Interannual variation of a 12,760 km transequatorial ionospheric - - PowerPoint PPT Presentation

interannual variation of a 12 760 km transequatorial
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Interannual variation of a 12,760 km transequatorial ionospheric - - PowerPoint PPT Presentation

Interannual variation of a 12,760 km transequatorial ionospheric channel availability and its dependence on ionization Ferran Orga 1 , David Altadill 2 , Marcos Hervs 1 and Rosa Ma Alsina-Pags 1 1 GTM Grup de Recerca en Tecnologies Mdia,


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Interannual variation of a 12,760 km transequatorial ionospheric channel availability and its dependence on ionization

1 GTM – Grup de Recerca en Tecnologies Mèdia, La Salle – Universitat Ramon Llull;

forga@salleurl.edu, mhervas@salleurl.edu, ralsina@salleurl.edu

2 Observatori de l'Ebre, CSIC – Universitat Ramon Llull; david_altadill@obsebre.es

Ferran Orga 1, David Altadill 2, Marcos Hervás 1 and Rosa Ma Alsina-Pagès 1

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ECAS 2016

  • F. Orga, D. Altadill, M. Hervás and R.M. Alsina-Pagès

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Index

  • 1. Description of the link and the antennas
  • 2. Goals of our paper are presented
  • 3. Sounding diagram
  • 4. General dependence study for the last four surveys
  • 5. Detailed interday dependence for the 2012-13 survey
  • 6. Conclusions
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ECAS 2016

  • F. Orga, D. Altadill, M. Hervás and R.M. Alsina-Pagès

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Our HF long-haul link

La Salle and the Observatori de l’Ebre have been sounding the 12,760 km ionospheric channel from Antarctica (62.7ºS, 299.6ºE) to Spain (41.0ºN, 1.0ºE) during the last 11 years.

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ECAS 2016

  • F. Orga, D. Altadill, M. Hervás and R.M. Alsina-Pagès

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System Antennas

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ECAS 2016

  • F. Orga, D. Altadill, M. Hervás and R.M. Alsina-Pagès

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Goals

➔To prove the relation between the channel availability and the

Sun phenomena afgecting the ionization in four consecutive sounding campaigns

➔To demonstrate the importance of the Sunspot Number index

concerning the ionization of the channel

➔To study a first comparison between the four surveys and to

focus in some specific transmissions as examples

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ECAS 2016

  • F. Orga, D. Altadill, M. Hervás and R.M. Alsina-Pagès

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Diagram of the sounding

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ECAS 2016

  • F. Orga, D. Altadill, M. Hervás and R.M. Alsina-Pagès

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A Narrowband-Sounding Frame

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ECAS 2016

  • F. Orga, D. Altadill, M. Hervás and R.M. Alsina-Pagès

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Availability and FLA for the last four surveys

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SLIDE 9

ECAS 2016

  • F. Orga, D. Altadill, M. Hervás and R.M. Alsina-Pagès

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Frequencies of Large Availability

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SLIDE 10

ECAS 2016

  • F. Orga, D. Altadill, M. Hervás and R.M. Alsina-Pagès

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Two examples of covariance in 2012-13 survey

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SLIDE 11

ECAS 2016

  • F. Orga, D. Altadill, M. Hervás and R.M. Alsina-Pagès

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Conclusions

➔The narrowband propagation has strong dependence on the

solar variations due to its influence in the ionospheric performance

➔1st study: the higher the SSN, the higher the Sun activity and the

better the performance of our channel in general terms

➔2nd study: when analyzing the interday variation, a strong

inverse dependency of the SNR and SSN is shown, delayed around 6 days