Magnetic Kelvin–Helmholtz instability in the solar atmosphere H Cavus, D Kazkapan New Astronomy 25, 89-94, 2013 | 22 | 2013 |
On the effects of viscosity on the shock waves for a hydrodynamical case—part I: basic mechanism H Cavus Advances in Astronomy 2013, 2013 | 12 | 2013 |
Predicting CME arrival time through data integration and ensemble learning KA Alobaid, Y Abduallah, JTL Wang, H Wang, H Jiang, Y Xu, ... Frontiers in Astronomy and Space Sciences 9, 1013345, 2022 | 10 | 2022 |
Can Solar Cycle 25 Be a New Dalton Minimum? GC Coban, A Raheem, H Cavus, M Asghari-Targhi Solar Physics 296 (11), 1-15, 2021 | 8 | 2021 |
On the viscosity effects in the shock wave observed in the solar wind after the December 13, 2006 coronal mass ejection H Çavuş Astrophysical Bulletin 70, 117-122, 2015 | 8 | 2015 |
Correlation between sunspots and interplanetary shocks measured by ACE during 1998–2014 and some estimations for the 22nd solar cycle and the years between 2015 and 2018 with … H Cavus, G Araz, GC Coban, A Raheem, AI Karafistan Advances in Space Research 65 (3), 1035-1047, 2020 | 7 | 2020 |
A magnetohydrodynamic model applied to the lower convective region in the Sun H Cavus, AI Karafistan Monthly Notices of the Royal Astronomical Society 380 (1), 142-148, 2007 | 6 | 2007 |
A viscous magnetohydrodynamic Kelvin–Helmholtz instability in the interface of two fluid layers: Part I. Basic mechanism GA Hoshoudy, H Cavus, A Mahdy Astrophysics and Space Science 364, 1-16, 2019 | 5 | 2019 |
Kelvin–Helmholtz instability of two finite-thickness fluid layers with continuous density and velocity profiles GA Hoshoudy, H Cavus Journal of Astrophysics and Astronomy 39, 1-10, 2018 | 5 | 2018 |
Effects of viscosity on the behavior of entropy change in the shock wave that occurred after the December 13, 2006 coronal mass ejection H Çavuş, A Kurt Astrophysical Bulletin 70, 220-225, 2015 | 5 | 2015 |
On the modelling of rotational effects in the lower convective region of the sun H Cavus, AI Karafistan Brazilian journal of physics 40, 160-165, 2010 | 5 | 2010 |
Modelling the magnetic field and differential rotation effects for the vicinity of the base of convective zone in the Sun H Cavus New Astronomy 14 (4), 349-355, 2009 | 4 | 2009 |
An investigation of the causal relationship between sunspot groups and coronal mass ejections by determining source active regions A Raheem, H Cavus, GC Coban, AC Kinaci, H Wang, JTL Wang Monthly Notices of the Royal Astronomical Society 506 (2), 1916-1926, 2021 | 2 | 2021 |
Predicting the physical parameters of interplanetary shock waves using Artificial Neural Networks trained on NASA’s ACE and WIND spacecrafts GC Coban, A Raheem, H Cavus 2020 4th International Symposium on Multidisciplinary Studies and Innovative …, 2020 | 2 | 2020 |
A viscous magnetohydrodynamic Kelvin–Helmholtz instability in the interface of two fluid layer: Part II. An application to the atmosphere of the Sun H Cavus, GA Hoshoudy Astrophysics and Space Science 364, 1-7, 2019 | 2 | 2019 |
Effect of viscosity on shock waves observed after two different coronal mass ejection activities CME20/11/2003 and CME11/04/2010 H Cavus, G Zeybek Astrophysics 60 (1), 100-110, 2017 | 2 | 2017 |
Treatment of viscosity in the shock waves observed after two consecutive coronal mass ejection activities CME08/03/2012 and CME15/03/2012 H Cavus Earth, Moon, and Planets 118, 91-101, 2016 | 2 | 2016 |
Son Yıllarda Temel Bilimlerde Oluşan Üniversite Sınavlarındaki Kontenjan Problemi ve Çözüm Önerileri H Cavus, O Demircan International Conference on Quality in Higher Education 2016, 2016 | 2 | 2016 |
A magnetohydrodynamic model applied to the lower convective region in the Sun including the radial components of magnetic field and flow H Cavus New Astronomy 14 (8), 700-707, 2009 | 2 | 2009 |
Güneş kabuğundaki konvektif olayların manyetohidrodinamik (mhd) yaklaşımla modellenmesi H Çavuş Fen Bilimleri Enstitüsü, 2007 | 2 | 2007 |