Low Solar Coronal Thermal Structure Derived from Magnetohydrostatic Model
| dc.contributor.author | Setiahadi, Bambang | |
| dc.date.accessioned | 2017-10-31T03:51:29Z | |
| dc.date.available | 2017-10-31T03:51:29Z | |
| dc.date.issued | 2017-05 | |
| dc.identifier.citation | Aschwanden, M.J., Poland, A.I., Rabin, D.M. (2001), The New Solar Corona, Annu. Rev. Astron. Astrophys., Vol. 39, pp. 175-210. [2]. Miller, D., De Groof, A., Hansteen, V.H., Peter, H. (2004), Thermal Non- 4 Equilibrium in Coronal Loops: A Road to Complex Evolution, , Multi-Wavelength Investigation of Solar Activity, Proceedings IAU Symp. No. 223, eds. A.V. Stepanov, E.E. Benevolenskaya, A.G. Kosovichev., pp. 289-294. [3]. Ofman, L., Wang, T. (2002), Hot Coronal Loop Oscillations Observed by SUMER: Slow Magnetosonoc Wave Damping by Thermal Conduction, The Astrophysical Journal, Vol. 580, pp. L85-l88. [4]. Schmieder, B., Rust, D.M., Georgoulis, M.K., Demoulin, P., Bernasconi, P.N. (2004), Emerging Flux and the Heating of Coronal Loops, The Astrophysical Journal, vol 601, pp. 530-545. [5]. Singh, J., Mineer, S., Sakurai, T., Ichimoto, K. (2007), Magnetic Nature of Coronal Loops, Bull. Astr. Soc. India, Vol. 35, pp. 437-445. [6]. Wiegelmann, T., Solanski, S.K. (2004), Similarities and Differnces Between Coronal Holes and the Quiet Sun: Are Loop Statistics the Key?, Solar Physics, Vol. 225, pp. 227-247. | in_ID |
| dc.identifier.issn | 2527-533X | |
| dc.identifier.uri | http://hdl.handle.net/11617/9361 | |
| dc.description.abstract | By assuming the Sun in quiet condition we derived coronal thermal structure for low solar coronal magnetoplasma atmosphere. Ideal gas law in a static equilibrium configuration in coronal magnetic plasma state is derived and the solution may be directed to figure-out the thermal structure in mixed plasma and magnetic fields within the low corona. The results show that corona may have hot and ‘cool’ solution in low corona under the condition when the Sun in quiet condition. | in_ID |
| dc.language.iso | id | in_ID |
| dc.publisher | Prosiding SNPBS (Seminar Nasional Pendidikan Biologi dan Saintek) Ke-2 | in_ID |
| dc.subject | Coronal equilibrium | in_ID |
| dc.subject | magnetohydrostatic | in_ID |
| dc.subject | thermal structure | in_ID |
| dc.title | Low Solar Coronal Thermal Structure Derived from Magnetohydrostatic Model | in_ID |
| dc.type | Article | in_ID |
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