Sunspot monitoring by using optical telescope / Amira Atiya Zal'ulya Mohd Amir
Sunspots are temporary phenomena on the sun's photosphere that appears as spots darker than surroundings area. It is the regions where the temperature is lowers than others region. It is caused by the concentrations of magnetic field flux that inhibit convection. This spots may last for a fe...
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| Format: | Student Project |
| Language: | English |
| Published: |
Faculty of Applied Sciences
2018
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| Subjects: | |
| Online Access: | https://ir.uitm.edu.my/id/eprint/24815/ |
| _version_ | 1848806092094570496 |
|---|---|
| author | Mohd Amir, Amira Atiya Zal'ulya |
| author_facet | Mohd Amir, Amira Atiya Zal'ulya |
| author_sort | Mohd Amir, Amira Atiya Zal'ulya |
| building | UiTM Institutional Repository |
| collection | Online Access |
| description | Sunspots are temporary phenomena on the sun's photosphere that appears as spots
darker than surroundings area. It is the regions where the temperature is lowers than
others region. It is caused by the concentrations of magnetic field flux that inhibit
convection. This spots may last for a few months, however it will eventually decay.
It comes in many shapes and sizes but often appear in groups. The numbers of
sunspots follows on 11 year cycle. The objectives of this research to assist potential
data user in the data mining and retrieving process, to study the sun's behavior from
sunspot monitoring, to compare the image of the sun atf different wavelength, to
understand how the sun work and also to develop a future capacity of sunspot
prediction, thereby contributing to the global forecasting the variable, space weather
conditions. To monitor the sunspot, we need to observe it and take a picture of it
everyday. From the picture we will compare it day by day with the data from the
Solar Dynamic Observatory at different wavelength. This research can be perform
efficiently if the weather is clear for the optical telescope. |
| first_indexed | 2025-11-14T22:21:25Z |
| format | Student Project |
| id | uitm-24815 |
| institution | Universiti Teknologi MARA |
| institution_category | Local University |
| language | English |
| last_indexed | 2025-11-14T22:21:25Z |
| publishDate | 2018 |
| publisher | Faculty of Applied Sciences |
| recordtype | eprints |
| repository_type | Digital Repository |
| spelling | uitm-248152019-07-19T02:45:40Z https://ir.uitm.edu.my/id/eprint/24815/ Sunspot monitoring by using optical telescope / Amira Atiya Zal'ulya Mohd Amir Mohd Amir, Amira Atiya Zal'ulya QC Physics Optics. Light Sunspots are temporary phenomena on the sun's photosphere that appears as spots darker than surroundings area. It is the regions where the temperature is lowers than others region. It is caused by the concentrations of magnetic field flux that inhibit convection. This spots may last for a few months, however it will eventually decay. It comes in many shapes and sizes but often appear in groups. The numbers of sunspots follows on 11 year cycle. The objectives of this research to assist potential data user in the data mining and retrieving process, to study the sun's behavior from sunspot monitoring, to compare the image of the sun atf different wavelength, to understand how the sun work and also to develop a future capacity of sunspot prediction, thereby contributing to the global forecasting the variable, space weather conditions. To monitor the sunspot, we need to observe it and take a picture of it everyday. From the picture we will compare it day by day with the data from the Solar Dynamic Observatory at different wavelength. This research can be perform efficiently if the weather is clear for the optical telescope. Faculty of Applied Sciences 2018 Student Project NonPeerReviewed text en https://ir.uitm.edu.my/id/eprint/24815/1/PPb_AMIRA%20ATIYA%20ZAL%27ULYA%20MOHD%20AMIR%20AS%20C%2018_5.PDF Mohd Amir, Amira Atiya Zal'ulya (2018) Sunspot monitoring by using optical telescope / Amira Atiya Zal'ulya Mohd Amir. (2018) [Student Project] <http://terminalib.uitm.edu.my/24815.pdf> (Unpublished) |
| spellingShingle | QC Physics Optics. Light Mohd Amir, Amira Atiya Zal'ulya Sunspot monitoring by using optical telescope / Amira Atiya Zal'ulya Mohd Amir |
| title | Sunspot monitoring by using optical telescope / Amira Atiya Zal'ulya Mohd Amir |
| title_full | Sunspot monitoring by using optical telescope / Amira Atiya Zal'ulya Mohd Amir |
| title_fullStr | Sunspot monitoring by using optical telescope / Amira Atiya Zal'ulya Mohd Amir |
| title_full_unstemmed | Sunspot monitoring by using optical telescope / Amira Atiya Zal'ulya Mohd Amir |
| title_short | Sunspot monitoring by using optical telescope / Amira Atiya Zal'ulya Mohd Amir |
| title_sort | sunspot monitoring by using optical telescope / amira atiya zal'ulya mohd amir |
| topic | QC Physics Optics. Light |
| url | https://ir.uitm.edu.my/id/eprint/24815/ |