Beryllium (Be) is a lithophile trace element with an abundance in Earth's crust at ppm levels (Ryan, 2002).
9Be is the only stable isotope of beryllium with nearly 100% relative abundance, while cosmogenic radionuclides 10 Be (t 1/2 = 1.39 million years (Chmeleff et al., 2010)) and 7 Be (t 1/2 = 53.2 days) are its two cosmogenic radionuclides. Meteoric 10 Be is produced by spallation of nitrogen and oxygen atoms in the stratosphere and upper troposphere, thereafter mixed in the atmosphere and scavenged to the Earth's surface by wet and dry precipitation (Lal & Peters, 1967). 10 Be can also be produced at the Earth's surface, but production rate of this in-situ 10 Be is negligible compared to the meteoric 10 Be (Willenbring & von Blanckenburg, 2010). The production rate of meteoric 10 Be is mainly modulated by geomagnetic field and solar activity. The modern global average production rate of 10 Be in the atmosphere is about 0.0209 atoms/cm 2 /s (Masarik & Beer, 2009). The residence time of 10 Be in the stratosphere is on the order of 1 year (Raisbeck et al., 1981), long enough to ensure stratospheric mixing. Thus, the global distribution of the atmospheric deposition flux for 10 Be on the Earth is almost independent from that of the atmosphere production rate, but is more