Loading…

The Sun and Heliosphere at Solar Maximum

Recent Ulysses observations from the Sun's equator to the poles reveal fundamental properties of the three-dimensional heliosphere at the maximum in solar activity. The heliospheric magnetic field originates from a magnetic dipole oriented nearly perpendicular to, instead of nearly parallel to,...

Full description

Saved in:
Bibliographic Details
Published in:Science (American Association for the Advancement of Science) 2003-11, Vol.302 (5648), p.1165-1169
Main Authors: Smith, E. J., Marsden, R. G., Balogh, A., Gloeckler, G., Geiss, J., McComas, D. J., McKibben, R. B., MacDowall, R. J., Lanzerotti, L. J., Krupp, N., Krueger, H., Landgraf, M.
Format: Article
Language:English
Subjects:
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-c782t-789f06267c45d19aa1e2a296ee0ba32b7cdd47d09a82f1d033d100a45cb07bab3
cites cdi_FETCH-LOGICAL-c782t-789f06267c45d19aa1e2a296ee0ba32b7cdd47d09a82f1d033d100a45cb07bab3
container_end_page 1169
container_issue 5648
container_start_page 1165
container_title Science (American Association for the Advancement of Science)
container_volume 302
creator Smith, E. J.
Marsden, R. G.
Balogh, A.
Gloeckler, G.
Geiss, J.
McComas, D. J.
McKibben, R. B.
MacDowall, R. J.
Lanzerotti, L. J.
Krupp, N.
Krueger, H.
Landgraf, M.
description Recent Ulysses observations from the Sun's equator to the poles reveal fundamental properties of the three-dimensional heliosphere at the maximum in solar activity. The heliospheric magnetic field originates from a magnetic dipole oriented nearly perpendicular to, instead of nearly parallel to, the Sun's rotation axis. Magnetic fields, solar wind, and energetic charged particles from low-latitude sources reach all latitudes, including the polar caps. The very fast high-latitude wind and polar coronal holes disappear and reappear together. Solar wind speed continues to be inversely correlated with coronal temperature. The cosmic ray flux is reduced symmetrically at all latitudes.
doi_str_mv 10.1126/science.1086295
format article
fullrecord <record><control><sourceid>gale_proqu</sourceid><recordid>TN_cdi_proquest_miscellaneous_743520626</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><galeid>A111203661</galeid><jstor_id>3835484</jstor_id><sourcerecordid>A111203661</sourcerecordid><originalsourceid>FETCH-LOGICAL-c782t-789f06267c45d19aa1e2a296ee0ba32b7cdd47d09a82f1d033d100a45cb07bab3</originalsourceid><addsrcrecordid>eNqN0ttr2zAUB2AzVta02_NexjCD7vLgVBfr4scubGkhWx7S7VUcy8epgy-ZZEP3308lZiUlbEEPAp3vSEj6RdFrSqaUMnnpbYWtxSklWrJMPIsmlGQiyRjhz6MJIVwmmihxGp15vyEk1DL-IjqlqaRCMDmJPt7eYbwa2hjaIr7Guur89g4dxtDHq64GF3-D-6oZmpfRSQm1x1fjfB79-PrldnadLJbzm9nVIrFKsz5ROiuJZFLZVBQ0A6DIgGUSkeTAWa5sUaSqIBloVtKCcF5QQiAVNicqh5yfRx92-25d92tA35um8hbrGlrsBm9UygV7OCHI9_-WlMuMcvVfSLXmXAkS4LsncNMNrg3XNYxyoRVPdUDJDq2hRlO1Zdc7sGts0UHdtVhWYfmKhu8Jry9p8NMDPowCm8oebPi01xBMj_f9Ggbvzc3q-_F2-fN4-3l-tNXzxb5NDlnb1TWu0YR0zJb7_nLnreu8d1iarasacL8NJeYh1WZMtRlTHTrejv8y5A0Wj36McQAXIwBvoS4dtLbyj05wmiqZBvdm5za-79zfOtdcpDrlfwBYjwCS</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>213587348</pqid></control><display><type>article</type><title>The Sun and Heliosphere at Solar Maximum</title><source>American Association for the Advancement of Science</source><source>JSTOR Archival Journals and Primary Sources Collection</source><source>Social Science Premium Collection</source><source>Alma/SFX Local Collection</source><source>Education Collection</source><creator>Smith, E. J. ; Marsden, R. G. ; Balogh, A. ; Gloeckler, G. ; Geiss, J. ; McComas, D. J. ; McKibben, R. B. ; MacDowall, R. J. ; Lanzerotti, L. J. ; Krupp, N. ; Krueger, H. ; Landgraf, M.</creator><creatorcontrib>Smith, E. J. ; Marsden, R. G. ; Balogh, A. ; Gloeckler, G. ; Geiss, J. ; McComas, D. J. ; McKibben, R. B. ; MacDowall, R. J. ; Lanzerotti, L. J. ; Krupp, N. ; Krueger, H. ; Landgraf, M.</creatorcontrib><description>Recent Ulysses observations from the Sun's equator to the poles reveal fundamental properties of the three-dimensional heliosphere at the maximum in solar activity. The heliospheric magnetic field originates from a magnetic dipole oriented nearly perpendicular to, instead of nearly parallel to, the Sun's rotation axis. Magnetic fields, solar wind, and energetic charged particles from low-latitude sources reach all latitudes, including the polar caps. The very fast high-latitude wind and polar coronal holes disappear and reappear together. Solar wind speed continues to be inversely correlated with coronal temperature. The cosmic ray flux is reduced symmetrically at all latitudes.</description><identifier>ISSN: 0036-8075</identifier><identifier>EISSN: 1095-9203</identifier><identifier>DOI: 10.1126/science.1086295</identifier><identifier>PMID: 14615526</identifier><identifier>CODEN: SCIEAS</identifier><language>eng</language><publisher>Washington, DC: American Association for the Advancement of Science</publisher><subject>Astronomy ; Charged particles ; Cosmic rays ; Earth, ocean, space ; Exact sciences and technology ; Geophysics ; Heliosphere ; Magnetic fields ; Magnetic flux ; Magnetic polarity ; Observations ; Particle radiation, solar wind ; Polar caps ; Review ; Solar energy ; Solar flares ; Solar physics ; Solar system ; Solar wind ; Sun ; Sunspots ; Tropical regions</subject><ispartof>Science (American Association for the Advancement of Science), 2003-11, Vol.302 (5648), p.1165-1169</ispartof><rights>Copyright 2003 American Association for the Advancement of Science</rights><rights>2004 INIST-CNRS</rights><rights>COPYRIGHT 2003 American Association for the Advancement of Science</rights><rights>COPYRIGHT 2003 American Association for the Advancement of Science</rights><rights>Copyright American Association for the Advancement of Science Nov 14, 2003</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c782t-789f06267c45d19aa1e2a296ee0ba32b7cdd47d09a82f1d033d100a45cb07bab3</citedby><cites>FETCH-LOGICAL-c782t-789f06267c45d19aa1e2a296ee0ba32b7cdd47d09a82f1d033d100a45cb07bab3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://www.proquest.com/docview/213587348/fulltextPDF?pq-origsite=primo$$EPDF$$P50$$Gproquest$$H</linktopdf><linktohtml>$$Uhttps://www.proquest.com/docview/213587348?pq-origsite=primo$$EHTML$$P50$$Gproquest$$H</linktohtml><link.rule.ids>314,780,784,2884,2885,21378,21394,27924,27925,33611,33612,33877,33878,43733,43880,58238,58471,74221,74397</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&amp;idt=15314764$$DView record in Pascal Francis$$Hfree_for_read</backlink><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/14615526$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink></links><search><creatorcontrib>Smith, E. J.</creatorcontrib><creatorcontrib>Marsden, R. G.</creatorcontrib><creatorcontrib>Balogh, A.</creatorcontrib><creatorcontrib>Gloeckler, G.</creatorcontrib><creatorcontrib>Geiss, J.</creatorcontrib><creatorcontrib>McComas, D. J.</creatorcontrib><creatorcontrib>McKibben, R. B.</creatorcontrib><creatorcontrib>MacDowall, R. J.</creatorcontrib><creatorcontrib>Lanzerotti, L. J.</creatorcontrib><creatorcontrib>Krupp, N.</creatorcontrib><creatorcontrib>Krueger, H.</creatorcontrib><creatorcontrib>Landgraf, M.</creatorcontrib><title>The Sun and Heliosphere at Solar Maximum</title><title>Science (American Association for the Advancement of Science)</title><addtitle>Science</addtitle><description>Recent Ulysses observations from the Sun's equator to the poles reveal fundamental properties of the three-dimensional heliosphere at the maximum in solar activity. The heliospheric magnetic field originates from a magnetic dipole oriented nearly perpendicular to, instead of nearly parallel to, the Sun's rotation axis. Magnetic fields, solar wind, and energetic charged particles from low-latitude sources reach all latitudes, including the polar caps. The very fast high-latitude wind and polar coronal holes disappear and reappear together. Solar wind speed continues to be inversely correlated with coronal temperature. The cosmic ray flux is reduced symmetrically at all latitudes.</description><subject>Astronomy</subject><subject>Charged particles</subject><subject>Cosmic rays</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>Geophysics</subject><subject>Heliosphere</subject><subject>Magnetic fields</subject><subject>Magnetic flux</subject><subject>Magnetic polarity</subject><subject>Observations</subject><subject>Particle radiation, solar wind</subject><subject>Polar caps</subject><subject>Review</subject><subject>Solar energy</subject><subject>Solar flares</subject><subject>Solar physics</subject><subject>Solar system</subject><subject>Solar wind</subject><subject>Sun</subject><subject>Sunspots</subject><subject>Tropical regions</subject><issn>0036-8075</issn><issn>1095-9203</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2003</creationdate><recordtype>article</recordtype><sourceid>ALSLI</sourceid><sourceid>CJNVE</sourceid><sourceid>M0P</sourceid><recordid>eNqN0ttr2zAUB2AzVta02_NexjCD7vLgVBfr4scubGkhWx7S7VUcy8epgy-ZZEP3308lZiUlbEEPAp3vSEj6RdFrSqaUMnnpbYWtxSklWrJMPIsmlGQiyRjhz6MJIVwmmihxGp15vyEk1DL-IjqlqaRCMDmJPt7eYbwa2hjaIr7Guur89g4dxtDHq64GF3-D-6oZmpfRSQm1x1fjfB79-PrldnadLJbzm9nVIrFKsz5ROiuJZFLZVBQ0A6DIgGUSkeTAWa5sUaSqIBloVtKCcF5QQiAVNicqh5yfRx92-25d92tA35um8hbrGlrsBm9UygV7OCHI9_-WlMuMcvVfSLXmXAkS4LsncNMNrg3XNYxyoRVPdUDJDq2hRlO1Zdc7sGts0UHdtVhWYfmKhu8Jry9p8NMDPowCm8oebPi01xBMj_f9Ggbvzc3q-_F2-fN4-3l-tNXzxb5NDlnb1TWu0YR0zJb7_nLnreu8d1iarasacL8NJeYh1WZMtRlTHTrejv8y5A0Wj36McQAXIwBvoS4dtLbyj05wmiqZBvdm5za-79zfOtdcpDrlfwBYjwCS</recordid><startdate>20031114</startdate><enddate>20031114</enddate><creator>Smith, E. J.</creator><creator>Marsden, R. G.</creator><creator>Balogh, A.</creator><creator>Gloeckler, G.</creator><creator>Geiss, J.</creator><creator>McComas, D. J.</creator><creator>McKibben, R. B.</creator><creator>MacDowall, R. J.</creator><creator>Lanzerotti, L. J.</creator><creator>Krupp, N.</creator><creator>Krueger, H.</creator><creator>Landgraf, M.</creator><general>American Association for the Advancement of Science</general><general>The American Association for the Advancement of Science</general><scope>IQODW</scope><scope>NPM</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>8GL</scope><scope>IBG</scope><scope>IOV</scope><scope>ISN</scope><scope>0-V</scope><scope>3V.</scope><scope>7QF</scope><scope>7QG</scope><scope>7QL</scope><scope>7QP</scope><scope>7QQ</scope><scope>7QR</scope><scope>7SC</scope><scope>7SE</scope><scope>7SN</scope><scope>7SP</scope><scope>7SR</scope><scope>7SS</scope><scope>7T7</scope><scope>7TA</scope><scope>7TB</scope><scope>7TK</scope><scope>7TM</scope><scope>7U5</scope><scope>7U9</scope><scope>7X2</scope><scope>7X7</scope><scope>7XB</scope><scope>88A</scope><scope>88B</scope><scope>88E</scope><scope>88I</scope><scope>8AF</scope><scope>8BQ</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>8FH</scope><scope>8FI</scope><scope>8FJ</scope><scope>8FK</scope><scope>8G5</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>ALSLI</scope><scope>ARAPS</scope><scope>ATCPS</scope><scope>AZQEC</scope><scope>BBNVY</scope><scope>BEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>BHPHI</scope><scope>BKSAR</scope><scope>C1K</scope><scope>CCPQU</scope><scope>CJNVE</scope><scope>D1I</scope><scope>DWQXO</scope><scope>F28</scope><scope>FR3</scope><scope>FYUFA</scope><scope>GHDGH</scope><scope>GNUQQ</scope><scope>GUQSH</scope><scope>H8D</scope><scope>H8G</scope><scope>H94</scope><scope>HCIFZ</scope><scope>JG9</scope><scope>JQ2</scope><scope>K9-</scope><scope>K9.</scope><scope>KB.</scope><scope>KR7</scope><scope>L6V</scope><scope>L7M</scope><scope>LK8</scope><scope>L~C</scope><scope>L~D</scope><scope>M0K</scope><scope>M0P</scope><scope>M0R</scope><scope>M0S</scope><scope>M1P</scope><scope>M2O</scope><scope>M2P</scope><scope>M7N</scope><scope>M7P</scope><scope>M7S</scope><scope>MBDVC</scope><scope>P5Z</scope><scope>P62</scope><scope>P64</scope><scope>PATMY</scope><scope>PCBAR</scope><scope>PDBOC</scope><scope>PQEDU</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope><scope>PYCSY</scope><scope>Q9U</scope><scope>R05</scope><scope>RC3</scope><scope>7TG</scope><scope>KL.</scope><scope>7X8</scope></search><sort><creationdate>20031114</creationdate><title>The Sun and Heliosphere at Solar Maximum</title><author>Smith, E. J. ; Marsden, R. G. ; Balogh, A. ; Gloeckler, G. ; Geiss, J. ; McComas, D. J. ; McKibben, R. B. ; MacDowall, R. J. ; Lanzerotti, L. J. ; Krupp, N. ; Krueger, H. ; Landgraf, M.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c782t-789f06267c45d19aa1e2a296ee0ba32b7cdd47d09a82f1d033d100a45cb07bab3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2003</creationdate><topic>Astronomy</topic><topic>Charged particles</topic><topic>Cosmic rays</topic><topic>Earth, ocean, space</topic><topic>Exact sciences and technology</topic><topic>Geophysics</topic><topic>Heliosphere</topic><topic>Magnetic fields</topic><topic>Magnetic flux</topic><topic>Magnetic polarity</topic><topic>Observations</topic><topic>Particle radiation, solar wind</topic><topic>Polar caps</topic><topic>Review</topic><topic>Solar energy</topic><topic>Solar flares</topic><topic>Solar physics</topic><topic>Solar system</topic><topic>Solar wind</topic><topic>Sun</topic><topic>Sunspots</topic><topic>Tropical regions</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Smith, E. J.</creatorcontrib><creatorcontrib>Marsden, R. G.</creatorcontrib><creatorcontrib>Balogh, A.</creatorcontrib><creatorcontrib>Gloeckler, G.</creatorcontrib><creatorcontrib>Geiss, J.</creatorcontrib><creatorcontrib>McComas, D. J.</creatorcontrib><creatorcontrib>McKibben, R. B.</creatorcontrib><creatorcontrib>MacDowall, R. J.</creatorcontrib><creatorcontrib>Lanzerotti, L. J.</creatorcontrib><creatorcontrib>Krupp, N.</creatorcontrib><creatorcontrib>Krueger, H.</creatorcontrib><creatorcontrib>Landgraf, M.</creatorcontrib><collection>Pascal-Francis</collection><collection>PubMed</collection><collection>CrossRef</collection><collection>Gale In Context: High School</collection><collection>Biography (Gale in Context)</collection><collection>Gale In Context: Opposing Viewpoints</collection><collection>Gale In Context: Canada</collection><collection>ProQuest Social Sciences Premium Collection</collection><collection>ProQuest Central (Corporate)</collection><collection>Aluminium Industry Abstracts</collection><collection>Animal Behavior Abstracts</collection><collection>Bacteriology Abstracts (Microbiology B)</collection><collection>Calcium &amp; Calcified Tissue Abstracts</collection><collection>Ceramic Abstracts</collection><collection>Chemoreception Abstracts</collection><collection>Computer and Information Systems Abstracts</collection><collection>Corrosion Abstracts</collection><collection>Ecology Abstracts</collection><collection>Electronics &amp; Communications Abstracts</collection><collection>Engineered Materials Abstracts</collection><collection>Entomology Abstracts (Full archive)</collection><collection>Industrial and Applied Microbiology Abstracts (Microbiology A)</collection><collection>Materials Business File</collection><collection>Mechanical &amp; Transportation Engineering Abstracts</collection><collection>Neurosciences Abstracts</collection><collection>Nucleic Acids Abstracts</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>Virology and AIDS Abstracts</collection><collection>Agricultural Science Collection</collection><collection>Health &amp; Medical Collection</collection><collection>ProQuest Central (purchase pre-March 2016)</collection><collection>Biology Database (Alumni Edition)</collection><collection>Education Database (Alumni Edition)</collection><collection>Medical Database (Alumni Edition)</collection><collection>Science Database (Alumni Edition)</collection><collection>STEM Database</collection><collection>METADEX</collection><collection>Technology Research Database</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Natural Science Collection</collection><collection>Hospital Premium Collection</collection><collection>Hospital Premium Collection (Alumni Edition)</collection><collection>ProQuest Central (Alumni) (purchase pre-March 2016)</collection><collection>Research Library (Alumni Edition)</collection><collection>Materials Science &amp; Engineering Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</collection><collection>Social Science Premium Collection</collection><collection>Advanced Technologies &amp; Aerospace Collection</collection><collection>Agricultural &amp; Environmental Science Collection</collection><collection>ProQuest Central Essentials</collection><collection>Biological Science Collection</collection><collection>eLibrary</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>Natural Science Collection</collection><collection>Earth, Atmospheric &amp; Aquatic Science Collection</collection><collection>Environmental Sciences and Pollution Management</collection><collection>ProQuest One Community College</collection><collection>Education Collection</collection><collection>ProQuest Materials Science Collection</collection><collection>ProQuest Central Korea</collection><collection>ANTE: Abstracts in New Technology &amp; Engineering</collection><collection>Engineering Research Database</collection><collection>Health Research Premium Collection</collection><collection>Health Research Premium Collection (Alumni)</collection><collection>ProQuest Central Student</collection><collection>Research Library Prep</collection><collection>Aerospace Database</collection><collection>Copper Technical Reference Library</collection><collection>AIDS and Cancer Research Abstracts</collection><collection>SciTech Premium Collection</collection><collection>Materials Research Database</collection><collection>ProQuest Computer Science Collection</collection><collection>Consumer Health Database (Alumni Edition)</collection><collection>ProQuest Health &amp; Medical Complete (Alumni)</collection><collection>Materials Science Database</collection><collection>Civil Engineering Abstracts</collection><collection>ProQuest Engineering Collection</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>ProQuest Biological Science Collection</collection><collection>Computer and Information Systems Abstracts – Academic</collection><collection>Computer and Information Systems Abstracts Professional</collection><collection>Agriculture Science Database</collection><collection>Education Database</collection><collection>Consumer Health Database</collection><collection>Health &amp; Medical Collection (Alumni Edition)</collection><collection>Medical Database</collection><collection>ProQuest research library</collection><collection>Science Database</collection><collection>Algology Mycology and Protozoology Abstracts (Microbiology C)</collection><collection>Biological Science Database</collection><collection>Engineering Database</collection><collection>Research Library (Corporate)</collection><collection>ProQuest advanced technologies &amp; aerospace journals</collection><collection>ProQuest Advanced Technologies &amp; Aerospace Collection</collection><collection>Biotechnology and BioEngineering Abstracts</collection><collection>Environmental Science Database</collection><collection>Earth, Atmospheric &amp; Aquatic Science Database</collection><collection>Materials Science Collection</collection><collection>ProQuest One Education</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 China</collection><collection>Engineering collection</collection><collection>Environmental Science Collection</collection><collection>ProQuest Central Basic</collection><collection>University of Michigan</collection><collection>Genetics Abstracts</collection><collection>Meteorological &amp; Geoastrophysical Abstracts</collection><collection>Meteorological &amp; Geoastrophysical Abstracts - Academic</collection><collection>MEDLINE - Academic</collection><jtitle>Science (American Association for the Advancement of Science)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Smith, E. J.</au><au>Marsden, R. G.</au><au>Balogh, A.</au><au>Gloeckler, G.</au><au>Geiss, J.</au><au>McComas, D. J.</au><au>McKibben, R. B.</au><au>MacDowall, R. J.</au><au>Lanzerotti, L. J.</au><au>Krupp, N.</au><au>Krueger, H.</au><au>Landgraf, M.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The Sun and Heliosphere at Solar Maximum</atitle><jtitle>Science (American Association for the Advancement of Science)</jtitle><addtitle>Science</addtitle><date>2003-11-14</date><risdate>2003</risdate><volume>302</volume><issue>5648</issue><spage>1165</spage><epage>1169</epage><pages>1165-1169</pages><issn>0036-8075</issn><eissn>1095-9203</eissn><coden>SCIEAS</coden><abstract>Recent Ulysses observations from the Sun's equator to the poles reveal fundamental properties of the three-dimensional heliosphere at the maximum in solar activity. The heliospheric magnetic field originates from a magnetic dipole oriented nearly perpendicular to, instead of nearly parallel to, the Sun's rotation axis. Magnetic fields, solar wind, and energetic charged particles from low-latitude sources reach all latitudes, including the polar caps. The very fast high-latitude wind and polar coronal holes disappear and reappear together. Solar wind speed continues to be inversely correlated with coronal temperature. The cosmic ray flux is reduced symmetrically at all latitudes.</abstract><cop>Washington, DC</cop><pub>American Association for the Advancement of Science</pub><pmid>14615526</pmid><doi>10.1126/science.1086295</doi><tpages>5</tpages></addata></record>
fulltext fulltext
identifier ISSN: 0036-8075
ispartof Science (American Association for the Advancement of Science), 2003-11, Vol.302 (5648), p.1165-1169
issn 0036-8075
1095-9203
language eng
recordid cdi_proquest_miscellaneous_743520626
source American Association for the Advancement of Science; JSTOR Archival Journals and Primary Sources Collection; Social Science Premium Collection; Alma/SFX Local Collection; Education Collection
subjects Astronomy
Charged particles
Cosmic rays
Earth, ocean, space
Exact sciences and technology
Geophysics
Heliosphere
Magnetic fields
Magnetic flux
Magnetic polarity
Observations
Particle radiation, solar wind
Polar caps
Review
Solar energy
Solar flares
Solar physics
Solar system
Solar wind
Sun
Sunspots
Tropical regions
title The Sun and Heliosphere at Solar Maximum
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-29T19%3A29%3A36IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-gale_proqu&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=The%20Sun%20and%20Heliosphere%20at%20Solar%20Maximum&rft.jtitle=Science%20(American%20Association%20for%20the%20Advancement%20of%20Science)&rft.au=Smith,%20E.%20J.&rft.date=2003-11-14&rft.volume=302&rft.issue=5648&rft.spage=1165&rft.epage=1169&rft.pages=1165-1169&rft.issn=0036-8075&rft.eissn=1095-9203&rft.coden=SCIEAS&rft_id=info:doi/10.1126/science.1086295&rft_dat=%3Cgale_proqu%3EA111203661%3C/gale_proqu%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c782t-789f06267c45d19aa1e2a296ee0ba32b7cdd47d09a82f1d033d100a45cb07bab3%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=213587348&rft_id=info:pmid/14615526&rft_galeid=A111203661&rft_jstor_id=3835484&rfr_iscdi=true