Terrestrial gamma-ray flashes observed up to 20 MeV

被引:378
作者
Smith, DM
Lopez, LI
Lin, RP
Barrington-Leigh, CP
机构
[1] Univ Calif Santa Cruz, Dept Phys, Santa Cruz, CA 95064 USA
[2] Univ Calif Santa Cruz, Santa Cruz Inst Particle Phys, Santa Cruz, CA 95064 USA
[3] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA
[4] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
[5] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA
[6] Univ British Columbia, Vancouver, BC V6T 1Z4, Canada
关键词
D O I
10.1126/science.1107466
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
Terrestrial gamma-ray flashes (TGFs) from Earth's upper atmosphere have been detected with the Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) satellite. The gamma-ray spectra typically extend up to 10 to 20 megaelectron volts (MeV); a simple bremsstrahlung model suggests that most of the electrons that produce the gamma rays have energies on the order of 20 to 40 MeV. RHESSI detects 10 to 20 TGFs per month, corresponding to similar to50 per day globally, perhaps many more if they are beamed. Both the frequency of occurrence and maximum photon energy are more than an order of magnitude higher than previously known for these events.
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页码:1085 / 1088
页数:4
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