Results 211 to 220 of about 29,430 (259)

Polymethylhydrosiloxane-Coated Ammonium Dinitramide: A Simple Strategy to Moisture-Resistant and Insensitive Energetic Microspheres. [PDF]

ACS Omega
Bui AT, Pham QH, Pham VT, Vu MT, Cao HT.
europepmc   +1 more source

Correlations and Kappa Distributions: Numerical Experiment with 3D Collisions and Debye-like Shielding. [PDF]

Entropy (Basel)
McComas DJ, Livadiotis G, Sarlis N.
europepmc   +1 more source

The role of ultrasound in the nucleation kinetics and Modification of product properties of 3-Nitro-1,2,4-triazol-5-one. [PDF]

Ultrason Sonochem
Hu X, Wu H, Chang P, Zhang Y, Xu C, Zhai L, Wang B.   +6 more
europepmc   +1 more source

Harnessing non-equilibrium forces to optimize work extraction. [PDF]

Nat Commun
Olsen KS, Goerlich R, Roichman Y, Löwen H.   +3 more
europepmc   +1 more source

Nonlinear spatiotemporal signatures of whistler-mode wave activity around Mercury during six flybys of BepiColombo mission. [PDF]

Nat Commun
Ozaki M, Yagitani S, Kasaba Y, Kasahara Y, Matsuda S, Omura Y, Hikishima M, Sahraoui F, Mirioni L, Chanteur G, Murakami G.   +10 more
europepmc   +1 more source

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Energetic Particle Observations

Space Science Reviews, 2006
The characteristics of solar energetic particles (SEP) as observed in interplanetary space provide fundamental information about the origin of these particles, and the acceleration and propagation processes at the Sun and in interplanetary space. Furthermore, energetic particles provide information on the development and structure of coronal mass ...
Berndt Klecker, Karoly Kecskeméty, David Lario   +2 more
exaly   +5 more sources

Energetic Particle Influence on the Earth’s Atmosphere [PDF]

Space Science Reviews, 2015
This manuscript gives an up-to-date and comprehensive overview of the effects of energetic particle precipitation (EPP) onto the whole atmosphere, from the lower thermosphere/mesosphere through the stratosphere and troposphere, to the surface. The paper summarizes the different sources and energies of particles, principally\ud galactic cosmic rays ...
Keri Nicoll, Ilya Usoskin, Esa Turunen   +2 more
exaly   +4 more sources

Energetic Particles in the Jovian Magnetotail

Science, 2007
When the solar wind hits Jupiter's magnetic field, it creates a long magnetotail trailing behind the planet that channels material out of the Jupiter system. The New Horizons spacecraft traversed the length of the jovian magnetotail to >2500 jovian radii ( R J ; 1 R J
R L, McNutt, D K, Haggerty, M E, Hill, S M, Krimigis, S, Livi, G C, Ho, R S, Gurnee, B H, Mauk, D G, Mitchell, E C, Roelof, D J, McComas, F, Bagenal, H A, Elliott, L E, Brown, M, Kusterer, J, Vandegriff, S A, Stern, H A, Weaver, J R, Spencer, J M, Moore   +19 more
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Energetic Particles at High Latitudes

Space Science Reviews, 1995
We review work on diffusion coefficients of energetic particles with an attempt to extract implications on their behaviour at high latitudes. In the ecliptic plane results from solar energetic particle propagation between the Sun and about 5 AU can be described by an effective radial mean free path λ r which is approximately constant as a function of ...
R. M�ller-Mellin, G. Wibberenz
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Energetic particle experiment ERNE

Solar Physics, 1995
The Energetic and Relativistic Nuclei and Electron (ERNE) experiment will investigate the solar atmosphere and the heliosphere by detecting particles produced in various kinds of energy release processes. ERNE is at the upper end in energy among the SOHO particle instruments.
Torsti, Jarmo, Valtonen, Eino, Lumme, Markku, Peltonen, Petri, Eronen, Timo, Louhola, M., Riihonen, E., Schultz, Göran, Teittinen, M., Ahola, Kimmo, Holmlund, Christer, Kelhä, Väinö, Leppälä, Kari, Ruuska, Pekka, Strömmer, Esko   +15 more
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