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Chaos in Sunspots
2012 (English)Independent thesis Advanced level (professional degree), 20 credits / 30 HE creditsStudent thesis
Abstract [en]

The Sun's activity varies with time. The most obvious period is the one of 11 years between twominimas. The degree of maximum activity between the minimas varies from period to period. The thesis will answer the question if there can be more and longer periods in the solar activity or if the sets are random or chaotic. The investigations are made by analyzing daily solar data in a chaos data analyzer computer program and see what results come out of the tests. The results shows signs of a chaotic behavior with small signs of a period. This period is the 11 year solar cycle. In the set of geomagnetic data it was more mysterious with signs of three periods. One is the solar period but how about the other two? This could be a further study.

Place, publisher, year, edition, pages
2012. , 65 p.
Keyword [en]
Physics Chemistry Maths, Sunspot, chaos, solar, physics
Keyword [sv]
Fysik, Kemi, Matematik
Identifiers
URN: urn:nbn:se:ltu:diva-46726Local ID: 4594e446-7fc7-4522-a993-efe0da928acbOAI: oai:DiVA.org:ltu-46726DiVA: diva2:1020041
Subject / course
Student thesis, at least 30 credits
Educational program
Space Engineering, master's level
Supervisors
Note
Validerat; 20120415 (anonymous)Available from: 2016-10-04 Created: 2016-10-04Bibliographically approved

Open Access in DiVA

fulltext(1631 kB)65 downloads
File information
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55afe5ad9c23a616773aa2f4118d7af4c825189177663caf43f34beb8365f1993d86645bf06d8417ef9d0e520d6f39358fd28d0aede19246ebc3b5fe8e9761cf
Type fulltextMimetype application/pdf

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Total: 65 downloads
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CiteExportLink to record
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Citation style
  • apa
  • ieee
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  • vancouver
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Language
  • de-DE
  • en-GB
  • en-US
  • fi-FI
  • nn-NO
  • nn-NB
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  • Other locale
More languages
Output format
  • html
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