费米太空望远镜在2009年就曾发现这一与正电子有关的特征现象的线索，地点正是在源于雷暴的地表伽马射线中。
The Fermi Space Telescope found hints in 2009 of the telltale pattern associated with positrons in terrestrial gamma rays stemming from lightning storms.
费米太空望远镜对这些伽马射线脉冲很灵敏，以至于它甚至不需要调整位置对准雷暴的正上方，就能来探测TGF信号。
The Fermi Space Telescope is so sensitive to these gamma ray bursts that it doesn't even need to be positioned right over a thunderstorm to detect the TGFs.
发射成功后不久，费米太空望远镜即开始收集伽马射线爆发(GRBs)的迹象，通常这种强烈的爆发是由濒死的恒星造成的。
Soon after launch, Fermi started picking up gamma-ray bursts (GRBs), powerful explosions usually triggered by dying stars.
PS r J 0357最初是通过费米·伽玛射线太空望远镜(Fermi Gamma Ray Space Telescope)于2009年发现的。
PSR J0357 was originally discovered by the Fermi Gamma Ray Space Telescope in 2009.
费米望远镜所具备的侦测超高能伽马射线能力，能够锁定太空中的坐标，非常适于进行这一实验。
With Fermi's ability to detect very-high-energy gamma rays, and pin down their sky coordinates, it is uniquely suited to carry out this experiment.
费米望远镜所具备的侦测超高能伽马射线能力，能够锁定太空中的坐标，非常适于进行这一实验。
With Fermi's ability to detect very-high-energy gamma rays, and pin down their sky coordinates, it is uniquely suited to carry out this experiment.
应用推荐