scholarly journals Composition, density and biomass of fish community from the surf zone as a function of the lunar cycle at Miramar Beach in Cabedelo, Paraíba

2019 ◽  
Vol 17 (2) ◽  
Author(s):  
Willy Vila Nova Pessoa ◽  
Jonas de Assis Almeida Ramos ◽  
Paulo Guilherme Vasconcelos de Oliveira
Keyword(s):  
Surf Zone ◽  
Abundant Species ◽  
Lunar Cycle ◽  
Species Group ◽  
Biological Interactions ◽  
The Moon ◽  
Group I ◽  
The Mean ◽  
New Moon ◽  
Density And Biomass

ABSTRACT The influence of the moon cycles on the ichthyofauna has been little studied in the surf zone. In this study, the number of species, density and biomass were evaluated as a function of the moon. A total of 49 species distributed in 24 families were captured in two areas of Miramar beach. The mean density was significant high in the weaning and low in the new moon, while density and biomass together showed differences for areas. The most abundant species were Anchoa tricolor and Trachinotus falcatus (new moon), and Anchovia clupeoides showed significant differences in the waning moon. The RDA indicates that turbidity influenced significantly the presence of two species group. The group I were represented by Stellifer brasiliensis, Trachinotus goodei, A. clupeoides, Chilomycterus spinosus and Conodon nobilis that occurred on the waning and new phases in both areas, while the group II were represented by Polydactylus virginicus and Haemulopsis corvinaeformis in the full moon. The surf zones may also be strongly governed by the lunar phases. Therefore, the results found in this study, showed that the biological interactions between the species with turbidity and moon might explain the density and biomass variations for some species in the surf zone.

scholarly journals On certain variations of the mean height of the barometer, mean temperature and depth of rain, connected with the lunar phases, in the cycle of years from 1815 to 1823

1843 ◽  
Vol 4 ◽  
pp. 211-211
Keyword(s):  
Full Moon ◽  
Lunar Cycle ◽  
Lunar Phase ◽  
The Moon ◽  
Lunar Phases ◽  
Mean Temperature ◽  
The Mean ◽  
New Moon ◽  
Made In

The table given in this paper contains the results of calculations relating to the objects specified in the title; cast into periods of six, seven, or eight days, so as to bring the day of the lunar phase belonging to it in the middle of the time. The observations were all made in the neighbourhood of London. It appears from them that in the period of the last quarter of the moon the barometer is highest, the temperature a little above the mean, and the depth of rain the smallest. In the period of the new moon, both the barometer and temperature are considerably depressed, and the rain increased in quantity. The influence of the first quarter shows itself by the further depression of the barometer; but the temperature rises almost to the point from which it had fallen, and the rain still increases, but not in an equal ratio. Lastly, the full moon again reduces the temperature; while the barometer attains its maximum mean height, and the quantity of rain is the greatest. Thus it appears, that during this lunar cycle, the approach of the last quarter is the signal for the clearing up of the air, and the return of sunshine.

Lunar Cycle Influences Reproductive Performance of Crossbred Brahman Cows Under Tropical Conditions

2021 ◽  
pp. 074873042098363
Author(s):  
Alejandro A. Aguirre ◽  
Roberto A. Palomares ◽  
Aitor D. De Ondiz ◽  
Eleazar R. Soto ◽  
Mariana S. Perea ◽  
...  
Keyword(s):  
Reproductive Performance ◽  
Full Moon ◽  
Lunar Cycle ◽  
The Moon ◽  
Crossbred Cows ◽  
Lunar Phases ◽  
Tropical Conditions ◽  
Service Conception ◽  
New Moon ◽  
Postpartum Estrus

Evidence has accumulated over the years indicating that the moon influences some aspects of the reproductive activity in animals and humans. However, little is known about the influence of the lunar cycle on the reproductive performance of cows under tropical conditions, where the environment strongly affects reproduction. This retrospective study was conducted with the aim of assessing the influence of the lunar cycle on some reproductive traits of tropical crossbred cows managed in a pasture-based system. Data from 5869 reproductive records from two commercial farms localized in the Maracaibo Lake Basin of Zulia State, Venezuela, were analyzed. Variables studied were first service conception rate, calving frequency, first postpartum estrous frequency, and pregnancy frequency. In addition to the lunar cycle, the effects of farm, season, and predominant breed were also considered. Data were analyzed using logistic regression and general linear model from SAS. First service conception was affected by lunar phases and predominant breed, but not by farm or season. For frequencies of calving, first postpartum estrus, and pregnancy, there was no main effect of farm, season, and predominant breed, whereas the effect of lunar phases was highly significant. First service conception was significantly greater in waning than in crescent phase of the lunar cycle. Frequencies of calving, first estrus, and pregnancy were highly correlated and showed greater figures around full moon and new moon. In conclusion, lunar cycle influenced first service conception, attaining greater values in the waning phase of the moon cycle. Frequencies of calving, first postpartum estrus, and pregnancy in crossbred cows showed a clear bimodal rhythm, whose greatest values coincided with new moon and full moon.

The biting habits of Culicoides furens (Poey) and C. barbosai Wirth & Blanton. III. Seasonal cycle, with a note on the relative importance of ten factors that might influence the biting rate

1972 ◽  
Vol 61 (3) ◽  
pp. 565-576 ◽  
Author(s):  
D. S. Kettle
Keyword(s):  
Seasonal Cycle ◽  
Full Moon ◽  
Lunar Cycle ◽  
Relative Importance ◽  
The Moon ◽  
Illumination Time ◽  
Biting Rate ◽  
New Moon ◽  
Phases Of The Moon ◽  
Cycle Temperature

The biting rates of Culicoides furens (Poey) and C. barbosai Wirth & Blanton on Florida Beach, Jamaica, were observed in 50 trials conducted 40–115 min after dawn from 5 February 1960 to 10 February 1961. The data were logarithmically transformed and non-zero biting rates standardised. Biting rates of both species varied markedly from week to week but monthly mean rates were significantly higher and lower for C. furens in September (111·4) and March (13·7), respectively. Monthly mean rates for C. barbosai fell into three groups, (i) March-June (15·3); (ii) November–December (9·1); (iii) January–February and July–October (3·1). These changes were negatively correlated with mean sea level. Biting rates of C. barbosai were highest at new moon (10·3) and lower but similar (4·3–5·2) for the other three phases of the moon. Those of C. furens were maximal at new moon (62·8), minimal at full moon (20·4) and intermediate (35·9, 39·5) at the quarters. The lunar effect is assumed to act through the tides. There were no significant differences between the standardised biting rates at different times after dawn. In a comparison of the quantitative effects of ten factors on the biting rates of C. furens, C. barbosai and Leptoconops becquaerti (Kieff.), most important were month of year and wind speed; of less importance were lunar cycle, temperature, collector and limb exposed; while site position, intensity of illumination, time after dawn, saturation deficit were of minor or no importance. It is concluded that the biting rate of L. becquaerti should be the least affected by changes in these factors, C. barbosai more affected and C. furens most affected.

The Earliest Visible Phase of the Moon

1920 ◽  
Vol 14 (3-4) ◽  
pp. 172-172
Author(s):  
T. Rice Holmes
Keyword(s):  
Early Spring ◽  
The Moon ◽  
Naked Eye ◽  
Fine Weather ◽  
Interesting Paper ◽  
The Mean ◽  
New Moon ◽  
The University ◽  
First Time ◽  
Clear Atmosphere

I AM glad that Dr. Fotheringham in the interesting paper which appeared in the Classical Quarterly (April, 1920, pp. 97–8) adhered to the view that ‘Caesar calculated the new moon for January 1 [45 B.C]…and that this calculation determined the inaugural day of the Julian calendar.’ As the object of my brief note, on which he commented, was merely to show that Groebe had failed to prove that the day in question was January 2, I have only a few questions to ask. But first, in justice to Judeich, I ought to say that his calculations, which Dr. Fotheringham notices, were made with the help of the assistant-astronomer attached to the observatory of the University of Strassburg. While Dr. Fotheringham admits that I was right in maintaining that the new moon of January 2, 45 B.C. (1.26 a.m.) was not visible on the evening of that day, he holds that Groebe was ‘fairly entitled to say’ that the new moon of March 24, 58 B.C. (4.40 p.m.), was visible on March 25. Dr. Fotheringham may be justified in saying that it ought ‘in normal [or abnormally fine ?] weather to have been visible that evening’; but, as I observed in my note, Groebe affirmed that in calculating the time of visibility of the crescent we should accept the mean of the Babylonian estimates, 36 hours—less, I should have added, in the early spring and the winter, more in the summer and autumn. Was he entitled to deduct 9 hours from the mean for an observation made not in the clear atmosphere of the East, but in Switzerland? Dr. Fotheringham tells us that ‘the shortest interval between a new moon and the observation of the moon by Schmidt's naked eye comes’ not, as Groebe said, to 29, but ‘to 25.7 hours.’ But forty-eight of Schmidt's forty-nine observations were made at Athens, where the atmosphere is clearer than in Switzerland. The great difference in visibility which a clear atmosphere makes must strike everyone who goes from this country or from Switzerland to the East or to Northern Africa. I realized it for the first time when I was exploring in Tunisia before the war. Has Dr. Fotheringham or any other trustworthy observer ever seen with the naked eye in an atmosphere no clearer than that of Geneva a moon not more than 27 hours old? If so, is it not remarkable that, as Dr. Fotheringham has said, ‘Hitherto it has been the practice to assume that [in the early spring or the winter and in favourable weather ?] the moon becomes visible on the first evening when she is more than 30 hours old at sunset’?

scholarly journals Singing in the moonlight: dawn song performance of a diurnal bird varies with lunar phase

2014 ◽  
Vol 10 (1) ◽  
pp. 20130970 ◽  
Author(s):  
Jennifer E. York ◽  
Andrew J. Young ◽  
Andrew N. Radford
Keyword(s):  
Animal Communication ◽  
Lunar Cycle ◽  
Lunar Phase ◽  
Moon Phase ◽  
Communication Research ◽  
The Moon ◽  
Research Attention ◽  
Dawn Song ◽  
New Moon ◽  
Diurnal Species

It is well established that the lunar cycle can affect the behaviour of nocturnal animals, but its potential to have a similar influence on diurnal species has received less research attention. Here, we demonstrate that the dawn song of a cooperative songbird, the white-browed sparrow weaver ( Plocepasser mahali ), varies with moon phase. When the moon was above the horizon at dawn, males began singing on average 10 min earlier, if there was a full moon compared with a new moon, resulting in a 67% mean increase in performance period and greater total song output. The lack of a difference between full and new moon dawns when the moon was below the horizon suggests that the observed effects were driven by light intensity, rather than driven by other factors associated with moon phase. Effects of the lunar cycle on twilight signalling behaviour have implications for both pure and applied animal communication research.

scholarly journals Genetic diversity of Clarias anguillaris from the Bakoye River in Mali

2021 ◽  
Vol 1 (2) ◽  
pp. 145-152
Author(s):  
Ramata Diop ◽  
Adama Konate ◽  
Rokiatou Fane ◽  
Nanourou Dembele ◽  
Sognan Dao ◽  
...  
Keyword(s):  
Genetic Diversity ◽  
Polymorphism Information Content ◽  
Fish Farming ◽  
River Basins ◽  
Species Group ◽  
Senegal River ◽  
Expected Heterozygosity ◽  
Group I ◽  
Hardy Weinberg Equilibrium ◽  
The Mean

Clarias anguillaris is a wild species found in River basins in Mali. It is the species most commonly used in fish farming in community stockings. However, it excites little study on the genetic diversity of this species in the natural environment in Mali. The present study focused on the genetic diversity of Clarias anguillaris from the Bakoye River, a tributary of the Senegal River in Mali. A total of (8) microsatellite markers were applied to 47 samples taken at random from the River. The markers were Cga02, Cga03, Cga06, Cga10, Cba11, Cba19, Cba20 and Cma12. The number of alleles, the number of genotype, genetic diversity, Polymorphism Information content (PIC), observed and expected heterozygosity were determined. The results showed that the number of alleles ranged from 1 to 7, with an average of 4.25 per locus. The mean rate of observed heterozygosity was 0.34 lower than that of expected heterozygosity which was 0.48 indicating nonconformity of the Hardy-Weinberg equilibrium. The allele frequency ranged from 0.35 at the Cba19 locus to 1 at the Cba11 locus, with a mean of 0.62. Genetic diversity ranged from 0 for Cba11 to 0.75 for Cba19. The markers Cga02, Cga03, Cga06, Cba19, Cba20 and Cma12 were polymorphic with an average peak of 0.42. The phylogenetic tree presented two groups of genotypes showing diversity within the species. Group I comprised 60.42% of individuals and group II presented 39.58% with 3 subgroups (A, B and C). The genetic distance (0.05) indicates little differentiation between individuals.

scholarly journals Plankton population and physico-chemical properties of a lake of Jahangirnagar University campus, Bangladesh at various lunar rhythms

2016 ◽  
Vol 4 (2) ◽  
pp. 31-36
Author(s):  
Most Fahima Ahmed Anny ◽  
Ismot Ara
Keyword(s):  
Full Moon ◽  
Chemical Properties ◽  
Abundant Species ◽  
Lunar Cycle ◽  
Moon Phase ◽  
University Campus ◽  
Physico Chemical ◽  
Free Carbon Dioxide ◽  
New Moon ◽  
Abundant Phytoplankton

Planktonic biomass and physico-chemical properties of water from a lake at Jahangirnagar University, Bangladesh were studied during new moon, first quarter, full moon and last quarter phases from 16th June to 15th July 2015. Twenty four species of phytoplankton belonging to Chlorophyceae, Bacillariophyceae and Euglenophyceae were recorded. Maximum abundance (162-301 unit/l) of Chlorophyceae was recorded in first quarter phase followed by full moon phase (112-224 unit/l), new moon phase (85-222unit/l) and last quarter phase (60-125 unit/l), respectively. Chlorella vulgaris and Biddulphia aurita were the most abundant phytoplankton throughout the lunar period. Among the zooplankton, 5 species of Protozoa, 2 species of Rotifer, 3 species of Cladocera and 1 species of Ostracoda were recorded. Highest zooplankton was recorded in full moon phase (54-105 unit/l) and Daphnia cephalata was the most abundant species throughout the lunar cycle. Physico-chemical parameters indicate that the water temperature, colour, odour and pH were almost similar throughout the lunar cycle, whereas maximum dissolved oxygen (7.16 mg/l) and minimum (4.43 mg/l) were found during the last quarter and the full moon phase, respectively. The highest content of free carbon dioxide (4.36 mg/l) and chloride (22.8 mg/l) were recorded during first quarter and full moon phase accordingly.Jahangirnagar University J. Biol. Sci. 4(2): 31-36, 2015 (December)

scholarly journals Study the variation of synodic month for the moon through 2000-2100

2019 ◽  
Vol 14 (29) ◽  
pp. 138-144
Author(s):  
Abdul Rahman H.S.
Keyword(s):  
Research Study ◽  
The Moon ◽  
The Earth ◽  
The Mean ◽  
New Moon ◽  
The Moment ◽  
The Relationship

In this research study the synodic month for the moon and theirrelationship with the mean anomaly for the moon orbit and date A.Dand for long periods of time (100 years), we was design a computerprogram that calculates the period of synodic months, and thecoordinates of the moon at the moment of the new moon with highaccuracy. During the 100 year, there are 1236 period of synodicmonths.We found that the when New Moon occurs near perigee (meananomaly = 0°), the length of the synodic month at a minimum.Similarly, when New Moon occurs near apogee (mean anomaly =180°), the length of the synodic month reaches a maximum. Theshortest synodic month on 2053 /1/ 16 and lasted (29.27436) days.The longest synodic month began on 2008 /11/ 27 and lasted(29.81442) days. The mean synodic month (29.53109) days. Wefound the relationship between synodic month with months. Theshortest synodic month are correlated with date (June and July) whenthe Earth is near aphelion. And the longest Synodic month arecorrelated with date (December and January) when the Earth is nearperihelion.

scholarly journals Secular pattern of aneurismal rupture with the lunar cycle and season

2016 ◽  
Vol 23 (1) ◽  
pp. 60-63 ◽  
Author(s):  
Jillian C Banfield ◽  
Mohamed Abdolell ◽  
Jai S Shankar
Keyword(s):  
Intracranial Aneurysm ◽  
Intracranial Aneurysms ◽  
Full Moon ◽  
Lunar Cycle ◽  
Aneurysm Rupture ◽  
Endovascular Coiling ◽  
The Moon ◽  
Moon Phases ◽  
Ruptured Intracranial Aneurysm ◽  
New Moon

Background The lunar cycle and seasons may be associated with rates of rupture of intracranial aneurysms, but the literature is mixed. Studies of the association between the lunar cycle and rates of aneurysm rupture used the eight qualitative moon phases. The purpose of this study was to assess any association of aneurysm rupture with the lunar cycle and with the season. Materials and methods We retrospectively reviewed all cases of subarachnoid haemorrhage secondary to ruptured intracranial aneurysm treated with endovascular coiling in our institution over a 10-year period. We included only cases with a known rupture date. We used the degree of illumination of the moon to quantitatively code the lunar cycle. Results A total of 212 cases were included in our analyses. The odds of aneurysm rupture were significantly greater ( p < 0.001) when the moon was least (new moon) and most (full moon) illuminated, as compared to the middle of the lunar cycle. The odds of rupture tended to be higher ( p = 0.059) in the summer, compared to autumn. Conclusions The odds of aneurysm rupture were greater when the moon was least illuminated (new moon) and most illuminated (full moon), compared to the middle of the lunar cycle.

The motion of a lunar orbiter

1966 ◽  
Vol 25 ◽  
pp. 373
Author(s):  
Y. Kozai
Keyword(s):  
Degrees Of Freedom ◽  
Dimensional Space ◽  
Artificial Satellite ◽  
Equations Of Motion ◽  
Triaxial Ellipsoid ◽  
The Moon ◽  
Secular Motion ◽  
The Earth ◽  
Close Satellite ◽  
The Mean

The motion of an artificial satellite around the Moon is much more complicated than that around the Earth, since the shape of the Moon is a triaxial ellipsoid and the effect of the Earth on the motion is very important even for a very close satellite.The differential equations of motion of the satellite are written in canonical form of three degrees of freedom with time depending Hamiltonian. By eliminating short-periodic terms depending on the mean longitude of the satellite and by assuming that the Earth is moving on the lunar equator, however, the equations are reduced to those of two degrees of freedom with an energy integral.Since the mean motion of the Earth around the Moon is more rapid than the secular motion of the argument of pericentre of the satellite by a factor of one order, the terms depending on the longitude of the Earth can be eliminated, and the degree of freedom is reduced to one.Then the motion can be discussed by drawing equi-energy curves in two-dimensional space. According to these figures satellites with high inclination have large possibilities of falling down to the lunar surface even if the initial eccentricities are very small.The principal properties of the motion are not changed even if plausible values ofJ3andJ4of the Moon are included.This paper has been published in Publ. astr. Soc.Japan15, 301, 1963.

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