Influence of Solar Wind High‐Speed Streams on the Brazilian Low‐Latitude Ionosphere During the Descending Phase of Solar Cycle 24
Abstract This study investigates the Brazilian low‐latitude ionospheric response to CIR/HSS‐driven geomagnetic storms during the declining phase of solar cycle 24, from 2016 to 2017. In this period the geomagnetic storms were mostly moderate, SymHmin ≈ −72 nT, AEmax ≈ 1580 nT, Vswmax ≈ 690 km/s and...
Saved in:
| Main Authors: | , , , , , , , |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
Wiley
2024-12-01
|
| Series: | Space Weather |
| Online Access: | https://doi.org/10.1029/2024SW003873 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
| _version_ | 1832575421830397952 |
|---|---|
| author | S. P. Moraes‐Santos C. M. N. Cândido F. Becker‐Guedes B. Nava V. Klausner C. Borries F. S. Chingarandi T. O. Osanyin |
| author_facet | S. P. Moraes‐Santos C. M. N. Cândido F. Becker‐Guedes B. Nava V. Klausner C. Borries F. S. Chingarandi T. O. Osanyin |
| author_sort | S. P. Moraes‐Santos |
| collection | DOAJ |
| description | Abstract This study investigates the Brazilian low‐latitude ionospheric response to CIR/HSS‐driven geomagnetic storms during the declining phase of solar cycle 24, from 2016 to 2017. In this period the geomagnetic storms were mostly moderate, SymHmin ≈ −72 nT, AEmax ≈ 1580 nT, Vswmax ≈ 690 km/s and lasted, on average, for 6 days. We analyze the variations in Vertical Total Electron Content (VTEC) at three representative regions: bele, over the equatorial region; boav and cuib, at the northern and southern crests of the Equatorial Ionization Anomaly. Our findings reveal the role of High‐Speed Solar Wind Streams and Corotating Interaction Region—driven geomagnetic storms. The VTEC intensifications were up to 30 TECu, during the daytime and nighttime. Additionally, three categories of nighttime enhancements were observed and analyzed with distinct characteristics and levels of pre‐reversal strengthening; Depletions up to 20 TECu also occurred during the day and nighttime. The delay between the storm commencement and the positive and negative variations were, on average, 7 and 20 hours, respectively. We discuss the Prompt Penetration Electric Fields and Disturbance Dynamo Electric Fields following the magnetic reconnection between Earth's and interplanetary magnetic field, using observational data and modeling. Furthermore, this study presents catalogs of low‐latitude ionospheric storms, providing detailed information for space weather applications and ionospheric modeling. |
| format | Article |
| id | doaj-art-5d073ae9a6a141e9878ddea3d1fd23d0 |
| institution | Kabale University |
| issn | 1542-7390 |
| language | English |
| publishDate | 2024-12-01 |
| publisher | Wiley |
| record_format | Article |
| series | Space Weather |
| spelling | doaj-art-5d073ae9a6a141e9878ddea3d1fd23d02025-02-01T08:10:33ZengWileySpace Weather1542-73902024-12-012212n/an/a10.1029/2024SW003873Influence of Solar Wind High‐Speed Streams on the Brazilian Low‐Latitude Ionosphere During the Descending Phase of Solar Cycle 24S. P. Moraes‐Santos0C. M. N. Cândido1F. Becker‐Guedes2B. Nava3V. Klausner4C. Borries5F. S. Chingarandi6T. O. Osanyin7National Institute for Space Research São José dos Campos BrazilUniversity of the Vale of Paraíba UNIVAP São José dos Campos BrazilNational Institute for Space Research São José dos Campos BrazilThe Abdus Salam International Centre for Theoretical Physics (ICTP) Trieste ItalyUniversity of the Vale of Paraíba UNIVAP São José dos Campos BrazilGerman Aerospace Center (DLR) Institute for Solar‐Terrestrial Physics Neustrelitz GermanyNational Institute for Space Research São José dos Campos BrazilNational Institute for Space Research São José dos Campos BrazilAbstract This study investigates the Brazilian low‐latitude ionospheric response to CIR/HSS‐driven geomagnetic storms during the declining phase of solar cycle 24, from 2016 to 2017. In this period the geomagnetic storms were mostly moderate, SymHmin ≈ −72 nT, AEmax ≈ 1580 nT, Vswmax ≈ 690 km/s and lasted, on average, for 6 days. We analyze the variations in Vertical Total Electron Content (VTEC) at three representative regions: bele, over the equatorial region; boav and cuib, at the northern and southern crests of the Equatorial Ionization Anomaly. Our findings reveal the role of High‐Speed Solar Wind Streams and Corotating Interaction Region—driven geomagnetic storms. The VTEC intensifications were up to 30 TECu, during the daytime and nighttime. Additionally, three categories of nighttime enhancements were observed and analyzed with distinct characteristics and levels of pre‐reversal strengthening; Depletions up to 20 TECu also occurred during the day and nighttime. The delay between the storm commencement and the positive and negative variations were, on average, 7 and 20 hours, respectively. We discuss the Prompt Penetration Electric Fields and Disturbance Dynamo Electric Fields following the magnetic reconnection between Earth's and interplanetary magnetic field, using observational data and modeling. Furthermore, this study presents catalogs of low‐latitude ionospheric storms, providing detailed information for space weather applications and ionospheric modeling.https://doi.org/10.1029/2024SW003873 |
| spellingShingle | S. P. Moraes‐Santos C. M. N. Cândido F. Becker‐Guedes B. Nava V. Klausner C. Borries F. S. Chingarandi T. O. Osanyin Influence of Solar Wind High‐Speed Streams on the Brazilian Low‐Latitude Ionosphere During the Descending Phase of Solar Cycle 24 Space Weather |
| title | Influence of Solar Wind High‐Speed Streams on the Brazilian Low‐Latitude Ionosphere During the Descending Phase of Solar Cycle 24 |
| title_full | Influence of Solar Wind High‐Speed Streams on the Brazilian Low‐Latitude Ionosphere During the Descending Phase of Solar Cycle 24 |
| title_fullStr | Influence of Solar Wind High‐Speed Streams on the Brazilian Low‐Latitude Ionosphere During the Descending Phase of Solar Cycle 24 |
| title_full_unstemmed | Influence of Solar Wind High‐Speed Streams on the Brazilian Low‐Latitude Ionosphere During the Descending Phase of Solar Cycle 24 |
| title_short | Influence of Solar Wind High‐Speed Streams on the Brazilian Low‐Latitude Ionosphere During the Descending Phase of Solar Cycle 24 |
| title_sort | influence of solar wind high speed streams on the brazilian low latitude ionosphere during the descending phase of solar cycle 24 |
| url | https://doi.org/10.1029/2024SW003873 |
| work_keys_str_mv | AT spmoraessantos influenceofsolarwindhighspeedstreamsonthebrazilianlowlatitudeionosphereduringthedescendingphaseofsolarcycle24 AT cmncandido influenceofsolarwindhighspeedstreamsonthebrazilianlowlatitudeionosphereduringthedescendingphaseofsolarcycle24 AT fbeckerguedes influenceofsolarwindhighspeedstreamsonthebrazilianlowlatitudeionosphereduringthedescendingphaseofsolarcycle24 AT bnava influenceofsolarwindhighspeedstreamsonthebrazilianlowlatitudeionosphereduringthedescendingphaseofsolarcycle24 AT vklausner influenceofsolarwindhighspeedstreamsonthebrazilianlowlatitudeionosphereduringthedescendingphaseofsolarcycle24 AT cborries influenceofsolarwindhighspeedstreamsonthebrazilianlowlatitudeionosphereduringthedescendingphaseofsolarcycle24 AT fschingarandi influenceofsolarwindhighspeedstreamsonthebrazilianlowlatitudeionosphereduringthedescendingphaseofsolarcycle24 AT toosanyin influenceofsolarwindhighspeedstreamsonthebrazilianlowlatitudeionosphereduringthedescendingphaseofsolarcycle24 |