Advanced in Geosciences, V2: Solar Terrestrial(St) by Wing-huen Ip PDF

By Wing-huen Ip

"Advances in Geosciences" is the results of a concerted attempt in bringing the most recent effects and making plans actions concerning earth and area technology in Asia and the overseas area. the quantity editors are all best scientists of their learn fields protecting 5 sections: sturdy Earth (SE), sun Terrestrial (ST), Planetary technology (PS), Hydrological technological know-how (HS), and Oceans and Atmospheres (OA). the most objective is to spotlight the clinical matters necessary to the research of earthquakes, tsunamis, weather switch, drought, flood, typhoons, area weathers, and planetary exploration.

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We synthesized the images in microwaves and in HXRs around the time of this peak, and examined the spectroscopic features of the coronal emission sources. Figure 3 shows the results. In the right panel we present a NoRH 34 GHz image. We overlaid the counter image with the gray line to show the coronal emission source. 1. 8, if we assume the gyro-synchrotron emission for the microwave emission source. We also overlaid the HXR contour images on the TRACE (left) and NoRH (right) images with black lines.

Stuiver, P. J. Reimer and T. F. Braziunas, Radiocarbon 40, 3 (1998) 1127. J. , Nature 331 (1988) 675. J. , Nature 347 (1990) 164. J. Beer, S. Tobias and N. Weiss, Solar Phys. 181 (1998) 237. A. N. Peristykh and P. E. Damon, Solar Phys. 177 (1998) 343. H. Miyahara, H. Masuda, Y. Muraki, H. Furuzawa, H. Menjo and T. Nakamura, Sol. Phys. 224 (2004) 317. H. Miyahara, K. Masuda, H. Furuzawa, H. Menjo, Y. Muraki, H. Kitagawa and T. Nakamura, Radiocarbon 46 (2004) 965. H. Miyahara, K. Masuda, H. Menjo, K.

9. 10. 11. 12. 13. 14. 15. 16. 17. 18. 19. 20. 21. 22. 23. F. W. G. Sp¨ orer, Vierteljahrsschr. Astron. Ges. (Leipzig) 22 (1887) 323. F. W. G. Sp¨ orer, Bull. Astron. 6 (1889) 60. E. W. Maunder, Mon. Not. R. Astron. Soc. 50 (1894) 251. W. -H. Soon and S. H. Yaskell, Maunder Minimum and the Variable SunEarth Connections (World Scientific Printers, Singapore, 2003), p. 278. J. A. Eddy, Science 192 (1976) 1189. J. A. Eddy, Sci. Am. 236 (1977) 80. J. A. Eddy, Solar Phys. 89 (1983) 195. E. -C. Ribes and R.

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