The cosmic ray differential diurnal variation dependences on the zenith angle and the geomagnetic disturbance
Simultaneous and continuous muon measurements in two opposite azimuthal directions under equal zenith angles demonstrated the importance of this method for cosmic ray diurnal variation investigations. Lately these measurements were extended by means of improved telescopes. The obtained cosmic ray di...
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creator | Kavlakov, S. Georgiev, L. |
description | Simultaneous and continuous muon measurements in two opposite azimuthal directions under equal zenith angles demonstrated the importance of this method for cosmic ray diurnal variation investigations. Lately these measurements were extended by means of improved telescopes. The obtained cosmic ray diurnal variations were presented as intensity differential curves. Theoretical investigations connected the properties of these curves with some interplanetary spece parameters. The harmonics of these curves were interpreted physically. Some order difference curves were introduced. In earlier works some dependences between the parameters characterizing the first and the second harmonics of the differential intensity curves and the geomagnetic activity were found. Then all measurements were carried out under only one zenith angle. The results of investigations of similar dependences using data of simultaneous measurements under three different zenith angles are presented. |
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Lately these measurements were extended by means of improved telescopes. The obtained cosmic ray diurnal variations were presented as intensity differential curves. Theoretical investigations connected the properties of these curves with some interplanetary spece parameters. The harmonics of these curves were interpreted physically. Some order difference curves were introduced. In earlier works some dependences between the parameters characterizing the first and the second harmonics of the differential intensity curves and the geomagnetic activity were found. Then all measurements were carried out under only one zenith angle. The results of investigations of similar dependences using data of simultaneous measurements under three different zenith angles are presented.</description><language>eng</language><publisher>Legacy CDMS</publisher><subject>Space Radiation</subject><creationdate>1985</creationdate><rights>Copyright Determination: GOV_PUBLIC_USE_PERMITTED</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>309,776,796</link.rule.ids><linktorsrc>$$Uhttps://ntrs.nasa.gov/citations/19850026720$$EView_record_in_NASA$$FView_record_in_$$GNASA$$Hfree_for_read</linktorsrc></links><search><creatorcontrib>Kavlakov, S.</creatorcontrib><creatorcontrib>Georgiev, L.</creatorcontrib><title>The cosmic ray differential diurnal variation dependences on the zenith angle and the geomagnetic disturbance</title><description>Simultaneous and continuous muon measurements in two opposite azimuthal directions under equal zenith angles demonstrated the importance of this method for cosmic ray diurnal variation investigations. Lately these measurements were extended by means of improved telescopes. The obtained cosmic ray diurnal variations were presented as intensity differential curves. Theoretical investigations connected the properties of these curves with some interplanetary spece parameters. The harmonics of these curves were interpreted physically. Some order difference curves were introduced. In earlier works some dependences between the parameters characterizing the first and the second harmonics of the differential intensity curves and the geomagnetic activity were found. Then all measurements were carried out under only one zenith angle. The results of investigations of similar dependences using data of simultaneous measurements under three different zenith angles are presented.</description><subject>Space Radiation</subject><fulltext>true</fulltext><rsrctype>conference_proceeding</rsrctype><creationdate>1985</creationdate><recordtype>conference_proceeding</recordtype><sourceid>CYI</sourceid><recordid>eNqFjMEKwkAMRHvxIOofeNgfEGpFq2dR_IDeS-xmt4FuKtlU0K83iHcvM8wMb-ZFanp03ZgTdU7g5TyFgIKsBIOFSdj8CUKgNLLz-ED2yB1mZ1ENfiOT9g44Dmjqv2XEMUFkVLv1lHWSOxi0LGYBhoyrny-K9fXSnG8bhgwtq-R2ezruy7I61FW5-zN_ANZVPmY</recordid><startdate>19850801</startdate><enddate>19850801</enddate><creator>Kavlakov, S.</creator><creator>Georgiev, L.</creator><scope>CYE</scope><scope>CYI</scope></search><sort><creationdate>19850801</creationdate><title>The cosmic ray differential diurnal variation dependences on the zenith angle and the geomagnetic disturbance</title><author>Kavlakov, S. ; Georgiev, L.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-nasa_ntrs_198500267203</frbrgroupid><rsrctype>conference_proceedings</rsrctype><prefilter>conference_proceedings</prefilter><language>eng</language><creationdate>1985</creationdate><topic>Space Radiation</topic><toplevel>online_resources</toplevel><creatorcontrib>Kavlakov, S.</creatorcontrib><creatorcontrib>Georgiev, L.</creatorcontrib><collection>NASA Scientific and Technical Information</collection><collection>NASA Technical Reports Server</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Kavlakov, S.</au><au>Georgiev, L.</au><format>book</format><genre>proceeding</genre><ristype>CONF</ristype><atitle>The cosmic ray differential diurnal variation dependences on the zenith angle and the geomagnetic disturbance</atitle><date>1985-08-01</date><risdate>1985</risdate><abstract>Simultaneous and continuous muon measurements in two opposite azimuthal directions under equal zenith angles demonstrated the importance of this method for cosmic ray diurnal variation investigations. Lately these measurements were extended by means of improved telescopes. The obtained cosmic ray diurnal variations were presented as intensity differential curves. Theoretical investigations connected the properties of these curves with some interplanetary spece parameters. The harmonics of these curves were interpreted physically. Some order difference curves were introduced. In earlier works some dependences between the parameters characterizing the first and the second harmonics of the differential intensity curves and the geomagnetic activity were found. Then all measurements were carried out under only one zenith angle. The results of investigations of similar dependences using data of simultaneous measurements under three different zenith angles are presented.</abstract><cop>Legacy CDMS</cop><oa>free_for_read</oa></addata></record> |
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subjects | Space Radiation |
title | The cosmic ray differential diurnal variation dependences on the zenith angle and the geomagnetic disturbance |
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