The satellite-borne PAMELA experiment has been continuously collecting data since 2006. This apparatus is designed to study charged particles in the cosmic radiation. The combination of a permanent magnet, a silicon strip tracker and a silicon-tungsten imaging calorimeter, and the redundancy of instrumentation allow very precise studies on the physics of cosmic rays in a wide energy range and with high statistics. This makes PAMELA a very suitable instrument for Solar Energetic Particle (SEP) observations. Not only does it span the energy range between the ground-based neutron monitor data and the observations of SEPs from space, but PAMELA also carries out the first direct measurements of the composition for the highest energy SEP events, ...
The PAMELA (Payload for Antimatter Matter Exploration and Light-nuclei Astro-physics) space-borne ex...
The nature of particle acceleration at the Sun, whether through flare reconnection processes or thro...
The PAMELA magnetic spectrometer was launched into a near-Earth orbit on board the Resurs-DK1 satell...
The satellite-borne PAMELA experiment has been continuously collecting data since 2006. This apparat...
The satellite-borne PAMELA experiment has been continuously collecting data since 2006.This apparatu...
The charged particle acceleration and transport during solar events have been widely studied in the ...
The PAMELA (Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics) satellite-borne...
Despite the significant progress achieved in recent years, the physical mechanisms underlying the or...
Its main task is investigation of the high-energy cosmic rays including electrons, protons, and nucl...
The origin of the high-energy solar energetic particles (SEPs) may conceivably be found in compositi...
The nature of particle acceleration at the Sun, whether through flare reconnection processes or thro...
The PAMELA (Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics) satellite-borne...
The PAMELA space experiment is providing first direct observations of Solar Energetic Particles (SEP...
The PAMELA space experiment is providing first direct observations of Solar Energetic Particles (SEP...
The PAMELA (Payload for Antimatter Matter Exploration and Light-nuclei Astro-physics) space-borne ex...
The nature of particle acceleration at the Sun, whether through flare reconnection processes or thro...
The PAMELA magnetic spectrometer was launched into a near-Earth orbit on board the Resurs-DK1 satell...
The satellite-borne PAMELA experiment has been continuously collecting data since 2006. This apparat...
The satellite-borne PAMELA experiment has been continuously collecting data since 2006.This apparatu...
The charged particle acceleration and transport during solar events have been widely studied in the ...
The PAMELA (Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics) satellite-borne...
Despite the significant progress achieved in recent years, the physical mechanisms underlying the or...
Its main task is investigation of the high-energy cosmic rays including electrons, protons, and nucl...
The origin of the high-energy solar energetic particles (SEPs) may conceivably be found in compositi...
The nature of particle acceleration at the Sun, whether through flare reconnection processes or thro...
The PAMELA (Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics) satellite-borne...
The PAMELA space experiment is providing first direct observations of Solar Energetic Particles (SEP...
The PAMELA space experiment is providing first direct observations of Solar Energetic Particles (SEP...
The PAMELA (Payload for Antimatter Matter Exploration and Light-nuclei Astro-physics) space-borne ex...
The nature of particle acceleration at the Sun, whether through flare reconnection processes or thro...
The PAMELA magnetic spectrometer was launched into a near-Earth orbit on board the Resurs-DK1 satell...