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Characteristics of equatorial plasma bubbles observed by TEC map over South America Barros, D.; Takahashi, H.; Wrasse, C. M.; Figueiredo, C. A. Instituto Nacional de Pesquisas Espaciais S ao Jos e dos Campos, S ao Paulo, Brazil


  1. Characteristics of equatorial plasma bubbles observed by TEC map over South America Barros, D.; Takahashi, H.; Wrasse, C. M.; Figueiredo, C. A. Instituto Nacional de Pesquisas Espaciais S˜ ao Jos´ e dos Campos, S˜ ao Paulo, Brazil April/2017 Diego Barros — April/2017 plasma bubles observed by tec map 1

  2. Outline 1. Introduction What are plasma bubbles? 2. Instrumentation and Metodology TEC dTEC 3. Results Characteristics of plasma bubbles observed by TEC map 4. Summary Diego Barros — April/2017 plasma bubles observed by tec map 2

  3. Outline 1. Introduction What are plasma bubbles? 2. Instrumentation and Metodology TEC dTEC 3. Results Characteristics of plasma bubbles observed by TEC map 4. Summary Diego Barros — April/2017 plasma bubles observed by tec map 2

  4. Outline 1. Introduction What are plasma bubbles? 2. Instrumentation and Metodology TEC dTEC 3. Results Characteristics of plasma bubbles observed by TEC map 4. Summary Diego Barros — April/2017 plasma bubles observed by tec map 2

  5. Outline 1. Introduction What are plasma bubbles? 2. Instrumentation and Metodology TEC dTEC 3. Results Characteristics of plasma bubbles observed by TEC map 4. Summary Diego Barros — April/2017 plasma bubles observed by tec map 2

  6. Outline 1. Introduction What are plasma bubbles? 2. Instrumentation and Metodology TEC dTEC 3. Results Characteristics of plasma bubbles observed by TEC map 4. Summary Diego Barros — April/2017 plasma bubles observed by tec map 2

  7. INTRODUCTION Diego Barros — April/2017 plasma bubles observed by tec map 3

  8. Introduction What are plasma bubbles? Plasma Bubbles are equatorial plasma irregularities; Are characterized to be a depletion of the ionospheric plasma density along the magnetic field lines; It has serious implication in trans-ionospheric communications and navigation systems. Diego Barros — April/2017 plasma bubles observed by tec map 4

  9. Introduction What are plasma bubbles? Plasma Bubbles are equatorial plasma irregularities; Are characterized to be a depletion of the ionospheric plasma density along the magnetic field lines; It has serious implication in trans-ionospheric communications and navigation systems. Diego Barros — April/2017 plasma bubles observed by tec map 4

  10. Introduction What are plasma bubbles? Plasma Bubbles are equatorial plasma irregularities; Are characterized to be a depletion of the ionospheric plasma density along the magnetic field lines; It has serious implication in trans-ionospheric communications and navigation systems. Diego Barros — April/2017 plasma bubles observed by tec map 4

  11. Introduction Plasma bubbles signatures VHF radar All Sky imager Photometer EMBRACE De Paula et al. (2011) Pimenta (2005) Diego Barros — April/2017 plasma bubles observed by tec map 5

  12. Introduction Plasma bubbles signatures VHF radar All Sky imager Photometer EMBRACE De Paula et al. (2011) Pimenta (2005) Diego Barros — April/2017 plasma bubles observed by tec map 5

  13. Introduction Plasma bubbles signatures VHF radar All Sky imager Photometer EMBRACE De Paula et al. (2011) Pimenta (2005) Diego Barros — April/2017 plasma bubles observed by tec map 6

  14. Introduction Plasma bubbles signatures Rockets - Langmuir probe Ionosonde Pimenta (2005) Muralikrishna (2006) Diego Barros — April/2017 plasma bubles observed by tec map 7

  15. Introduction Plasma bubbles signatures Rockets - Langmuir probe Ionosonde Pimenta (2005) Muralikrishna (2006) Diego Barros — April/2017 plasma bubles observed by tec map 7

  16. INSTRUMENTATION AND METODOLOGY Diego Barros — April/2017 plasma bubles observed by tec map 8

  17. Instrumentation and Metodology Measurement limitations Most of the techniques mentioned above are not able to monitor plasma bubbles continuously in a sufficiently large two dimensional area. All-sky imager - Depend on favorable weather conditions; VHF radar and ionosonde - Cannot cover a wide range; Rocket and Satellite - Only in situ measeruments; Rocket - Sporadic launching. Diego Barros — April/2017 plasma bubles observed by tec map 9

  18. Instrumentation and Metodology Measurement limitations Most of the techniques mentioned above are not able to monitor plasma bubbles continuously in a sufficiently large two dimensional area. All-sky imager - Depend on favorable weather conditions; VHF radar and ionosonde - Cannot cover a wide range; Rocket and Satellite - Only in situ measeruments; Rocket - Sporadic launching. Diego Barros — April/2017 plasma bubles observed by tec map 9

  19. Instrumentation and Metodology Measurement limitations Most of the techniques mentioned above are not able to monitor plasma bubbles continuously in a sufficiently large two dimensional area. All-sky imager - Depend on favorable weather conditions; VHF radar and ionosonde - Cannot cover a wide range; Rocket and Satellite - Only in situ measeruments; Rocket - Sporadic launching. Diego Barros — April/2017 plasma bubles observed by tec map 9

  20. Instrumentation and Metodology Measurement limitations Most of the techniques mentioned above are not able to monitor plasma bubbles continuously in a sufficiently large two dimensional area. All-sky imager - Depend on favorable weather conditions; VHF radar and ionosonde - Cannot cover a wide range; Rocket and Satellite - Only in situ measeruments; Rocket - Sporadic launching. Diego Barros — April/2017 plasma bubles observed by tec map 9

  21. Instrumentation and Metodology Measurement limitations Most of the techniques mentioned above are not able to monitor plasma bubbles continuously in a sufficiently large two dimensional area. All-sky imager - Depend on favorable weather conditions; VHF radar and ionosonde - Cannot cover a wide range; Rocket and Satellite - Only in situ measeruments; Rocket - Sporadic launching. Diego Barros — April/2017 plasma bubles observed by tec map 9

  22. Instrumentation and Metodology Measurement limitations Most of the techniques mentioned above are not able to monitor plasma bubbles continuously in a sufficiently large two dimensional area. All-sky imager - Depend on favorable weather conditions; VHF radar and ionosonde - Cannot cover a wide range; Rocket and Satellite - Only in situ measeruments; Rocket - Sporadic launching. Diego Barros — April/2017 plasma bubles observed by tec map 9

  23. Instrumentation and Metodology TEC TEC = Total Electron Content satellite � TEC = N e · ds receiver TECU = 10 16 el´ etrons/m 2 Diego Barros — April/2017 plasma bubles observed by tec map 10

  24. Instrumentation and Metodology TEC TEC = Total Electron Content satellite � TEC = N e · ds receiver TECU = 10 16 el´ etrons/m 2 Diego Barros — April/2017 plasma bubles observed by tec map 10

  25. Instrumentation and Metodology TEC TEC = Total Electron Content satellite � TEC = N e · ds receiver TECU = 10 16 el´ etrons/m 2 Diego Barros — April/2017 plasma bubles observed by tec map 10

  26. Instrumentation and Metodology TEC TEC = Total Electron Content satellite � TEC = N e · ds receiver TECU = 10 16 el´ etrons/m 2 Diego Barros — April/2017 plasma bubles observed by tec map 10

  27. Instrumentation and Metodology GNSS receivers N ◦ of satellites GNSS network GPS 32 GLONASS 24 Galileo 18 BDS 22 Total 96 -80 -75 -70 -65 -60 -55 -50 -45 -40 -35 -30 5 5 Square GPS (2017) 0 0 -5 -5 o ) -10 -10 Latitude ( N ◦ of receivers Receivers network -15 -15 LISN 30 -20 -20 IGS 29 -25 -25 RAMSAC 67 -30 -30 RBMC 101 -35 -35 RBMC RBMC RBMC RBMC RBMC RBMC RAMSAC RAMSAC RAMSAC RAMSAC RAMSAC RAMSAC Total 227 LISN LISN LISN LISN LISN LISN IGS IGS IGS IGS IGS IGS -80 -75 -70 -65 -60 -55 -50 -45 -40 -35 -30 Longitude ( o ) Figueiredo (2017) Diego Barros — April/2017 plasma bubles observed by tec map 11

  28. Instrumentation and Metodology GNSS receivers N ◦ of satellites GNSS network GPS 32 GLONASS 24 Galileo 18 BDS 22 Total 96 -80 -75 -70 -65 -60 -55 -50 -45 -40 -35 -30 5 5 Square GPS (2017) 0 0 -5 -5 o ) -10 -10 Latitude ( N ◦ of receivers -15 -15 Receivers network -20 -20 LISN 30 -25 -25 IGS 29 -30 -30 RAMSAC 67 RBMC 101 -35 -35 RBMC RBMC RBMC RBMC RBMC RBMC RAMSAC RAMSAC RAMSAC RAMSAC RAMSAC RAMSAC LISN LISN LISN LISN LISN LISN IGS IGS IGS IGS IGS IGS Total 227 -80 -75 -70 -65 -60 -55 -50 -45 -40 -35 -30 Longitude ( o ) Figueiredo (2017) Diego Barros — April/2017 plasma bubles observed by tec map 12

  29. Instrumentation and Metodology TEC map -80 -75 -70 -65 -60 -55 -50 -45 -40 -35 -30 5 5 0 0 -5 -5 o ) -10 -10 Latitude ( -15 -15 -20 -20 -25 -25 -30 -30 -35 -35 RBMC RBMC RBMC RBMC RBMC RBMC RAMSAC RAMSAC RAMSAC RAMSAC RAMSAC RAMSAC LISN LISN LISN LISN LISN LISN IGS IGS IGS IGS IGS IGS -80 -75 -70 -65 -60 -55 -50 -45 -40 -35 -30 Longitude ( o ) Diego Barros — April/2017 plasma bubles observed by tec map 13

  30. Instrumentation and Metodology TEC map Diego Barros — April/2017 plasma bubles observed by tec map 13

  31. Instrumentation and Metodology TEC map Diego Barros — April/2017 plasma bubles observed by tec map 13

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