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                <identifier>ezaposleni.singidunum.ac.rs/rest/sciNaucniRezultati/oai:2:9893</identifier>
                <datestamp>2025-01-27T13:46:26Z</datestamp>
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                <dim:dim>
                    <dim:field mdschema="dc" element="title" lang="en">Space Weather and Hurricanes Irma, Jose and Katia</dim:field>
                    <dim:field mdschema="dc" element="date" qualifier="issued">2019</dim:field>
                    <dim:field mdschema="dc" element="identifier" qualifier="uri">http://ezaposleni.singidunum.ac.rs/rest/sciNaucniRezultati/oai/record/2/9893</dim:field>
                    <dim:field mdschema="dc" element="identifier" qualifier="uri">file:///C:/Users/Japan/Downloads/s10509-019-3646-5.pdf</dim:field>
                    <dim:field mdschema="dc" element="contributor" qualifier="author" authority="id:44929" confidence="-1">Y. Vyklyuk</dim:field>
                    <dim:field mdschema="dc" element="contributor" qualifier="author" authority="id:44930" confidence="-1">M. Radovanović</dim:field>
                    <dim:field mdschema="dc" element="contributor" qualifier="author" authority="id:44931" confidence="-1">B. Milovanović</dim:field>
                    <dim:field mdschema="dc" element="contributor" qualifier="author" authority="id:44932" confidence="-1">M. Milan</dim:field>
                    <dim:field mdschema="dc" element="contributor" qualifier="author" authority="id:44933" confidence="-1">P. Marko</dim:field>
                    <dim:field mdschema="dc" element="contributor" qualifier="author" authority="id:44934" confidence="-1">D. Doljak</dim:field>
                    <dim:field mdschema="dc" element="contributor" qualifier="author" authority="id:44935" confidence="-1">S. Miličević-Malinović</dim:field>
                    <dim:field mdschema="dc" element="contributor" qualifier="author" authority="id:44936" confidence="-1">N. Vujković</dim:field>
                    <dim:field mdschema="dc" element="contributor" qualifier="author" authority="orcid::0000-0001-8684-4228" confidence="-1">A. Vujko</dim:field>
                    <dim:field mdschema="dc" element="contributor" qualifier="author" authority="id:44938" confidence="-1">N. Matskiuk</dim:field>
                    <dim:field mdschema="dc" element="contributor" qualifier="author" authority="id:44939" confidence="-1">S. Mukherjee</dim:field>
                    <dim:field mdschema="dc" element="description" qualifier="abstract">This research is devoted to the determination of
the causal relationship between the flow of particles that are
coming from the Sun and the hurricanes Irma, Jose, and Katia.
To accomplish this, the lag correlation analysis was performed.
High correlation coefficients confirmed a preliminary
conclusion about the relationship between solar activities
and the hurricane phenomenon, which allows further research.
Five parameters i.e. characteristics of solar activity
(10.7 cm solar radio flux (F10.7), the flows of protons and
electrons with maximum energy, speed and density of solar
wind particles) were chosen as model input, while the wind
speed and air pressure of Irma, Jose, and Katia hurricaneswere used as model output. Input data were sampled to a six
hours interval in order to adapt the time interval to the observed
data about hurricanes, in the period between September
28 and December 21, 2017. As a result of the preliminary
analysis, using 12,274,264 linear models by parallel
calculations, six of them were chosen as best. The identified
lags were the basis for refinement of models with the
artificial neural networks. Multilayer perceptrons with back
propagation and recurrent LSTM have been chosen as commonly
used artificial neural networks. Comparison of the accuracy
of both linear and artificial neural networks results
confirmed the adequacy of these models and made it possible
to take into account the dynamics of the solar wind. Sensitivity
analysis has shown that F10.7 has the greatest impact
on the wind speed of the hurricanes. Despite low sensitivity
of pressure to change the parameters of the solar wind, their
strong fluctuations can cause a sharp decrease in pressure,
and therefore the appearance of hurricanes.</dim:field>
                    <dim:field mdschema="dc" element="type">article</dim:field>
                    <dim:field mdschema="dc" element="identifier" qualifier="doi">https://doi.org/10.1007/s10509-019-3646-5</dim:field>
                    <dim:field mdschema="dc" element="citation" qualifier="volume">364</dim:field>
                    <dim:field mdschema="dc" element="citation" qualifier="issue">154</dim:field>
                    <dim:field mdschema="dc" element="citation" qualifier="spage">1</dim:field>
                    <dim:field mdschema="dc" element="citation" qualifier="epage">15</dim:field>
                    <dim:field mdschema="dc" element="identifier" qualifier="issn">0004-640X</dim:field>
                    <dim:field mdschema="dc" element="source">ASTROPHYSICS AND SPACE SCIENCE</dim:field>
                </dim:dim>
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