LATHAM. You mean if it was cloudy--

NIEMAND. No, no. The weather had nothing to do with it. I mean the Sun

had to be above the horizon at both places. A person might undergo an

attack soon after sunrise in New York but there would be no

corresponding record of an attack in California where it was still dark.

Conversely, a person might be stricken late in the afternoon in

California without a corresponding attack in New York where the Sun had

set. Dr. Hillyard and I had been searching desperately for a clue. We

had both noticed that the attacks occurred only during the daylight

hours but this had not seemed especially significant. Here we had

evidence pointing directly to the source of trouble. It must have some

connection with the Sun.

LATHAM. That must have had you badly puzzled at first.

NIEMAND. It certainly did. It looked as if we were headed back to the

Middle Ages when astrology and medicine went hand in hand. But since it

was our only lead we had no other choice but to follow it regardless of

the consequences. Here luck played somewhat of a part, for Hillyard

happened to have a contact that proved invaluable to us. Several years

before Hillyard had gotten to know a young astrophysicist, Henry

Middletown, who had come to him suffering from a severe case of myositis

in the arms and shoulders. Hillyard had been able to effect a complete

cure for which the boy was very grateful, and they had kept up a

desultory correspondence. Middletown was now specializing in radio

astronomy at the government's new solar observatory on Turtle Back

Mountain in Arizona. If it had not been for Middletown's help I'm afraid

our investigation would never have gotten past the clinical stage.

LATHAM. In what way was Middletown of assistance?

NIEMAND. It was the old case of workers in one field of science being

completely ignorant of what was going on in another field. Someday we

will have to establish a clearing house in science instead of keeping it

in tight little compartments as we do at present. Well, Hillyard and I

packed up for Arizona with considerable misgivings. We were afraid

Middletown wouldn't take our findings seriously but somewhat to our

surprise he heard our story with the closest attention. I guess

astronomers have gotten so used to hearing from flying saucer

enthusiasts and science-fiction addicts that nothing surprises them any

more. When we had finished he asked to see our records. Hillyard had

them all set down for easy numerical tabulation. Middletown went to work

with scarcely a word. Within an hour he had produced a chart that was

simply astounding.

* * * * *

LATHAM. Can you describe this chart for us?

NIEMAND. It was really quite simple. But if it had not been for

Middletown's experience in charting other solar phenomena it would never

have occurred to us to do it. First, he laid out a series of about

thirty squares horizontally across a sheet of graph paper. He dated

these beginning March 1, 1955, when our records began. In each square he

put a number from 1 to 10 that was a rough index of the number and

intensity of the attacks reported on that day. Then he laid out another

horizontal row below the first one dated twenty-seven days later. That

is, the square under March 1st in the top row was dated March 28th in

the row below it. He filled in the chart until he had an array of dozens

of rows that included all our data down to May, 1958.

When Middletown had finished it was easy to see that the squares of

highest index number did not fall at random on the chart. Instead they

fell in slightly slanting parallel series so that you could draw

straight lines down through them. The connection with the Sun was

obvious.

LATHAM. In what way?

NIEMAND. Why, because twenty-seven days is about the synodic period of

solar rotation. That is, if you see a large spot at the center of the

Sun's disk today, there is a good chance if it survives that you will

see it at the same place twenty-seven days later. But that night

Middletown produced another chart that showed the connection with the

Sun in a way that was even more convincing.

LATHAM. How was that?

NIEMAND. I said that the lines drawn down through the days of greatest

mental disturbance slanted slightly. On this second chart the squares

were dated under one another not at intervals of twenty-seven days, but

at intervals of twenty-seven point three days.

LATHAM. Why is that so important?

NIEMAND. Because the average period of solar rotation in the sunspot

zone is not twenty-seven days but twenty-seven point three days. And on

this chart the lines did not slant but went vertically downward. The

correlation with the synodic rotation of the Sun was practically

perfect.

LATHAM. But how did you get onto the S-Regions?

NIEMAND. Middletown was immediately struck by the resemblance between

the chart of mental disturbance and one he had been plotting over the

years from his radio observations. Now when he compared the two charts

the resemblance between the two was unmistakable. The pattern shown by

the chart of mental disturbance corresponded in a striking way with the

solar chart but with this difference. The disturbances on the Earth

started two days later on the average than the disturbances due to the

S-Regions on the Sun. In other words, there was a lag of about

forty-eight hours between the two. But otherwise they were almost

identical.

LATHAM. But if these S-Regions of Middletown's are invisible how could

he detect them?

NIEMAND. The S-Regions are invisible to the eye through an _optical_

telescope, but are detected with ease by a _radio_ telescope. Middletown

had discovered them when he was a graduate student working on radio

astronomy in Australia, and he had followed up his researches with the

more powerful equipment at Turtle Back Mountain. The formation of an

S-Region is heralded by a long series of bursts of a few seconds

duration, when the radiation may increase up to several thousand times

that of the background intensity. These noise storms have been recorded

simultaneously on wavelengths of from one to fifteen meters, which so

far is the upper limit of the observations. In a few instances, however,

intense bursts have also been detected down to fifty cm.

LATHAM. I believe you said the periods of mental disturbance last for

about ten or twelve days. How does that tie-in with the S-Regions?

NIEMAND. Very closely. You see it takes about twelve days for an

S-Region to pass across the face of the Sun, since the synodic rotation

is twenty-seven point three days.

LATHAM. I should think it would be nearer thirteen or fourteen days.

NIEMAND. Apparently an S-Region is not particularly effective when it is

just coming on or just going off the disk of the Sun.

LATHAM. Are the S-Regions associated with sunspots?

NIEMAND. They are connected in this way: that sunspot activity and

S-Region activity certainly go together. The more sunspots the more

violent and intense is the S-Region activity. But there is not a

one-to-one correspondence between sunspots and S-Regions. That is, you

cannot connect a particular sunspot group with a particular S-Region.

The same thing is true of sunspots and magnetic storms.

LATHAM. How do you account for this?

NIEMAND. We don't account for it.

* * * * *

LATHAM. What other properties of the S-Regions have you discovered?

NIEMAND. Middletown says that the radio waves emanating from them are

strongly circularly polarized. Moreover, the sense of rotation remains

constant while one is passing across the Sun. If the magnetic field

associated with an S-Region extends into the high solar corona through

which the rays pass, then the sense of rotation corresponds to the

ordinary ray of the magneto-ionic theory.

LATHAM. Does this mean that the mental disturbances arise from some form

of electromagnetic radiation?

NIEMAND. We doubt it. As I said before, the charts show a lag of about

forty-eight hours between the development of an S-Region and the onset

of mental disturbance. This indicates that the malignant energy

emanating from an S-Region consists of some highly penetrating form of

corpuscular radiation, as yet unidentified.[A]

[Footnote A: Middletown believes that the Intense radiation recently

discovered from information derived from Explorer I and III has no

connection with the corpuscular S-radiation.]

LATHAM. A question that puzzles me is why some people are affected by

the S-Regions while others are not.

NIEMAND. Our latest results indicate that probably _no one_ is

completely immune. All are affected in _some_ degree. Just why some

should be affected so much more than others is still a matter of

speculation.

LATHAM. How long does an S-Region last?

NIEMAND. An S-Region may have a lifetime of from three to perhaps a

dozen solar rotations. Then it dies out and for a time we are free from

this malignant radiation. Then a new region develops in perhaps an

entirely different region of the Sun. Sometimes there may be several

different S-Regions all going at once.

LATHAM. Why were not the S-Regions discovered long ago?

NIEMAND. Because the radio exploration of the Sun only began since the

end of World War II.

LATHAM. How does it happen that you only got patients suffering from

S-radiation since about 1955?

NIEMAND. I think we did get such patients previously but not in large

enough numbers to attract attention. Also the present sunspot cycle

started its rise to maximum about 1954.

LATHAM. Is there no way of escaping the S-radiation?

NIEMAND. I'm afraid the only sure way is to keep on the unilluminated

side of the Earth which is rather difficult to do. Apparently the

corpuscular beam from an S-Region is several degrees wide and not very

sharply defined, since its effects are felt simultaneously over the

entire continent. Hillyard and Middletown are working on some form of

shielding device but so far without success.

LATHAM. What is the present state of S-Region activity?

NIEMAND. At the present moment there happens to be no S-Region activity

on the Sun. But a new one may develop at any time. Also, the outlook for

a decrease in activity is not very favorable. Sunspot activity continues

at a high level and is steadily mounting in violence. The last sunspot

cycle had the highest maximum of any since 1780, but the present cycle

bids fair to set an all time record.

LATHAM. And so you believe that the S-Regions are the cause of most of

the present trouble in the world. That it is not ourselves but something

outside ourselves--

NIEMAND. That is the logical outcome of our investigation. We are

controlled and swayed by forces which in many cases we are powerless to

resist.

LATHAM. Could we not be warned of the presence of an S-Region?

NIEMAND. The trouble is they seem to develop at random on the Sun. I'm

afraid any warning system would be worse than useless. We would be

crying WOLF! all the time.

LATHAM. How may a person who is not particularly susceptible to this

malignant radiation know that one of these regions is active?

NIEMAND. If you have a feeling of restlessness and anxiety, if you are

unable to concentrate, if you feel suddenly depressed and discouraged

about yourself, or are filled with resentment toward the world, then you

may be pretty sure that an S-Region is passing across the face of the

Sun. Keep a tight rein on yourself. For it seems that evil will always

be with us ... as long as the Sun shall continue to shine upon this

little world.

Disturbing Sun · 第 6 / 8 题