Results 1 to 10 of about 25,490 (221)
Dust in the Interplanetary Medium [PDF]
Plasma Physics and Controlled Fusion, 2010 The mass density of dust particles that form from asteroids and comets in the interplanetary medium of the solar system is, near 1 AU, comparable to the mass density of the solar wind.
Czechowski, Andrzej +4 more
core +5 more sources
The Astrophysical Journal, 2023 Low-frequency fluctuations in the interplanetary medium represent a turbulent environment where universal scaling behavior, generated by an energy cascade, has been investigated.
Federica Chiappetta +4 more
doaj +1 more source
INFLUENCE OF THE SOLAR WIND ON INTERFEROMETRIC OBSERVATIONS AT THE DECAMETER WAVELENGTHS [PDF]
Radio Physics and Radio Astronomy, 2020 Purpose: The effect of the Earth’s ionosphere and interplanetary plasma on the radio astronomy observations, in particular, interferometric ones, at decameter waves has been investigated.
V. O. Shepelev +3 more
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On the solar origin of interplanetary disturbances observed in the vicinity of the Earth [PDF]
Annales Geophysicae, 2003 The solar origin of 40 interplanetary disturbances observed in the vicinity of the Earth between January 1997 and June 1998 is investigated in this paper.
N. Vilmer +4 more
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Transport in the interplanetary medium of coronal mass ejections [PDF]
Geofísica Internacional, 2008 Coronal mass ejections (CMEs) are large scale structures of plasma and magnetic field expelled from the Sun to the interplanetary medium and generally observed in white light coronagraphs.
A. Ventura, A. Lara, A. Borgazzi
doaj +3 more sources
Case studies of space weather events from their launching on the Sun to their impacts on power systems on the Earth [PDF]
Annales Geophysicae, 2002 Active geomagnetic conditions on 12–13, 15–16, and 22–23 September 1999 resulted in geomagnetically induced currents (GIC) measurable in power systems in Canada and the United States.
H.-L. Lam +3 more
doaj +1 more source
Frontiers in Physics, 2021 Low–frequency fluctuations in the interplanetary medium have been extensively investigated and described in the framework of turbulence, and the observed universal scaling behavior represents a clear signature of the underlying energy cascade.
Vincenzo Carbone +7 more
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Heliospheric consequences of solar activity in geophysical and interplanetary phenomena [PDF]
Geofísica Internacional, 2004 We have done an analysis of the total solar magnetic flux, polar coronal hole area and sunspots. We investigate their long term evolution over several solar cycles and their possible relationship with interplanetary shocks, sudden storm commencements at ...
D. Maravilla +2 more
doaj +3 more sources
Interplanetary Shocks between 0.3 and 1.0 au: Helios 1 and 2 Observations
The Astrophysical Journal, 2023 The Helios 1 (H1) and Helios 2 (H2) spacecraft measured the solar winds at a distance between ∼0.3 and 1.0 au from the Sun. With increasing heliocentric distance ( r _h ), the plasma speed is found to increase at ∼34–40 km s ^−1 au ^−1 and the density ...
Rajkumar Hajra +5 more
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Reconstruction of the Parker spiral with the Reverse In situ data and MHD APproach – RIMAP
Journal of Space Weather and Space Climate, 2021 The reconstruction of plasma parameters in the interplanetary medium is very important to understand the interplanetary propagation of solar eruptions and for Space Weather application purposes.
Biondo Ruggero +3 more
doaj +1 more source