Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Indriani Sukma"'
Autor:
Zubaidah Indriani Sukma
Melesatnya kemajuan teknologi baik di dalam maupun luar negeri memberikan dampak yang luar biasa bagi seluruh aspek dalam kehidupan, termasuk dunia pendidikan. Untuk menyokong kemajuan mutu pendidikan dan sekolah, pendidikan sendiri harus memiliki in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ad356fd466e3cbddbb2d9a57fcf99430
https://doi.org/10.31219/osf.io/mq3rw
https://doi.org/10.31219/osf.io/mq3rw
Autor:
Indriani Sukma, Zamri Zainal Abidin
Publikováno v:
Indian Journal of Physics. 91:595-606
The study of the solar cycle and geomagnetic index associated with the seismic activity from the year 1901 to the end of 2015 has been done for an area that covers the majority of China and its bordering countries. Data of sunspot number, solar wind
Autor:
Nur Nafhatun Md Shariff, Noor Aqma Iryani Aziz, Zainol Abidin Ibrahim, N. M. Anim, Zamri Zainal Abidin, Zety Sharizat Hamidi, Nabilah Ramli, Roslan Umar, Indriani Sukma, Christian Monstein
Publikováno v:
New Astronomy Reviews. 67:18-33
Compact Astronomical Low-frequency, Low-cost Instrument for Spectroscopy in Transportable Observatories (CALLISTO) is a global network of spectrometer system with the purpose to observe the Sun's activities. There are 37 stations (using 68 instrument
Publikováno v:
Advanced Studies in Theoretical Physics. 7:1231-1234
We derived Reissner-Nordstrom solution for non-rotating charged celestial objects with Elliptical in shaped, such as stars and/or elliptical galaxies. This metric is capable to describing the behavior of gravitational field outside any charged ellips
Autor:
Zamri Zainal Abidin, Zainol Abidin Ibrahim, Zety Sharizat Hamidi, N. N.S. Hakimi, A. Mokhtar, S. Rohizat, Indriani Sukma, N. Syukri, Nur Nafhatun Md Shariff, N. M. Anim, Christian Monstein, N. Hamzan
Publikováno v:
International Journal of Fundamental Physical Sciences. :72-75
The Sun is considered as one of the strongest radio sources and observation in radio region can provide information on structures throughout the solar atmosphere. In radio wavelengths, we could possible to investigate high quality images within an ar