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Impact of Solar Activities on Global Temperature | |||||||
Paper Id :
16421 Submission Date :
2022-08-16 Acceptance Date :
2022-08-19 Publication Date :
2022-08-22
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Abstract |
The Energy that drives the Earth’sClimate is undoubtedly provided by the Sun. Thevariations in the intensity of radiation hitting the Earth are quite significant on regional climate but also on a global scale so it is essential to give due importance to natural causes including sunspot activity. The present paper has been structured using significant studies carried out by researchers. It offers statistical approach towards the dramatic changes of the climatecaused by small solar irradiance.
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Keywords | Solar Activities, Natural Causes, Sunspots, Climate Change. | ||||||
Introduction |
1.The Sun-Ultimate source of energy of all the planets including Earth.
Earth is the only place that has all the right conditions for life to exist. The main reason for this is the right spot of Earth to receive the Sun's abundant energy that is needed for proper chemical reaction. The Sun is vital to life on Earth. Its heat influences the environment of all the planets, Moon andComets in our Solar System. Variations in the intensity of solar radiation hitting the Earth may produce changes in global and regional climate which are both different and additional to those from man-made climate change.
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Objective of study | The solar-climate connection has often been disregarded by meteorologists until the late20thcentury. Nowadays computer models of the atmosphere are providing a route to understand this complex process involved. The main objective of this paper is to find a suitable explanation for globally changed climate. |
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Review of Literature | Since 90’s scientific research on climate
change has included multiple disciplines and expanded. FromCharless Grelly
Abott’s theory(1930) that persistently connected the sunspot as a main cause of
climate change to Milutin Milankovitch’s (1950)improved theory of James Crall
with tedious calculations of varying distances and angles of the Sun’s
radiations convinced that sunspot variations were a main cause of climate
change. Early 1970’s also brought claims that far slower variations in the
Earth’s magnetic field correlated with climate, however it failed to convince.
In 1973 Jack Eddy drew attention to a spell of low Carbon-14 and thus high
solar activity. By the early 21st century all the trends in the Sun that could have an influence on the
earth’s climate has been in the opposite direction to that required to explain
the observed rise in global mean temperature. Recent reviews have been
presented by Haigh(2007), Lockwood (2012), Olayinka S. Ohunakin (2015), Jesse
L.Reynlds (2019),Seleshi G. Yalew (2020). |
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Main Text |
Fig.
(1) Earth and Sun The Solar
energy to the Earth is significant even after passing through millions of
kilometers of the Earth’s atmosphere. It is generally considered to
produce a constant amount of power in spite of small variations. Average
radiation that hits the edge of the Earth's atmosphere is known as the Solar
Constant, that varies 7.1% according to the distance of the Earth from the
Sun.There are two main sources of variation in solar radiation. The first one
is the Inter stellar process that affect the radiant energy emitted by the Sun
and the second is the Earth's orbit that directly affect the amount of energy
hitting the Earth and its distribution around the Globe. 2.Effect of
Earth’s Orbit-The solar
energy flux i.e.,total amount of solar energy reaching the Earth in a given
time period depends upon the distance of Earth to the Sun.Seasons exist because
of the elliptical orbit of Earth that varies during the year. As Earth’s axis
is tilted from the direction perpendicular to the plane of its orbits, so when
one pole is tilted towards the Sun at a particular point in the orbit it is
summer in the associated hemisphere and winter in the other hemisphere. Another
parameter that measures the wobble of the Earth’s axis affecting the timing of
the seasons relative to the Earth’s position is the elliptical orbit.On time
scale of many millennia the amount of radiation received at the Earth is
affected by variations in these orbital parameters. The Earth -Sun geometry
play the major role in the variation of magnetic flux.The total solar energy
that hits the Earth is basically depends upon its distance from the Sun and Its
elliptical path. But the distribution radiation over the globe depends on the
tilt & precession. Fig.
(2)The different parameters responsible for solar energy flux. The amount of energy arriving in summer at high latitudes determines whether the winter growth of the ice cap will recede or the climate will be precipitated into an ice age. Changes to the seasonal irradiance, when amplified by other mechanism such as greenhouse gases released by the initial warming can lead to much longer- term shifts in climate regime. Data showing a connection between solar variations and climate are often dismissed as mere correlations since there is no generally accepted theoretical basis to explain these correlations. This is hardly an acceptable position given that the strongest arguments in approval of carbon dioxide in the atmosphere, mostly due to human activities. In the case of carbon dioxide, there is a generallyaccepted mechanism for linking changes in climate to variations in the concentration of this gas since it is an absorber of long wavelength infrared radiation and simple dimensional radiative equilibrium model illustrates the connection. It is defined as the change in net downward radiative flux at the troposphere resulting from any process that acts to perturb the climate system and measured in w/m2. It
is convenient to characterize the response of the Earth’s surface and
troposphere to a radiative perturbation after the stratosphere has come to
thermal equilibrium considering the case of carbon dioxide, labeled as “the
most important” greenhouse gas. Fig. (3) Daily
average solar radiation (Wm-2) entering the top of the atmosphere as a function
of time, year and latitude. If we increase the carbon dioxide by a factor of two
it does not double the amount of infrared radiation absorbed by this. The reason
for this is the position of carbon dioxide absorption bands relative to the
earth’s emission spectrum CO2 has three absorption bands at
wavelength of 4.25, 7.52 and 14.99 microns. The Earth’s emission spectrum peaks
at b/w 15 and 20 microns and falls off rapidly with decreasing wavelength.As a
result, the CO2 absorption band at 4.26 and 7.52 microns absorb
negligible amounts of thermal radiation compound to the band at 14.99
microns.Accordingly adding more carbon dioxide to the atmosphere would
contribute nothing to greenhouse gas effect.However, 14.99-micron band is
essentially saturated so additional carbon dioxide may have some disturbance at
the edge of the band. Because of this marginal effect, the change in forcing
due to a change in carbon dioxide concentration is proportional to the natural
logarithm of the fractional change in concentration of this gas. ΔF=
α/n(c/co) Where c is the
concentration of carbon dioxide at the time c0 is the
concentration at a given reference time and is the sensitivity of the
climate to changes in carbon dioxide concentration.The approximation is valid
in the range of practical interest therefore the earth’s temperature is
relatively insensitive to changes in carbon dioxide concentrations. 3.Solar
Influence on Surface Climate - Climate variability and climate change depends crucially on the existence and accuracy of records of meteorological parameters. That would consist of long time series of measurements made by well calibrated instruments located with high density across the globe. But measurements with global coverage have only been made since the start of the satellite era just about thirty years ago. Fig (4)- The most recent
activity of solar cycle. A key concern of contemporary climate science is to attribute causes, including the contribution of solar variability to the observed variations in temperature. Many approaches have been used but the simplest is to calculate the correlation of the time series of the temperature with that of the factor of interest, another approach is that of multiple linear regression analysis which seeks to drive simultaneously the magnitudes of signals due to a number of pre-determined factors. If the known uncertainties in both the data and the forcing factors are taken into account the result can be improved. (a) Millennial Time Scale-On long time scales changes in the earth’s orbit as well as variations in solar activity must be considered. Fig. (4) shows how interglacial periods tend to be associated with higher irradiance in summer high latitudes and also how the recovery from a cold period proceeds much faster than the rate at which it originally developed. This is probably due to a feedback effect whereby an initial warming is amplified by the release of the natural greenhouse gases. In this case the initial warming is assumed due to an increase in solar irradiance. Fig-(5)Temperature
deduced from18O records in air bubbles trapped in the Vostok ice core. (b) Centennial Time Scale-On these timescales, long term changes in the Earth’s orbit may be disregarded. Fig (5) presents reconstructions of the Northern Hemisphere surface temperature record over the past centuries. In long term variability, it is clear that current temperature is higher than the past two millennia climate change records suggests that the climate has been changing over the past century include the retreat of mountain glaciers, sea lever rise, thinner Arctic ice sheets and an increased frequency of extreme precipitation events. Fig (6) Temperature
change with the passing of years. Different factors in the past century affecting the climate are
represented in fig (2). This suggests
that the sun may have introducean overall global warming approximately 0.070 C
before 1960 but had little effect, since than studies using other solar indices
have produced a larger signal of temperature increase before mid-century and a
better match between observations and regressions model during that period. Confirmation of
hypotheses and validation of models can only be obtained by the
continuingacquisition of long term, well-calibrated measurements of atmospheric
properties including temperature, cloud properties and ozone concentration with
sufficient spatial and temporal resolution. These need to be acquired as along
side properly calibrated solar spectral data. |
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Conclusion |
Modern satellite observations revolutionized understanding of how the Sun and Earth are changing and the linkages between them. Recognition that Earth might be changing because of human activities galvanized the acquisition of sustained, coordinated, validated space-based observations of the Sun and the Earth that continues today.Attributing warming of the globe to increasing concentrations of greenhouse gases necessitates knowledge of the Sun’s total radiative output, which heats the Earth, also changes. Detecting and understanding how chloro-fluorocarbons released into the atmosphere depute Earth’s protective ozone layer which necessitates knowledge of how solar ultra violet irradiance, which both produces and destroys ozone also changes.
It is a challenge to communicate the simultaneous limitations and potential of the changing Sun to change Earth’s climate and atmosphere and the complexity of the connection. Many researchers consider the sun to be a major cause of climate change while other insist that its influence is negligible. The most optimistic avenue for communicating connections between the changing Sun and Earth’s climate and atmosphere is to observemodel and project the ongoing changes with sufficient fidelity to alleviate uncertainty as to their extent and impact. |
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Suggestions for the future Study | Understanding the role of solar variability in solar activity is essential to the interpretation of past climate and for the prediction of the future. Solar activities changes might also play an important role in regional climate that we need to understand in the context of informing climate adaptation efforts. | ||||||
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