Abstract. The traditionally accepted source of Anomalous Cos-mic Rays (ACRs) is neutral atoms penetrating the heliosphere from the local interstellar cloud (LIC). The ACR composition should be depleted in easily ionized atoms such as C, Si, and Fe. However, sig-nificant fluxes of these ions are observed in ACRs and their source has not been previously identified. We show that there is an “outer source ” of pickup ions, and hence ACRs, caused by sputtered atoms (subsequently ionized and picked up by the solar wind) from small grains generated via collisions of objects in the Edgeworth-Kuiper Belt. The outer source accounts for the abundance and compo-sition of the additional population of ACRs. The discovery that ACRs are generated from mate...
We present a new determination of the relative abundances of the interstellar neutral atoms CI, NI,...
Interstellar pickup ions accelerated by the termination shock of the solar wind dominate the anomalo...
We present a new determination of the relative abundances of the interstellar neutral atoms CI, NI,...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95527/1/grl16222.pd
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...
Interstellar pickup ions accelerated by the termination shock of the solar wind dominate the anomalo...
We review the observed properties of anomalous cosmic rays and the present status of our knowledge o...
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...
Interstellar pickup ions and solar wind ions are two main sources of anomalous cosmic ray (ACR) ions...
A variety of heliospheric ion populations—from Anomalous Cosmic Rays (ACRs) to particles accelerated...
We present a new determination of the abundances (normalized to He I and Ne I) of neutral atoms HI, ...
We present a new determination of the abundances (normalized to He I and Ne I) of neutral atoms HI, ...
We present a new determination of the relative abundances of the interstellar neutral atoms CI, NI,...
Interstellar pickup ions accelerated by the termination shock of the solar wind dominate the anomalo...
We present a new determination of the relative abundances of the interstellar neutral atoms CI, NI,...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95527/1/grl16222.pd
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...
Interstellar pickup ions accelerated by the termination shock of the solar wind dominate the anomalo...
We review the observed properties of anomalous cosmic rays and the present status of our knowledge o...
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...
Interstellar pickup ions and solar wind ions are two main sources of anomalous cosmic ray (ACR) ions...
A variety of heliospheric ion populations—from Anomalous Cosmic Rays (ACRs) to particles accelerated...
We present a new determination of the abundances (normalized to He I and Ne I) of neutral atoms HI, ...
We present a new determination of the abundances (normalized to He I and Ne I) of neutral atoms HI, ...
We present a new determination of the relative abundances of the interstellar neutral atoms CI, NI,...
Interstellar pickup ions accelerated by the termination shock of the solar wind dominate the anomalo...
We present a new determination of the relative abundances of the interstellar neutral atoms CI, NI,...