Add to ORKGWe consider the acceleration of solar, interplanetary, and interstellar particles at the solar-wind termination shock, predict expected composition and energy spectra, and discuss possible observable consequences. The acceleration of a small fraction of solar wind ions incident on the termination shock may explain low-energy enhancements in the spectra of several elements observed by Voyager beyond ~ 60 AU. Other possible particle sources are also discussed
This work extends our previous two-dimensional self-consistent model of the cosmic rays interacting ...
Since the beginning of the space age, it was known that two main sources of energetic particles pe...
Since the beginning of the space age, it was known that two main sources of energetic particles pe...
We consider the acceleration of solar, interplanetary, and interstellar particles at the solar-wind ...
We consider the acceleration of solar, interplanetary, and interstellar particles at the solar-wind ...
We consider the acceleration of solar/interplanetary particles at the solar wind termination shock,...
Interstellar pickup ions and solar wind ions are two main sources of anomalous cosmic ray (ACR) ions...
The spacecraft Voyager 1 is at a distance greater than 85 au from the Sun, in the vicinity of the te...
The spacecraft Voyager 1 is at a distance greater than 85 au from the Sun, in the vicinity of the te...
We use energy spectra of anomalous cosmic rays (ACRs) measured with the Cosmic Ray instrument on the...
We use energy spectra of anomalous cosmic rays (ACRs) measured with the Cosmic Ray instrument on the...
We present energy spectra of e leven cosmic ray elements with energies from ~5 to ~500 MeV/nuc using...
We present energy spectra of e leven cosmic ray elements with energies from ~5 to ~500 MeV/nuc using...
We present energy spectra of e leven cosmic ray elements with energies from ~5 to ~500 MeV/nuc using...
The heliosphere, the volume inflated by the solar wind, is impenetrable to inter-stellar plasma, exc...
This work extends our previous two-dimensional self-consistent model of the cosmic rays interacting ...
Since the beginning of the space age, it was known that two main sources of energetic particles pe...
Since the beginning of the space age, it was known that two main sources of energetic particles pe...
We consider the acceleration of solar, interplanetary, and interstellar particles at the solar-wind ...
We consider the acceleration of solar, interplanetary, and interstellar particles at the solar-wind ...
We consider the acceleration of solar/interplanetary particles at the solar wind termination shock,...
Interstellar pickup ions and solar wind ions are two main sources of anomalous cosmic ray (ACR) ions...
The spacecraft Voyager 1 is at a distance greater than 85 au from the Sun, in the vicinity of the te...
The spacecraft Voyager 1 is at a distance greater than 85 au from the Sun, in the vicinity of the te...
We use energy spectra of anomalous cosmic rays (ACRs) measured with the Cosmic Ray instrument on the...
We use energy spectra of anomalous cosmic rays (ACRs) measured with the Cosmic Ray instrument on the...
We present energy spectra of e leven cosmic ray elements with energies from ~5 to ~500 MeV/nuc using...
We present energy spectra of e leven cosmic ray elements with energies from ~5 to ~500 MeV/nuc using...
We present energy spectra of e leven cosmic ray elements with energies from ~5 to ~500 MeV/nuc using...
The heliosphere, the volume inflated by the solar wind, is impenetrable to inter-stellar plasma, exc...
This work extends our previous two-dimensional self-consistent model of the cosmic rays interacting ...
Since the beginning of the space age, it was known that two main sources of energetic particles pe...
Since the beginning of the space age, it was known that two main sources of energetic particles pe...