Production of coronal mass ejections in relation with complex solar radio burst type III correlated with single solar radio burst type III

• Autorzy: Hussien N.H. , Hamidi Z.S. , Ali M.O. , Sabri S.N.U. , Zainol N.H. , Shariff N.M. , Moinstein C.
• Języki publikacji: EN

Abstrakty

EN

• Wydawca: -
• Czasopismo: World Scientific News
• Rocznik: 2016
• Tom: 36
• Opis fizyczny: p.96-108,fig.,ref.

Twórcy

autor

Hussien N.H.

• School of Physics and Material Sciences, Faculty of Sciences, MARA University of Technology, 40450, Shah Alam, Selangor, Malaysia

autor

Hamidi Z.S.

• School of Physics and Material Sciences, Faculty of Sciences, MARA University of Technology, 40450, Shah Alam, Selangor, Malaysia

autor

Ali M.O.

• School of Physics and Material Sciences, Faculty of Sciences, MARA University of Technology, 40450, Shah Alam, Selangor, Malaysia

autor

Sabri S.N.U.

• School of Physics and Material Sciences, Faculty of Sciences, MARA University of Technology, 40450, Shah Alam, Selangor, Malaysia

autor

Zainol N.H.

• School of Physics and Material Sciences, Faculty of Sciences, MARA University of Technology, 40450, Shah Alam, Selangor, Malaysia

autor

Shariff N.M.

• Academy of Contemporary Islamic Studies (ACIS), MARA University of Technology, 40450, Shah Alam, Selangor, Malaysia

autor

Moinstein C.

• Institute of Astronomy, Wolfgang-Pauli-Strasse 27, Building HIT, Floor J, 8093 Zurich, Switzerland