Interstellar pickup ions accelerated by the termination shock of the solar wind dominate the anomalous cosmic-ray (ACR) intensities observed by the Voyager spacecraft in the outer heliosphere. Using a two-dimensional acceleration and propagation model, we derive the relative abundances of these interstellar ACRs and determine the mass dependence of the injection/acceleration efficiency for the diffusive accelera
We present energy spectra of eleven cosmic ray elements with energies from rv5 to rv500 MeV/nuc usin...
The spacecraft Voyager 1 is at a distance greater than 85 au from the Sun, in the vicinity of the te...
We present energy spectra of eleven cosmic ray elements with energies from rv5 to rv500 MeV/nuc usin...
Interstellar pickup ions accelerated by the termination shock of the solar wind dominate the anomalo...
The “classic” anomalous cosmic ray (ACR) component originates as interstellar neutral atoms that dri...
The “classic” anomalous cosmic ray (ACR) component originates as interstellar neutral atoms that dri...
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...
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...
Since the beginning of the space age, it was known that two main sources of energetic particles pe...
Anomalous cosmic ray (ACR) acceleration at the heliospheric termination shock is described by a self...
We present energy spectra of eleven cosmic ray elements with energies from rv5 to rv500 MeV/nuc usin...
The spacecraft Voyager 1 is at a distance greater than 85 au from the Sun, in the vicinity of the te...
We present energy spectra of eleven cosmic ray elements with energies from rv5 to rv500 MeV/nuc usin...
Interstellar pickup ions accelerated by the termination shock of the solar wind dominate the anomalo...
The “classic” anomalous cosmic ray (ACR) component originates as interstellar neutral atoms that dri...
The “classic” anomalous cosmic ray (ACR) component originates as interstellar neutral atoms that dri...
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...
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...
Since the beginning of the space age, it was known that two main sources of energetic particles pe...
Anomalous cosmic ray (ACR) acceleration at the heliospheric termination shock is described by a self...
We present energy spectra of eleven cosmic ray elements with energies from rv5 to rv500 MeV/nuc usin...
The spacecraft Voyager 1 is at a distance greater than 85 au from the Sun, in the vicinity of the te...
We present energy spectra of eleven cosmic ray elements with energies from rv5 to rv500 MeV/nuc usin...