“Wow! 信号”的版本间差异

2013年5月14日 (二) 20:10的最新版本

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Wow! 信号

Wow! 信号

Wow! 信号是由工作在俄亥俄州立大学大耳无线电望远镜项目（SETI） Jerry R. Ehman 博士于1977年8月15日检测到的一个强大的窄带无线电信号，这个信号印证了潜在的非陆地和非太阳系的起源。它持续了72秒，整个期间由大耳无线电望远镜观察，但是它并没有再次被检测到。当谈论到 SETI 项目的成果时，它一直是主流媒体关注的焦点。

惊讶于它如此贴切用天线所期望得到的外星智能信号，Ehman 博士将在电脑上打印输出的信号圈出并在一旁写下注释“哇！”这个注释成为了信号的名称。

技术细节

被圈出来的字母代码 6EQUJ5 描述了信号的强度变化。每一个空隔表示介于 0到0.999之间。数字 1到9 表示对应带编号的强度（从1.000到9.999），高于 10.0的强度用字母表示（A的强度相当于10.0到10.999，B的强度相当于11.0到11.999，以此类推）。字母U所表示的值为30.0到30.999之间，是这台望远镜所曾检测到的最大值。在这种情况下的强度是无单位的信噪噪声比，是在数分钟之前这个频带上的平均值。

信号的位宽小于10kHz（在打印出的每一页对应着 10 kHz位宽的信道，信号是唯一的在一列之中）。已经给出了两个不同的频率值：1420.356MHz（J. D. Kraus）和1420.456MHz（J. R. Ehman），二者与氢线 1420.406 MHz 的差异小于 50 kHz 。两个可能的赤道坐标已给出：

R.A. = 19^h22^m22^s ± 5^s
R.A. = 19^h25^m12^s ± 5^s

两个坐标都在 = -27°03´ ± 20´ (epoch B1950.0).

大耳望远镜固定着随着地球的旋转扫描星空，依据地球自传的速率以及观测窗口的宽度。它可以在72秒内观察任何给出的点。因此，一个地球之外的信号将只能记录72秒钟，并且记录的强度在第36秒时会达到顶峰，直到信号到达了大耳望远镜观测窗口的中心，这时它会呈现逐步下降趋势。

Therefore, both the length of the Wow! signal, 72 seconds, and its shape would correspond to a possible extraterrestrial origin.

Searches for recurrence of the signal

The Big Ear telescope used two feed horns to search for signals, each pointing to a slightly different direction in the sky following Earth's rotation; the Wow! signal was detected in one of the horns but not in the other, although the data were processed in such a way that it is impossible to determine in which of the two horns the signal entered. In any case, the signal was expected to appear a mere three minutes apart in each of the horns, but this did not happen. Ehman unsuccessfully looked for recurrences of the signal using Big Ear in the month after the detection.

In 1987 and 1989, Robert Gray searched for the event using the META array at Oak Ridge Observatory, but did not re-detect it.

In 1995 and 1996, Gray also searched for the signal using the Very Large Array, which is significantly more powerful than Big Ear.

Gray and Dr. Simon Ellingsen later searched for recurrences of the event in 1999 using the University of Tasmania's Hobart 26m radio telescope.[5] Six 14-hour observations were made at positions in the vicinity, but did not detect anything similar to the Wow signal.

Speculations on the origin

Interstellar scintillation of a weaker continuous signal — similar, in effect, to atmospheric twinkling—could be a possible explanation, although this still would not exclude the possibility of the signal being artificial in its nature. However, even by using the significantly more sensitive Very Large Array, such a signal could not be detected, and the probability that a signal below the Very Large Array level could be detected by the Big Ear radio telescope due to interstellar scintillation is low.[4] Other speculations include a rotating lighthouse-like source, a signal sweeping in frequency, or a one time burst. Some have also suggested it could have come from a moving space vehicle of extraterrestrial origin.

Ehman has stated his doubts that the signal is of intelligent extraterrestrial origin: "We should have seen it again when we looked for it 50 times. Something suggests it was an Earth-sourced signal that simply got reflected off a piece of space debris."

He later recanted his skepticism somewhat after further research scientifically relegated an Earth-bound signal to be astronomically unlikely, due to the requirements of a space-borne reflector being bound to certain unrealistic requirements to sufficiently explain the nature of the signal. Also, the 1420 MHz signal is problematic in itself in that it is "protected spectrum" or bandwidth in which terrestrial transmitters are forbidden to transmit. In his most recent writings, Ehman resists "drawing vast conclusions from half-vast data."

Location of the signal

The location of the signal in celestial coordinates was, at (epoch J2000.0)

Right Ascension (On the positive horn): 19h25m31s ± 10s

Right Ascension (On the negative horn): 19h28m22s ± 10s

Declination (Is the same for both horns): -26d57m ± 20m

This region of the sky lies in the constellation Sagittarius, roughly 2.5 degrees south of the fifth-magnitude star Chi-1 Sagittarii.

@@ 第1行： / 第1行： @@
+{{Editing|zhouxiaobo|最近很累，又有许多事，需要在一个月后继续更新。}}
 <big>'''Wow! 信号'''</big>
+[[Image:Wow_signal.jpg|220px|right|thumb|Wow! 信号]]
-[[Image:Wow_signal.jpg|220px|right|thumb|Wow! 信号]]
-The Wow! signal was a strong, narrowband radio signal detected by Dr. Jerry R. Ehman on August 15, 1977, while working on a [[SETI]] project at the Big Ear radio telescope of Ohio State University. The signal bore expected hallmarks of potential non-terrestrial and non-solar system origin. It lasted for 72 seconds, the full duration Big Ear observed it, but has not been detected again. It has been the focus of attention in the mainstream media when talking about SETI results.
+Wow! 信号是由工作在俄亥俄州立大学大耳无线电望远镜项目（SETI） Jerry R. Ehman 博士于1977年8月15日检测到的一个强大的窄带无线电信号，这个信号印证了潜在的非陆地和非太阳系的起源。它持续了72秒，整个期间由大耳无线电望远镜观察，但是它并没有再次被检测到。当谈论到 SETI 项目的成果时，它一直是主流媒体关注的焦点。
+惊讶于它如此贴切用天线所期望得到的外星智能信号，Ehman 博士将在电脑上打印输出的信号圈出并在一旁写下注释“哇！”这个注释成为了信号的名称。
-Amazed at how closely the signal matched the expected signature of an interstellar signal in the antenna used, Ehman circled the signal on the computer printout and wrote the comment "Wow!" on its side. This comment became the name of the signal.
-=='''Technical details'''==
+=='''技术细节'''==
-The circled letter code 6EQUJ5 describes the intensity variation of the signal. A space denotes an intensity between 0 and 0.999.., the numbers 1-9 denote the correspondingly numbered intensities (from 1.000 to 9.999...), and intensities of 10.0 and above are denoted by a letter ('A' corresponds to intensities between 10.0 and 10.999..., 'B' to 11.0 to 11.999..., etc). The value 'U' (an intensity between 30.0 and 30.999...) was the highest ever detected by the telescope. The intensity in this case is the unitless signal-to-noise ratio, where noise was averaged for that band over the previous few minutes.
+被圈出来的字母代码 6EQUJ5 描述了信号的强度变化。每一个空隔表示介于 0到0.999之间。数字 1到9 表示对应带编号的强度（从1.000到9.999），高于 10.0的强度用字母表示（A的强度相当于10.0到10.999，B的强度相当于11.0到11.999，以此类推）。字母U所表示的值为30.0到30.999之间，是这台望远镜所曾检测到的最大值。在这种情况下的强度是无单位的信噪噪声比，是在数分钟之前这个频带上的平均值。
-The bandwidth of the signal is less than 10 kHz (each column on the printout corresponds to a 10 kHz-wide channel; the signal is only present in one column). Two different values for its frequency have been given: 1420.356 MHz (J. D. Kraus) and 1420.456 MHz (J. R. Ehman), both within 50 kHz of the frequency of the hydrogen line, which is at 1420.406 MHz. Two possible equatorial coordinates are given:
+信号的位宽小于10kHz（在打印出的每一页对应着 10 kHz位宽的信道，信号是唯一的在一列之中）。
+已经给出了两个不同的频率值：1420.356MHz（J. D. Kraus）和1420.456MHz（J. R. Ehman）
+，二者与氢线 1420.406 MHz 的差异小于 50 kHz 。两个可能的赤道坐标已给出：
@@ 第21行： / 第27行： @@
-Both coordinates give dec. = -27°03´ ± 20´ (epoch B1950.0).
+两个坐标都在 = -27°03´ ± 20´ (epoch B1950.0).
-The Big Ear telescope was fixed and used the rotation of the Earth to scan the sky. At the speed of the earth's rotation, and given the width of the Big Ear's observation "window", the Big Ear could observe any given point for just 72 seconds. An extraterrestrial signal, therefore, would be expected to register for exactly 72 seconds, and the recorded intensity of that signal would show a gradual peaking for the first 36 seconds – until the signal reached the center of Big Ear's observation "window" – at which time it would show a gradual decrease.
+大耳望远镜固定着随着地球的旋转扫描星空，依据地球自传的速率以及观测窗口的宽度。它可以在72秒内观察任何给出的点。因此，一个地球之外的信号将只能记录72秒钟，并且记录的强度在第36秒时会达到顶峰，直到信号到达了大耳望远镜观测窗口的中心，这时它会呈现逐步下降趋势。
 Therefore, both the length of the Wow! signal, 72 seconds, and its shape would correspond to a possible extraterrestrial origin.
 =='''Searches for recurrence of the signal'''==
@@ 第71行： / 第75行： @@
 *[[SETI]]
-[[Category:SETI]]
+[[Category:SETI]][[Category:待翻译]]