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Naufal, L., Mulki, F.A.M., Fatima, S., Widyanita, Zahirah, S., Satrya, C.D. and Herdiwijaya, D. (2019) Prominence Measurement of Total Solar Eclipse: March 9th 2016, Ternate, Indonesia. Journal of Physics, 771, 1-4.
http://iopscience.iop.org/article/10.1088/1742-6596/771/1/012007/pdf

has been cited by the following article:

• TITLE: Prominence Activity during the 2006 Total Solar Eclipse

  AUTHORS: Beshir Marzouk

  KEYWORDS: Total Solar Eclipse, Coronal and Chromospheric Structures, Prominence Activity, White Light Corona

  JOURNAL NAME: Natural Science, Vol.10 No.4, April 4, 2018

  ABSTRACT: During total solar eclipses, we can observe the outer atmospheric layers of the sun (chromosphere and corona). The solar corona extends to several solar radii depending on the sunspot cycle. Basic coronal structures such as polar streamers, helmet type structures wereobservedduring the 2006 total solar eclipse. Our total solar eclipse 2006 observations throughboth White light corona and H-Alpha filter allowed us to describe coronal structures and Prominence Activity. We found that the solar corona is extended to 4 times of solar radii, the existence different zones of white light corona were shown, moreover, we compared the defined features of solar corona at different observing locations along the track of total solar eclipse 2006. The solar limb activity was studied during both of partial and total eclipse phases by using H-Alpha and white light observations from Salloum, Egypt. We got same prominence activity during partial and total phases of the solar eclipse and recorded three prominences on solar limb. Finally, our processed image in a good agreement with the publishedprocessed imageswasobserved from different locations along the track of total eclipse,added, similar magnetic field structure shown in our processed image and published one.