Faculty Advisor
Jenesis Escobar
Faculty Advisor
Carlos Gutierrez, Rafael Gomez, Patrick Dandenault & Eduardo Araujo Pradere
Faculty Advisor
Carlos Gutierrez, Rafael Gomez, Patrick Dandenault & Eduardo Araujo Pradere
Location
FIU Wellness & Recreation Center
Start Date
8-4-2019 12:00 PM
End Date
8-4-2019 2:00 PM
Session
Poster Session 2
Abstract
This study describes the behavior of the peak value of the ionospheric concentration (foF2) during the descending phase of Solar Cycle 20. In order to understand the ionospheric dependency with the solar activity during the descending phase of solar cycle 20 (1970 to 1975), peak ionospheric values for multiple ionospheric stations have been downloaded from the National Oceanic and atmospheric Administration (NOAA)’s National Geophysics Data Center (NGDC) database and analyzed using a new approach: The study of daily maximum and minimum values. Many interesting characteristics of the ionospheric behavior were detected, while the trend of the maxima closely follows the trend of the solar activity (as captured by different indexes), the trend of the minima is 2 – 4 times less pronounced. The variability of both values seems to be consistently linked with the solar activity trend, but the clear picture does not emerge from this analysis. In order to clarify these trends, we plan to continue the exploration of the multiple dependencies of the ionospheric behavior with the solar activity.
File Type
Poster
Ionospheric Behavior During Descendant Phase of Solar Cycle 20
FIU Wellness & Recreation Center
This study describes the behavior of the peak value of the ionospheric concentration (foF2) during the descending phase of Solar Cycle 20. In order to understand the ionospheric dependency with the solar activity during the descending phase of solar cycle 20 (1970 to 1975), peak ionospheric values for multiple ionospheric stations have been downloaded from the National Oceanic and atmospheric Administration (NOAA)’s National Geophysics Data Center (NGDC) database and analyzed using a new approach: The study of daily maximum and minimum values. Many interesting characteristics of the ionospheric behavior were detected, while the trend of the maxima closely follows the trend of the solar activity (as captured by different indexes), the trend of the minima is 2 – 4 times less pronounced. The variability of both values seems to be consistently linked with the solar activity trend, but the clear picture does not emerge from this analysis. In order to clarify these trends, we plan to continue the exploration of the multiple dependencies of the ionospheric behavior with the solar activity.
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Comments
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