Fractions of proton, helium, middle and heavy nuclei in primary cosmic rays at energy 1016eV
Classification of gamma-hadron families, registered by the Pamir collaboration, on four groups of nuclei (P, He, middle and heavy), responsible for their generation, is made, and fractions of families in each of the groups are estimated. Results show, that below the knee of the energy spectrum the c...
Gespeichert in:
Veröffentlicht in: | arXiv.org 2001-07 |
---|---|
Hauptverfasser: | , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | |
---|---|
container_issue | |
container_start_page | |
container_title | arXiv.org |
container_volume | |
creator | Kalmakhelidze, Maia Roinishvili, Nina Svanidze, Manana |
description | Classification of gamma-hadron families, registered by the Pamir collaboration, on four groups of nuclei (P, He, middle and heavy), responsible for their generation, is made, and fractions of families in each of the groups are estimated. Results show, that below the knee of the energy spectrum the chemical composition of primary cosmic rays remains close to the normal one. |
format | Article |
fullrecord | <record><control><sourceid>proquest</sourceid><recordid>TN_cdi_proquest_journals_2092517416</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2092517416</sourcerecordid><originalsourceid>FETCH-proquest_journals_20925174163</originalsourceid><addsrcrecordid>eNqNjUsKwjAURYMgWLR7eOC0hXz60bFYXIA4EkpIU01pEk1SIbs3Axfg6MI5B-4KZZQxUh4qSjco937CGNOmpXXNMnTvHBdBWePBjvByNlhTwFPOatEFaDUMswRuhoT4J4JZxCwVKJNSpbmLIKzXSoDj0QMPII10jwgEk0bedmg98tnL_LdbtO_O19OlTD_vRfrQT3ZxJqme4iOtSVuRhv1XfQE2i0Ig</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2092517416</pqid></control><display><type>article</type><title>Fractions of proton, helium, middle and heavy nuclei in primary cosmic rays at energy 1016eV</title><source>Freely Accessible Journals</source><creator>Kalmakhelidze, Maia ; Roinishvili, Nina ; Svanidze, Manana</creator><creatorcontrib>Kalmakhelidze, Maia ; Roinishvili, Nina ; Svanidze, Manana</creatorcontrib><description>Classification of gamma-hadron families, registered by the Pamir collaboration, on four groups of nuclei (P, He, middle and heavy), responsible for their generation, is made, and fractions of families in each of the groups are estimated. Results show, that below the knee of the energy spectrum the chemical composition of primary cosmic rays remains close to the normal one.</description><identifier>EISSN: 2331-8422</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Chemical composition ; Cosmic rays ; Energy spectra ; Heavy nuclei ; Helium ; Knee ; Nuclei (nuclear physics) ; Organic chemistry ; Primary cosmic rays</subject><ispartof>arXiv.org, 2001-07</ispartof><rights>2001. This work is published under https://arxiv.org/licenses/assumed-1991-2003/license.html (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>781,785</link.rule.ids></links><search><creatorcontrib>Kalmakhelidze, Maia</creatorcontrib><creatorcontrib>Roinishvili, Nina</creatorcontrib><creatorcontrib>Svanidze, Manana</creatorcontrib><title>Fractions of proton, helium, middle and heavy nuclei in primary cosmic rays at energy 1016eV</title><title>arXiv.org</title><description>Classification of gamma-hadron families, registered by the Pamir collaboration, on four groups of nuclei (P, He, middle and heavy), responsible for their generation, is made, and fractions of families in each of the groups are estimated. Results show, that below the knee of the energy spectrum the chemical composition of primary cosmic rays remains close to the normal one.</description><subject>Chemical composition</subject><subject>Cosmic rays</subject><subject>Energy spectra</subject><subject>Heavy nuclei</subject><subject>Helium</subject><subject>Knee</subject><subject>Nuclei (nuclear physics)</subject><subject>Organic chemistry</subject><subject>Primary cosmic rays</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2001</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><recordid>eNqNjUsKwjAURYMgWLR7eOC0hXz60bFYXIA4EkpIU01pEk1SIbs3Axfg6MI5B-4KZZQxUh4qSjco937CGNOmpXXNMnTvHBdBWePBjvByNlhTwFPOatEFaDUMswRuhoT4J4JZxCwVKJNSpbmLIKzXSoDj0QMPII10jwgEk0bedmg98tnL_LdbtO_O19OlTD_vRfrQT3ZxJqme4iOtSVuRhv1XfQE2i0Ig</recordid><startdate>20010706</startdate><enddate>20010706</enddate><creator>Kalmakhelidze, Maia</creator><creator>Roinishvili, Nina</creator><creator>Svanidze, Manana</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope></search><sort><creationdate>20010706</creationdate><title>Fractions of proton, helium, middle and heavy nuclei in primary cosmic rays at energy 1016eV</title><author>Kalmakhelidze, Maia ; Roinishvili, Nina ; Svanidze, Manana</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-proquest_journals_20925174163</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2001</creationdate><topic>Chemical composition</topic><topic>Cosmic rays</topic><topic>Energy spectra</topic><topic>Heavy nuclei</topic><topic>Helium</topic><topic>Knee</topic><topic>Nuclei (nuclear physics)</topic><topic>Organic chemistry</topic><topic>Primary cosmic rays</topic><toplevel>online_resources</toplevel><creatorcontrib>Kalmakhelidze, Maia</creatorcontrib><creatorcontrib>Roinishvili, Nina</creatorcontrib><creatorcontrib>Svanidze, Manana</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Access via ProQuest (Open Access)</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></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Kalmakhelidze, Maia</au><au>Roinishvili, Nina</au><au>Svanidze, Manana</au><format>book</format><genre>document</genre><ristype>GEN</ristype><atitle>Fractions of proton, helium, middle and heavy nuclei in primary cosmic rays at energy 1016eV</atitle><jtitle>arXiv.org</jtitle><date>2001-07-06</date><risdate>2001</risdate><eissn>2331-8422</eissn><abstract>Classification of gamma-hadron families, registered by the Pamir collaboration, on four groups of nuclei (P, He, middle and heavy), responsible for their generation, is made, and fractions of families in each of the groups are estimated. Results show, that below the knee of the energy spectrum the chemical composition of primary cosmic rays remains close to the normal one.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | EISSN: 2331-8422 |
ispartof | arXiv.org, 2001-07 |
issn | 2331-8422 |
language | eng |
recordid | cdi_proquest_journals_2092517416 |
source | Freely Accessible Journals |
subjects | Chemical composition Cosmic rays Energy spectra Heavy nuclei Helium Knee Nuclei (nuclear physics) Organic chemistry Primary cosmic rays |
title | Fractions of proton, helium, middle and heavy nuclei in primary cosmic rays at energy 1016eV |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-11T19%3A09%3A12IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest&rft_val_fmt=info:ofi/fmt:kev:mtx:book&rft.genre=document&rft.atitle=Fractions%20of%20proton,%20helium,%20middle%20and%20heavy%20nuclei%20in%20primary%20cosmic%20rays%20at%20energy%201016eV&rft.jtitle=arXiv.org&rft.au=Kalmakhelidze,%20Maia&rft.date=2001-07-06&rft.eissn=2331-8422&rft_id=info:doi/&rft_dat=%3Cproquest%3E2092517416%3C/proquest%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2092517416&rft_id=info:pmid/&rfr_iscdi=true |