Solar radio burst type III due to M 2.9 class flare with a geomagnetic disturbance

• Autorzy: Hamidi Z.S. , Ali M.O. , Shariff N.N.M. , Monstein C. , Zainol N.H. , Hussien N.H. , Ramli N. , Farid M.S.
• Języki publikacji: EN

Abstrakty

EN

• Wydawca: -
• Czasopismo: World Scientific News
• Rocznik: 2016
• Tom: 44
• Opis fizyczny: p.155-167,fig.,ref.

Twórcy

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

Shariff N.N.M.

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

autor

Monstein C.

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

autor

Zainol N.H.

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

autor

Hussien N.H.

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

autor

Ramli N.

• Physics Department, Faculty of Science, University of Malaya, 50603, Kuala Lumpur, Malaysia

autor

Farid M.S.

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