Diagnostics of the electromagnetic characteristics of the interplanetary medium based on cosmic ray effects

We propose a model for the modulation of cosmic rays (CRs) based on changes in the CR energy in different regular electromagnetic fields of the interplanetary medium. Within the framework of the elaborated concept, an analytical expression for the CR rigidity spectrum has been obtained. It allows us...

Full description

Saved in:
Bibliographic Details
Published in:Geomagnetism and Aeronomy 2013-07, Vol.53 (4), p.430-440
Main Authors: Dvornikov, V. M., Kravtsova, M. V., Sdobnov, V. E.
Format: Article
Language:English
Subjects:
Anisotropy
Cosmic rays
Earth and Environmental Science
Earth Sciences
Electromagnetic fields
Electromagnetism
Geophysics/Geodesy
Magnetic fields
Rigidity
Solar activity
Solar flares
Citations: Items that this one cites
Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by cdi_FETCH-LOGICAL-c349t-7ffe0189aecad895d0fb2cdfa8297b942bc6eb3aaa4ae297fa78b9dab8dd463d3
cites cdi_FETCH-LOGICAL-c349t-7ffe0189aecad895d0fb2cdfa8297b942bc6eb3aaa4ae297fa78b9dab8dd463d3
container_end_page 440
container_issue 4
container_start_page 430
container_title Geomagnetism and Aeronomy
container_volume 53
creator Dvornikov, V. M.
Kravtsova, M. V.
Sdobnov, V. E.
description We propose a model for the modulation of cosmic rays (CRs) based on changes in the CR energy in different regular electromagnetic fields of the interplanetary medium. Within the framework of the elaborated concept, an analytical expression for the CR rigidity spectrum has been obtained. It allows us to describe variations in proton intensity observed in the energy range from several MeV to several tens of GeV per hour of observation. We give a description of a method for determining parameters of the model spectrum that reflect the electromagnetic characteristics of the interplanetary medium with a different nature. Using ground-based and satellite measurements of the CR intensity, we have examined variations in the CR rigidity spectrum and anisotropy and variations in the planetary system of geomagnetic cutoff rigidities during different manifestations of solar activity. A whole set of phenomena under observation has been interpreted.
doi_str_mv 10.1134/S0016793213040075
format article
fullrecord <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_1448220525</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1448220525</sourcerecordid><originalsourceid>FETCH-LOGICAL-c349t-7ffe0189aecad895d0fb2cdfa8297b942bc6eb3aaa4ae297fa78b9dab8dd463d3</originalsourceid><addsrcrecordid>eNp1kElLxEAQhRtRcBz9Ad4avHiJ9pqkj-IOAx5U8BYqvcxkTNJjd3KYf2-H8eCCp4L3vveoKoROKbmglIvLZ0JoXijOKCeCkELuoRmVUma5kG_7aDbZ2eQfoqMY14RwIiWdofebBpa9j0OjI_YODyuLbWv1EHyXDJt0rFcQQA82ND-wpk_SpoUEQdjizppm7HAN0Rrse6x97FI4wBZb51JjPEYHDtpoT77mHL3e3b5cP2SLp_vH66tFprlQQ1YkmtBSgdVgSiUNcTXTxkHJVFErwWqd25oDgACbJAdFWSsDdWmMyLnhc3S-690E_zHaOFRdE7Vtp1X9GCsqRMkYkUwm9OwXuvZj6NN2FeVKCSVoPlF0R-ngYwzWVZvQdOnoipJqen_15_0pw3aZmNh-acO35n9Dn3kGiYw</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1399494165</pqid></control><display><type>article</type><title>Diagnostics of the electromagnetic characteristics of the interplanetary medium based on cosmic ray effects</title><source>Springer Link</source><creator>Dvornikov, V. M. ; Kravtsova, M. V. ; Sdobnov, V. E.</creator><creatorcontrib>Dvornikov, V. M. ; Kravtsova, M. V. ; Sdobnov, V. E.</creatorcontrib><description>We propose a model for the modulation of cosmic rays (CRs) based on changes in the CR energy in different regular electromagnetic fields of the interplanetary medium. Within the framework of the elaborated concept, an analytical expression for the CR rigidity spectrum has been obtained. It allows us to describe variations in proton intensity observed in the energy range from several MeV to several tens of GeV per hour of observation. We give a description of a method for determining parameters of the model spectrum that reflect the electromagnetic characteristics of the interplanetary medium with a different nature. Using ground-based and satellite measurements of the CR intensity, we have examined variations in the CR rigidity spectrum and anisotropy and variations in the planetary system of geomagnetic cutoff rigidities during different manifestations of solar activity. A whole set of phenomena under observation has been interpreted.</description><identifier>ISSN: 0016-7932</identifier><identifier>EISSN: 1555-645X</identifier><identifier>EISSN: 0016-7940</identifier><identifier>DOI: 10.1134/S0016793213040075</identifier><language>eng</language><publisher>Boston: Springer US</publisher><subject>Anisotropy ; Cosmic rays ; Earth and Environmental Science ; Earth Sciences ; Electromagnetic fields ; Electromagnetism ; Geophysics/Geodesy ; Magnetic fields ; Rigidity ; Solar activity ; Solar flares</subject><ispartof>Geomagnetism and Aeronomy, 2013-07, Vol.53 (4), p.430-440</ispartof><rights>Pleiades Publishing, Ltd. 2013</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c349t-7ffe0189aecad895d0fb2cdfa8297b942bc6eb3aaa4ae297fa78b9dab8dd463d3</citedby><cites>FETCH-LOGICAL-c349t-7ffe0189aecad895d0fb2cdfa8297b942bc6eb3aaa4ae297fa78b9dab8dd463d3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27924,27925</link.rule.ids></links><search><creatorcontrib>Dvornikov, V. M.</creatorcontrib><creatorcontrib>Kravtsova, M. V.</creatorcontrib><creatorcontrib>Sdobnov, V. E.</creatorcontrib><title>Diagnostics of the electromagnetic characteristics of the interplanetary medium based on cosmic ray effects</title><title>Geomagnetism and Aeronomy</title><addtitle>Geomagn. Aeron</addtitle><description>We propose a model for the modulation of cosmic rays (CRs) based on changes in the CR energy in different regular electromagnetic fields of the interplanetary medium. Within the framework of the elaborated concept, an analytical expression for the CR rigidity spectrum has been obtained. It allows us to describe variations in proton intensity observed in the energy range from several MeV to several tens of GeV per hour of observation. We give a description of a method for determining parameters of the model spectrum that reflect the electromagnetic characteristics of the interplanetary medium with a different nature. Using ground-based and satellite measurements of the CR intensity, we have examined variations in the CR rigidity spectrum and anisotropy and variations in the planetary system of geomagnetic cutoff rigidities during different manifestations of solar activity. A whole set of phenomena under observation has been interpreted.</description><subject>Anisotropy</subject><subject>Cosmic rays</subject><subject>Earth and Environmental Science</subject><subject>Earth Sciences</subject><subject>Electromagnetic fields</subject><subject>Electromagnetism</subject><subject>Geophysics/Geodesy</subject><subject>Magnetic fields</subject><subject>Rigidity</subject><subject>Solar activity</subject><subject>Solar flares</subject><issn>0016-7932</issn><issn>1555-645X</issn><issn>0016-7940</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2013</creationdate><recordtype>article</recordtype><recordid>eNp1kElLxEAQhRtRcBz9Ad4avHiJ9pqkj-IOAx5U8BYqvcxkTNJjd3KYf2-H8eCCp4L3vveoKoROKbmglIvLZ0JoXijOKCeCkELuoRmVUma5kG_7aDbZ2eQfoqMY14RwIiWdofebBpa9j0OjI_YODyuLbWv1EHyXDJt0rFcQQA82ND-wpk_SpoUEQdjizppm7HAN0Rrse6x97FI4wBZb51JjPEYHDtpoT77mHL3e3b5cP2SLp_vH66tFprlQQ1YkmtBSgdVgSiUNcTXTxkHJVFErwWqd25oDgACbJAdFWSsDdWmMyLnhc3S-690E_zHaOFRdE7Vtp1X9GCsqRMkYkUwm9OwXuvZj6NN2FeVKCSVoPlF0R-ngYwzWVZvQdOnoipJqen_15_0pw3aZmNh-acO35n9Dn3kGiYw</recordid><startdate>20130701</startdate><enddate>20130701</enddate><creator>Dvornikov, V. M.</creator><creator>Kravtsova, M. V.</creator><creator>Sdobnov, V. E.</creator><general>Springer US</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope><scope>3V.</scope><scope>7TG</scope><scope>7XB</scope><scope>88I</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>8FK</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>GNUQQ</scope><scope>H8D</scope><scope>HCIFZ</scope><scope>KL.</scope><scope>L7M</scope><scope>M2P</scope><scope>P5Z</scope><scope>P62</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>Q9U</scope></search><sort><creationdate>20130701</creationdate><title>Diagnostics of the electromagnetic characteristics of the interplanetary medium based on cosmic ray effects</title><author>Dvornikov, V. M. ; Kravtsova, M. V. ; Sdobnov, V. E.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c349t-7ffe0189aecad895d0fb2cdfa8297b942bc6eb3aaa4ae297fa78b9dab8dd463d3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2013</creationdate><topic>Anisotropy</topic><topic>Cosmic rays</topic><topic>Earth and Environmental Science</topic><topic>Earth Sciences</topic><topic>Electromagnetic fields</topic><topic>Electromagnetism</topic><topic>Geophysics/Geodesy</topic><topic>Magnetic fields</topic><topic>Rigidity</topic><topic>Solar activity</topic><topic>Solar flares</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Dvornikov, V. M.</creatorcontrib><creatorcontrib>Kravtsova, M. V.</creatorcontrib><creatorcontrib>Sdobnov, V. E.</creatorcontrib><collection>CrossRef</collection><collection>ProQuest Central (Corporate)</collection><collection>Meteorological &amp; Geoastrophysical Abstracts</collection><collection>ProQuest Central (purchase pre-March 2016)</collection><collection>Science Database (Alumni Edition)</collection><collection>Technology Research Database</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Central (Alumni) (purchase pre-March 2016)</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</collection><collection>Advanced Technologies &amp; Aerospace Collection</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central</collection><collection>ProQuest Central Student</collection><collection>Aerospace Database</collection><collection>SciTech Premium Collection</collection><collection>Meteorological &amp; Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Science Database</collection><collection>Advanced Technologies &amp; Aerospace Database</collection><collection>ProQuest Advanced Technologies &amp; Aerospace Collection</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central Basic</collection><jtitle>Geomagnetism and Aeronomy</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Dvornikov, V. M.</au><au>Kravtsova, M. V.</au><au>Sdobnov, V. E.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Diagnostics of the electromagnetic characteristics of the interplanetary medium based on cosmic ray effects</atitle><jtitle>Geomagnetism and Aeronomy</jtitle><stitle>Geomagn. Aeron</stitle><date>2013-07-01</date><risdate>2013</risdate><volume>53</volume><issue>4</issue><spage>430</spage><epage>440</epage><pages>430-440</pages><issn>0016-7932</issn><eissn>1555-645X</eissn><eissn>0016-7940</eissn><abstract>We propose a model for the modulation of cosmic rays (CRs) based on changes in the CR energy in different regular electromagnetic fields of the interplanetary medium. Within the framework of the elaborated concept, an analytical expression for the CR rigidity spectrum has been obtained. It allows us to describe variations in proton intensity observed in the energy range from several MeV to several tens of GeV per hour of observation. We give a description of a method for determining parameters of the model spectrum that reflect the electromagnetic characteristics of the interplanetary medium with a different nature. Using ground-based and satellite measurements of the CR intensity, we have examined variations in the CR rigidity spectrum and anisotropy and variations in the planetary system of geomagnetic cutoff rigidities during different manifestations of solar activity. A whole set of phenomena under observation has been interpreted.</abstract><cop>Boston</cop><pub>Springer US</pub><doi>10.1134/S0016793213040075</doi><tpages>11</tpages></addata></record>
fulltext fulltext
identifier ISSN: 0016-7932
ispartof Geomagnetism and Aeronomy, 2013-07, Vol.53 (4), p.430-440
issn 0016-7932
1555-645X
0016-7940
language eng
recordid cdi_proquest_miscellaneous_1448220525
source Springer Link
subjects Anisotropy
Cosmic rays
Earth and Environmental Science
Earth Sciences
Electromagnetic fields
Electromagnetism
Geophysics/Geodesy
Magnetic fields
Rigidity
Solar activity
Solar flares
title Diagnostics of the electromagnetic characteristics of the interplanetary medium based on cosmic ray effects
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-29T18%3A33%3A30IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Diagnostics%20of%20the%20electromagnetic%20characteristics%20of%20the%20interplanetary%20medium%20based%20on%20cosmic%20ray%20effects&rft.jtitle=Geomagnetism%20and%20Aeronomy&rft.au=Dvornikov,%20V.%20M.&rft.date=2013-07-01&rft.volume=53&rft.issue=4&rft.spage=430&rft.epage=440&rft.pages=430-440&rft.issn=0016-7932&rft.eissn=1555-645X&rft_id=info:doi/10.1134/S0016793213040075&rft_dat=%3Cproquest_cross%3E1448220525%3C/proquest_cross%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c349t-7ffe0189aecad895d0fb2cdfa8297b942bc6eb3aaa4ae297fa78b9dab8dd463d3%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=1399494165&rft_id=info:pmid/&rfr_iscdi=true