Results 51 to 60 of about 490,789 (126)

Acceleration of protons by interplanetary shocks [PDF]

open access: yes, 1970
Acceleration of protons by interplanetary ...
Arens, J. F., Ogilvie, K. W.
core  

Features of Ground Level Enhancement (GLE #74) Event on 11 May 2024

open access: yesJournal of Geophysical Research: Space Physics, Volume 131, Issue 10, October 2026.
Abstract Ground Level Enhancement (GLE #74) occurred on 11 May 2024 following an X5.8 solar flare from active region AR 13668 and the associated halo coronal mass ejection. The event was observed by both ground‐based neutron monitors (NMs) and space‐borne instruments and occurred during a deep Forbush decrease and one of the strongest geomagnetic ...
Alexander Mishev   +5 more
wiley   +1 more source

Global Magnetospheric Response to an Interplanetary Shock: THEMIS Observations [PDF]

open access: yes, 2011
We investigate the global response of geospace plasma environment to an interplanetary shock at approx. 0224 UT on May 28, 2008 from multiple THEMIS spacecraft observations in the magnetosheath (THEMIS B and C) and the mid-afternoon (THEMIS A) and dusk ...
Zhang, Hui   +6 more
core  

A case study of large-amplitude ULF waves in the Martian foreshock

open access: yesEarth and Planetary Physics, 2020
Foreshock ultralow frequency (ULF) waves constitute a significant physical phenomenon in the plasma environment of terrestrial planets. The occurrence of these waves, associated with backstreaming particles reflected and accelerated at the bow shock ...
LiCan Shan, YaSong Ge, AiMin Du
doaj   +1 more source

Statistical Mapping of ULF Wave Power in the Vicinity of Earth's Bow Shock Using Cluster Magnetic Field Data

open access: yesJournal of Geophysical Research: Space Physics, Volume 131, Issue 10, October 2026.
Abstract Ultra‐low frequency (ULF) waves with frequencies 10–140 s are a characteristic feature of the foreshock, playing important roles in transient formation, shock reformation, and particle acceleration. We utilize 23 years of Cluster data to map ULF wave power and compressibility in the vicinity of Earth's bow shock, combining Cluster data with ...
R. L. Atkinson   +4 more
wiley   +1 more source

On the stability and structure of shock waves in interplanetary space [PDF]

open access: yes, 1965
Structure of interplanetary shock waves formed by interaction of geomagnetic field and solar wind - earth bow ...
Hinton, F. L.
core  

Interplanetary Shocks Observed from Multipoints at Venus and 1 au

open access: yesThe Astrophysical Journal
We present a database of 12 fast forward interplanetary (IP) shocks observed in situ by radially aligned spacecraft (Venus Express, Wind, and/or STEREO) between 2006 and 2014.
Can Wang   +8 more
doaj   +1 more source

Kelvin–Helmholtz Spectral Redistribution by Flow and Density Structure at the Dusk Dayside Magnetopause

open access: yesJournal of Geophysical Research: Space Physics, Volume 131, Issue 10, October 2026.
Abstract We study the development of the Kelvin‐Helmholtz instability (KHI) along the dusk dayside Earth's magnetopause with and without the presence of enhanced plasma density at the shear interface. Using three‐dimensional MAGE global simulations, we establish general KHI growth rate diagrams, which depend sensitively on the transverse profiles of ...
G. Peyrichon   +8 more
wiley   +1 more source

Response of Thermospheric Nitric Oxide (NO) Cooling During Events of Strong Solar Wind Pressure

open access: yesJournal of Geophysical Research: Space Physics, Volume 131, Issue 10, October 2026.
Abstract Nitric oxide (NO) infrared emissions are a notable indicator for varying thermospheric energy budget during geomagnetic storms while the Interplanetary Magnetic Field (IMF) is southward. In this study, we present the first investigation on the response of NO cooling emissions during northward IMF conditions.
Alok Kumar Ranjan   +2 more
wiley   +1 more source

Solar Orbiter IRFU Interplanetary Shock List

open access: yes
<p>This is a list of interplanetary shocks observed by Solar Orbiter. Some were found by eye but the majority have been detected automatically using MAG and SWA-PAS measuremetns.
Dimmock, Andrew
core   +1 more source

Home - About - Disclaimer - Privacy