Results 31 to 40 of about 932,549 (275)

Modelling interplanetary CMEs using magnetohydrodynamic simulations [PDF]

Annales Geophysicae, 2002
The dynamics of Interplanetary Coronal Mass Ejections (ICMEs) are discussed from the viewpoint of numerical modelling. Hydrodynamic models are shown to give a good zero-order picture of the plasma properties of ICMEs, but they cannot model the ...
P. J. Cargill, P. J. Cargill, J. M. Schmidt   +2 more
doaj   +1 more source

Disappearance of plasmaspheric hiss following interplanetary shock [PDF]

, 2015
Plasmaspheric hiss is one of the important plasma waves controlling radiation belt dynamics. Its spatiotemporal distribution and generation mechanism are presently the object of active research.
Abel, Agapitov, Albert, Baker, Baker, Baker, Blake, Blake, Bortnik, Bortnik, Bortnik, Bortnik, C. A. Kletzing, Chao Shen, Chen, Chen, Chen, Chen, Chen, Chen, D. N. Baker, Foster, Fu, Fuliang Xiao, Funsten, G. B. Hospodarsky, G. D. Reeves, Glauert, Golden, Goldstein, Gonzalez, Gonzalez, Green, H. E. Spence, H. O. Funsten, Hayakawa, Heppner, Horne, Hudson, Hui Zhu, Huinan Zheng, J. B. Blake, J. R. Wygant, Kennel, Kennel, Kletzing, Kurth, Li, Li, Li, Li, Li, Lyons, Mauk, McComas, Meredith, Meredith, Meurant, Min Zhang, Mourenas, Ni, Nunn, Omura, Peng, Reeves, Ronnmark, Russell, Samsonov, Sheeley, Shklyar, Shprits, Shue, J., Shui Wang, Smith, Sonwalkar, Spence, H. E., Stone, Su, Su, Su, Su, Su, Z., Subbotin, Summers, Summers, Summers, Thorne, Thorne, Thorne, Thorne, R. M., Tsurutani, Tsurutani, B. T., Tu, Turner, Ukhorskiy, W. S. Kurth, Wang, Wygant, J., Yuming Wang, Zhang, Zhenpeng Su, Zhou, Zong   +102 more
core   +3 more sources

Turbulence Upstream and Downstream of Interplanetary Shocks

Frontiers of Physics, 2021
The paper reviews the interaction of collisionless interplanetary (IP) shocks with the turbulent solar wind. The coexistence of shocks and turbulence plays an important role in understanding the acceleration of particles via Fermi acceleration mechanisms,
A. Pitňa, J. Šafránková, Z. Němeček, T. Ďurovcová, A. Kis   +4 more
semanticscholar   +1 more source

The Isotropic Interplanetary Dust Cloud and Near-infrared Extragalactic Background Light Observed with COBE/DIRBE [PDF]

Astrophysical Journal, 2020
We report observation of isotropic interplanetary dust (IPD) by analyzing the infrared (IR) maps of the Diffuse Infrared Background Experiment (DIRBE) on board the Cosmic Background Explorer (COBE) spacecraft.
K. Sano, S. Matsuura, Kazuma Yomo, Aoi Takahashi College of Science, Engineering, S. O. Mathematics, Physics, K. University, D. Physics, School of Materials Science, Kwansei Gakuin University, Department of Electrical Engineering, T. University, Astrobiology Center   +13 more
semanticscholar   +1 more source

Observations of interplanetary scintillation during the 1998 Whole Sun Month: a comparison between EISCAT, ORT and Nagoya data [PDF]

Annales Geophysicae, 2000
Observations of interplanetary scintillation (IPS) allow accurate solar wind velocity measurements to be made at all heliographic latitudes and at a range of distances from the Sun.
P. J. Moran, P. J. Moran, P. J. Moran, S. Ananthakrishnan, V. Balasubramanian, A. R. Breen, A. Canals, R. A. Fallows, P. Janardhan, P. Janardhan, M. Tokumaru, P. J. S. Williams   +11 more
doaj   +1 more source

Physical Properties of the Interplanetary Dust [PDF]

International Astronomical Union Colloquium, 1971
The interplanetary dust may be composed of cometary material, interstellar grains, debris from asteroidal collisions, primordial material formed by direct condensation, or contributions from all of these sources. Before we can determine the origin of the dust, we need to know its physical nature, spatial distribution, and the dynamical forces that act ...
openaire   +1 more source

Interplanetary mesoscale observatory (InterMeso): A mission to untangle dynamic mesoscale structures throughout the heliosphere

Frontiers in Astronomy and Space Sciences, 2022
Mesoscale dynamics are a fundamental process in space physics, but fall within an observational gap of current and planned missions. Particularly in the solar wind, measurements at the mesoscales (100s RE to a few degrees heliographic longitude at 1 au ...
R. Allen, Evan J. Smith, B. Anderson, J. Borovsky, G. Ho, L. Jian, S. Krucker, S. Lepri, Gang Li, S. Livi, N. Lugaz, D. Malaspina, B. Maruca, P. Mostafavi, J. Raines, D. Verscharen, J. Vievering, S. Vines, P. Whittlesey, L. Wilson III, R. Wimmer–Schweingruber   +20 more
semanticscholar   +1 more source

Band-splitting of coronal and interplanetary type II bursts [PDF]

Astronomy & Astrophysics, 2003
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Vršnak, Bojan, Magdalenić, Jasmina, Zlobec, Paolo   +2 more
openaire   +2 more sources

Beyond Basic Drag in Interplanetary CME Modeling: Effects of Solar Wind Pileup and High‐Speed Streams

Space Weather, 2022
Coronal mass ejections (CMEs) cause severe space weather effects throughout our solar system. As a fast CME propagates through interplanetary space, it accumulates solar wind materials at its front.
C. Kay, T. Nieves-chinchilla, S. Hofmeister, E. Palmerio   +3 more
semanticscholar   +1 more source

Predictions of the arrival time of Coronal Mass Ejections at 1AU: an analysis of the causes of errors [PDF]

Annales Geophysicae, 2004
Three existing models of Interplanetary Coronal Mass Ejection (ICME) transit between the Sun and the Earth are compared to coronagraph and in situ observations: all three models are found to perform with a similar level of accuracy (i.e.
M. Owens, P. Cargill
doaj   +1 more source