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COCKE: The Crab pulsar has two pulses in ita big one, the primary one, and a shorter, fatter, secondary pulse. They come more or less spaced evenly between each other. The radio pulse looks like that, and so we had felt probably that's what the optical pulse would look like too.
DISNEY: Well, for a few moments we were quite excited because we really thought that Baade's Star would be the place to find this pulsar. And, in fact, there was no sign of a pulsar at all, so we were all a little bit let down. And Don decided that he had to go back to the University in Tucson. So, the next day he showed us how to work all the equipment. By now we were pretty familiar with it and realized it really wasn't as terrifying as it all looked at first. And so on the third night, John and I observed on our own. We weren't exactly on our own at all, in fact, we had Bob McCallister, you know, prevented us from making a lot of mistakes, and was actually working some of the electronic equipment for us. We repeated essentially what we had done the previous night, and we didn't find any pulsar at all.
COCKE: I do remember feeling pretty discouraged about the whole thing. Of course, we weren't very optimistic to begin withor at least, I wasn't. And so, I wasn't feeling as discouraged as I would have if I'd had really high hopes.
DISNEY: We had two more nights to go, and then it turned out they were both cloudy, so there was nothing we could do anyway. And then it just happened. The person who was observing after usBill Tifft, his name washe said that his wife was sick and he couldn't come observingthere were a couple of more days we could have. So we decided well, anyway, we might as well use them.
COCKE: The next two days then were spent more or less walking around the mountain under the clouds, trying to think what to do next. Until then I remembered that it would probably be a good thing to go and re-check the calculations that I did.
DISNEY: And when I came up the mountain in the evening of the next day, John and I cooked dinner and he told me something very interesting. Because the earth is moving around the sun, the actual periodthe apparent periodof these pulses from the pulsar changes as the earth is moving either towards the pulsar or away from it. When the earth is moving towards the pulsar, the pulse is going to appear to come more quickly than they would normally. And when we're moving away, they'd rather come more slowly. It's like a train coming towards you. The note drops, it's what's called the Doppler effect. And so we'd had to make corrections to the known period, the radio period of the pulse. |
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