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News
Breaking News | Escape route found for Jupiter's particlesspaceflightnow.com › news
spaceflightnow.com
Jun 1, · "The dusk flank of Jupiter's magnetosphere is a surprising contrast to the dawn flank," said Dr. Stamatios (Tom) Krimigis, ...
News | Jupiter Particles' Escape Route Found
www.jpl.nasa.gov
May 31, · "The dusk flank of Jupiter's magnetosphere is a surprising contrast to the dawn flank," said Dr. Stamatios (Tom) Krimigis, a Cassini scientist who heads the space department of the Johns Hopkins University's Applied Physics Laboratory, Laurel, Md. Cassini spent most of January and February skating along the magnetosphere's dusk flank, which is on the side of the planet turning away from the …
Space and Atmospheric Physics Group - News Page
www.sp.ph.ic.ac.uk
... persisted for lower energy ions (below a "cross-over" energy of about 26 keV) but reversed sense to give higher fluxes on the dusk flank at ...
Unique gathering of spacecraft yields new views, clues on Jupiter's...
spaceref.com
Unique gathering of spacecraft yields new views, clues on Jupiter's Magnetosphere - SpaceRef
Interests
Jupiter Particles' Escape Route Found -- ScienceDaily
www.sciencedaily.com
Jun 25, · "The dusk flank of Jupiter's magnetosphere is a surprising contrast to the dawn flank," said Dr. Stamatios (Tom) Krimigis, a Cassini scientist who …
Books & Literature
Dayside Magnetosphere Interactionsbooks.google.com › books
books.google.de
(2012) found more KH waves at the dayside dusk flank magnetopause, this is not in contrast with the results of Nykyri (2013) because for many of the events ...
28th International Symposium on Shock Waves - Google Books
books.google.de
The University of Manchester hosted the 28th International Symposium on Shock Waves between 17 and 22 July The International Symposium on Shock Waves...
CADAM Proceedings - Google Books
books.google.de
The regular solution exists practically only on the dusk flank on which the tangential discontinuity impinges. When the density and, consequently, the dynamic ...
Earth's Magnetosphere: Formed by the Low-Latitude Boundary Layer -...
books.google.co.uk
The author argues that, after five decades of debate about the interactive of solar wind with the magnetosphere, it is time to get back to basics. Starting...
Music
Full text of "Magnetic field configuration in the magnetotail near
archive.org
5 near the dusk flank and gradually increases to + 3 near the dawn flank, revealing a non-uniform lati- tudinal divergence along Y, even though the js! has an ...
Related Documents
Prolonged Kelvin-Helmholtz Waves at Dawn and Dusk Flank ...
www.diva-portal.org
Prolonged Kelvin-Helmholtz Waves at Dawn and Dusk Flank Magnetopause: Simultaneous Observations by MMS and THEMIS Lu, S. W. Chinese Acad Sci, State Key Lab Space Weather, Natl Space Sci Ctr, Beijing , Peoples R China;Univ Chinese Acad Sci, Chinese Acad Sci, Beijing , Peoples R China.
Waves on the dusk flank boundary layer during very northward...
ui.adsabs.harvard.edu
Title: Waves on the dusk flank boundary layer during very northward interplanetary magnetic field conditions: Observations and simulation: Authors:
Electric structure of dipolarization front at sub-proton scale
www.diva-portal.org
We find that there is an electric field at ion inertia scale directed normal to the DF; it has a duskward component at the dusk flank of DF but a ...
Evolution of Kelvin-Helmholtz activity on the dusk flank magnetopause
ui.adsabs.harvard.edu
Title: Evolution of Kelvin-Helmholtz activity on the dusk flank magnetopause: Authors: Foullon, C.; Farrugia, C. J.; Fazakerley, A. N.; Owen, C. J.; Gratton, F. T.; ...
Scientific Publications
Polar Cusps - an overview | ScienceDirect Topics
www.sciencedirect.com
Jul 12, · At closer distances the particles execute normal drift motion confined to the equatorial plane and show higher flux because of longer trapping time; at larger distances these particles reach the dusk flank in the equatorial plane and are lost to the interplanetary medium.
The dusk flank of Jupiter's magnetosphere - PubMedpubmed.ncbi.nlm.nih.gov › ...
pubmed.ncbi.nlm.nih.gov
Limited single-spacecraft observations of Jupiter's magnetopause have been used to infer that the boundary moves inward or outward in response to variations ...
Publications
Evolution of Kelvin-Helmholtz activity on the dusk\ud flank...
core.ac.uk
dusk flank magnetopause. ByC Foullon, C Farrugia, A Fazakerley, C Owen, F Gratton and Roy Torbert ...
Cold and Dense Plasma Sheet Caused by Solar Wind Entry - MDPIwww.mdpi.com › htm
www.mdpi.com
[Google Scholar] [CrossRef]; Fuselier, S.A.; Elphic, R.C.; Gosling, J.T. Composition measurements in the dusk flank magnetopause. J. Geophys. Res.
Plasma Pressure under Magnetopause on the Dusk Flank in the...
link.springer.com
The crossings of the magnetopause and low-latitude boundary layer by the THEMIS-B satellite in the spring of on the dusk flank under large negative XG
"A Statistical Study Into the Spatial Distribution and Dawn-Dusk...
commons.erau.edu
We present evidence that the dawn flank is consistently hotter than the dusk flank for a variety of upstream conditions. Our statistical data also suggest a dependency on solar wind speed such that the level of asymmetry increases with faster speeds. We conclude that the dawn-favored asymmetry of the magnetosheath seed population is ...
Reports & Statements
Steam Community :: spidey002
steamcommunity.com
Dusk Flank United States Level Winged Laser Pony XP . This is the first thing you see and it's telling you what you already know. AKA: Wandering Love Nest, White Mystery Time is like a sifter. Eventually, if you shake it enough, everything falls apart. Like a scrotum, here it is in a nutshell: I …
The dusk flank of Jupiter's magnetosphere | Nature
www.nature.com
Limited single-spacecraft observations of Jupiter's magnetopause have been used to infer that the boundary moves inward or outward in response to variations in...
Project SHOCK - Sodium gyro-resonance with Kelvin-Helmholtz waves at...
project-shock.eu
The official blog of the project SHOCK including own RSS feed.
Dawn–dusk asymmetry in the Kelvin–Helmholtz instability at ...
www.nature.com
The simulations also reveal that as vortices move along the dusk flank, they continue to grow convectively within the bulk flow. Results. MESSENGER spacecraft observations of the KHI at Mercury.
Miscellaneous
Astronomynews - Yahoo Grupos
br.groups.yahoo.com
"The dusk flank of Jupiter's magnetosphere is a surprising contrast to the dawn flank," said Dr. Stamatios (Tom) Krimigis, a Cassini scientist who heads the space ...
Evolution of Kelvin-Helmholtz activity on the dusk flank magnetopause...
wrap.warwick.ac.uk
Our purpose is to characterize the evolution of the magnetopause Kelvin-Helmholtz (KH) wave activity with changes in thickness of the adjacent boundary layer ...
THEMIS Science Nuggets.
www.igpp.ucla.edu
THEMIS encountered an HFA on 4 July The spacecraft were on the dusk flank of the bow shock, and the ground-based observatories were aligned on the dawn side of ...
(PDF) The dusk flank of Jupiter's magnetosphere | W Kurth und Steven...
www.academia.edu
(PDF) The dusk flank of Jupiter's magnetosphere | W Kurth and Steven joy - Academia.edu Academia.edu is a platform for academics to share research papers.
Evidence of surface wave on the dusk flank of Saturn's magnetopause...
www.tib.eu
Title: Evidence of surface wave on the dusk flank of Saturn's magnetopause possibly caused by the Kelvin-Helmholtz instability. Author / Creator: Cutler, J.C. ...
Low latitude dusk flank magnetosheath magnetopause and boundary layer...
www.invenzone.com
Discuss about this paper : Low-latitude dusk flank magnetosheath, magnetopause, and boundary layer for low magnetic shear: wind observations. Platform for...
Motion of the dusk flank boundary layer caused by solar wind -...
www.tib.eu
Title: Motion of the dusk flank boundary layer caused by solar wind pressure changes and the Kelvin-Helmholtz instability: January (DOI ...
Evidence of surface wave on the dusk flank of Saturn's ProQuestsearch.proquest.com › openview
www.proquest.com
First time boundary waves have been observed on the Kronian dusk flank These waves are similar to those observed at dawn by Masters et al.
Evolution of Kelvin-Helmholtz activity on the dusk flank magnetopause
ore.exeter.ac.uk
Title: Evolution of Kelvin-Helmholtz activity on the dusk flank magnetopause. Author: Foullon, Claire Farrugia, Charles J. Fazakerley, Andrew Owen, Christopher ...
Waves on the dusk flank boundary layer during very northward...
deepblue.lib.umich.edu
Waves on the dusk flank boundary layer during very northward interplanetary magnetic field conditions: Observations and simulation
Evolution of Kelvin-Helmholtz activity on the dusk flank magnetopause...
eprints.ucl.ac.uk
UCL Discovery is UCL's open access repository, showcasing and providing access to UCL research outputs from all UCL disciplines.
Results & submissions : REF : Output details
results.ref.ac.uk
Evolution of Kelvin-Helmholtz activity on the dusk flank magnetopause. Type. D - Journal article. DOI JA Title of journal. J GEOPHYS ...
Stable reconnection at the dusk flank magnetopause
ulysses.phys.wvu.edu
Observations of the dusk flank magnetopause by MMS on 28 August show that antiparallel magnetic reconnection is a stable process even at the dawn-dusk terminator. During this magnetopause encounter, motion of the reconnection site appears not to be …
The dusk flank of Jupiter's magnetosphere
deepblue.lib.umich.edu
Abstract: Limited single-spacecraft observations of Jupiter's magnetopause have been used to infer that the boundary moves inward or outward in response to variations ...
1.3 Mission Phases and Science Regions of Interest - MMS ...
lasp.colorado.edu
Extended Mission Year 2 Phase 4a:. September 28, R E Dusk Flank (Dwell time outside BS (0.3 nPa < 10 hrs) MMS_4A_SROIs_v2.pptx: 3 SROI. 20 km Oct 18. Phase 4b: November 29, 2018
ANGEO - Relation between the asymmetric ring current ...
angeo.copernicus.org
The high-latitude anti-sunward currents are connected at their noon and midnight ends to field-aligned currents that lead the currents to the outer magnetosphere. The auroral net current branch on the morning side is closed along the dawn flank near the magnetopause, and the evening side currents flow along the dusk flank magnetosphere.
AGU Chapman Conference on …
agu.confex.com
Abstract: In September 2015, the Magnetospheric Multiscale (MMS) mission begins science operations at the dusk flank magnetopause. This multi-spacecraft mission ...
Dawn-dusk asymmetry in particles of solar wind origin within the...
hal.archives-ouvertes.fr
Ions then need less energy to drift to the dusk flank, so that the cross-over energy, at which the asymmetry changes sense, is reduced.
Abstract: Distinct sources of particles near …
agu.confex.com
This would imply that two distinct sources were active at the same time on the dusk flank of the magnetosphere. In addition, ...
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