Results 61 to 70 of about 34,498 (251)

Effect of Finite Larmor Radius on the Cosmic Ray Penetration into an Interplanetary Magnetic Flux Rope

open access: yes, 2010
We discuss a mechanism for cosmic ray penetration into an interplanetary magnetic flux rope, particularly the effect of the finite Larmor radius and magnetic field irregularities.
Cane   +18 more
core   +1 more source

Magnetic field disturbances in the sheath region of a super-sonic interplanetary magnetic cloud [PDF]

open access: yesAnnales Geophysicae, 2008
It is well-known that interplanetary magnetic clouds can cause strong geomagnetic storms due to the high magnetic field magnitude in their interior, especially if there is a large negative Bz component present.
E. Romashets, M. Vandas, S. Poedts
doaj   +1 more source

The Characteristics of Energetic Electron Precipitation Based on Low Altitude FY‐3E Satellite Measurements

open access: yesGeophysical Research Letters, Volume 52, Issue 14, 28 July 2025.
Abstract This study statistically analyzes the electron precipitation patterns from 40 to 600 keV on dawnside and duskside and their correlations with geomagnetic activities and solar wind conditions based on Low‐Earth Orbit Fengyun‐3E (FY‐3E) satellite during July 2021 to May 2024.
Yu‐Xuan Li   +11 more
wiley   +1 more source

Estimating the Magnetic Structure of an Erupting CME Flux Rope From AR12158 Using Data-Driven Modeling

open access: yesFrontiers in Astronomy and Space Sciences, 2021
We investigate here the magnetic properties of a large-scale magnetic flux rope related to a coronal mass ejection (CME) that erupted from the Sun on September 12, 2014 and produced a well-defined flux rope in interplanetary space on September 14–15 ...
Emilia K. J. Kilpua   +4 more
doaj   +1 more source

Slow Solar Wind: Origin in an Independent Small‐Scale Solar Dynamo

open access: yesGeophysical Research Letters, Volume 52, Issue 13, 16 July 2025.
Abstract Separation of the solar wind (SW) into three flow types (coronal mass ejections (CMEs), high speed streams (HSSs), and slow solar wind (SSW)) reveals an inverse relationship between the percentage of time Earth spends in SSW during a year and its annually averaged magnetic field strength (B).
E. W. Cliver   +2 more
wiley   +1 more source

Conjugate auroras and the interplanetary magnetic field [PDF]

open access: yesJournal of Geophysical Research: Space Physics, 1997
Earlier results from analyses of auroral all‐sky data obtained on several series of conjugate flights along the College, Alaska, magnetic meridian are reevaluated, and it is suggested that while the diffuse aurora is conjugate, the discrete aurora is nonconjugate but still on closed field lines.
H. C. Stenbaek-Nielsen, A. Otto
openaire   +2 more sources

Statistical Analysis of the Short Large‐Amplitude Magnetic Structures: Evolution and Ion Resonance

open access: yesGeophysical Research Letters, Volume 52, Issue 13, 16 July 2025.
Abstract Short large‐amplitude magnetic structures (SLAMS) play a fundamental role in the formation and energy conversion of the collisionless shock. Nevertheless, the evolution and the ion dynamics inside SLAMS are still unclear. In this study, we performed a superposed analysis of SLAMS near the Earth's bow shock to investigate their properties and ...
Shi‐Chen Bai   +6 more
wiley   +1 more source

Development of Space Magnetometers in Austria

open access: yesProceedings, 2018
With spaceborne magnetic field measurements it is possible to investigate the interior of planets,moons and asteroids which have either an intrinsic or a crustal magnetic field.
Werner Magnes   +12 more
doaj   +1 more source

Can an interplanetary magnetic field reach the surface of Venus? [PDF]

open access: yesAnnales Geophysicae, 2018
We address the question of whether there is a possibility of an interplanetary magnetic field reaching Venus' surface by magnetic diffusion across the ionosphere.
Y. Narita   +3 more
doaj   +1 more source

Upstream IMF Influence on Closed Magnetic Field Orientation on Mars

open access: yesGeophysical Research Letters, Volume 52, Issue 13, 16 July 2025.
Abstract Closed magnetic fields play an important role in plasma transport and atmospheric escape from the Martian dayside ionosphere. Leveraging in‐situ magnetic field data from the Mars Atmosphere and Volatile EvolutioN (MAVEN) mission, we conduct a statistical analysis of closed magnetic field behavior under varying upstream conditions. Our findings
JunFeng Qin   +5 more
wiley   +1 more source

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