDEFIX rover

Progress in Earth and Planetary Science
A CNES/DLR rover called IDEFIX will be deployed on the surface of Phobos in late 2028 or early 2029 as part of JAXA’s Martian Moons eXploration (MMX) mission.
Pierre Vernazza, Laurent Jorda, Simon Tardivel, Julien Baroukh, Olivier Groussin, Celia Pimorin, Axel Poulain, Pierre-Yves Chabaud, Emilie Robert, Jean Bertrand, Valerian Lalucaa, Emile Remetean, Nicolas Théret, Cedric Virmontois, Naomi Murdoch, Stéphane Le Mouélic, Pierre Beck, Ottaviano Rüsch, Jessica Flahaut, Sebastien Charnoz, Jeremie Lasue, Maria-Antonietta Barucci, Alain Doressoundiram, Patrick Michel, Stephan Ulamec   +24 more
doaj   +1 more source

Editorial: Methods and applications in emotion regulation and processing. [PDF]

Front Behav Neurosci, 2023
Cicvaric A.
europepmc   +1 more source

Science operations of IDEFIX, the MMX Phobos rover

Progress in Earth and Planetary Science
IDEFIX, a rover to be delivered to the martian moon Phobos, is part of the Martian Moons eXploration (MMX) mission by the Japan Aerospace Exploration Agency, JAXA.
Stephan Ulamec, Patrick Michel, N. Murdoch, P. Vernazza, M. Grott, J. Knollenberg, S. Schröder, H.-W. Hübers, Y. Cho, O. Prieto-Ballesteros, J. Biele, S. Tardivel, F. Buse, H. Miyamoto, C. Krause, D. May, C. Delmas, J. Baroukh, S. Mary, M. Grebenstein   +19 more
doaj   +1 more source

Exploring the recycling model of Phobos formation: rubble-pile satellites

, 2022
Gustavo Madeira, S. Charnoz
openalex   +2 more sources