Some MHD solutions for the bottom of the solar convective layer
| dc.authorid | Cavus, Huseyin/0000-0003-4224-7039 | |
| dc.contributor.author | Cavus, H. | |
| dc.contributor.author | Karafistan, A. I. | |
| dc.date.accessioned | 2025-01-27T21:05:48Z | |
| dc.date.available | 2025-01-27T21:05:48Z | |
| dc.date.issued | 2007 | |
| dc.department | Çanakkale Onsekiz Mart Üniversitesi | |
| dc.description | Workshop on Solar and Stellar Physics through Eclipses -- MAR 27-29, 2006 -- Ankara Univ, ORSEM Campus, Side, Antalya, TURKEY | |
| dc.description.abstract | The magnetic field responsible for the solar activity is stored in the base of the convective zone. Applying this knowledge to the bottom of the convection zone in the Sun our objective was to investigate some magnetohydrodynamical (MHD) solutions. The first order perturbation approximation was used in order to calculate the small perturbations on the physical parameters of a Standard Solar Model (SSM) excluding both rotation and magnetic field (Christensen-Dalsgaard et al. 1996) in the unperturbed equilibrium case. The validity of each approximation is tested and examined from the SSM. The MHD results thus obtained are presented graphically and compared with those of the SSM. | |
| dc.description.sponsorship | Research Foundation of the Canakkale 18 Mart University [2005/113] | |
| dc.description.sponsorship | We acknowledge with thanks partial support from the Research Foundation of the Canakkale 18 Mart University (Project No: 2005/113). We thank also Ismail Tarhan for his help in using LaTeX. | |
| dc.identifier.endpage | + | |
| dc.identifier.isbn | 978-1-583812-38-9 | |
| dc.identifier.startpage | 74 | |
| dc.identifier.uri | https://hdl.handle.net/20.500.12428/27798 | |
| dc.identifier.volume | 370 | |
| dc.identifier.wos | WOS:000246823600010 | |
| dc.identifier.wosquality | N/A | |
| dc.indekslendigikaynak | Web of Science | |
| dc.language.iso | en | |
| dc.publisher | Astronomical Soc Pacific | |
| dc.relation.ispartof | Solar and Stellar Physics Through Eclipses | |
| dc.relation.publicationcategory | Konferans Öğesi - Uluslararası - Kurum Öğretim Elemanı | |
| dc.rights | info:eu-repo/semantics/closedAccess | |
| dc.snmz | KA_WoS_20250125 | |
| dc.subject | Zone | |
| dc.subject | Models | |
| dc.title | Some MHD solutions for the bottom of the solar convective layer | |
| dc.type | Conference Object |
