The secular imprint of the interplanetary magnetic field drift on 10Be data

Geophysical Research Letters

Volumn 31, Issue 12, 2004, Pages

  Valdes Galicia J F ^a   Mendoza, B ^a  

^a UNIVERSIDAD NACIONAL AUTÓNOMA DE MÉXICO   (Mexico)

Author keywords

[No Author keywords available]

Indexed keywords

CORRELATION METHODS; GEOMAGNETISM; GEOPHYSICS; SOLAR SYSTEM; COSMOLOGY; MAGNETIC FIELDS; MAGNETIC POLARITY; MAGNETISM; SOLAR ENERGY; UPPER ATMOSPHERE;

INTERPLANETARY MAGNETIC FIELDS; SOLAR CYCLES; SOLAR MAGNETIC FIELDS;

MAGNETIC FIELD EFFECTS;

GEOMAGNETIC FIELD; SOLAR ACTIVITY;

CORRELATION COEFFICIENT; DRIFT EFFECTS; GOOD CORRELATIONS; INTERPLANETARY MAGNETIC FIELDS; LOW CORRELATION; NEGATIVE POLARITY; SOLAR CYCLE; SOLAR MAGNETIC FIELDS;

EID: 6044269306     PISSN: 00948276     EISSN: None     Source Type: Journal    
DOI: 10.1029/2003GL018123     Document Type: Article

References (19)

1. Beer, J. (2000), Long-term indirect indices of solar variability, Space Sci. Rev., 94, 53-66.
2. Beer, J., St. Baumgartner, B. Dittrich-Hannen, J. Hauenstein, P. Kubik, Ch. Lukasczyk, W. Mende, R. Stellmacher, and M. Suter (1994), Solar variability traced by cosmogmic isotopes, in The Sun as a Variable Star: Solar and Stellar Variations, Cambridge Univ. Press, edited by J. M. Pap, C. Fröhlich, H. S. Hudson, and S. K. Solanki, 291-300.
3. Chrernosky, E. J. (1996), Double sunspot-cycle variation in terrestrial magnetic activity, 1884-1963,. J. Geophys. Res., 71(3), 965-974.
4. Gibbons, J. D. (1976), Non parameric methods for quantitative analysis, Holt, Reinhart and Winston, 242 pp., New York.
5. Hays, W. L. (1981), Statistics, 3rd edition, Holt, Reinhart and Winston, 425 pp., New York.
6. Kota, J., and J. R. Jokipii (1983), Effects of drift on the transport of cosmic rays, VI. A three dimensional model including diffusion, Astrophys. J., 249, 573.
7. Lockwood, M. (2001), Long term variations in the magnetic field of the sun and the heliosphere: Their origin, effects and implications, J. Geophys. Res., 106, 16,021-16,038.
8. Lockwood, M. (2003), Twenty three cycles of changing open solar magnetic flux, J. Geophys. Res., 108(A3), 1128, doi:10.1029/2002JA009431.
9. Lockwood, M., R. Stamper, and M. N. Wild (1999), A doubling of the Sun's coronal magnetic field during the past 100 years, Nature, 399, 437-439.
10. Mayaud, P. N. (1972), The aa indices: A 100-year series characterizing the magnetic activity, J. Geophys. Res., 77, 6870-6874.
11. 10Be due to the 11 year modulation of the cosmic radiation, and variations in the vector geomagnetic dipole, Proceedings of 27th ICRC, 4129-4132.
12. McCracken, K. G., J. Beer, and F. B. McDonald (2003), A typical cosmic ray propagation during the qA > 0 sunspot minimum of 1954, Proceedings of 28th ICRC, 7, 4031-4034.
13. Mursula, K., I. G. Usoskin, and G. A. Kovaltsov (2001), Long term cosmic ray intensity vs. solar proxies: A simple linear relation does not work, Proceedings of 28th ICRC, 8, 3838-3841.
14. Potgieter, M., R. A. Burger, and S. E. Ferreira (2001), Modulation of cosmic rays from solar minimum to solar maximum: A theoretical pespective, Space Sci Rev., 97, 295-307.
15. Shea, M. A., and D. Smart (1981), Preliminary search for cosmic radiation and solar terrestrial parameters correlated with the reversal of the solar magnetic field, Adv. Space Res., 1, 165-168.
16. Shea, M. A., and D. Smart (1985), An update of the correlation between the cosmic radiation intensity and the geomagnetic aa index, Proceedings of 19th ICRC, 4, 501-504.
17. Solanki, S. K., M. Schlusser, and M. Fligge (2002), Secular variations of the sun's magnetic field, Astronom. Astrophys., 383, 706-712.
18. Usoskin, I., K. Mursula, S. M. Solanki, M. Schlusser, and G. A. Kovaltsov (2002), A physical reconstruction of cosmic ray intensity since 1610, J. Geophys. Res., 107(A11), 1374, doi:10.1029/2002JA009343.
19. Wang, Y.-M., J. Lean, and N. R. Sheeley (2000), The long-term variation of the Sun's open magnetic flux, Geophys. Res. Lett., 27, 505-508.