Abstract

A total solar eclipse occurred on 20 March 2015, with a totality path passing mostly above the North Atlantic Ocean, which resulted in a partial solar eclipse over Belgium and large parts of Europe. In anticipation of this event, a dedicated observational campaign was set up at the Belgian Solar-Terrestrial Centre of Excellence (STCE). The objective was to perform high-quality observations of the eclipse and the associated effects on the geospace environment by utilising the advanced space- and ground-based instrumentation available to the STCE in order to further our understanding of these effects, particularly on the ionosphere. The study highlights the crucial importance of taking into account the eclipse geometry when analysing the ionospheric behaviour during eclipses and interpreting the eclipse effects. A detailed review of the eclipse geometry proves that considering the actual obscuration level and solar zenith angle at ionospheric heights is much more important for the analysis than at the commonly referenced Earth’s surface or at the plasmaspheric heights. The eclipse occurred during the recovery phase of a strong geomagnetic storm which certainly had an impact on (some of) the ionospheric characteristics and perhaps caused the omission of some “low-profile” effects. However, the analysis of the ionosonde measurements, carried out at unprecedented high rates during the eclipse, suggests the occurrence of travelling ionospheric disturbances (TIDs). Also, the high temporal and spatial resolution measurements proved very important in revealing and estimating some finer details of the delay in the ionospheric reaction and the ionospheric disturbances.

Highlights

  • A solar eclipse occurs when the Moon passes between the Sun and the Earth, obscuring the Sun from view on part of the Earth’s surface, totally or partially

  • A partial solar eclipse was observed over Belgium in the morning hours of 20 March 2015

  • The Solar-Terrestrial Centre of Excellence (STCE) observational campaign aimed at carrying out high-quality measurements that would help further our current understanding of the eclipse effects on the geospace environment, on the local ionosphere

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Summary

Introduction

A solar eclipse occurs when the Moon passes between the Sun and the Earth, obscuring the Sun from view on part of the Earth’s surface, totally or partially. Total solar eclipses provide unique conditions for observation of the Sun’s outer atmospheric layers, the solar corona, chromosphere and prominences. This paper presents observations of the total solar eclipse that occurred on 20 March 2015. The paper presents eclipse observations carried out by the Belgian Solar-Terrestrial Centre of Excellence (STCE) with various instruments at its disposal. The instrumentation and measurement techniques used in this study are presented, followed by a description of the models and operational monitoring systems developed by the STCE and used for investigating the various phenomena associated with the eclipse. The following section presents the results of the solar and plasmasphere-ionosphere observations and modelling during both the eclipse day and a control day (A). The paper concludes with a summary of all results and an outlook for further investigations

Instrumentation and measurement techniques
SWAP and LYRA instruments onboard PROBA2 satellite
Solar radio telescope
GNSS receivers and network
Digital ionospheric sounder
Ionosphere monitoring systems
Background conditions prior to and during the eclipse
Observations during the eclipse
Eclipse geometry effects on the ionospheric response
Comparison with ionospheric observations from the eclipse on 3 October 2005
Findings
Summary
Full Text
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