Solar energetic particle fluxes (Ee > 38 keV) observed by the ULYSSES/HI-SCALE experiment are utilized as diagnostic tracers of the large-scale structure and topology of the Interplanetary Magnetic Field (IMF) embedded within two well-identified Interplanetary Coronal Mass Ejections (ICMEs) detected at 56° and 62° south heliolatitudes by ULYSSES during the solar maximum southern high-latitude pass. On the basis of the energetic solar particle observations it is concluded that: (A) the high-latitude ICME magnetic structure observed in May 2000 causes a depression in the solar energetic electron intensities which can be accounted for by either a detached or an attached magnetic field topology for the ICME; (B) during th...
This work presents in situ solar wind observations of three magnetic clouds (MCs) that contain cold ...
Context. Relating in-situ measurements of relativistic solar particles to their parent act...
Coronal Mass Ejections (CMEs) are extremely dynamical events in which the solar plasma is ejected in...
International audienceSolar energetic particle fluxes (Ee > 38 keV) observed by the ULYSSES/HI-SCALE...
International audienceIn this work, solar flare energetic particle fluxes (Ee ? 42 keV) observed by ...
[1] In late October and early November 2003 the ACE spacecraft at 1 AU detected two shock-associated...
On 15 May 2005, a huge interplanetary coronal mass ejection (ICME) was observed near Earth. It trigg...
In late October and early November 2003, the ACE spacecraft at 1 AU detected two Interplanetary Coro...
International audienceOn 15 May 2005, a huge interplanetary coronal mass ejection (ICME) was observe...
We examine the near-Earth Interplanetary Coronal Mass Ejection (ICME) apparently related to the inte...
[1] At the time of the solar flare on the Bastille Day of 2000, the Ulysses spacecraft was at 3.17 A...
We study the influence of the large-scale interplanetary magnetic field configuration on the solar e...
At the time of the solar flare on July 14 (Bastille Day) of 2000, the Ulysses spacecraft was at 3.17...
International audienceWe study interplanetary coronal mass ejections (ICMEs) measured by probes at d...
On 2015 January 6&-7, an interplanetary coronal mass ejection (ICME) was observed at L1. This event,...
This work presents in situ solar wind observations of three magnetic clouds (MCs) that contain cold ...
Context. Relating in-situ measurements of relativistic solar particles to their parent act...
Coronal Mass Ejections (CMEs) are extremely dynamical events in which the solar plasma is ejected in...
International audienceSolar energetic particle fluxes (Ee > 38 keV) observed by the ULYSSES/HI-SCALE...
International audienceIn this work, solar flare energetic particle fluxes (Ee ? 42 keV) observed by ...
[1] In late October and early November 2003 the ACE spacecraft at 1 AU detected two shock-associated...
On 15 May 2005, a huge interplanetary coronal mass ejection (ICME) was observed near Earth. It trigg...
In late October and early November 2003, the ACE spacecraft at 1 AU detected two Interplanetary Coro...
International audienceOn 15 May 2005, a huge interplanetary coronal mass ejection (ICME) was observe...
We examine the near-Earth Interplanetary Coronal Mass Ejection (ICME) apparently related to the inte...
[1] At the time of the solar flare on the Bastille Day of 2000, the Ulysses spacecraft was at 3.17 A...
We study the influence of the large-scale interplanetary magnetic field configuration on the solar e...
At the time of the solar flare on July 14 (Bastille Day) of 2000, the Ulysses spacecraft was at 3.17...
International audienceWe study interplanetary coronal mass ejections (ICMEs) measured by probes at d...
On 2015 January 6&-7, an interplanetary coronal mass ejection (ICME) was observed at L1. This event,...
This work presents in situ solar wind observations of three magnetic clouds (MCs) that contain cold ...
Context. Relating in-situ measurements of relativistic solar particles to their parent act...
Coronal Mass Ejections (CMEs) are extremely dynamical events in which the solar plasma is ejected in...