Observations of solar pulsations

We have modified our solar magnetograph to measure velocities at the solar surface, rather than magnetic fields. Using this apparatus, we have observed fluctuations of period 2 h 40 min, which are remarkably stable. The interpretation of this phenomenon seems to cause much theoretical difficulty.

Saved in:
Bibliographic Details
Published in:Nature (London) 1976-01, Vol.259 (5539), p.87-89
Main Authors: Severny, A. B., Kotov, V. A., Tsap, T. T.
Format: Article
Language:English
Subjects:
Humanities and Social Sciences
multidisciplinary
Science
Science (multidisciplinary)
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-c290t-cb45dda788a4e1982e9d46d9cb8db9c4fe819cef296783764dcd90f4852fd3063
cites cdi_FETCH-LOGICAL-c290t-cb45dda788a4e1982e9d46d9cb8db9c4fe819cef296783764dcd90f4852fd3063
container_end_page 89
container_issue 5539
container_start_page 87
container_title Nature (London)
container_volume 259
creator Severny, A. B.
Kotov, V. A.
Tsap, T. T.
description We have modified our solar magnetograph to measure velocities at the solar surface, rather than magnetic fields. Using this apparatus, we have observed fluctuations of period 2 h 40 min, which are remarkably stable. The interpretation of this phenomenon seems to cause much theoretical difficulty.
doi_str_mv 10.1038/259087a0
format article
fullrecord <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_22530594</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>22530594</sourcerecordid><originalsourceid>FETCH-LOGICAL-c290t-cb45dda788a4e1982e9d46d9cb8db9c4fe819cef296783764dcd90f4852fd3063</originalsourceid><addsrcrecordid>eNpl0EtLxDAUBeAgCtZR8Cd0Jbqo3qRpHksZfMHAbHQd0jykQ6epuVPBf2-lunJ14PBx4R5CLincUqjVHWs0KGnhiBSUS1FxoeQxKQCYqkDV4pScIe4AoKGSF6Tcthjypz10acAyxRJTb3M5Tj0u3Tk5ibbHcPGbK_L2-PC6fq4226eX9f2mckzDoXItb7y3UinLA9WKBe258Nq1yrfa8RgU1S5EpoVUtRTcO68hctWw6GsQ9YpcLXfHnD6mgAez79CFvrdDSBMaxpoaGs1neL1AlxNiDtGMudvb_GUomJ8JzN8EM71ZKM5keA_Z7NKUh_mN__Ybyr5adQ</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>22530594</pqid></control><display><type>article</type><title>Observations of solar pulsations</title><source>Nature Journals Online</source><creator>Severny, A. B. ; Kotov, V. A. ; Tsap, T. T.</creator><creatorcontrib>Severny, A. B. ; Kotov, V. A. ; Tsap, T. T.</creatorcontrib><description>We have modified our solar magnetograph to measure velocities at the solar surface, rather than magnetic fields. Using this apparatus, we have observed fluctuations of period 2 h 40 min, which are remarkably stable. The interpretation of this phenomenon seems to cause much theoretical difficulty.</description><identifier>ISSN: 0028-0836</identifier><identifier>EISSN: 1476-4687</identifier><identifier>DOI: 10.1038/259087a0</identifier><language>eng</language><publisher>London: Nature Publishing Group UK</publisher><subject>Humanities and Social Sciences ; multidisciplinary ; Science ; Science (multidisciplinary)</subject><ispartof>Nature (London), 1976-01, Vol.259 (5539), p.87-89</ispartof><rights>Springer Nature Limited 1976</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c290t-cb45dda788a4e1982e9d46d9cb8db9c4fe819cef296783764dcd90f4852fd3063</citedby><cites>FETCH-LOGICAL-c290t-cb45dda788a4e1982e9d46d9cb8db9c4fe819cef296783764dcd90f4852fd3063</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,27898,27899</link.rule.ids></links><search><creatorcontrib>Severny, A. B.</creatorcontrib><creatorcontrib>Kotov, V. A.</creatorcontrib><creatorcontrib>Tsap, T. T.</creatorcontrib><title>Observations of solar pulsations</title><title>Nature (London)</title><addtitle>Nature</addtitle><description>We have modified our solar magnetograph to measure velocities at the solar surface, rather than magnetic fields. Using this apparatus, we have observed fluctuations of period 2 h 40 min, which are remarkably stable. The interpretation of this phenomenon seems to cause much theoretical difficulty.</description><subject>Humanities and Social Sciences</subject><subject>multidisciplinary</subject><subject>Science</subject><subject>Science (multidisciplinary)</subject><issn>0028-0836</issn><issn>1476-4687</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1976</creationdate><recordtype>article</recordtype><recordid>eNpl0EtLxDAUBeAgCtZR8Cd0Jbqo3qRpHksZfMHAbHQd0jykQ6epuVPBf2-lunJ14PBx4R5CLincUqjVHWs0KGnhiBSUS1FxoeQxKQCYqkDV4pScIe4AoKGSF6Tcthjypz10acAyxRJTb3M5Tj0u3Tk5ibbHcPGbK_L2-PC6fq4226eX9f2mckzDoXItb7y3UinLA9WKBe258Nq1yrfa8RgU1S5EpoVUtRTcO68hctWw6GsQ9YpcLXfHnD6mgAez79CFvrdDSBMaxpoaGs1neL1AlxNiDtGMudvb_GUomJ8JzN8EM71ZKM5keA_Z7NKUh_mN__Ybyr5adQ</recordid><startdate>19760101</startdate><enddate>19760101</enddate><creator>Severny, A. B.</creator><creator>Kotov, V. A.</creator><creator>Tsap, T. T.</creator><general>Nature Publishing Group UK</general><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>19760101</creationdate><title>Observations of solar pulsations</title><author>Severny, A. B. ; Kotov, V. A. ; Tsap, T. T.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c290t-cb45dda788a4e1982e9d46d9cb8db9c4fe819cef296783764dcd90f4852fd3063</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1976</creationdate><topic>Humanities and Social Sciences</topic><topic>multidisciplinary</topic><topic>Science</topic><topic>Science (multidisciplinary)</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Severny, A. B.</creatorcontrib><creatorcontrib>Kotov, V. A.</creatorcontrib><creatorcontrib>Tsap, T. T.</creatorcontrib><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Nature (London)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Severny, A. B.</au><au>Kotov, V. A.</au><au>Tsap, T. T.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Observations of solar pulsations</atitle><jtitle>Nature (London)</jtitle><stitle>Nature</stitle><date>1976-01-01</date><risdate>1976</risdate><volume>259</volume><issue>5539</issue><spage>87</spage><epage>89</epage><pages>87-89</pages><issn>0028-0836</issn><eissn>1476-4687</eissn><abstract>We have modified our solar magnetograph to measure velocities at the solar surface, rather than magnetic fields. Using this apparatus, we have observed fluctuations of period 2 h 40 min, which are remarkably stable. The interpretation of this phenomenon seems to cause much theoretical difficulty.</abstract><cop>London</cop><pub>Nature Publishing Group UK</pub><doi>10.1038/259087a0</doi><tpages>3</tpages></addata></record>
fulltext fulltext
identifier ISSN: 0028-0836
ispartof Nature (London), 1976-01, Vol.259 (5539), p.87-89
issn 0028-0836
1476-4687
language eng
recordid cdi_proquest_miscellaneous_22530594
source Nature Journals Online
subjects Humanities and Social Sciences
multidisciplinary
Science
Science (multidisciplinary)
title Observations of solar pulsations
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-03-05T18%3A32%3A54IST&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=Observations%20of%20solar%20pulsations&rft.jtitle=Nature%20(London)&rft.au=Severny,%20A.%20B.&rft.date=1976-01-01&rft.volume=259&rft.issue=5539&rft.spage=87&rft.epage=89&rft.pages=87-89&rft.issn=0028-0836&rft.eissn=1476-4687&rft_id=info:doi/10.1038/259087a0&rft_dat=%3Cproquest_cross%3E22530594%3C/proquest_cross%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c290t-cb45dda788a4e1982e9d46d9cb8db9c4fe819cef296783764dcd90f4852fd3063%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=22530594&rft_id=info:pmid/&rfr_iscdi=true