Academic literature on the topic 'Lunar variations'

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Journal articles on the topic "Lunar variations"

1

Winch, Denis E. "Lunar magnetic variations." Pure and Applied Geophysics PAGEOPH 131, no. 3 (1989): 533–49. http://dx.doi.org/10.1007/bf00876844.

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2

Palumbo, A. "Lunar daily variations in rainfall." Journal of Atmospheric and Terrestrial Physics 48, no. 2 (1986): 145–48. http://dx.doi.org/10.1016/0021-9169(86)90078-4.

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3

Winch, D. E. "Solar and Lunar Daily Geomagnetic Variations." Exploration Geophysics 24, no. 2 (1993): 147–50. http://dx.doi.org/10.1071/eg993147.

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4

Edwards, B. C., J. J. Bloch, D. Roussel-Dupré, T. E. Pfafman, and Sean Ryan. "ALEXIS Lunar Observations." International Astronomical Union Colloquium 152 (1996): 465–70. http://dx.doi.org/10.1017/s0252921100036393.

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The ALEXIS small satellite was designed as a large area monitor operating at extreme ultraviolet wavelengths (130 − 190 Å). At these energies, the moon is the brightest object in the night sky and was the first source identified in the ALEXIS data. Due to the design of ALEXIS and the lunar orbit, the moon is observed for two weeks of every month. Since lunar emissions in the extreme ultraviolet are primarily reflected solar radiation these observations may be useful as a solar monitor in the extreme ultraviolet. The data show distinct temporal and spectral variations indicating similar changes
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5

Zaman, Fahad, Lawrence W. Townsend, Wouter C. de Wet, et al. "Composition variations of major lunar elements: Possible impacts on lunar albedo spectra." Icarus 369 (November 2021): 114629. http://dx.doi.org/10.1016/j.icarus.2021.114629.

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6

TRIVEDI, NB, and RG RASTOGI. "Lunar tidal oscillations in horizontal magnetic intensity at Kodaikanal during periods of low and high sunspots." MAUSAM 20, no. 3 (2022): 235–46. http://dx.doi.org/10.54302/mausam.v20i3.5452.

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The paper describes the lunar daily (L) variations at fixed lunar ages and the lunar monthly (M) variations at fixed solar hours in horizontal magnetic intensity (.H) at Kodaikanal for the low sunspot period, Jan, 1951 to Dec, 1955; and for the high sunspot period Jan. 1956 to Dec, 1960. The lunar daily variations at any of the seasons or solar activity epochs are found to follow Chapman's phase law: L=Cn sin [n~+(.n-2)v+an]. With the increase of solar activity the phase of Ls wave remains constant for each of the seasons, but the amplitude increases during D. and E. months and slightly decrea
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7

Pearce, Steven J., and H. J. Melosh. "Terrace width variations in complex lunar craters." Geophysical Research Letters 13, no. 13 (1986): 1419–22. http://dx.doi.org/10.1029/gl013i013p01419.

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8

McKnight, J. D. "Lunar daily geomagnetic variations in New Zealand." Geophysical Journal International 122, no. 3 (1995): 889–98. http://dx.doi.org/10.1111/j.1365-246x.1995.tb06844.x.

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9

Antonov, Yu V. "ABOUT A POSSIBLE CONNECTION BETWEEN EARTHQUAKES AND LUNAR-SOLAR GRAVITY VARIATIONS." Proceedings of higher educational establishments. Geology and Exploration, no. 3 (June 25, 2018): 51–57. http://dx.doi.org/10.32454/0016-7762-2018-3-51-57.

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A possible correlation between the destructive earthquakes of magnitude M = 7 and above and luni-solar gravity variations between 1975 and 2015 has been analyzed. The lunar-solar variations are characterized by three extreme points: the maximum and minimum values of gravity, and the maximum rate of change of variations. At this time, there is an extreme impact of lunar-solar attraction on the earth’s crust and the Earth as a whole. Variations can be a source of irreversible deformation in the earth’s crust. If in this case, there is an additional external impact of space factors, the probabili
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10

McGee, J. J. "Lunar ferroan anorthosites: Mineralogy, compositional variations, and petrogenesis." Journal of Geophysical Research: Planets 98, E5 (1993): 9089–105. http://dx.doi.org/10.1029/93je00400.

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