An analysis of active regions 11036 characteristics leads to solar flare class C7.2 phenomena

• Autorzy: Zainol N.H. , Hamidi Z.S. , Husien N. , Ali M.O. , Sabri S.N.U. , Shariff N.N.M. , Faid M.S. , Monstein C. , Ramli N.
• Języki publikacji: EN

Abstrakty

EN

• Wydawca: -
• Czasopismo: World Scientific News
• Rocznik: 2016
• Tom: 45
• Numer: 2
• Opis fizyczny: p.80-91,fig.,ref.

Twórcy

autor

Zainol 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

Husien N.

• 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

Shariff N.N.M.

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

autor

Faid M.S.

• 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

Ramli N.

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