Ulysses observations of the high-latitude solar wind have shown that on time scales of \u3c 1 day, the polar wind is dominated by pressure balance structures (PBSs). Fluctuations of the plasma beta within PBSs appear to be strongly correlated with fluctuations in the helium abundance. The correlation occurs in both the northern and southern hemispheres. In addition, a mechanism is apparently at work in the high-latitude solar wind that dissipates the beta/He correlation over a distance of a few AU. Solar wind composition is established at the base of the corona; thus, the He abundance signature strongly suggests the observed solar wind PBSs are associated with structures low in the solar atmosphere. In particular, high-beta structures appea...
International audienceA sizable total-pressure (magnetic pressure plus kinetic pressure) enhancement...
International audienceAbstract The solar wind measured in situ by Parker Solar Probe in the very inn...
[1] Time variations in plasma beta and a parameter which measures isotropy in suprathermal electron ...
Ulysses observations of the high-latitude solar wind have shown that on time scales of \u3c 1 day, t...
Observations from the second Ulysses fast latitude scan show that the global structure of solar wi...
Solar wind compressive fluctuations at MHD scales have been extensively studied in the past using d...
The solar wind properties depend on λ, the heliomagnetic latitude with respect to the helios...
The Ulysses mission is providing the first opportunity to observe variations in solar wind plasma pa...
The mass flux density and velocity of the solar wind at polar latitudes can provide strong constrain...
The hot solar atmosphere continually expands out into space to form the solar wind, which drags with...
Spacecraft observations from the interplanetary medium of our solar system reveal the presence of a ...
Context: The recent launches of Parker Solar Probe, Solar Orbiter (SO), and BepiColombo, along with ...
The solar wind measured in situ by Parker Solar Probe in the very inner heliosphere is studied in co...
Observations of the corona and solar wind are analyzed and compared with generalized results derived...
49heights up to 10 or more solar radii by various coronal instruments in the EUV and VL channels (fi...
International audienceA sizable total-pressure (magnetic pressure plus kinetic pressure) enhancement...
International audienceAbstract The solar wind measured in situ by Parker Solar Probe in the very inn...
[1] Time variations in plasma beta and a parameter which measures isotropy in suprathermal electron ...
Ulysses observations of the high-latitude solar wind have shown that on time scales of \u3c 1 day, t...
Observations from the second Ulysses fast latitude scan show that the global structure of solar wi...
Solar wind compressive fluctuations at MHD scales have been extensively studied in the past using d...
The solar wind properties depend on λ, the heliomagnetic latitude with respect to the helios...
The Ulysses mission is providing the first opportunity to observe variations in solar wind plasma pa...
The mass flux density and velocity of the solar wind at polar latitudes can provide strong constrain...
The hot solar atmosphere continually expands out into space to form the solar wind, which drags with...
Spacecraft observations from the interplanetary medium of our solar system reveal the presence of a ...
Context: The recent launches of Parker Solar Probe, Solar Orbiter (SO), and BepiColombo, along with ...
The solar wind measured in situ by Parker Solar Probe in the very inner heliosphere is studied in co...
Observations of the corona and solar wind are analyzed and compared with generalized results derived...
49heights up to 10 or more solar radii by various coronal instruments in the EUV and VL channels (fi...
International audienceA sizable total-pressure (magnetic pressure plus kinetic pressure) enhancement...
International audienceAbstract The solar wind measured in situ by Parker Solar Probe in the very inn...
[1] Time variations in plasma beta and a parameter which measures isotropy in suprathermal electron ...