Please use this identifier to cite or link to this item: https://repository.sustech.edu/handle/123456789/9317
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dc.contributor.authorHamid, Hamid Altaher
dc.contributor.authorHassan, Abubakr Abdalmonim
dc.contributor.authorSupervisor - Magdi Elfadil Yousif Suliman
dc.date.accessioned2014-12-28T10:03:39Z
dc.date.available2014-12-28T10:03:39Z
dc.date.issued2014-06-20
dc.identifier.citationHamid,Hamid Altaher.SUNSPOTS RELATION WITH GEOMAGNETIC INDICES/Hamid Altaher Hamid,Abubakr Abdalmonim Hassan;Magdi Elfadil Yousif Suliman.-khartoum:Sudan University of Science and Technology,College of Science,2014.-36p. :ill;28cm.-Basheors,search .en_US
dc.identifier.urihttp://repository.sustech.edu/handle/123456789/9317
dc.descriptionBachelors,searchen_US
dc.description.abstractIn this project we studied the Sun, its structure and the relation of sunspots to the geomagnetic indices. The geomagnetic indices have been very well defined to describe the conditions on the Sun-Earth system; in this regard, it is worth to mention that the Sun heats the Earth’s atmosphere and a degree of ionization in the ionosphere increases at the dayside and this causes convection in ionosphere. Solar wind sweeps towards Earth at supersonic speed ranging from 300 to 1000 km/s distorts the Earth’s magnetic field and shape the magnetosphere. And when calculating the disturbance storm time index (Dst) we shall find that the negative Dst value means that the Earth's magnetic field is weakened. This is particularly the case during solar storms, which weakened the Earth’s magnetic field at or near the magnetic equator.en_US
dc.description.sponsorshipSudan University of Science and Technologyen_US
dc.language.isoenen_US
dc.publisherSudan University of Science and Technologyen_US
dc.subjectScientific Laboratoriesen_US
dc.subjectSUNSPOTS RELATIONen_US
dc.subjectGEOMAGNETICen_US
dc.subjectionosphere increasesen_US
dc.titleSUNSPOTS RELATION WITH GEOMAGNETIC INDICESen_US
dc.typeThesisen_US
Appears in Collections:Bachelor of Science

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