Results 81 to 90 of about 20,985 (231)
Switchbacks, characterized by large-angle deflections of the local interplanetary magnetic field relative to the background, are frequently observed throughout the heliosphere and play a crucial role in the solar wind dynamics.
Hui Li +4 more
doaj +1 more source
Hybrid Simulations of the Cusp and Dayside Magnetosheath Dynamics Under Quasi-Radial Interplanetary Magnetic Fields. [PDF]
Ng J +4 more
europepmc +1 more source
Magnetic Field Variations in Interplanetary Space [PDF]
Magnetic field variations and structures in interplanetary space are described and related to the sun. Discrete flare-related effects in the interplanetary medium occur within a large-scale interplanetary sector pattern related to a solar sector pattern that is ordered over a large extent in heliographic latitude and longitude.
openaire +1 more source
Interplanetary magnetic fields as a cause of comet tails [PDF]
Interplanetary magnetic fields as cause of comet ...
Beard, D. B., Nakada, M. P.
core +1 more source
Identifying MESSENGER Magnetospheric Boundary Crossings Using a Random Forest Region Classifier
Abstract We present a new list of bow shock and magnetopause crossings based on automated region classification for the MESSENGER (Mercury Surface, Space Environment, Geochemistry and Ranging) mission. We fit a random forest model to magnetometer and ephemeris data to classify the solar wind, magnetosheath, and magnetosphere regions surrounding Mercury.
Daragh M. Hollman +6 more
wiley +1 more source
Surface Waves at Switchback Boundaries in the Young Solar Wind from Parker Solar Probe Observations
Switchbacks (SBs) are localized magnetic field deflections in the solar wind, marked by abrupt changes in the magnetic field direction relative to the ambient solar wind.
Kyung-Eun Choi +4 more
doaj +1 more source
Intermittent character of interplanetary magnetic field fluctuations
Interplanetary magnetic field magnitude fluctuations are notoriously more intermittent than velocity fluctuations in both fast and slow wind. This behavior has been interpreted in terms of the anomalous scaling observed in passive scalars in fully developed hydrodynamic turbulence.
Bruno, R. +5 more
openaire +5 more sources
On the flow of a magnetized solar wind around the moon [PDF]
Effects of interplanetary magnetic fields on flow of plasma around ...
Jokipii, J. R.
core +1 more source
SOLAR ERUPTION ON 4 JANUARY 2011: CASE STUDY FOR SPACE EARLY WARNING [PDF]
We perform intuitive analysis for solar eruption on 4 January 2011. Since we do not have magnetic observational data from the eruption, we perform first order calculation and expands it as interplanetary total effect of energy propagation by retro ...
Bambang, Setiahadi
core
We analyze the well observed flare-CME event from October 1, 2011 (SOL2011-10-01T09:18) covering the complete chain of action - from Sun to Earth - for a better understanding of the dynamic evolution of the CME and its embedded magnetic field.
Dissauer, K. +6 more
core +1 more source

