SlideShare a Scribd company logo
Advances in Physics Theories and Applications www.iiste.org
ISSN 2224-719X (Paper) ISSN 2225-0638 (Online)
Vol.22, 2013
10
Correlative Analysis of Long Term Cosmic Ray Variation in
Relation with Sunspot Number
UMA PANDEY
Department of Physics, MVM, Bhopal-462003 (M.P.)
Contact No: 07697312643 Email: uma.pandey185@gmail.com
MAHENDRA SINGH
Department of Physics, MVM, Bhopal-462003 (M.P.)
Contact No: 09425608307 Email: asbplin@rediffmail.com
PANKAJ K. SHRIVASTAVA
Department of Physics Govt. Model Science College ,Rewa(M.P.)-486001
Contact No: 09893328379 Email:pankaj_in_2001@rediffmail.com
Abstract
In this paper we will study about the relation between Cosmic ray Intensity(CRI) and Sunspot Number for solar
cycle 22, 23 and 24.For this we have taken the data of cosmic ray intensity from various neutron Monitor
stations .These neutron monitor stations are well maintained stations and provide reliable cosmic ray data for
variation study. A detail correlative study have been done by running cross correlation method. The cosmic ray
intensity and sunspot number shows high and negative correlation among themselves. Sunspot number shows
anti phase with Cosmic ray Intensity (CRI).
Keywords:- Cosmic –ray; Solar Cycle; Solar activity; Sunspot number
Introduction
In the past a lot of work has been done to correlate the solar parameters with cosmic ray intensity on long term
basis. In the recent past two ideas have motivated much to modulation research.The first originally proposed by
Lockwood (1960), is that the long term modulation of cosmic ray intensity i.e. 11 year variation result from
pileup of individual intensity decreases caused by shock’s and other disturbance in solar wind. The second major
idea is that gradient end curvature drifts, long neglected in theories of modulation may be significant and in some
cases dominant in governing the modulation of cosmic rays [1-3]. Generally sunspot numbers have been used as
a representative of solar activity index for various studies. Solar terrestrial relationships provide an important
factor to explain the aspects of the 11 and 22 year variation of galactic cosmic ray.The 11 year variation in
Cosmic ray Intensity observed on the earth is anti-correlated with sunspot number[4-5]. The Cosmic ray
Intensity curve follow a 22 year cycle with alternate maxima being flat topped and peaked as predicted by
models of Cosmic ray modulation based on the observed reversal of the sun’s magnetic field polarity after
every 11 year and curvature and gradient drifts in the large scale magnetic field of the heliosphere[6-10]..In this
paper we have made an attempt to derive the correlation between Sunspot number and Cosmic ray Intensity for
solar cycle22, 23 and 24.The solar cycle 22 have been started in the September 1986 and ended in the year
1996(May). The solar cycle 23 lasted in 12.6 years, beginning in May 1996 and ending in December 2008. The
maximum smoothed sunspot number (monthly number of sunspots averaged over a twelve-month period)
observed during the solar cycle 23 was 120.8, and the minimum was 1.7. There were a total of 805 days with no
sunspots during this cycle.[11]
METHOD OF ANALYSIS
In this paper we will find the correlation between Cosmic ray intensity and solar parameter sunspot number for
solar cycle22, 23 and 24(incomplete) .For this monthly mean values of sunspot number (Rz) are taken from the
Solar Geophysical Data books. The pressure corrected monthly mean value of cosmic ray data of Moscow,
Russia (Cutoff Rigidity=2.42GV) neutron monitor station have been taken for analysis. In this paper we will also
make comparative study of solar cycle 22, 23 and 24.
RESULTS AND DISCUSSION
Solar activity rises and falls with a period of about 11 years .The number of sunspots indicates the level of solar
activity. The emissions of matter and electromagnetic fields from the sun increases during high solar activity,
making it harder for Galactic Cosmic Ray to reach the earth. Cosmic ray intensity is lower when solar activity is
high and vice versa. The long term modulation of cosmic ray intensity has been studied by several scholars in
relation with sunspot number, and a high negative correlation is found between them. The fig.3 shows
correlation between sunspot number and Cosmic ray intensity(CRI) for solar cycle 22, 23 and 24(incomplete).
Advances in Physics Theories and Applications www.iiste.org
ISSN 2224-719X (Paper) ISSN 2225-0638 (Online)
Vol.22, 2013
11
Figure 1 & 2 shows the linear plot of Sunspot number and Cosmic ray intensity with year. From fig.3&4 it is
clear that sunspot number and CRI are anti- correlated. Following conclusions can be drawn:
1) The solar 22 started in September 1986 and ended in May 1996.The total length of cycle 22 is 9.7 years. The
solar cycle 23 started in May 1996 and ended in December 2008 and total length of cycle is 12.6 yrs. Thus solar
cycle 23 is longer than solar cycle 22.The solar cycle 24 has started in the year 2008( December ) and is
incomplete.
2) The solar activity of solar cycle 22 shows increasing phase from 1986 to 1989 and then decreasing phase from
1989 to 1996.At the same time Cosmic ray intensity(CRI )decreases for the period 1986-1991 and shows
increasing phase from 1991 to 1996.Thus from the figure it is clear that as sunspot activity increases ,at the same
time Cosmic ray intensity (CRI) decreases. Thus both sunspot number and cosmic ray intensity shows anti-phase
with each other.
3) The solar activity of solar cycle 23 shows increasing phase from 1996 to 2000 and then decreasing phase from
2000 to 2008.At the same time CRI decreases for the period 1996-2000 and shows increasing phase from 2000
to 2008.Thus it is clear from fig 3. that for cycle 23 also sunspot activity and Cosmic ray intensity(CRI) are anti-
correlated.
4) The solar cycle 24 has started in the year 2008(Dec) and is incomplete. But it seems to be that solar cycle 24
is weaker in solar activity as comparison to cycle 22 and 23.
5)From fig.4 the correlation coefficient between sunspot number and Cosmic ray intensity (CRI) for solar cycle
22,23 and 24 is found to be -0.90057 which is highly negative correlated.
References
[1] Lockwood,J.A.,1960,J Geophysics.Res, 65,19
[2] Webber W.R. and Lockwood JA.,1988, Journal of Geophysical research,93 ,8735
[3] Sharma,N.I.,29th
International Cosmic ray Conference Pune ,2005,00, 101-104
[4] Forbush, S.E. 1954, J. Geophys. Res.,59,525
[5] Forbush,S.E. 1958, J. Geophys. Res.,63,651
[6] Dorman I V & Dorman L I, 1967,J Geophys Res(USA) ,72,1513
[7] Jokipii,J.R.,Thomas, B.T. 1981,Astrophys.. J.,243,1115
[8] Jokipii, J.R.,Levy, E.H.,Hubbard,W.B. 1977,Astrophys. J.,213,861
[9] Nagashima K & Morishitha I,Proc of 16th
ICRC, 1979,Tokyo,Japan,.3 ,325
[10] Gupta Meera,Mishra,V.K.,Mishra A.P. June 2006,Indian Journal of Radio
and space Physics, 35,167
[11] Solar Cycle 23 Wikipedia free encyclopedia
Advances in Physics Theories and Applications www.iiste.org
ISSN 2224-719X (Paper) ISSN 2225-0638 (Online)
Vol.22, 2013
12
Graphs:
Fig:1 Year Vs average yearly values of sunspot number(Rz) for solar
cycle 22,23 and 24
Fig:2 Year Vs average yearly values of Cosmic Ray Intensity(Moscow Neutron Station)
for solar cycle 22,23 and24
Advances in Physics Theories and Applications www.iiste.org
ISSN 2224-719X (Paper) ISSN 2225-0638 (Online)
Vol.22, 2013
13
Fig:3 Shows cross-plot curve between yearly value of sunspot number(Rz)
and Cosmic Ray Intensity (Moscow Neutron Station) for solar cycle 22,23
and24
Fig:4 Shows Correlation curve between yearly value of sunspot number(Rz) and
Cosmic Ray Intensity(CRI) for solar cycle 22,23 and24
This academic article was published by The International Institute for Science,
Technology and Education (IISTE). The IISTE is a pioneer in the Open Access
Publishing service based in the U.S. and Europe. The aim of the institute is
Accelerating Global Knowledge Sharing.
More information about the publisher can be found in the IISTE’s homepage:
http://www.iiste.org
CALL FOR JOURNAL PAPERS
The IISTE is currently hosting more than 30 peer-reviewed academic journals and
collaborating with academic institutions around the world. There’s no deadline for
submission. Prospective authors of IISTE journals can find the submission
instruction on the following page: http://www.iiste.org/journals/ The IISTE
editorial team promises to the review and publish all the qualified submissions in a
fast manner. All the journals articles are available online to the readers all over the
world without financial, legal, or technical barriers other than those inseparable from
gaining access to the internet itself. Printed version of the journals is also available
upon request of readers and authors.
MORE RESOURCES
Book publication information: http://www.iiste.org/book/
Recent conferences: http://www.iiste.org/conference/
IISTE Knowledge Sharing Partners
EBSCO, Index Copernicus, Ulrich's Periodicals Directory, JournalTOCS, PKP Open
Archives Harvester, Bielefeld Academic Search Engine, Elektronische
Zeitschriftenbibliothek EZB, Open J-Gate, OCLC WorldCat, Universe Digtial
Library , NewJour, Google Scholar

More Related Content

PDF
Öncel Akademi: İstatistiksel Sismoloji
PDF
Effect of Solar Variability on the Helioshphere and Cosmic Rays
PPT
Ii 3 magn_mooney
PDF
Magnetic interaction of_a_super_cme_with_the_earths_magnetosphere_scenario_fo...
PDF
Proper-motion age dating of the progeny of Nova Scorpii ad 1437
PDF
Four new planets_around_giant_stars_and_the_mass_metallicity_correlation_of_p...
PDF
Streamer waves, final version
PDF
Exocometary gas in_th_hd_181327_debris_ring
Öncel Akademi: İstatistiksel Sismoloji
Effect of Solar Variability on the Helioshphere and Cosmic Rays
Ii 3 magn_mooney
Magnetic interaction of_a_super_cme_with_the_earths_magnetosphere_scenario_fo...
Proper-motion age dating of the progeny of Nova Scorpii ad 1437
Four new planets_around_giant_stars_and_the_mass_metallicity_correlation_of_p...
Streamer waves, final version
Exocometary gas in_th_hd_181327_debris_ring

What's hot (18)

PDF
The completeness-corrected rate of stellar encounters with the Sun from the f...
PDF
Kepler monitoring l_dwarfs_spot
PDF
Daily variability of_ceres_albedo_detected_by_m_eans_of_radial_velocities_cha...
PDF
Evidence for a_distant_giant_planet_in_the_solar_system
PDF
The colision between_the_milky_way_and_andromeda
PDF
F04414145
PDF
DAQScienceTeamMeetingPosterV1
PDF
Large turbulent reservoirs of cold molecular gas around high-redshift starbur...
PDF
Variability in a_young_lt_transition_planetary_mass_object
PDF
Models of cosmic ray modulations in light of new data from AMS-02
PDF
Asassn 15ih a_highly_super_luminous_supernova
DOCX
Multiple choices questions 4-
PDF
A nearby yoiung_m_dwarf_with_wide_possibly_planetary_m_ass_companion
PDF
Cosmic radiation in australia carpenter
PDF
The parkes hi zone of avoidance survey
PDF
End point of_black_ring_instabilities_and_the_weak_cosmic_censorship_conjecture
PDF
Öncel Akademi: İstatistiksel Sismoloji
PPTX
Pre assessment
The completeness-corrected rate of stellar encounters with the Sun from the f...
Kepler monitoring l_dwarfs_spot
Daily variability of_ceres_albedo_detected_by_m_eans_of_radial_velocities_cha...
Evidence for a_distant_giant_planet_in_the_solar_system
The colision between_the_milky_way_and_andromeda
F04414145
DAQScienceTeamMeetingPosterV1
Large turbulent reservoirs of cold molecular gas around high-redshift starbur...
Variability in a_young_lt_transition_planetary_mass_object
Models of cosmic ray modulations in light of new data from AMS-02
Asassn 15ih a_highly_super_luminous_supernova
Multiple choices questions 4-
A nearby yoiung_m_dwarf_with_wide_possibly_planetary_m_ass_companion
Cosmic radiation in australia carpenter
The parkes hi zone of avoidance survey
End point of_black_ring_instabilities_and_the_weak_cosmic_censorship_conjecture
Öncel Akademi: İstatistiksel Sismoloji
Pre assessment
Ad

Similar to Correlative analysis of long term cosmic ray variation in relation with sunspot number (20)

PDF
Study of Solar Interplanetary and Geomagnetic Disturbances in Solar Cycle 23
PDF
Heliospheric Modulation of CRI Due to Solar Activity
PDF
Solar Interplanetary and Geomagnetic Activity in Solar Cycle 23
PDF
Long term modulation of cosmic ray intensity in statistical relation with cor...
PDF
Solar activity indices and their Impact on Helioshphere and GCR Modulation
PDF
Impact of Solar Outputs on the Helioshphere and Cosmic Ray Modulation
PDF
Acorrelation between sunspot observations and solar Ca II H&K activity proxies
PPTX
Sunspots.pptx This ppt is all about sunspots
PDF
Analysis of high energy charge particle in the Heliosphere
PDF
Analysis of high energy charge particle in the Heliosphere
PPT
Cycle 24 hbarc talk
PPTX
The Sun and Life on Planets by Saku Tsuneta
PDF
Discovery of a relation between the decay rate of the Sun’s magnetic dipole a...
PDF
10
 
PDF
Variability of solar eruptions during cycle 23
PPT
Dtu10e lecture ppt_ch10 2
PDF
The Sun A Guide To Stellar Physics 1st Edition Engvold Oddbj Skumanich
PPTX
Determination of Solar Rotation
PDF
Solar Variability And Planetary Climates Space Sciences Series Of Issi 1st Ed...
PPT
Properties of the sun
Study of Solar Interplanetary and Geomagnetic Disturbances in Solar Cycle 23
Heliospheric Modulation of CRI Due to Solar Activity
Solar Interplanetary and Geomagnetic Activity in Solar Cycle 23
Long term modulation of cosmic ray intensity in statistical relation with cor...
Solar activity indices and their Impact on Helioshphere and GCR Modulation
Impact of Solar Outputs on the Helioshphere and Cosmic Ray Modulation
Acorrelation between sunspot observations and solar Ca II H&K activity proxies
Sunspots.pptx This ppt is all about sunspots
Analysis of high energy charge particle in the Heliosphere
Analysis of high energy charge particle in the Heliosphere
Cycle 24 hbarc talk
The Sun and Life on Planets by Saku Tsuneta
Discovery of a relation between the decay rate of the Sun’s magnetic dipole a...
10
 
Variability of solar eruptions during cycle 23
Dtu10e lecture ppt_ch10 2
The Sun A Guide To Stellar Physics 1st Edition Engvold Oddbj Skumanich
Determination of Solar Rotation
Solar Variability And Planetary Climates Space Sciences Series Of Issi 1st Ed...
Properties of the sun
Ad

More from Alexander Decker (20)

PDF
Abnormalities of hormones and inflammatory cytokines in women affected with p...
PDF
A validation of the adverse childhood experiences scale in
PDF
A usability evaluation framework for b2 c e commerce websites
PDF
A universal model for managing the marketing executives in nigerian banks
PDF
A unique common fixed point theorems in generalized d
PDF
A trends of salmonella and antibiotic resistance
PDF
A transformational generative approach towards understanding al-istifham
PDF
A time series analysis of the determinants of savings in namibia
PDF
A therapy for physical and mental fitness of school children
PDF
A theory of efficiency for managing the marketing executives in nigerian banks
PDF
A systematic evaluation of link budget for
PDF
A synthetic review of contraceptive supplies in punjab
PDF
A synthesis of taylor’s and fayol’s management approaches for managing market...
PDF
A survey paper on sequence pattern mining with incremental
PDF
A survey on live virtual machine migrations and its techniques
PDF
A survey on data mining and analysis in hadoop and mongo db
PDF
A survey on challenges to the media cloud
PDF
A survey of provenance leveraged
PDF
A survey of private equity investments in kenya
PDF
A study to measures the financial health of
Abnormalities of hormones and inflammatory cytokines in women affected with p...
A validation of the adverse childhood experiences scale in
A usability evaluation framework for b2 c e commerce websites
A universal model for managing the marketing executives in nigerian banks
A unique common fixed point theorems in generalized d
A trends of salmonella and antibiotic resistance
A transformational generative approach towards understanding al-istifham
A time series analysis of the determinants of savings in namibia
A therapy for physical and mental fitness of school children
A theory of efficiency for managing the marketing executives in nigerian banks
A systematic evaluation of link budget for
A synthetic review of contraceptive supplies in punjab
A synthesis of taylor’s and fayol’s management approaches for managing market...
A survey paper on sequence pattern mining with incremental
A survey on live virtual machine migrations and its techniques
A survey on data mining and analysis in hadoop and mongo db
A survey on challenges to the media cloud
A survey of provenance leveraged
A survey of private equity investments in kenya
A study to measures the financial health of

Recently uploaded (20)

PPTX
20250228 LYD VKU AI Blended-Learning.pptx
PDF
Shreyas Phanse Resume: Experienced Backend Engineer | Java • Spring Boot • Ka...
PPTX
MYSQL Presentation for SQL database connectivity
PPTX
Big Data Technologies - Introduction.pptx
PPTX
VMware vSphere Foundation How to Sell Presentation-Ver1.4-2-14-2024.pptx
PDF
KodekX | Application Modernization Development
PPT
Teaching material agriculture food technology
PDF
Empathic Computing: Creating Shared Understanding
PDF
Mobile App Security Testing_ A Comprehensive Guide.pdf
PDF
Machine learning based COVID-19 study performance prediction
PPTX
Cloud computing and distributed systems.
PDF
Encapsulation theory and applications.pdf
PPTX
Understanding_Digital_Forensics_Presentation.pptx
DOCX
The AUB Centre for AI in Media Proposal.docx
PDF
How UI/UX Design Impacts User Retention in Mobile Apps.pdf
PDF
Unlocking AI with Model Context Protocol (MCP)
PDF
Architecting across the Boundaries of two Complex Domains - Healthcare & Tech...
PPTX
Effective Security Operations Center (SOC) A Modern, Strategic, and Threat-In...
PDF
Modernizing your data center with Dell and AMD
PDF
Building Integrated photovoltaic BIPV_UPV.pdf
20250228 LYD VKU AI Blended-Learning.pptx
Shreyas Phanse Resume: Experienced Backend Engineer | Java • Spring Boot • Ka...
MYSQL Presentation for SQL database connectivity
Big Data Technologies - Introduction.pptx
VMware vSphere Foundation How to Sell Presentation-Ver1.4-2-14-2024.pptx
KodekX | Application Modernization Development
Teaching material agriculture food technology
Empathic Computing: Creating Shared Understanding
Mobile App Security Testing_ A Comprehensive Guide.pdf
Machine learning based COVID-19 study performance prediction
Cloud computing and distributed systems.
Encapsulation theory and applications.pdf
Understanding_Digital_Forensics_Presentation.pptx
The AUB Centre for AI in Media Proposal.docx
How UI/UX Design Impacts User Retention in Mobile Apps.pdf
Unlocking AI with Model Context Protocol (MCP)
Architecting across the Boundaries of two Complex Domains - Healthcare & Tech...
Effective Security Operations Center (SOC) A Modern, Strategic, and Threat-In...
Modernizing your data center with Dell and AMD
Building Integrated photovoltaic BIPV_UPV.pdf

Correlative analysis of long term cosmic ray variation in relation with sunspot number

  • 1. Advances in Physics Theories and Applications www.iiste.org ISSN 2224-719X (Paper) ISSN 2225-0638 (Online) Vol.22, 2013 10 Correlative Analysis of Long Term Cosmic Ray Variation in Relation with Sunspot Number UMA PANDEY Department of Physics, MVM, Bhopal-462003 (M.P.) Contact No: 07697312643 Email: uma.pandey185@gmail.com MAHENDRA SINGH Department of Physics, MVM, Bhopal-462003 (M.P.) Contact No: 09425608307 Email: asbplin@rediffmail.com PANKAJ K. SHRIVASTAVA Department of Physics Govt. Model Science College ,Rewa(M.P.)-486001 Contact No: 09893328379 Email:pankaj_in_2001@rediffmail.com Abstract In this paper we will study about the relation between Cosmic ray Intensity(CRI) and Sunspot Number for solar cycle 22, 23 and 24.For this we have taken the data of cosmic ray intensity from various neutron Monitor stations .These neutron monitor stations are well maintained stations and provide reliable cosmic ray data for variation study. A detail correlative study have been done by running cross correlation method. The cosmic ray intensity and sunspot number shows high and negative correlation among themselves. Sunspot number shows anti phase with Cosmic ray Intensity (CRI). Keywords:- Cosmic –ray; Solar Cycle; Solar activity; Sunspot number Introduction In the past a lot of work has been done to correlate the solar parameters with cosmic ray intensity on long term basis. In the recent past two ideas have motivated much to modulation research.The first originally proposed by Lockwood (1960), is that the long term modulation of cosmic ray intensity i.e. 11 year variation result from pileup of individual intensity decreases caused by shock’s and other disturbance in solar wind. The second major idea is that gradient end curvature drifts, long neglected in theories of modulation may be significant and in some cases dominant in governing the modulation of cosmic rays [1-3]. Generally sunspot numbers have been used as a representative of solar activity index for various studies. Solar terrestrial relationships provide an important factor to explain the aspects of the 11 and 22 year variation of galactic cosmic ray.The 11 year variation in Cosmic ray Intensity observed on the earth is anti-correlated with sunspot number[4-5]. The Cosmic ray Intensity curve follow a 22 year cycle with alternate maxima being flat topped and peaked as predicted by models of Cosmic ray modulation based on the observed reversal of the sun’s magnetic field polarity after every 11 year and curvature and gradient drifts in the large scale magnetic field of the heliosphere[6-10]..In this paper we have made an attempt to derive the correlation between Sunspot number and Cosmic ray Intensity for solar cycle22, 23 and 24.The solar cycle 22 have been started in the September 1986 and ended in the year 1996(May). The solar cycle 23 lasted in 12.6 years, beginning in May 1996 and ending in December 2008. The maximum smoothed sunspot number (monthly number of sunspots averaged over a twelve-month period) observed during the solar cycle 23 was 120.8, and the minimum was 1.7. There were a total of 805 days with no sunspots during this cycle.[11] METHOD OF ANALYSIS In this paper we will find the correlation between Cosmic ray intensity and solar parameter sunspot number for solar cycle22, 23 and 24(incomplete) .For this monthly mean values of sunspot number (Rz) are taken from the Solar Geophysical Data books. The pressure corrected monthly mean value of cosmic ray data of Moscow, Russia (Cutoff Rigidity=2.42GV) neutron monitor station have been taken for analysis. In this paper we will also make comparative study of solar cycle 22, 23 and 24. RESULTS AND DISCUSSION Solar activity rises and falls with a period of about 11 years .The number of sunspots indicates the level of solar activity. The emissions of matter and electromagnetic fields from the sun increases during high solar activity, making it harder for Galactic Cosmic Ray to reach the earth. Cosmic ray intensity is lower when solar activity is high and vice versa. The long term modulation of cosmic ray intensity has been studied by several scholars in relation with sunspot number, and a high negative correlation is found between them. The fig.3 shows correlation between sunspot number and Cosmic ray intensity(CRI) for solar cycle 22, 23 and 24(incomplete).
  • 2. Advances in Physics Theories and Applications www.iiste.org ISSN 2224-719X (Paper) ISSN 2225-0638 (Online) Vol.22, 2013 11 Figure 1 & 2 shows the linear plot of Sunspot number and Cosmic ray intensity with year. From fig.3&4 it is clear that sunspot number and CRI are anti- correlated. Following conclusions can be drawn: 1) The solar 22 started in September 1986 and ended in May 1996.The total length of cycle 22 is 9.7 years. The solar cycle 23 started in May 1996 and ended in December 2008 and total length of cycle is 12.6 yrs. Thus solar cycle 23 is longer than solar cycle 22.The solar cycle 24 has started in the year 2008( December ) and is incomplete. 2) The solar activity of solar cycle 22 shows increasing phase from 1986 to 1989 and then decreasing phase from 1989 to 1996.At the same time Cosmic ray intensity(CRI )decreases for the period 1986-1991 and shows increasing phase from 1991 to 1996.Thus from the figure it is clear that as sunspot activity increases ,at the same time Cosmic ray intensity (CRI) decreases. Thus both sunspot number and cosmic ray intensity shows anti-phase with each other. 3) The solar activity of solar cycle 23 shows increasing phase from 1996 to 2000 and then decreasing phase from 2000 to 2008.At the same time CRI decreases for the period 1996-2000 and shows increasing phase from 2000 to 2008.Thus it is clear from fig 3. that for cycle 23 also sunspot activity and Cosmic ray intensity(CRI) are anti- correlated. 4) The solar cycle 24 has started in the year 2008(Dec) and is incomplete. But it seems to be that solar cycle 24 is weaker in solar activity as comparison to cycle 22 and 23. 5)From fig.4 the correlation coefficient between sunspot number and Cosmic ray intensity (CRI) for solar cycle 22,23 and 24 is found to be -0.90057 which is highly negative correlated. References [1] Lockwood,J.A.,1960,J Geophysics.Res, 65,19 [2] Webber W.R. and Lockwood JA.,1988, Journal of Geophysical research,93 ,8735 [3] Sharma,N.I.,29th International Cosmic ray Conference Pune ,2005,00, 101-104 [4] Forbush, S.E. 1954, J. Geophys. Res.,59,525 [5] Forbush,S.E. 1958, J. Geophys. Res.,63,651 [6] Dorman I V & Dorman L I, 1967,J Geophys Res(USA) ,72,1513 [7] Jokipii,J.R.,Thomas, B.T. 1981,Astrophys.. J.,243,1115 [8] Jokipii, J.R.,Levy, E.H.,Hubbard,W.B. 1977,Astrophys. J.,213,861 [9] Nagashima K & Morishitha I,Proc of 16th ICRC, 1979,Tokyo,Japan,.3 ,325 [10] Gupta Meera,Mishra,V.K.,Mishra A.P. June 2006,Indian Journal of Radio and space Physics, 35,167 [11] Solar Cycle 23 Wikipedia free encyclopedia
  • 3. Advances in Physics Theories and Applications www.iiste.org ISSN 2224-719X (Paper) ISSN 2225-0638 (Online) Vol.22, 2013 12 Graphs: Fig:1 Year Vs average yearly values of sunspot number(Rz) for solar cycle 22,23 and 24 Fig:2 Year Vs average yearly values of Cosmic Ray Intensity(Moscow Neutron Station) for solar cycle 22,23 and24
  • 4. Advances in Physics Theories and Applications www.iiste.org ISSN 2224-719X (Paper) ISSN 2225-0638 (Online) Vol.22, 2013 13 Fig:3 Shows cross-plot curve between yearly value of sunspot number(Rz) and Cosmic Ray Intensity (Moscow Neutron Station) for solar cycle 22,23 and24 Fig:4 Shows Correlation curve between yearly value of sunspot number(Rz) and Cosmic Ray Intensity(CRI) for solar cycle 22,23 and24
  • 5. This academic article was published by The International Institute for Science, Technology and Education (IISTE). The IISTE is a pioneer in the Open Access Publishing service based in the U.S. and Europe. The aim of the institute is Accelerating Global Knowledge Sharing. More information about the publisher can be found in the IISTE’s homepage: http://www.iiste.org CALL FOR JOURNAL PAPERS The IISTE is currently hosting more than 30 peer-reviewed academic journals and collaborating with academic institutions around the world. There’s no deadline for submission. Prospective authors of IISTE journals can find the submission instruction on the following page: http://www.iiste.org/journals/ The IISTE editorial team promises to the review and publish all the qualified submissions in a fast manner. All the journals articles are available online to the readers all over the world without financial, legal, or technical barriers other than those inseparable from gaining access to the internet itself. Printed version of the journals is also available upon request of readers and authors. MORE RESOURCES Book publication information: http://www.iiste.org/book/ Recent conferences: http://www.iiste.org/conference/ IISTE Knowledge Sharing Partners EBSCO, Index Copernicus, Ulrich's Periodicals Directory, JournalTOCS, PKP Open Archives Harvester, Bielefeld Academic Search Engine, Elektronische Zeitschriftenbibliothek EZB, Open J-Gate, OCLC WorldCat, Universe Digtial Library , NewJour, Google Scholar