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The interference that Red Coast had to deal with was similar, but the source of interference (the sun) was between the source of the transmission (outer space) and the ground-based receiver. Compared to communication satellites, the solar outages suffered by Red Coast were more frequent and more severe. Red Coast Base as constructed was also much more modest than its original design, such that the transmission and monitoring systems shared the same antenna. This made the times available for monitoring even more precious, and solar outages even more of a problem.

Lei and Yang’s idea for eliminating interference was very simple: ascertain the frequency spectrum and characteristics of solar radiation in the monitored range, and then filter it out digitally. Both of them were technical, and at that time, when the ignorant often led the knowledgeable, that was a rare bit of fortune. But Yang wasn’t a specialist in astrophysics, and Lei had taken the path of becoming a political officer, which prevented him from accruing in-depth technical know-how. In reality, electromagnetic radiation from the sun is only stable within the limited range from near-ultraviolet to mid-infrared (including visible light). In other ranges, the radiation is quite volatile and unpredictable.

To set the right expectations, Ye made it clear in her first research report that during periods of intense solar activity—sunspots, solar flares, coronal mass ejections, and so on—it was impossible to eliminate solar interference. Thus, her research target was limited to radiation within the frequency ranges monitored by Red Coast during periods of normal solar activity.

Research conditions at the base weren’t too bad. The library could obtain foreign-language materials related to the topic, including timely European and American academic journals. In those years, this was no easy feat. Ye also could use the military phone line to connect to the two groups conducting solar science research within the Chinese Academy of Sciences and obtain their observation data by fax.

After half a year of study, Ye saw no glimpse of hope. She quickly discovered that within the frequency ranges monitored by Red Coast, solar radiation fluctuated unpredictably. By analyzing large amounts of observed data, Ye discovered a puzzling mystery. Sometimes, during one of the sudden fluctuations in solar radiation, the surface of the sun was calm. Since hundreds of thousands of kilometers of solar material would absorb any shortwave and microwave radiation originating from the core of the sun, the radiation must have come from activities on its surface, so there should have been observable surface activity when these fluctuations occurred. If there were no corresponding surface disturbances, what caused these sudden changes to the narrow frequency ranges? The more she thought about it, the more mysterious it seemed.

Eventually Ye ran out of ideas and decided to give up. In her last report, she conceded that she could not solve the problem. This shouldn’t have been a big deal. The military had asked several groups within universities and the Chinese Academy of Sciences to research the same issue, and all of those efforts had failed. But Yang wanted to try one more time, relying on Ye’s extraordinary talent.

Lei’s agenda was even simpler: He just wanted Ye’s paper. The research topic was highly theoretical and would show off his expertise and skill. Now that the chaos in society was finally subsiding, the demands on cadres were also changing. There was an acute need for men like him, politically mature and academically accomplished. Of course he would have a bright future. As to whether the problem of interference from solar outages could be solved, he didn’t really care.

But in the end, Ye didn’t hand in her report. She thought that if the research project were terminated, the base library would stop receiving foreign language journals and other research materials, and she would no longer have access to such a rich trove of astrophysics references. So she nominally continued her research, while in reality she focused on refining her mathematical model of the sun.

One night, Ye was, as usual, the only person in the cold reading room of the base library. On the long table in front of her, a pile of documents and journals were spread open. After completing a set of tedious and cumbersome matrix calculations, she blew on her hands to warm them, and picked up the latest issue of the Journal of Astrophysics to take a break. As she flipped through it, a brief note about Jupiter caught her attention: