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Galactic Astronomy

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Cosmogenic Radionuclides

Part of the book series: Physics of Earth and Space Environments ((EARTH))

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Abstract

As discussed in Sect. 5.4, and in Chap. 17, the cosmogenic data provide us with information about the past. In particular, we have studied the variability of the Sun, and in Chap. 21 will study the secular changes in the geomagnetic field.

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References

  • Aschenbach B, Iyudin AF, Schonfelder V (1999) Constraints of age, distance and progenitor of the supernova remnant RX J0852.0-4622/GRO J0852-4642. Astron Astrophys 350(3):997–1006

    ADS  Google Scholar 

  • Berezinskii VS, Ptuskin VS (1989) Diffusive shock acceleration of cosmic ray and gamma radiation from young supernova shells. Astrophys J 340:351–354

    Article  ADS  Google Scholar 

  • Berezinsky VS, Bulanov SV, Dogiel VA, Ginzburg VL, Ptuskin VS (1990) Astrophysics of cosmic rays. North Holland, Amsterdam

    Google Scholar 

  • Busching I, Potgieter MS (2008) The variability of the proton cosmic ray flux on the Sun’s way around the galactic center. Adv Space Res 42(3):504–509

    Article  ADS  Google Scholar 

  • Florinski V, Zank GP, Axford WI (2003) The Solar System in a dense interstellar cloud: implications for cosmic-ray fluxes at Earth and Be-10 records. Geophys Res Lett 30:GL2206

    Google Scholar 

  • Frisch PC, Mueller H-R (2011) Time variability in the interstellar boundary conditions of the Heliosphere over the past 60,000 years: impact of the solar journey on the galactic cosmic ray flux at Earth. Space Sci Rev (in press)

    Google Scholar 

  • Mueller HR, Frisch PC, Florinski V, Zank GP (2006) Heliospheric response to different possible interstellar environments. Astrophys J 647(2):1491

    Article  ADS  Google Scholar 

  • Rood RT, Sarazin CL, Zeller EJ, Parker BC (1979) X-rays or gamma-rays from super-novae in glacial ice. Nature 282(5740):701–703

    Article  ADS  Google Scholar 

  • Shaviv NJ (2003) The spiral structure of the Milky Way, cosmic rays, and ice age epochs on Earth. New Astron 8(1):39–77

    Article  ADS  Google Scholar 

  • Sonett CP, Morfill GE, Jokipii JR (1987) Interstellar shock-waves and Be-10 from ice cores. Nature 330(6147):458–460

    Article  ADS  Google Scholar 

  • Zank GP, Frisch PC (1999) The interaction of the solar wind with a high density cloud. AIP Conf Proc 471:831–834

    Article  ADS  Google Scholar 

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Correspondence to Jürg Beer .

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© 2012 Springer-Verlag Berlin Heidelberg

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Beer, J., McCracken, K., von Steiger, R. (2012). Galactic Astronomy. In: Cosmogenic Radionuclides. Physics of Earth and Space Environments. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-14651-0_18

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