dc.contributor | Universidade Estadual Paulista (UNESP) | |
dc.creator | Bryant, Jeff | |
dc.date | 2016-10-26T17:57:26Z | |
dc.date | 2016-10-26T17:57:26Z | |
dc.date.accessioned | 2017-04-06T12:16:56Z | |
dc.date.available | 2017-04-06T12:16:56Z | |
dc.identifier | http://acervodigital.unesp.br/handle/unesp/365480 | |
dc.identifier | http://objetoseducacionais2.mec.gov.br/handle/mec/10586 | |
dc.identifier.uri | http://repositorioslatinoamericanos.uchile.cl/handle/2250/961762 | |
dc.description | The number of sunspots observed on the sun has an 11-year cycle. It is easy to see the regularity of the sunspot cycle by examining observations taken over many years. Besides the 11-year cycle, there is an 80- to 90-year Gleisberg Cycle. From 1640 to 1710, an unusually low number of sunspots were observed. This period is known as the Maunder minimum. It coincided with a period of colder-than-average temperatures in northern Europe called the Little Ice Age | |
dc.description | Componente Curricular::Ensino Médio::Matemática | |
dc.publisher | Wolfram Demonstration Project | |
dc.relation | AnnualSunspotNumbers.nbp | |
dc.rights | Demonstration freeware using MathematicaPlayer | |
dc.subject | Data analysis | |
dc.subject | Educação Básica::Ensino Médio::Matemática::Análise de dados e probabilidade | |
dc.title | Annual sunspot numbers | |
dc.type | Otro | |