Cosmic rays that are produced by nuclear interactions during propagation and decay only by electron capture can be used to determine the level of cosmic ray reacceleration that has occurred. The high resolution, large statistical sample of cosmic rays collected by the Cosmic Ray Isotope Spectrometer (CRIS) aboard the Advanced Composition Explorer (ACE) spacecraft provides a data set that allows precision measurements of these isotopic abundances. We discuss electron capture decay, the signatures of reacceleration, and the sensitivity with which reacceleration models can be tested
The Cosmic Ray Isotope Spectrometer on the ACE spacecraft measures the isotopic composition of cosmi...
Precise measurements of predominantly secondary cosmic-ray Li, Be, and B together with current well-...
The Cosmic Ray Isotope Spectrometer (CRIS) instrument on board the Advanced Composition Explorer (AC...
Cosmic rays that are produced by nuclear interactions during propagation and decay only by electronc...
The secondary isotopes ^(37)Ar, ^(44)Ti, ^(49)V, ^(51)Cr, ^(55)Fe, and ^(57)Co decay only by electro...
Radioactive cosmic ray nuclei produced by nuclear interactions during cosmic ray propagation through...
We report the first observation of an energy dependence in the titanium, vanadium, and chromium isot...
The elemental abundances of galactic cosmic rays (GCR) observed near Earth provide information about...
Galactic cosmic rays (GCR) interact to produce secondary fragments as they pass through the interste...
The Cosmic Ray Isotope Spectrometer (CRIS) instrument on the Advanced Composition Explorer (ACE) mis...
The Advanced Composition Explorer (ACE), which carries instrumentation for making high-precision mea...
International audienceElectron capture (EC) decay relies on attachment and stripping cross-sections,...
We present measurements of the nickel and cobalt isotopes from the Cosmic Ray Isotope Spectrometer ...
Measurements by the Cosmic Ray Isotope Spectrometer (CRIS) on the Advanced Composition Explorer (ACE...
We report direct evidence of the energy loss of galactic cosmic rays as they diffuse in magnetic irr...
The Cosmic Ray Isotope Spectrometer on the ACE spacecraft measures the isotopic composition of cosmi...
Precise measurements of predominantly secondary cosmic-ray Li, Be, and B together with current well-...
The Cosmic Ray Isotope Spectrometer (CRIS) instrument on board the Advanced Composition Explorer (AC...
Cosmic rays that are produced by nuclear interactions during propagation and decay only by electronc...
The secondary isotopes ^(37)Ar, ^(44)Ti, ^(49)V, ^(51)Cr, ^(55)Fe, and ^(57)Co decay only by electro...
Radioactive cosmic ray nuclei produced by nuclear interactions during cosmic ray propagation through...
We report the first observation of an energy dependence in the titanium, vanadium, and chromium isot...
The elemental abundances of galactic cosmic rays (GCR) observed near Earth provide information about...
Galactic cosmic rays (GCR) interact to produce secondary fragments as they pass through the interste...
The Cosmic Ray Isotope Spectrometer (CRIS) instrument on the Advanced Composition Explorer (ACE) mis...
The Advanced Composition Explorer (ACE), which carries instrumentation for making high-precision mea...
International audienceElectron capture (EC) decay relies on attachment and stripping cross-sections,...
We present measurements of the nickel and cobalt isotopes from the Cosmic Ray Isotope Spectrometer ...
Measurements by the Cosmic Ray Isotope Spectrometer (CRIS) on the Advanced Composition Explorer (ACE...
We report direct evidence of the energy loss of galactic cosmic rays as they diffuse in magnetic irr...
The Cosmic Ray Isotope Spectrometer on the ACE spacecraft measures the isotopic composition of cosmi...
Precise measurements of predominantly secondary cosmic-ray Li, Be, and B together with current well-...
The Cosmic Ray Isotope Spectrometer (CRIS) instrument on board the Advanced Composition Explorer (AC...