International audienceA flare east of central meridian on 2003 October 28 produced a relativistic particle event at Earth, although it was located far from the footpoint of the nominal interplanetary Parker spiral. From a study of the onset times of the event at different neutron monitors we conclude that the earliest arriving solar particles may be neutrons. The first relativistic protons (prompt component) arrived a few minutes later. Metre wave imaging suggests that electrons are not only accelerated in the flaring active regions, but at several places far away, including the western hemisphere. Simultaneous Type III emission and associated Langmuir waves demonstrates that these regions are connected to the Earth. We suggest that, like i...
Protons accelerated to relativistic energies by transient solar and interplanetary phenomena caused ...
Abstract We analyze the high-energy particle emission from the Sun in two extreme solar particle eve...
An X17.2 solar flare occurred on 2003 October 28, accompanied by multi-wavelength emissions and a hi...
International audienceA flare east of central meridian on 2003 October 28 produced a relativistic pa...
International audienceA flare on 2003 October 28 produced a relativistic particle event at Earth, al...
International audienceAims. We analyse particle, radio, and X-ray observations during the first rela...
International audienceThe origin of relativistic solar protons during large flare/CME events has not...
Context. The highest energies of solar energetic nucleons detected in space or through gamma-ray emi...
The large solar flare of 14 July 2000 10 UT occurred in an active region near the central meridian. ...
Context. Relating in-situ measurements of relativistic solar particles to their parent activity in t...
Abstract We performed an analysis of high-energy particle emission from the Sun in two extreme sola...
Context. Relating in-situ measurements of relativistic solar particles to their parent act...
Timing discrepancies between signatures of accelerated particles at the sun and the arrival times of...
Understanding the energy budget in large solar flares requires a good knowledge of how and where th...
Mildly relativistic electrons appear during the solar energetic particle events. A detailed investig...
Protons accelerated to relativistic energies by transient solar and interplanetary phenomena caused ...
Abstract We analyze the high-energy particle emission from the Sun in two extreme solar particle eve...
An X17.2 solar flare occurred on 2003 October 28, accompanied by multi-wavelength emissions and a hi...
International audienceA flare east of central meridian on 2003 October 28 produced a relativistic pa...
International audienceA flare on 2003 October 28 produced a relativistic particle event at Earth, al...
International audienceAims. We analyse particle, radio, and X-ray observations during the first rela...
International audienceThe origin of relativistic solar protons during large flare/CME events has not...
Context. The highest energies of solar energetic nucleons detected in space or through gamma-ray emi...
The large solar flare of 14 July 2000 10 UT occurred in an active region near the central meridian. ...
Context. Relating in-situ measurements of relativistic solar particles to their parent activity in t...
Abstract We performed an analysis of high-energy particle emission from the Sun in two extreme sola...
Context. Relating in-situ measurements of relativistic solar particles to their parent act...
Timing discrepancies between signatures of accelerated particles at the sun and the arrival times of...
Understanding the energy budget in large solar flares requires a good knowledge of how and where th...
Mildly relativistic electrons appear during the solar energetic particle events. A detailed investig...
Protons accelerated to relativistic energies by transient solar and interplanetary phenomena caused ...
Abstract We analyze the high-energy particle emission from the Sun in two extreme solar particle eve...
An X17.2 solar flare occurred on 2003 October 28, accompanied by multi-wavelength emissions and a hi...