International Journal for Quality Research 11(3) 717–728
ISSN 1800-6450
Tadeja Jere Jakulin 1
Rudi Čop
Article info:
Received 06.03.2017
Accepted 12.07.2017
UDC – 91
DOI – 10.18421/IJQR11.03-14
SUNSPOT CYCLES IMPACTS ON TOURISM
AND QUALITY OF LIFE
Abstract: We live under the influence of natural cycles caused
by the rotation of our planet and its revolution around the sun.
The nature of our nearest star is also subject to cyclical
change. This article presents a study of a correlation between
sunspot cycles and foreign tourists arrivals in Slovenia, based
on historical data between sunspot cycles and sea salt
production in Slovenia’s Municipality of Piran during the
Maunder Minimum period (1645–1715). The production of
salt by the solar evaporation of brine in salt pans and tourist
industry are seasonal economic activities that are affected by
changes to the weather. The paper looks at sea salt production
in Piran during a particular period in the past. The repetition
of the sea salt production in the past is not possible. For this
reason, the study uses mathematical tools and an additional
case study, which analyses arrivals of foreign tourists to
Slovenia over the past 65 years (1948–2012). The study has
two purposes: to identify a linear correlation coefficient, which
provides evidence of a correlation between arrivals of foreign
tourists to Slovenia and sunspot cycles and to develop a causal
loop diagram (CLD) or so called qualitative model of a
complex tourism system, which shows the interdependency of
sunspot cycles, tourism system, and quality of life.
Keywords: sunspot cycles, Maunder minimum, foreign
tourist arrivals, CLD modelling, quality of life
1. Introduction1
The theoretical assumptions underlying this
study stem from the results of data, operating
in a reverse fashion when compared with
traditional research. Our assumptions, based
on these data, used inductive reasoning
(Cassell & Symon, 2004; Heath & Cowley,
2004). With inductive reasoning, the theory
should more or less match the data, be
relevant to it and it should be possible to
1
Corresponding author: Tadeja Jere Jakulin
email: tadeja.jerejakulin@upr.si
work with and modify the theory according
to new data or newly organised data sets. As
with all scientific research, any theoretical
assumptions derived from data should be
provable and repeatable (Kennett, 2014).
From the outset, such assumptions should be
internally consistent, coherent and without
error. In the process of building a theory,
additional research on similar examples
helps in the formulation and validation of the
theory, and in the identification of any
contradictions that might otherwise lead to
unrealistic results. Such a treatment enables
mathematical modelling and the use of
scientific methods. It is a form of
717
epistemology, which is the theory of
knowledge (Moglia et al., 2011; Hoda et al.,
2012).
The research described in this article bases
on data from various archives. As the
phenomena occured in the past, they are
unique, and any repetition is impossible. We
extracted periodic events from these
phenomena, which occurred in twelve-year
cycles. From these results, we established a
theory that seasonal economic activities,
which are influenced by changes in the
weather, are also affected by sunspot cycles.
The basic research idea arouses from the
curiosity and the wish for greater
understanding. We anticipate that the results
of the research will provide useful
knowledge on how to make long-term
predictions for seasonal economic activities.
These long-term predictions are more
convenient for managing processes and their
regulation than providing a complete
analysis of all the factors that contribute to
the success of these economic activities
(Adolpha et al., 2012; Dunne, 2011). The
most important processes comprise key
decisions at the highest level of management
together with staff education and experience.
2. Sunspots
The existence of spots on the sun and their
variation knew the scholars in the antique
time. Sunspots had been observed and
described more than two thousand years
before the invention of the telescope. Their
appearance correlated with changes in the
weather (Galilei & Scheiner, 2010). The
introduction of the telescope to astronomy at
the beginning of the seventeenth century
changed astronomical observations forever
and also accelerated the development of
optics and epistemology. The telescope was
used to observe and describe the heavenly
bodies, the moon, the sun and its sunspots.
The discovery of sunspot cycles at the
beginning of the nineteenth century was one
of the most important discoveries in
718
astronomy (Arlt, 2011). All our knowledge
about the nature of the sun, which directly
affects the earth and life on it, is a result of
that discovery. From a combination of
sunspot numbers and their distribution on the
solar disc in the past 150 years, it follows
that the maximum number of solar activities
repeated between every 9.5 and 11 years.
Wolf’s number is another name for this
repeating period (Clette, 2007). These cycles
take too long to impinge directly on our
everyday life. As a result, we either fail to
notice their influence or simply forget it. The
identification of the nature of sunspots
started at the beginning of the twentieth
century. They appear because of an anomaly
in the sun’s magnetic field (Hale et al.,
1919). Later on Milanković published his
calculations on the temperature at different
points on the surface of Earth at different
times of year from axioms, or first principles
in Théorie mathématique des phénomènes
thermiques produits par la radiation solaire
(Mathematical
Theory
of
Thermal
Phenomena Caused by Solar Radiation). The
calculations gave results that were roughly in
line with empirical data concerning early
20th-century temperatures,
and they
immediately attracted the attention of
meteorologists. Together with astronomer
Köppen
and
geophysicist
Wegener,
Milanković presented the effect of known
regular changes in three astronomical
parameters: the obliquity (tilt) of Earth’s axis
of rotation, the precession (wobblelike
movement) of the rotation axis, and the
eccentricity (a measure of the elliptical
shape) of Earth’s orbit around the Sun.
Those three parameters govern the amount
of solar radiation (insolation) that strikes
Earth’s surface at different latitudes in
different seasons. Because they operate on
different timescales, the parameters affect
climate by interacting in a manner that
sometimes
increases
and sometimes
decreases the insolation at a particular
location (Macdougal 2014, Milanković,
1941).
T. Jere Jakulin, R. Čop
At the time of the Maunder Minimum, the
observation of the sun was 68% (± 7%) of
available days (Hoyt & Schatten, 1996).
During that period appeared the sunspots
notification and the observation of few polar
lights, which reinforces the existence of the
Maunder Minimum. Radioactive isotopes
produced by cosmic rays in the upper layers
of the atmosphere are a confirmation of its
existence in the past. Deposits of
cosmogenic carbon-14 and beryllium-10
were particles in the remains of living bodies
and in Antarctic ice (Beer, 2000).
In this article, we used yearly sunspot
numbers from two different sources: the
estimated numbers for the period from 1610
to 1700 (National Geophysical Data Center
(NOAA), 2007) and the average numbers of
sunspots since the year 1700 (SILSO, 2014).
These verified and systematically arranged
data sets were used to calculate a linear
correlation coefficient with data sets from
two local commercial activities that are
seasonally affected: sea salt production in
Piran during the time of the Maunder
Minimum and arrivals of foreign tourists to
Slovenia between 1948 and 2012.
3. Historical data - maunder
minimum in Piran
Studies about possible connections between
space weather and storms in earth markets
numbers are more than 300 years old
(Jonathan Swift, 1726, William Hershel,
1801, William Jevons, 1878) The Republic
of Venice (Serenissima Repubblica di
Venezia) lasted from the 7th century until
1797. Initially, fishing and salt production
were the main sectors of its economy. The
development of the shipping trade led
indirectly to the development of other
activities. A typical characteristic of
Venetian economic policy was the
unacceptability of a market surplus for any
type of goods. State monopolies were
carefully maintained to ensure steady prices.
The state prohibited the import of goods or
their production to prevent any reductions in
price (Bonin, 2005).
In the thirteenth century, the Senate of the
Venetian Republic appointed a large number
of magistrates, which restricted the authority
of the Doge. An administrative body for salt
was also established (Magistrato sopra i
sali). This body had four overseers, political
appointees held by noblemen for two years
and later 18 months. They issued salt
contracts for the production and trading of
salt for every salt field in the territory of the
Republic. These contracts ensured a state
monopoly over salt in the domain of the
Adriatic Sea. Despite the administrative
restrictions, significant levels of salt
smuggling happened. The overseers received
reports on smuggling, which increased,
especially in those periods when the price of
salt was high (Bonin, 2005). Salt was one of
the most important additions to food since
people used it for food preservation.
The city of Piran, which now lies in
Slovenian Istria, was part of the Venetian
Republic from the end of the thirteenth
century until its decline. The first known salt
contract between the Venetian Republic and
the Municipality of Piran dates from 1375
(Bonin, 2001). Venetian government,
represented by the administrative body for
salt, and the Municipality of Piran,
represented by the Council of Twenty for
Salt (Colleggio dei XX del sal) signed salt
contracts. The Council consisted of twenty
representatives of salt field owners in Piran.
At first, these contracts were valid for five
years. At the beginning of the eighteenth
century, however, this period was extended
to twelve and later increased to fifteen years.
The last salt contract between the Venetian
Republic and Piran, dating from 1780, was
made for 20 years. The main part of these
contracts was the price of salt. In a salt
contract set up in 1636, the yearly limit of
sea salt to be produced in Piran was 5200
modi (a modio is equivalent to 801 kg). This
quantity remained stable for a further 113
years. During this entire period, the amount
of salt produced in Piran changed very little.
A study on possible causal connections
719
between solar activity and wheat prices.
(Pustilnik & Yom Din, 2004), was shown
that a complex causal chain can have taken
place.
Figure 1. Correlation between the price of sea salt in the Republic of Venice and the number of
sunspots during the Maunder Minimum
The Piran Archives include data relating to
the quantities of salt harvested in Piran
(Bonin, 2001; Bonin & Čop, 2008). The
earliest data about salt production are from
1637. The data were regularly recorded until
1685 when their systematic registration
stopped. During this entire period of 48
years, only the data for 1657, 1658, 1663 and
1672 are not available. For the following 70
years, until 1744, there are data for five
separate years and a further two 5-year
periods (1730‒1734 (21,170 modi) and
1735‒1739 (21,327 modi)).
In Piran, salt contracts determined the price
of salt per modio in lire (1 lira veneziana =
1/2 ducato d'oro = 20 soldi = 240 denari)
from 1637 until 1744 (Figure 1). The linear
coefficient of correlation between (Stigler,
1989; Rodgers & Nicewander, 1988) the
price of salt and the average number of
720
sunspots in the observed period is = - 0.53.
The anti-correlation between these two
groups of data means that the price of salt
went up when the number of sunspots was
lower.
4. Foreign tourists arrivals
between 1948 – 2012
In the past 65 years, annual data relating to
the arrivals of foreign tourists have been
taken from different sources and then
arranged by year (Zavod Republike
Slovenije
za
Statistiko
[Slovenian
Department of Statistics], 1971, 1992; 2013).
Slovenian Department of Statistics recorded
extreme events in the data for the period
between 1948 and 2012.
T. Jere Jakulin, R. Čop
Figure 2. Arrivals of foreign tourists to Slovenia from 1948 to 2012
In 1973, a steady increase in the number of
tourists stopped abruptly and, in 1991, there
was a dramatic decrease in the number of
foreign tourists (Figure 2). These events
derived from the political situation in
Slovenia at the time, namely, the result of
political instability in 1973 and the breakup
of Yugoslavia in 1991. The time distance
between these two events is 16 ± one year.
Throughout the entire observed period of 65
years, there were shorter periods of change
with lower amplitudes, with periods of three
to five years and from six to eight years. The
shortest periods of decrease occurred in 1999
and 2009. The data relating to arrivals of
foreign tourists are not as reliable
statistically as data relating to overnight
stays. The political events at that time
influenced the data relating to overnight
stays. A linear correlation coefficient
between the annual numbers of foreign
tourists and annual sunspot numbers in the
past seven sun cycles is = - 0.30 (anticorrelation). As for the numbers of these
cycles in the past 65 years, there is a very
probable correlation in anti-phase.
A detailed analysis of the graph in Figure 3
shows that during the most rapid increase of
sunspot numbers, the number of arrivals of
foreign tourists decreased, and vice versa.
These roughly seven-year cycles had a lower
amplitude between 1948 and 1973 when
arrivals of foreign tourists increased steadily.
We carried out an FFT frequency analysis
(Cooly & Tukey, 1965; Bergland, 1969) of
the available data for the annual numbers of
arrivals of foreign tourist for the period
between 1948 and 2012.
The cyclical events at the 10.83 and 13-year
period points have nearly the same level of
power and coincide with well-known natural
cycles, namely, sunspot and geomagnetic
storm cycles (Cliver, 1994). Each has greater
power than the 16.25 year period point,
caused by the political events in Slovenia at
the time (Figure 4). The 10.84-year period
point is little higher than the average value
of 10.78 year periods for the sunspot cycles
numbered 19 to 23. Sunspot cycle 19 started
in April 1954, and sunspot cycle number 23
ended in January 2008 (SILSO, 2014;
Hathaway, 2015).
721
Figure 3. Correlation between the annual numbers of arrivals of foreign tourists to Slovenia
and sunspot numbers from the eighteenth to the twenty-fourth sunspot cycle
Figure 4. Results of frequency analysis (FFT) of annual arrivals of foreign tourists’ data in
Slovenia from 1948 to 2012
5. Results and CLD model
Comparison of the available data of sea salt
production in the Piran Municipality during
the time of Maunder Minimum with the
estimated data of sunspot numbers during
the same time did not give the expected
722
results (Bonin, Čop, 2008). The raised price
of salt at the time in Venetian Republic
shows a great shortage of this commodity on
the market at that time.
The linear correlation between the salt
production in the Piran Municipality and the
sunspot numbers during the time of Maunder
T. Jere Jakulin, R. Čop
Minimum does not exist. Also, other types of
correlations did not give any useful results
(Paliska et al., 2015) mainly for the lack of
continuous data. Behind the deficiency of
adequate data, the same question crops up as
it appears to the collector of data of
production: Are the data of salt production in
the Piran Municipality at the time of
Maunder Minimum correct? Between 1994
and 1997 the salt production was organized
in the Piran salt pans of the same dimensions
as those during the seventeenth century. The
harvest of sea salt was from 3.1 modi per salt
pan in the rainy year to 6.2 modi per salt pan
in the year with good weather conditions.
However, during the time of Maunder
Minimum, this production was limited by a
Salt Contract to 2 modi per salt pan (Bonin,
2001).
To obtain the expected results and to check
the data sets more easily we used the data
relating to the arrival of foreign tourists in
Slovenia for the past sixty-five years (19482012) for additional verification of linear
correlation with annual sunspot numbers.
The result of this mathematical operation is a
linear anti-correlation coefficient = - 0.30.
In parallel measurements with the same type
of magnetometers, but with different serial
numbers, in two neighboring observatories
on four successive geomagnetic very calm
days, the reckoning linear correlation
coefficients are ranging from = 0.81 to =
0.93 with the average value of = 0.85 (Čop
et al., 2011). The value of this correlation
significantly drops if the observatories are on
different geographic latitudes and longitudes,
and they can also reach negative values.
These measurements have something in
common; they represent the flux of energy
from the Sun to the Earth’s magnetosphere.
Following the results of the research and the
newest data of spectral analysis, we will
build a diagram – a model, which will serve
as a describer of the activity of basic mutual
influences among variables. We will use
systems methodology, which is due to its
transparency an excellent tool for modelling
of complex systems. Causal-loop (CLD)
model is a mental model, which is the basis
of causal connections among model
variables: sunspot cycles, tourists’ arrivals,
investments to tourism, tourism market,
science & research, and quality of life. We
present it in figure 5. Model is only a
graphic presentation of a real system, which
consists of elements and is greater than its
parts. If we connect the set of system’s
elements on the basis of their descriptions,
with arrows pointing in the same direction,
and denote them with the symbol (+)
opposite the symbol (-), we create an
influential diagram. We build a causal loop
diagram where we label a link polarity by
adding ‘+’ or a ‘–’ sign at each arrowhead to
convey more information. A ‘+’ is used if
the cause increase, the effect increases and if
the cause decrease, the effect decreases. A ‘’ is used if the cause increases, the effect
decreases and if the cause decreases, the
effect increases (Jere Jakulin, 2017).
Building causal-loop diagram has a strategic
meaning. It shows correlations among
parameters, which are important when we
want to show how the system in reality
works and what could be a strategy for its
development in the future. It is a good
presentation for decision-makers, who
become aware of correlations among
parameters of a model in our case aware of
the power of sunspot cycles. Thus, they can
develop a strategy and anticipate time for the
investments. The behavior of the model in
figure 5 is as follows: sunspot cycles
increase tourists’ arrivals (+), which
positively influence the investments (+),
increase mass tourism (+) and decrease (-)
attractiveness of the area. Area attractiveness
increases (+) tourism market, which
increases (+) science and research activities.
These influences (+) area attractiveness,
which gives positive feedback (+) to science
and research and quality of life. Quality of
life positively affects (+) science and
research and this increases (+) knowledge
about solar activities- sunspot cycles.
723
Figure 5. Causal loop diagram (CLD) of interdependency between sunspot cycles, tourists’
arrivals investments, area attractiveness, and quality of life
Above described interdependency among
elements of a complex tourism system
presents system dynamics as a methodology
for solving complex systems problems.
According to Sterman (Sterman, 2000),
system dynamics is:
A. Methodology for understanding
complex problems where there is
dynamic behaviour (quantities
changing over time) and where
feedback impacts significantly on
system behaviour.
B. Framework and rules for qualitative
description,
exploration
and
analysis of systems regarding their
processes, information, boundaries
and
strategies,
facilitating
quantitative simulation modelling
and analysis for the design of
system structure and control.
C. Rigorous study of organisational
problems, from a holistic or system
perspective, using the principles of
feedback, dynamics and simulation
(Jere Jakulin, Kljajić, 2006).
724
5. Conclusions
After the frequency analysis during the
sixty-five-year period, we see that the power
of influence of solar cycles on the tourist
industry in Slovenia is comparable with the
power of political events. This industry is in
major part a long-term investment,
especially in hotels. For a long-term
planning of this industry, it would also be
very useful to study the influence of solar
cycles on it. Therefore, it would also be
necessary to use adequate data sets from
other
tourism-orientated
countries.
Moreover, the standard verification of
economic efficiency of the tourist industry in
those countries would help in decisionmaking to take seriously into concern the
influence of sunspot cycles upon tourist
arrivals and consequently to rethink
investments to tourism.
There is not only the cycle of sunspot
numbers which the Sun creates. In the time
of its minimum, the circumstances in the
T. Jere Jakulin, R. Čop
space around the Earth are not calm; they are
only changed (Eddy, 2009). In that time the
flux of cosmic rays are bigger which
influence the formation of the clouds
(Svensmark, 2000, National Academies,
2011). The Sun with its activity also directly
influence on the health of the people (Palmer
et al., 2006) and the nowadays technology
(Čop, 2015). All these phenomena change
our way of life and also change the direction
and intensity of tourist’s currents flow. To
present this practically, we used a systems
methodology. System dynamics enhances
learning in complex systems, which features
are in a quantity of parameters tightly
interconnected and interdependent: such as
tourism, economy, industry, science, Sun. It
is a method for developing management
flight simulators, often computer simulation
models, to help us learn about dynamic
complexity, understand the sources of policy
resistance, and design more effective
policies. With a causal-loop diagram, which
we build in a frame of system dynamics, we
presented correlations among elements
described in this study and the elements that
are important when we research tourism and
quality of life. From this diagram, one can
derive the dynamic equations that are
necessary for a computer simulation. We
showed the equivalence of different
methodologies, whose differences or
similarities can be judged only in context of
a problem and the aims of researches.
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Tadeja Jere Jakulin
Rudi Čop
University of Primorska,
Faculty of Tourism Studies
Obala 11a, Portorož
Slovenia
tadeja.jerejakulin@upr.si
Terra Viva Institute,
Geophysical Observatory
Sv.Peter 115, 6330 Piran
Slovenia
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T. Jere Jakulin, R. Čop