M. Derouich

King Abdulaziz University — Saudi Arabia

Physics and Astronomy · Physical Sciences

13h-index417citations77works0.92yr avg
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Research Topics

Solar and Space Plasma Dynamics(56), Ionosphere and magnetosphere dynamics(22), Atmospheric Ozone and Climate(19), Stellar, planetary, and galactic studies(18), Geomagnetism and Paleomagnetism Studies(16)

Publications76 total

Collisional and magnetic effects on the polarization of the solar oxygen infrared triplet
Astronomy and Astrophysics·2025Open Access
Collisional and magnetic effects on the polarization of the solar oxygen infrared triplet
arXiv (Cornell University)·2025Open Access
Ensuring outcome-based curriculum coherence through systematic CLO–PLO alignment and feedback loops
Discover Education·2025Open Access
Geo-effectiveness of ICMES/MCs of different magnetic-polarity configurations
Astrophysics and Space Science·2025
Forbush decreases during strong geomagnetic storms: time delays, rigidity effects, and ICME-driven modulation
Astrophysics and Space Science·2025
Depolarization and polarization transfer rates for the C<sub>2</sub> (X<sup>1</sup> Σ<sup>+</sup><sub>g</sub>, a <sup>3</sup>Π<sub>u</sub>) + H(<sup>2</sup>S<sub>1/2</sub>) collisions in the solar photosphere
Astronomy and Astrophysics·2025Open Access
Depolarization and polarization transfer rates for the C$_2$ $(X ^1Σ^+_g, a ^3Π_u)$ + H$(^2S_{1/2})$ collisions in the solar photosphere
arXiv (Cornell University)·2025Open Access
Forbush decreases in cosmic rays during intensegeomagnetic storms
2024Open Access
On the collisional sensitivity of polarized Mg II solar lines
arXiv (Cornell University)·2024Open Access
Dynamics and solar wind control of the recovery of strong geomagnetic storms
arXiv (Cornell University)·2024Open Access
Dynamics and solar wind control of the recovery of strong geomagnetic storms
Astrophysics and Space Science·2024· 3 cited
Characteristics and development of the main phase disturbance in geomagnetic storms (<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si189.svg"><mml:mrow><mml:mi mathvariant="normal">Dst</mml:mi><mml:mo>⩽</mml:mo><mml:mo linebreak="badbreak">-</mml:mo><mml:mn>50</mml:mn><mml:mi mathvariant="normal">nT</mml:mi></mml:mrow></mml:math>)
Advances in Space Research·2024· 9 citedOpen Access
Collisional effects in modeling solar polarized lines
Astronomy and Astrophysics·2024· 1 citedOpen Access
On the collisional sensitivity of polarised Mg II solar lines
Publications of the Astronomical Society of Australia·2024
Collisions of Electrons with Alkali, Alkaline and Complex Atoms Relevant to Solar and Stellar Atmospheres
Universe·2022Open Access
Polarization Transfer Rates by Isotropic Collisions between Astrophysical SiO Molecule and Electrons
Universe·2022Open Access
Study of the development of geomagnetic storms in the magnetosphere using solar wind data of three different time resolutions
Astrophysics and Space Science·2022· 6 cited
Study of the development and mechanism of large amplitude decreases in cosmic ray intensity during geomagnetic disturbances in the magnetosphere
Advances in Space Research·2021· 5 cited
Study of the recovery characteristics of intense cosmic-ray decreases
Astrophysics and Space Science·2021· 3 cited
Depolarization of MgH Solar Lines by Collisions with Hydrogen Atoms
The Astrophysical Journal·2021Open Access
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Frequent Co-authors

B. Badruddin(16), P. S. Barklem(10), S. Sahal−Bréchot(9), V. Bommier(7), Saleh Qutub(7), O. P. M. Aslam(4), E. Landi Degl’Innocenti(3), O. Ahmed(3), F. Mustajab(3), Yulia N. Kalugina(3), G. Molodij(2), H. Asiri(2), M. Faurobert(2), R. Manso Sainz(2), Anand Kumar(2), A. Alruhaili(2), K. Kudela(1), B. J. O’Mara(1), J. Arnaud(1), Jean-Marie Malherbe(1)