"We can detect sunspots at a depth of 60,000 kilometers, but if we try to detect them deeper or closer to the surface, the travel-time shift becomes weaker," Ilonidis says.
“我们能探测六万公里深处的黑子,但如果探测更深些或者更靠近太阳表面的位置时,(声波的)传播时间的变化将变得不明显,”Ilonidis说。
"We can detect sunspots at a depth of 60, 000 kilometers, but if we try to detect them deeper or closer to the surface, the travel-time shift becomes weaker," Ilonidis says.
“我们能探测六万公里深处的黑子,但如果探测更深些或者更靠近太阳表面的位置时,(声波的)传播时间的变化将变得不明显,”Ilonidis说。
"We can detect sunspots at a depth of 60, 000 kilometers, but if we try to detect them deeper or closer to the surface, the travel-time shift becomes weaker," Ilonidis says.
“我们能探测六万公里深处的黑子,但如果探测更深些或者更靠近太阳表面的位置时,(声波的)传播时间的变化将变得不明显,”Ilonidis说。
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