Histograms constructed from the data of [sup.239]Pu alpha-activity manifest a tendency for change in the similar way as at the moments when the Sun, the Moon, Venus, Mars and Mercury intersect the celestial equator.
A many-year monitoring of the alpha-activity of [sup.239]Pu samples (performed with devices constructed by one of the authors, I. A. Rubinstein ) was used as a basis for this study. Round-the-clock once-a-second measurements were made in Pushchino, at the Institute of Theoretical and Experimental Biophysics, Russian Academy of Sciences, and at Novolazarevskaya Antarctic Polar Station of the Arctic and Antarctic Institute.
Semi-conductor detectors used were either collimator-free or equipped with collimators limiting the beam of registered alpha-particles by a spatial angle (about 0.1 radian) within which the particles travelled along a certain direction: towards the Sun, Polar Star, West or East. The number of registered alpha-particles during one-second interval was the measured parameter. Results of the continuous once-a-second measurements of the decay activity were stored in a computer databank.
One-minute histograms constructed from 60 results of the once-a-second measurements of activity were the main objects of analysis in our study. The histograms were visually compared with each other in order to estimate the resemblance of their shape. The estimation was made by the method of expert judgment. This analysis was performed with the assistance of Edwin Pozharsky's computer program (described in ) which allowed to construct histograms for each one-minute interval in a series of measurements and, further, to smooth and scale them, and to mirror (if needed) in order to superimpose the histograms and visually compare their shape. At the final step of analysis, we constructed the distribution of the number of pairs of similar histograms versus the interval separating the histograms in each pair. Fig. 1 presents a diagram explaining three kinds of comparison of the series of histograms.
Method A; direct alignment (parallel). These two compared histogram series are aligned with each other as parallel sequences in which the equinox moments occur at the same place. Then each i-th histogram of one series is compared with the number of neighboring histograms of the other series, as shown in Fig. 1, case A.
[FIGURE 1 OMITTED]
Method B; inverse alignment (anti-parallel). These two series are aligned in the same way but the second one is reversed at the point of equinox. This is illustrated in Fig. 1B.
Method C; "palindrome" alignment. Two parts of the same sequence are compared with each other. To do that, we assume the equinox moment to be the inversion center of a palindrome. Therefore, the second half of the sequence (following the center) is reversed and aligned with the first half as shown in Fig. 1C. Then the two halves of the sequence are compared with each other.
Fig. 2 presents an extract from the laboratory log-file to illustrate what shapes are considered similar from the expert's viewpoint. Final results are presented as the plots of the frequency of similar pairs of histograms versus the interval (measured in minutes) separating the position of items in the pairs (Fig. 3, e.g.).
The true equinox moments and the equivalent moments when the Moon, Mars, Venus or Mercury intersect the celestial equator (called here, by analogy, "planetary equinoxes") were determined by nonlinear interpolation of the data tabulated in the annual astronomy tables ; the residual error of this interpolation was much within the time resolution of our observations.
[FIGURE 2 OMITTED]
2.1 Comparison of the histogram series obtained at the successive (in turn) "equinoxes"
It had been found earlier [2, 5, 6], in studying the variation of shape of the successive sequences of histograms obtained at vernal and autumnal equinoxes, the sequences related to "homonymous" equinoxes (vernal-and-vernal or autumnal-and-autumnal ones) display the similarity higher than that of "heteronymous" equinoxes. This fact gave a hint for a hypothesis that the histogram shape may depend not only on the proximity to the equinox moment, but also on the direction the Sun is moving to the celestial equator: from the northern or from the southern hemisphere. The hypothesis has been confirmed by comparison of the direct series of the autumn histograms with the inverse series of the spring histograms [2, 5, 6] (cf. in Fig. 1, method B).
[FIGURE 3 OMITTED]
In this work, the same analysis is applied to the data including "planetary equinoxes". Namely, not only solar but also lunar, venusian, martian and mercurian "equinoxes" have been considered. Fig. 3 summarizes the results of 24 pairs of such "equinox" events. Only the pairs of successive "equinoxes" were here compared; i.e., a series of histograms obtained at one "equinox" was compared with that of just next "equinox" for the same celestial body. The series were compared with use of either procedure A (parallel) and B (anti-parallel) (cf. in Fig. 1).
Fig. 3 shows that:
1. The phenomenon of similarity of the temporal change of the histogram shape near the moments of intersection of the celestial equator by a celestial body appears to be independent of the nature of the body (whatever the Sun, the Moon, Venus, Mars or Mercury). Hence, the sequential changes of histograms do not show any gravitational influence of the bodies;
2. Neither does it depend on the geographic point where the measurements have been performed: the data obtained in Pushchino and Novolazarevskaya (Antarctic) display similarity of histograms at the same absolute time, to within one-minute accuracy;
3. Neither does it depend on the velocity a celestial body moves across the equator. Despite a great difference in both angular and linear velocities of the bodies, the changes of histogram shape are correlated in the sequences aligned along the same time scale. This is a surprising result that has not a simple kinematic explanation. This fact, again, is an indication of that the phenomenon observed is not a matter of any "influence" exerted by a celestial bodies on the observable value;
4. What we can learn from the fact that the similarity of histogram sequences is higher in the case of anti-parallel orientation of compared sequences is as follows. The variation of histogram shape shows not only the extent of proximity of the Sun or a planet to the celestial equator but also their location in one or another celestial hemisphere. In other words, the "northern" histograms of a vernal equinox display higher similarity to the "southern" histograms of the next autumnal equinox despite the movement of the body on the sky sphere are reciprocal at these two cases.
[FIGURE 4 OMITTED]
The fact that the histogram shape variations do not depend on the nature of celestial body is confirmed also by pairwise comparison of the "equinoxes" of different planets. For example, Fig. 4 presents the results of comparison of a Venus "equinox" (2001-October-18 ([down arrow])) with three Moon "equinoxes" (2005-March-11([up arrow]); 2005-March-25([down arrow]), and 2005- April-7([right arrow])). The figure shows that:
1. The histogram series adjusted to "equinox" moments are similar even if the events considered are separated by years (four years in this particular case);
2. The similarity of histograms depends on the direction of movement towards the celestial equator. However, in this particular case, symbate "equinoxes" (Venus 2001-October-18([down arrow]) and Moon-2005-March-25([down arrow])) happened to be less similar then the counter-directed ones (Venus-2001-October-18([down arrow]) and the other two Moon "equinoxes", both rising).
[FIGURE 5 OMITTED]
2.2 Comparison of direct and inverse halves of the same series of histograms (the "palindrome" effect)
The "palindrome effect" has been described in a number of earlier works; this is the presence of specific inversion points in the time series of histograms after which the same histograms occur in the reverse order [2, 5, 6]. Over a daily period, 6 am and 6 pm of local time have been found to be such inversion points. Any point on the Earth's surface participates in two movements, one due to the rotation of the Earth about its axis and another due to the movement of the center of the Earth along its circumsolar orbit. One finds that, the projections of the two movements onto the circumsolar orbit are counter-directional during the daytime (6 am to 6 pm) and co-directional during the nighttime (6 pm to 6 am). This is a probable "kinematic" reason for these two time moments are featured.
A question arose if there are a number of such "palindrome" centers existing at the equinoxes and "planetary equinoxes", separating the celestial body movement towards and away from the celestial equator. This supposition has proved to be true. Indeed, the histogram sequences preceding the equinox moments were similar to the inverse sequences following this moments. The palindrome effect (detected with the procedure C; cf. Fig. 1), is illustrated in Fig. 5. As revealed from the picture, the probability to find similar histograms is 3-fold higher if one of the compared half-sequences is inverted--this is exact the essence of the palindrome effect.
[FIGURE 6 OMITTED]
Phenomenological meaning of this observation is that the "equinox" moments are just the points at which the order of changing the histogram shapes is reverted. Sharpness of the peak is an indication of a high accuracy (one minute) of detection of the "equinox" moment. Mirror symmetry of the histogram sequences around an equinox means that histogram shape depends on how far distant is the celestial body from the equator plane, whatever on the northern or southern side of the celestial sphere. This result might seem to conflict with the data presented in Fig. 3 indicating that the direction of the movement also does matter. However, the seeming conflict is resolved by the fact (revealed from our special investigation) that these two phenomena are determined by different, not overlapping sets of similar histograms.
2.3 Equinox effects in the data obtained with collimators
The phenomena presented in Figs. 3-5 have been observed in the data on the alpha-activity measured with either collimator-free detectors and those supplied with the collimator permanently directed towards West or East or towards the Sun. No dependence of the observed phenomenology on the orientation of the collimator was found in these cases. The only dramatic difference has been found for the case where the collimator was directed towards the Polar Star.
In this series of data, the sequences of histograms obtained at the sequential (neighboring) "equinoxes" displayed higher similarity when they were compared as parallel sequences (procedure A in Fig. 1) and lesser similarity when they were anti-parallel. This observation is illustrated in Fig. 6, summarizing the results of eight equinox events with the Moon, the Sun and Mars. Therefore, the difference between the northern and southern hemispheres is not reflected in the measurements with the collimator directed to Northern Pole.
A number of phenomenological conclusions follow from the results presented herein:
1. The shape of histograms obtained from the measurements performed in different geographic locations near the time of "equinoxes" is changing synchronously, within one minute accuracy. For instance, they occur simultaneously in Pushchino and Novolazarevskaya despite 104 minutes of local time difference between these two places. This means this is a global phenomenon independent of the Earth axial rotation;
2. The changes of histograms obtained near the solar or planetary "equinoxes" do not depend on the nature of the "acting" celestial body, whatever the Sun, Mercury, Mars, Venus or Mercury. Individual features of the bodies--different masses and different rates of their orbital movement--are not essential;
3. At very equinox moments, the inversion of the sequence of the histogram shapes occurs: the sequence preceding this moment is reciprocal to that observed after it. A moment when the celestial equator is intersected by a celestial body is a particular point in the histogram series. Its position on the time scale can be determined, with a high accuracy, from the palindrome effect;
4. Changes of histograms near the "equinoxes" depend on the direction in which the celestial body intersects the equator plane (from the northern or from southern hemisphere);
5. Seeming contradiction between these two phenomena--the similarity of the anti-parallel sequences obtained at successive equinoxes, and the mirror similarity of two halves of each histogram sequence (the "palindrome effect")--is, probably, resolved by the fact that these two kinds of symmetry are determined by different, not overlapping sets of similar histograms;
6. Phenomena observed with collimators can be considered as an indication of the anisotropy of space. Vanishing of the "palindrome" phenomena when the collimator is oriented towards the Polar Star is, perhaps, the most indicative fact favoring the conclusion on the anisotropy. Analysis of this phenomenon should be subjected to further studies.
B. V. Komberg attracted our attention to the fact that the direction of the equinox line (the line of intersection of the equatorial and ecliptic planes) may coincide with direction of the line of the minimum temperature of the Cosmic Microwave Backgroud (relict) Radiation, called the "axis of evil" in the scientific literature .
We sincerely appreciate A. E. Shnoll and A. E. Rodin's participation in the calculation of the moments the celestial equator is intersected by the Moon, Venus and Mars and valuable advice in the data analysis. We sincerely appreciate valuable discussion with S. A. Vasiliev and his interpretation of our results . We sincerely appreciate A. A. Andreyeva's work as a "second expert" in the analysis of similarity of histograms. We are much obliged to our colleagues from the Laboratory for Physical Biochemistry of the Institute for Theoretical and Experimental Biophysics of RAS and from Chair of Biophysics at Physics Department of MSU, for useful discussions at our seminars, and especially to O. Yu. Seraya for discussion and English translation of the article. We appreciate T. A. Zenchenko's systematic job on the development and support of a computer databank for radioactivity monitoring. We are grateful to D. D. Rabounski for his valuable discussion. The work would be impossible without M. N. Kondrashova and her continuous attention, support and discussion of results. Financial support from D. B. Zimin is greatly appreciated.
Submitted on January 01, 2011/Accepted on January 05, 2011
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Simon E. Shnoll * ([dagger])([section]), Ilya A. Rubinstein ([double dagger]), Sergey N. Shapovalov (#), Valery A. Kolombet ([dagger]), Dmitri P. Kharakoz ([dagger])
* Department of Physics, Moscow State University, Moscow, Russia ([dagger]) Institute of Theor. and Experim. Biophysics, Russ. Acad. Sci., Pushchino, Russia ([double dagger]) Skobeltsin Inst. of Nuclear Physics at Moscow State Univ., Moscow, Russia ([section]) Pushchino State University, Pushchino, Russia (#) Arctic and Antarctic Research Institute, St. Petersburg, Russia
E-mail: firstname.lastname@example.org (Simon E. Shnoll, the corresponding author)
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|Author:||Shnoll, Simon E.; Rubinstein, Ilya A.; Shapovalov, Sergey N.; Kolombet, Valery A.; Kharakoz, Dmitri|
|Publication:||Progress in Physics|
|Date:||Apr 1, 2011|
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