Measurement of the Secondary Radionuclides 10Be, 26Al, 36Cl, 54Mn, and 14C and Implications for the Galactic Cosmic-Ray Age

By N. Yanasak, M. Wiedenbeck, R. Mewaldt, A. Davis, A. Cummings, J. George, R. Leske, E. Stone, E. Christian, T. T. Rosenvinge and 3 more. 2001

156 citations recorded by the source corpus.

Subfields: Global and Planetary Change, Nuclear and High Energy Physics, Radiological and Ultrasound Technology

View Paper: https://www.semanticscholar.org/paper/ec74c1ce59d7506e339d82b1e49a1a397d79e7ea

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In Global and Planetary Change

1. M. Fukugita

In Nuclear and High Energy Physics

1. A. Strong
2. E. Orlando
3. Troy A. Porter
4. Igor V. Moskalenko
5. G. Jóhannesson
6. A. Bykov
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8. S. Digel

Citations in the corpus

• A Markov Chain Monte Carlo technique to sample transport and source parameters of Galactic cosmic rays - II. Results for the diffusion model combining B/C and radioactive nuclei (2010, methodology): “– G1: as F, but with new ACE 1997-1998 data, 31 data points; – G2: as F, but with new ACE 2001-2003 data only, 31 data points; – G1/2: using both 1997-1998 and 2001-2003 ACE data, 37 data points; –”
• GLOBAL COSMIC-RAY-RELATED LUMINOSITY AND ENERGY BUDGET OF THE MILKY WAY (2010, background): “These halo sizes cover the range consistent with available CR data for B/C and10Be/9Be (Engelmann et al. 1990; Yanasak et al. 2001; de Nolfo et al. 2006, and references therein).”
• Proton, helium, and electron spectra during the large solar particle events of October-November 2003 (2005, background): “It is interesting that galactic cosmic rays apparently extract a similar fraction of the kinetic energy from supernova shocks in order to sustain the energy density of cosmic rays in the galaxy ( 1 eV/cm3) over the average cosmic ray lifetime of 15 million years [Yanasak et al., 2001].”
• A database of charged cosmic rays (2013, unknown): “– Balloon (1982/10): Garcia-Munoz et al. (1986) – Balloon (1984/09): Garcia-Munoz et al. (1986) – Balloon (1987/08): Evenson et al. (1995) – Balloon (1990/08): Evenson et al. (1995) – Balloon (1992/08): Evenson et al. (1995) – Balloon (1994/08): Evenson et al. (1995) – Balloon (1969/04+1970/11): Sil”
• Interstellar Turbulence II: Implications and Effects (2004, background): “Their flight time determined from isotope ratios ranges from ∼15 My for a leaky-box model with a small halo (Simpson & Garcia-Munoz 1988, Yanasak et al. 2001) to 108 years for a diffusion model in a ∼5 kpc halo (Ptuskin & Soutoul 1998).”
• Observational Signatures of Particle Acceleration in Supernova Remnants (2012, background): “Its age is just 1-2 Myr and its central density reaches 105 M pc −3 (Portegies Zwart et al., 2010).”
• ENERGY SPECTRA OF COSMIC-RAY NUCLEI AT HIGH ENERGIES (2009, background): “Likewise, their confinement time in the Galaxy can be determined through measurements of long-lived radioactive secondary nuclei (Longair 1994; Yanasak et al. 2001).”
• The Cosmic Energy Inventory (2004, methodology): “We take the cosmic ray mean life in the galaxy to be 2× 107 yr (Garcia-Munoz, Mason & Simpson 1977; Yanasak et al. 2001).”
• CONSTRAINTS ON COSMIC-RAY PROPAGATION MODELS FROM A GLOBAL BAYESIAN ANALYSIS (2010, unknown): “Therefore, we use the ACE measurements corresponding to the solar minimum conditions (George et al. 2009).”