Serendip

SERENDIP takes advantage of ongoing "mainstream" radio telescope observations as a "piggy-back" or "commensal" program.

SERENDIP利用运转中的主流射电望远镜作为“被扶持”或“共生”的一个计划。

Instead, SERENDIP scans the signal from the radio telescope in real time, right when it comes down from the receiver.

相反的，SERENDIP实时的从射电望远镜扫描信号，当信号失衡的时候从接收器中纠正。

The tapes with the recorded signals are then packed up and sent to the SERENDIP team in Berkeley, with an additional copy going to colleagues at Cornell University in Ithaca, New York.

磁带会记录这些信号并递交给伯克利分校的SERENDIP团队，同时一个副本会发送给纽约伊萨卡的康奈尔大学团队。

The increased bandwidth will enable SERENDIP V to listen to the entire spectrum of the Arecibo receiver that will be collecting its data.

提高了带宽将是SERENDIP V有足够能力聆听阿雷西博接收器说接收的数据的整个频谱。

Rather than having its own observation program, SERENDIP analyzes deep space radio telescope data that it obtains while other astronomers are using the telescope.

尽管SERENDIP并不拥有自属的观察安排，但它可以在其他天文学家在利用望远镜的同时分析来自深层太空的无线电数据。

Like every previous generation of the project, SERENDIP V represents a giant step forward over its predecessors.

如同项目的所有上一代，SERENDIP V代表着比前任有着一个巨大的进步。