1 Ocak 2018 Dergi makalesi Açık Erişim

Kilcik, A.; Yurchyshyn, V; Sahin, S.; Sarp, V; Obridko, V; Ozguc, A.; Rozelot, J. P.

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  <identifier identifierType="URL">https://aperta.ulakbim.gov.tr/record/28649</identifier>
  <creators>
    <creator>
      <creatorName>Kilcik, A.</creatorName>
      <givenName>A.</givenName>
      <familyName>Kilcik</familyName>
      <affiliation>Akdeniz Univ, Fac Sci, Dept Space Sci &amp; Technol, TR-07058 Antalya, Turkey</affiliation>
    </creator>
    <creator>
      <creatorName>Yurchyshyn, V</creatorName>
      <givenName>V</givenName>
      <familyName>Yurchyshyn</familyName>
    </creator>
    <creator>
      <creatorName>Sahin, S.</creatorName>
      <givenName>S.</givenName>
      <familyName>Sahin</familyName>
      <affiliation>Akdeniz Univ, Fac Sci, Dept Space Sci &amp; Technol, TR-07058 Antalya, Turkey</affiliation>
    </creator>
    <creator>
      <creatorName>Sarp, V</creatorName>
      <givenName>V</givenName>
      <familyName>Sarp</familyName>
      <affiliation>Akdeniz Univ, Fac Sci, Dept Space Sci &amp; Technol, TR-07058 Antalya, Turkey</affiliation>
    </creator>
    <creator>
      <creatorName>Obridko, V</creatorName>
      <givenName>V</givenName>
      <familyName>Obridko</familyName>
      <affiliation>Russian Acad Sci, IZMIRAN, Pushkov Inst Terr Magnetism Ionosphere &amp; Radio Wa, Moscow 142190, Russia</affiliation>
    </creator>
    <creator>
      <creatorName>Ozguc, A.</creatorName>
      <givenName>A.</givenName>
      <familyName>Ozguc</familyName>
    </creator>
    <creator>
      <creatorName>Rozelot, J. P.</creatorName>
      <givenName>J. P.</givenName>
      <familyName>Rozelot</familyName>
    </creator>
  </creators>
  <titles>
    <title>The Evolution Of Flaring And Non-Flaring Active Regions</title>
  </titles>
  <publisher>Aperta</publisher>
  <publicationYear>2018</publicationYear>
  <dates>
    <date dateType="Issued">2018-01-01</date>
  </dates>
  <resourceType resourceTypeGeneral="Text">Journal article</resourceType>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://aperta.ulakbim.gov.tr/record/28649</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsIdenticalTo">10.1093/mnras/sty388</relatedIdentifier>
  </relatedIdentifiers>
  <rightsList>
    <rights rightsURI="http://www.opendefinition.org/licenses/cc-by">Creative Commons Attribution</rights>
    <rights rightsURI="info:eu-repo/semantics/openAccess">Open Access</rights>
  </rightsList>
  <descriptions>
    <description descriptionType="Abstract">According to the modified Zurich classification, sunspot groups are classified into seven different classes (A, B, C, D, E, F and H) based on their morphology and evolution. In this classification, classes A and B, which are small groups, describe the beginning of sunspot evolution, while classes D, E and F describe the large and evolved groups. Class C describes the middle phase of sunspot evolution and the class H describes the end of sunspot evolution. Here, we compare the lifetime and temporal evolution of flaring and non-flaring active regions (ARs), and the flaring effect on ARs in these groups in detail for the last two solar cycles (1996 through 2016). Our main findings are as follows: (i) Flaring sunspot groups have longer lifetimes than non-flaring ones. (ii) Most of the class A, B and C flaring ARs rapidly evolve to higher classes, while this is not applicable for non-flaring ARs. More than 50 per cent of the flaring A, B and C groups changed morphologically, while the remaining D, E, F and H groups did not change remarkably after the flare activity. (iii) 75 per cent of all flaring sunspot groups are large and complex. (iv) There is a significant increase in the sunspot group area in classes A, B, C, D and H after flaring activity. In contrast, the sunspot group area of classes E and F decreased. The sunspot counts of classes D, E and F decreased as well, while classes A, B, C and H showed an increase.</description>
  </descriptions>
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