Context. The formation of the slow solar wind remains unclear as we lack a complete understanding of its transient outflows. Aims. In a previous work we analysed the white-light coronal brightness as a function of elongation and time from Wide-Field Imager (WISPR) observations on board the Parker Solar Probe (PSP) mission when PSP reached a minimum heliocentric distance of ≈28 R⊙. We found 4–5 transient outflows per day over a narrow wedge in the PSP orbital plane, which is close to the solar equatorial plane. However, the elongation versus time map (J-map) analysis supplied only lower limits on the number of released density structures due to the small spatial-scales of the transient outflows and line-of-sight integration effects. In this ...
Quasi-periodic density structures are important mesoscale structures that constitute the slow solar ...
International audienceThe release of density structures at the tip of the coronal helmet streamers, ...
In paper 1, we showed that the Heliospheric Imager (HI) instruments on the pair of NASA STEREO space...
Context. The formation of the slow solar wind remains unclear as we lack a complete understanding of...
We analyse the signature and origin of transient structures embedded in the slow solar wind, and obs...
Aims. Our goal is to develop methodologies to seamlessly track transient solar wind flows viewed by ...
International audienceThe physical mechanisms that produce the slow solar wind are still highly deba...
Improved space weather diagnostics depend critically on improving our understanding of the evolution...
International audienceA subset at least of the slow solar wind is released in the form of transients...
Two distinct plasma states of slow solar wind are identified from in-situ measurements of the local ...
International audienceIn a recent study, we took advantage of a highly tilted coronal neutral sheet ...
This thesis examines a proposed source of the slow solar wind at the boundaries of active regions. ...
International audienceIn contrast with the fast solar wind, which originates in coronal holes, the s...
International audienceDuring the solar minimum, when the Sun is at its least active, the solar wind(...
The Heliospheric Imager (HI) instruments on board the STEREO spacecraft are used to analyze the sola...
Quasi-periodic density structures are important mesoscale structures that constitute the slow solar ...
International audienceThe release of density structures at the tip of the coronal helmet streamers, ...
In paper 1, we showed that the Heliospheric Imager (HI) instruments on the pair of NASA STEREO space...
Context. The formation of the slow solar wind remains unclear as we lack a complete understanding of...
We analyse the signature and origin of transient structures embedded in the slow solar wind, and obs...
Aims. Our goal is to develop methodologies to seamlessly track transient solar wind flows viewed by ...
International audienceThe physical mechanisms that produce the slow solar wind are still highly deba...
Improved space weather diagnostics depend critically on improving our understanding of the evolution...
International audienceA subset at least of the slow solar wind is released in the form of transients...
Two distinct plasma states of slow solar wind are identified from in-situ measurements of the local ...
International audienceIn a recent study, we took advantage of a highly tilted coronal neutral sheet ...
This thesis examines a proposed source of the slow solar wind at the boundaries of active regions. ...
International audienceIn contrast with the fast solar wind, which originates in coronal holes, the s...
International audienceDuring the solar minimum, when the Sun is at its least active, the solar wind(...
The Heliospheric Imager (HI) instruments on board the STEREO spacecraft are used to analyze the sola...
Quasi-periodic density structures are important mesoscale structures that constitute the slow solar ...
International audienceThe release of density structures at the tip of the coronal helmet streamers, ...
In paper 1, we showed that the Heliospheric Imager (HI) instruments on the pair of NASA STEREO space...