scholarly journals Climate, the Earth, and God – Entangled narratives of cultural and climatic change in the Peruvian Andes

2018 ◽  
Vol 110 ◽  
pp. 345-359 ◽  
Author(s):  
Morgan Scoville-Simonds

2019 ◽  
Vol 55 (1) ◽  
pp. 260
Author(s):  
Constantinos Perisoratis

The climate changes are necessarily related to the increase of the Earth’s temperature, resulting in a sea level rise. Such continuous events, were taking place with minor and greater intensity, during the alternation of warm and cool periods in the Earth during the Late Quaternary and the Holocene periods. However, a particularly significant awareness has taken place in the scientific community, and consequently in the greater public, in the last decades: that a climatic change will take place soon, or it is on-going, and that therefore it is important to undertake drastic actions. However, such a climatic change has not been recorded yet, and hence the necessary actions are not required, for the time being.



1990 ◽  
Vol 17 (4) ◽  
pp. 397-414 ◽  
Author(s):  
Geoffrey O. Seltzer ◽  
Christine A. Hastorf


2007 ◽  
Vol 34 (1) ◽  
pp. 1-9 ◽  
Author(s):  
Nicholas P. Branch ◽  
Rob A. Kemp ◽  
Barbara Silva ◽  
Frank M. Meddens ◽  
Alan Williams ◽  
...  


Author(s):  
K. Anandan ◽  
V.P. Venkatamuthu

The two types of atoms stable and unstable atoms play the major role in the universe. The space consists of majority of stable atoms in controversy to earth consists of majority of unstable atoms. The attraction and repulsion of unstable atom by stable atom produces a torque. This torque depends on temperature and magnetic field. Thus, the earth rotates about itself. Due to the increase of temperature the diameter of earth increases, that decreases the speed and the spinning of earth; causes climatic change.



1976 ◽  
Vol 6 (4) ◽  
pp. 481-493 ◽  
Author(s):  
J. Murray Mitchell

A variance spectrum of climatic variability is presented that spans all time scales of variability from about one hour (10−4 years) to the age of the Earth (4 × 109 years). An interpretive overview of the spectrum is offered in which a distinction is made between sources of variability that arise through stochastic mechanisms internal to the climatic system (atmosphere-ocean-cryosphere) and those that arise through forcing of the system from the outside. All identifiable mechanisms, both internal and external, are briefly defined and clarified as to their essential nature. It is concluded that most features of the spectrum of climatic variability can be given tentatively reasonable interpretations, whereas some features (in particular the quasi-biennial oscillation and the neoglacial cycle of the Holocene) remain fundamentally unexplained. The overall spectrum suggests the existence of a modest degree of deterministic forms of climatic change, but sufficient nonsystematic variability to place significant constraints both on the extent to which climate can be predicted, and on the extent to which significant events in the paleoclimatic record can ever manage to be assigned specific causes.



2017 ◽  
Author(s):  
Sara Manafzadeh ◽  
Yannick M. Staedler ◽  
Hamid Moazzeni ◽  
David Masson ◽  
Jürg Schönenberger ◽  
...  

AbstractSince the Industrial Revolution, human activities have contributed substantially to climate change, by adding CO2to the atmosphere, especially since the mid-20thcentury (the “Great Acceleration”). Climatic change does not have the same impact on different regions of the Earth, neither in the recorded past, nor in models of the future. Therefore, to anticipate on these changes, we need to understand and be able to predict the possible responses of the different regional vegetations of the world to these changes, and most significantly to increased drought conditions. The aim of this study is to understand the response of the xerophytes of the immense oriental Irano-Turanian bioregion to post-industrial global warming and to compare it with the response of the xerophytes of the neighbouring occidental Mediterranean bioregion. We measured stomata index and stomata density from 83 herbarium sheets (coll. 1821-2014) from species of the non-succulent xerophyte,Haplophyllum. We tested for differences before and after the “Great Acceleration” in both bioregions. SI decreased in the occidental species (significant only for abaxial leaf side), whereas SI significantly increased in the oriental species (both sides). We suggest that changes in both occidental and oriental species are linked to atmospheric CO2due to the different constraints that act on their growth. In light-limited occidental species, atmospheric CO2caused the stomata index decrease, whereas in the predominantly water-limited oriental species, increased drought stress and temperature (climatic change) caused stomata index increase. In conclusion, we propose that whereas atmospheric CO2directly caused a decrease in stomata index in occidental xerophytes, it indirectly caused an increase in stomata index in oriental xerophytesviaclimate change (increase in aridity, drought stress, and temperature). This study highlights the considerable potential of research based on historical herbarium collections to answer ecological questions, especially regarding climatic change.



1990 ◽  
Vol 17 (4) ◽  
pp. 397 ◽  
Author(s):  
Geoffrey O. Seltzer ◽  
Christine A. Hastorf


1966 ◽  
Vol 25 ◽  
pp. 373
Author(s):  
Y. Kozai

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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