Climatology of successive equatorial plasma bubbles observed by GPS ROTI over Malaysia

Author:

Buhari S. M.12ORCID,Abdullah M.13,Yokoyama T.4ORCID,Otsuka Y.5,Nishioka M.4ORCID,Hasbi A. M.3,Bahari S. A.13,Tsugawa T.4

Affiliation:

1. Space Science CentreUniversiti Kebangsaan Malaysia Bangi Malaysia

2. Department of PhysicsUniversiti Teknologi Malaysia Skudai Malaysia

3. Department of Electrical, Electronics and Systems EngineeringUniversiti Kebangsaan Malaysia Bangi Malaysia

4. National Institute of Information and Communications Technology Koganei Japan

5. Institute for Space‐Earth Environmental ResearchNagoya University Nagoya Japan

Funder

Fundamental Research Grant Scheme (FRGS)

Ministry of Education Malaysia National Institute of Communications and Information Technology JSPS Core-to-Core Program B, Asia-Africa Science Platforms

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Reference32 articles.

1. The longitudinal morphology of equatorial F‐layer irregularities relevant to their occurrence;Aarons J.;Space Sci. Rev.,1993

2. Equatorial spread F development and quiet time variability under solar minimum conditions;Abdu M.;Indian J. Radio Space Phys.,2012

3. Explicit characteristics of evolutionary-type plasma bubbles observed from Equatorial Atmosphere Radar during the low to moderate solar activity years 2010-2012

4. Continuous generation and two‐dimensional structure of equatorial plasma bubbles observed by high‐density GPS receivers in Southeast Asia

5. Seasonal-longitudinal variability of equatorial plasma bubbles

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