Two Memorable Green Bank experiments
I first met Don in 1971, my first year of grad school at UVa and he was on his NRAO PostDoc.
He was always willing to chat and support a callow grad student.
I remember two experiments he did over the years in Green Bank with especial awe because, as usual for Don,
he used equipment in extremely novel ways.
In the early 1970s he followed *individual* pulsar pulses in frequency by using all 5 GB telescope independently
tuned to different frequencies (the 140 ft, the 300 ft, and the 3 85 ft interferometer elements). This required
writing a complete operating system for the interferometer which had never at that point been used as
individual telescopes tuned to different frequencies.
In the mid 1980s he studied giant pulses from the Crab -- these things are 103 stronger than the mean pulse
intensity but are both infrequent, say, 1/5000, and sporadic. His pulsar back end in GB had finite bandwidth of
course and, in those days, finite storage capacity. So he couldn't just crank away and observe continuously.
His solution was to team with Tim Hankins who observed the Crab at L band at the VLA which had a mode
where they could observe constantly albeit at low resolution. When Tim found a giant pulse, he sent a
trigger signal to Don at the 140 ft *over the Internet* so he could turn on his pulsar backend to sample
at 800 MHz with 85-2. To make this work they had to synch the clocks of
their computers for days, again over the internet, taking out packet speed fluctuations by polling many,
many different clocks around the internet. At least that is what I recall.
As Jim Moran said in Physics Today, we are all much poorer now from the loss of his humanity as well as his technical gifts.