collaborators

5 papers

astro-ph.SR2018

The solar nitrogen abundance under the LTE assumption

Sameh I. S, M. M. Beheary, Abdelrazek M. K. Shaltout

The solar chemical abundances studied in considerable detail because of discrepant values of solar metallicity inferred from different indicators, where in the present work we have…

astro-ph.SR2018

Estimating the coronal and chromospheric magnetic fields of solar active regions as observed with the Nobeyama Radioheliograph Compared with the Extrapolated Linear Force-Free Field

A. Mouner, Abdelrazek M. K. Shaltout, M. M. Beheary +2

Adopting the thermal free-free emission mechanism, the coronal and chromospheric magnetic fields are derived from the polarization and spectral observations with the Nobeyama Radio…

astro-ph.SR2017

Inference of chromospheric magnetic fields in a sunspot derived from spectropolarimetry of Ca II 8542 A

Ali G. A. Abdelkawy, Abdelrazek M. K. Shaltout, M. M. Beheary +1

We analyze spectropolarimetric observations of the chromospheric Ca II 8542 A line taken by the Interferometric Bidimensional Spectrometer (IBIS) at the Dunn Solar Telescope. The d…

astro-ph.SR2017

The chromospheric magnetic field in active regions derived from spectropolarimetry of Ca II 8542

Ali G. A. Abdelkawy, Abdelrazek M. K. Shaltout, M. M. Beheary

We analyze spectropolarimetric observations of the chromospheric Ca II 8542 line taken by the Interferometric Bidimensional Spectrometer (IBIS) at the Dunn Solar Telescope and phot…

astro-ph.SR2017

The LTE solar abundance of neodymium

A. G. A. Abdelkawy, Abdelrazek M. K. Shaltout, M. M. Beheary +1

We study the solar photospheric abundance of singly ionized neodymium (Nd II) using high resolution spectroscopic data obtained by Fourier transform spectrograph (FTS). Based on th…