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NATIONAL RADIO ASTRONOMY OBSERVATORY ARCHIVES
Papers of Woodruff T. Sullivan III: Tapes SeriesInterview with A. Melvin Skellett By telephone from the University of Washington to his home in Sarasota, Florida August 26, 1977 Interview Time: 28 minutes Transcribed for Sullivan by Pamela M. Jernegan Note: The interview listed below was either transcribed as part of Sullivan's research for his book, Cosmic Noise: A History or Early Radio Astronomy (Cambridge University Press, 2009) or was transcribed in the NRAO Archives by Sierra Smith in 2012-2013. The transcription may have been read and edited for clarity by Sullivan, and may have also been read and edited by the interviewee. Any notes added in the reading/editing process by Sullivan, the interviewee, or others who read the transcript have been included in brackets. If the interview was transcribed for Sullivan, the original typescript of the interview is available in the NRAO Archives. Sullivan's notes about each interview are available on the individual interviewee's Web page. During processing, full names of institutions and people were added in brackets and if especially long the interview was split into parts reflecting the sides of the original audio cassette tapes. We are grateful for the 2011 Herbert C. Pollock Award from Dudley Observatory which funded digitization of the original cassette tapes, and for a 2012 grant from American Institute of Physics, Center for the History of Physics, which funded the work of posting these interviews to the Web. SullivanOkay, this is talking with A. Melvin Skellett over the telephone from the University of Washington to his retirement home in Sarasota, Florida on 26 August 1977 and we’re going to be taking this through a pickup mic on the telephone. Okay, to start off with your connection with the [Karl] Jansky discovery, I noticed that in Jansky's 1933 paper, he does give an acknowledgement to you for the help that you gave. Could you please relate how you remember the development of trying to figure out what this third kind of static was, how that went? SkellettWell, here's the story on it. Jansky was, you know, an associate of mine at the Laboratory, and he built this rotating antenna. His assignment was to study static electricity, I mean static interference with radio, all of its aspects. SullivanYou knew him before. SkellettOh, yes. We used to play bridge together and everything. We were very close friends. Well, at the same time, I was attending Princeton University, getting my doctorate degree in astronomy, see? SullivanI see, what was your bachelor's degree in, can I ask? SkellettI had my bachelor's degree in, I'd specialized in physics and my minor was math. SullivanWhat school was that? SkellettWashington University, St. Louis, Missouri. SullivanI see. The connection between astronomy and radio engineering is not the usual one for that time. How is it that you had these two interests? SkellettWell, I helped make them, put them together. SullivanThat's very true. SkellettAnyway, we were studying. I was trying to get a degree, a Ph.D. in astronomy. SullivanWho were the main professors you were working with? SkellettHenry Norris Russell and John Q. Stewart, these are all three professors in the Astronomy Department at Princeton. And the other one was named [Raymond Smith] Dugan. SullivanOh, yes. SkellettThey wrote a book. SullivanI know that textbook. SkellettYes. Well, anyway, so I was at the time in the Bell Lab. I was in the radio end of the thing, see. We were studying radio transmission across the ocean because they were starting to put the short wave radio telephones. This was before they had any radio between New York and London. So it occurred to me that the meteors shooting up there might be a contributing factor to the noise. So we set up an experiment, and we had a radar. They didn't call it radar then, but it was the same thing. SullivanThey called it a pulse method, or something like that. SkellettAnd we would get out there, boy, it was cold, at two o'clock in the morning, and shoot these pulses up at the meteor, see. And I'd lay on my back and whenever we saw a meteor overhead, I'd holler to the fellow inside who was looking at the cathode ray tube, and he'd say if there was any connection. Well, there was. SullivanThis was, before we get to the meteors, can we just now talk about the Jansky thing. So how was it that you heard about Jansky having this data that he couldn't figure out? SkellettWell, Jansky kept taking this data. He'd get this little hump in his data that happened about every 24 hours. And he came to me and he said, "Hey, I think I've got something here. I think that I'm getting static from the Sun." And I said, "Gee, it looks like it all right." So a month or two later, he says, "Something's wrong. It's gotten out at of phase with the Sun." He said, "It's not the same place; it's sliding." And then, of course, immediately I thought maybe it's not solar time but sidereal time. Now if it's sidereal time, it means that it's fixed in space but not fixed where the Sun is. Do you follow this? SullivanRight. SkellettSo, I said, "Why don't you try to fit sidereal time to your data?" He said, "I don't know anything about sidereal time." So I went out to him and we sat down together and we calculated, and sure enough, the darn thing came out that it was sidereal time and it was an easy step then to find where this thing was in space, and it was in Sagittarius, you see. SullivanRight. Okay, haw many months of data was accumulated before you made this connection with sidereal time? SkellettMy guess is a whole year, but it could be six months. But he had enough data so we weren't just guessing. SullivanIt was quite clear? SkellettYes. SullivanAnd so you found that it was in the constellation of Sagittarius and what did that mean to you at that time? SkellettWell, you see, Sagittarius is pretty close to the middle of our Galaxy, and we just thought it was coming from all the stars in the galaxy. SullivanRight. The middle of the galaxy as determined from [Harlow] Shapley's globular cluster work? SkellettYes, I guess so. There's a lot of ways of finding out where the middle of the Milky Way is. SullivanBut I was wondering, what was the main method then that you were relying on? SkellettGee, I don't remember. All I remember was that, yes, mostly Shapley's work, I think. This is a lot of years back, you know. It's hard to remember all the details. SullivanRight. Okay, now, one question to ask you is that in 1935 Jansky published another paper in which he looked back at those records he took in 1932 and he noticed that it wasn't just a single strong signal, but in fact, the entire plane of the Milky Way was giving emission. Do you have any ideas why you didn't catch that at first? SkellettI tell you, we had very little data to go on at first. He had just this one little hump in the records, see, and it happened every twenty-four hours roughly, not exactly. And we were just feeling our way along. Later then, he got to studying the thing and he got more data... SullivanWell, no, this was the same data. SkellettIt was? SullivanWell, he never took any more data, which brings me to another question while I think of it. Let me go back now. This is the same data, you can see the main peak of the galactic center, but then there are secondary peaks every time the antenna goes around, which corresponds to the Milky Way plane. SkellettYes. SullivanDo you have any idea why you didn't try well, what you would do today is make a contour map of the sky, more or less. SkellettWell, to tell you the honest truth, I don't remember the answer to that one. SullivanOkay. That's what I want to have is the honest truth. But okay, another question is if you're familiar with why Karl Jansky did not follow up his original measurements? SkellettEverybody asks me that question. And to the best of my knowledge, here's the reason. Karl did this work and he published it and it created a little bit of a stir, but nobody really was talking about, "Gee, we've opened up a whole new field of investigation, radio astronomy." They didn't think like that. So after he had taken all the data he could with that rotating antenna, he didn't know where to go from there, you see. And it was at the bottom of the Depression, and money for projects in the Bell Laboratories wasn't too easy to get anyway. So with the consent of everybody, and I'm pretty sure I can say rightly that Karl himself thought it was all right, that we drop the thing there, that he'd found out this stuff and published it, and what else could you do? You see, nobody dreamed that you could build a dish as big as the one at Arecibo or anything like that. So there wasn’t any real acrimonious thing going on between Karl and the... SullivanAnd [Harald T.] Friis? SkellettAnd Friis and the whole bunch, you know. Everything was in nice good faith and then later on, when the whole thing broke open, then they go back and they ask questions, "Why didn't Bell Labs push him into doing more stuff?" Oh, all kinds of things like that. But that's all... SullivanThat's all hindsight. SkellettThat's right. SullivanWere there other people asking these questions besides this fellow [John E.] Pfeiffer that wrote this book in the ‘50s? SkellettNo, no. There was very little interest in it. Believe me, I remember talking to my colleagues and professors at Princeton, because I was going there. And they said, "Gee, that's interesting. You mean there’s radio stuff coming from the stars?" I said, "Well, that's what it looks like." "Very interesting," and that's all they had to say about it. They didn't see any use for it or any reason to investigate or follow it any further. Everybody thought "Well, Karl did a nice job there, he got every bit of data he could get out of that big rotating antenna," and it was pretty big, you know. SullivanRight. SkellettSo everybody kind of threw up their hands and, "Nice job, where do you go from here?" No place to go. SullivanThe astronomers did believe the data. SkellettOh, well, anything from the Bell Labs they had to believe, you know. The reputation of the Bell Labs was behind this thing. SullivanBut there was no one at Princeton that was interested in trying to work out the theory of what might be causing this emission? SkellettNo, no one. SullivanAnd did you make some efforts to try to get people interested? SkellettNo. No, we didn't try to get publicity on it at all. We just thought we had made a very nice thing, published a paper, and then you go on to the next thing. SullivanDo you remember, did either you or Jansky ever give a talk at Princeton on this? SkellettI think Jansky gave some talks. I don't remember either of us talking at Princeton. No, the only thing I remember at Princeton was the informal discussion group. They were interested in what we were doing, but just kind of academically, you know. SullivanAnd do you think it was just that it was so far removed from their own type of astronomy that they didn't know what to do with it? SkellettYou hit the nail right on the head. That's exactly right. It was so far from the way they thought of astronomy that, you know, there was no real interest. If somebody had been fooling around with radio waves and even my paper on the meteors, I think that, no that was later. But anyway, they were interested in that, but I never did any more work on it. And the thing was just published, and I got my degree, and that was the whole thing. SullivanOkay, we'll get to the meteors very shortly. A couple of other questions about the Jansky thing. What ideas did you have about the possible origin of this emission? Did you think it was coming from the integrated effect of stars or did you think it was coming from the interstellar medium? SkellettWe didn't have the vaguest idea. We thought it must be coming from stars but that's just because that's what we knew were out there. We didn't try to speculate as to how it arose. SullivanBut then, of course, the question is: if it's coming from the stars, why don't you see it from the Sun? SkellettWell, they did later, you know. SullivanRight, but I'm talking about your thinking in the 1930s. SkellettNo, we didn't. All we knew was that the Sun's a great big hot body; there's an enormous amount of ionization which means that the surface of the Sun is an electric conductor and why wouldn't you get some radio from there? SullivanBut no one at that time thought about just pointing an antenna at the Sun? SkellettI don't think so. I don't recall that anybody did. It was [George] Southworth, wasn't it, that picked that up and got all the data on it? SullivanDuring World War II, right. SkellettAnd that was quite a bit later, wasn't it? SullivanThat was during the war, yes. SkellettRight. And as far as I know that was the first time anybody ever got any radio waves from the Sun. [Sullivan: Actually [James] Hey (1942) a bit earlier] SullivanBut I'm just puzzled why somebody didn't try this around 1930. SkellettWell, we didn't, that's all I can say. SullivanOkay. SkellettBut I tell you, you almost have to put yourself back into the thinking of those times to really understand this thing, because, golly, if something like this happened today with all our techniques and everything, now everybody would go to town on it, see? SullivanBut what was really different in that time, would you say? SkellettWell, what was different was that radio as a transmitting medium hadn't really been developed anywhere near like it is today. We didn't have any microwaves in those days, and it was very early in the game, I guess that's all I can say. Although I have to tell you as I've already said, it was a long time ago and it's hard to remember everything. SullivanOkay. I want to talk about the meteor ionization stuff now, but just let me check to make sure this recording is coming out okay. So I'll be back in about thirty seconds. Okay, it seems to be working. If you can remember to speak as loud as possible, that will help. SkellettOkay. SullivanNow about the meteor ionization, you say that was basically your idea that this might be a cause of ionization in the E layer, I believe. SkellettThat's right. SullivanAnd so, I guess you just worked out the numbers and that was the paper you published in 1932, which very interestingly directly follows Jansky's first paper. SkellettOh, yes. SullivanI don't know if you remember that. SkellettNo, but I know we were working on things at about the same time. SullivanWas there any design in trying to have those two together, since they both dealt with a bit of astronomy? SkellettNo, no. I'm pretty sure there wasn't at all. He was working quite independently of me, and I was working quite independently of him. SullivanI see. SkellettIn fact, we weren't in the same group, although the same basic area in the laboratory. SullivanYou were working at the Deal Laboratory? SkellettThat's right. And he was working at Homdel. SullivanAnd also, you did not know of any other work along the lines of calculating the radio effects of meteors? SkellettNo. I'm trying to remember, there was a fellow in Japan. SullivanThat's right. Naka... [WS: Nagaoka] SkellettNagasoki? SullivanSomething like that. Right. SkellettBut I think that his conclusion was that when a meteor goes through the atmosphere, what it leaves is just the opposite of mine. It would leave dust and the dust would be an insulator. Is that right? SullivanWell, that's correct. SkellettSo that that's the only other thing that I know of where anybody even remotely connected radio waves and meteor trails, see. SullivanRight. Do you remember at all how this idea came to you? SkellettNo, except that, you see that I was studying astronomy and I would go out and look at meteor showers just because I was very much interested in it. SullivanRight. SkellettAnd also, I was working in the radio group at the Bell Laboratories, and so it was almost logical that I would wonder if the thing didn't, you know, if there wasn't a connection. SullivanI see. SkellettYes. SullivanI'm still curious as to, the average graduate student at Princeton in astronomy would not be working at Bell Labs. I'm just curious as to how you came to be doing both of those things? SkellettWell, that is interesting. I got the job at Bell Labs before I went to Princeton, and I was working at Bell Laboratories and I wanted to get a doctorate degree. I only had a master's and a bachelor’s. So I went over there and I told them that I would like to be a candidate, see. And I remember the Dean saying, "Look, the requirements are that you have to live at Princeton if you're going to get a doctorate degree, at least a year's residence. So we'd have to pull the city limits of Princeton all the way over to the coast in order to get you in." I said, "Well, it wouldn't hurt to do that once, would it?" So they did. I used to go back and forth three or four times a week and at nights; you know. I had a little car and I'd drive those forty miles. SullivanSo what years was it that you were a student at Princeton? SkellettI think it was ‘30, ‘31, and, wait a minute, I got the degree in 1933. So it must have been 1931, '32, and '33. I was there three years. SullivanI see. And your thesis project was this meteor ionization? SkellettYes, that's what I was working on at Bell Laboratories. SullivanSo I can look that thesis up in the Princeton Library, I guess. SkellettOh, sure. SullivanWho was your advisor? SkellettI'm trying to think, I think it was Stewart, but it could have been Dugan. It could have been any one of the three. I can't remember. It's in there, I'm pretty sure, if you find the thesis. SullivanRight. Okay. Now looking more specifically at exactly what you did, I found a comment by [A. C. Bernard] Lovell who said the following: "The pre-World War II literature, had many proposals that meteors left an ionized trail which gave a detectable echo but there was no definite proof." Now would you agree with that? SkellettI didn't realize that so many people predicted it. I thought I was the only one. But he says there were, does he? SullivanWell, there are some other papers in which other people talk about the possibility and so forth, but would you agree that there was no real definite proof until Lovell's work that meteors did cause ionization? SkellettWho's Lovell? SullivanLovell in England, Sir Bernard. SkellettOh, yes. But was his stuff before mine? SullivanOh, no, no. This was after World War II. SkellettYes, I'd agree to that, I think because that's the way I remembered, I couldn't remember his name, but I remembered it was in England. SullivanBut what I'm saying is that he says that before World War II, there was no definite proof that an ionized trail could be caused by a meteor. SkellettWell, he's saying that I'm wrong then. SullivanWell, in a way. I'm saying do you feel that you definitely proved? SkellettOh, yes. We certainly thought we had. We saw them, and we saw the thing on the cathode ray tube, you know, the pulse coming back, and by eye as soon as the meteor trail died out. We were sure we had positive proof. SullivanI see. Well, you see, it looked like that to me, too, reading your papers. So let's talk about the individual papers. Well, the two of them together. There's your paper in 1932 in which you demonstrate the plausibility that meteors could cause sufficient ionization. SkellettThat was mostly theoretical. SullivanRight. And then there's the [J. P.] Schafer and [W. M.] Goodall paper right next to it, in which they looked at the November 1931 Leonid meteor shower, at your suggestion apparently. SkellettWell, I was with them, yes. SullivanBut they could not make any visual observations because it was cloudy. SkellettOh, yes, yes. I remember that. SullivanAnd so they had to rely on somebody else in New York State who looked at it, and so it wasn't a real tight argument that you could make. SkellettThat's right. SullivanBut what I'm wondering is why did they not mention the fact that you had looked at the Delta Aquarids the previous July, which was brought out in your later 1935 paper? For those August meteors, or July meteors, you had correlated visual and radio. SkellettGee, I'm so vague thinking back about that. See, Schafer and Goodall were really the radar experts over there. They were the ones that built the radio equipment, and we were all good friends and they were interested and worked with me, but I just don't remember the details of all that. I'm surprised, didn't I show, I remember there was something that had a chart in it and it had some meteors... SullivanThat's right; that's your 1935 paper. SkellettOh, yes. SullivanBut I'm curious why Schafer and Goodall didn't mention these previous observations because you did have them, simultaneous optical and radio observations. SkellettYou say the paper was in ‘35, but when was the data taken? SullivanOh, the data was in ‘31. SkellettOh, is that right? SullivanThat's another question I have for you, but okay, you don't remember then why Schafer and Goodall didn't mention the July ‘31 Delta Aquarids, I guess. SkellettNo, I'm sure there was a reason. One thing, I was not very much interested in publishing. I just didn't give a damn, you see. All I wanted was the doctor's degree. So my thinking in getting the data was to get it written up in a thesis and presented and get the doctor's degree and publish it, all right. I didn't care too much whether I published it or not. SullivanI see. Okay. Well, let's move on then. I notice that you gave a talk at the American Astronomical Society in Washington, D.C. in 1931 in which you presented these results about possible ionization from meteors. Can you remember what the reaction was from the astronomers? SkellettNo, I really don't. I remember giving the talk, but that's all I remember. I really don't remember. I think there was enough interest, though, that a few people asked questions, but there again, my memory is very vague.v SullivanDid you have any ideas at that time to try to look for daytime meteor showers? SkellettI don't think so. You can't see a meteor in the daytime very well. SullivanWell, but Lovell after the war did quite a bit of this. SkellettOh, I know. Lots was done afterwards, because, well, you know the literature better than I do now. SullivanBut you're saying the signal is a good bit weaker in the daytime. SkellettI don't know. We didn't shoot it up in the daytime, I don't think. SullivanBut what I'm asking is that this would seem to be something you could do and maybe really contribute, because there would be no other way of seeing these meteor showers. SkellettThat's right. SullivanDid this idea ever occur to you? SkellettI don't think so. One thing you have to remember is that our radar wasn't like the later ones were, sensitive enough. We only got signals back from a good, bright streak in the sky. The little guys that went by, we didn't get them. SullivanOkay. That's a big difference between after the war and before. SkellettYou know, radar really only came to its prime development due the war. SullivanRight. And that's of course, what really helped radio astronomy take off. SkellettSure. SullivanDid you ever think about trying to calculate velocities from the radar signals? SkellettNo. I know what you mean, no. I'm sure we didn't. SullivanWas it, once again, that it just couldn't be done? SkellettWell, we didn't see an easy way to do it. SullivanYou thought about it, though. SkellettI'm not sure. I just don't remember. SullivanOkay. Let's move on to the 1935 paper in which you discuss your visual observations and how they correlated with the radio from 1931 and 1932, and my first question is, why was there this delay in publishing this? [Sullivan: answered in his letter of 9/15/77] SkellettGee, I didn't realize there was a delay. I'll tell you what I'd like to do. Things are happening in my family. My sister died yesterday. SullivanOh, I see. I'm sorry. SkellettSo, I didn't do anything about looking anything up. But I'd like to go back, I've got some reprints and see if I can refresh my memory. Hey, incidentally, what are you going to do with this data? SullivanEventually, I'm going to write a book about the history and development of radio astronomy. SkellettOh, I see. SullivanIt's a few years off because it's going to be a very conclusive book, inclusive I mean, but that's the eventual goal. SkellettYes. Well, look, why don't I do this? I may be able to help you a little bit more if I look up the data and try to get some answers for you. Here's the thing, we're going to the funeral, which is up in St. Louis, so we'll be gone for at least a week. Can you wait another week or two? SullivanOkay. I'll give you a call again? SkellettYes. SullivanOkay, and then you have all of those papers? SkellettI think I can find them all. SullivanI'll call you up and ask you these questions and see if anything more comes back to you. SkellettYou've covered the field that you want pretty well, haven't you? SullivanI was just about at the end of it. Let me see what else I have here. So you don't remember why that paper was delayed? SkellettNo, I don't. That's what I'd like to check out. SullivanOkay. But you did get your degree in 1933. SkellettYes, I did. And the thesis was approved before I got the degree, see? So I had the data back in ‘33, so why, are you sure you've got all the publications? SullivanRight. Yes, I'm pretty sure. SkellettI'd like to check into that. And I'll do that within, as soon as I come back, and then if you'll call me in about two weeks. SullivanOkay. Do you remember at all why you did not do more pulse work during showers? There was only these three showers that were ever looked at. SkellettYes. I think it was pretty much like the Jansky thing. We had gone through the motions. We did quite a bit of work. There were quite a few nights we laid out there in the cold, and we finished this thing up and it was written up of course, in the Bell Laboratory’s records. We had ways of filing our data. And so I moved on to another job. SullivanYou considered it a closed case, more or less? SkellettPretty much, yes. We'd shown what we set out to show and what else can you do? Just keep taking data of the same kind of thing over and over? SullivanI guess you'd also shown that these were not of serious consequence for radio telephone communications. SkellettThat's right. SullivanSo it was rather analogous to Janksy's thing. Okay, one final question. I would imagine that you did not think of yourself as founding or beginning to found any kind of a field that might be called radar astronomy. SkellettNo, not at all. No, we didn't think like that. And I don't know whether Karl Jansky did or not, but I don't think so. SullivanBut it's rather ironic that I think that one can say that both radio and radar astronomy began at the same lab the same year. SkellettThat's right. That's interesting. SullivanBut not because of a group sort of working away at it, just by accident. Well, not really by accident in your case. No, it's not by accident in your case. Okay, well thank you very much, Dr. Skellett. I'll give you a ring back some evening about two weeks from now. SkellettYes. I hate to ask you again, but what was your name? SullivanW. T. Sullivan. Shall I give you my address? SkellettNo, I guess that's all right. You're going to call me, aren't you? SullivanAll right. I'll give you a call. SkellettShould I know you? Have we ever met? SullivanI don't think so, no. If you were located somewhere a bit more convenient to me, I'd love to come and visit, but I'm afraid I’ll never get to Sarasota. SkellettWhere are you? Washington, D.C.? SullivanNo, in Seattle. SkellettOh, out there! Sure. SullivanUniversity of Washington. SkellettWell, okay. SullivanThank you very much. I'll call you again. [Sullivan: not done until 6/83!] That finishes the first part of the interview with A. M. Skellett over the phone on 26 August ’77. Modified on Tuesday, 29-Jan-2013 08:50:31 EST by Ellen Bouton, Archivist (Questions or feedback) |