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<p class="MsoNormal" style="background:white"><span style="font-size:11.5pt;font-family:"Times New Roman",serif;color:black">Dear Colleagues,</span><span style="color:black"><o:p></o:p></span></p>
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<span style="font-size:11.5pt;font-family:"Times New Roman",serif;color:black">Please consider submitting an abstract to our session on ionospheric plasma irregularities and scintillation at EGU this spring. <span class="apple-converted-space"> </span></span><b><span style="font-family:"Times New Roman",serif;color:black">EGU
2021 will be fully online</span></b><span style="font-family:"Times New Roman",serif;color:black">. More information can be found at<span class="apple-converted-space"> </span></span><span style="color:black"><a href="https://gcc02.safelinks.protection.outlook.com/?url=https%3A%2F%2Fegu21.eu%2Fabout%2Fprovisional_format_of_egu21.html&data=04%7C01%7Cjeffrey.klenzing%40nasa.gov%7C4feb48fb43774bba029a08d8957f61f2%7C7005d45845be48ae8140d43da96dd17b%7C0%7C0%7C637423721618921246%7CUnknown%7CTWFpbGZsb3d8eyJWIjoiMC4wLjAwMDAiLCJQIjoiV2luMzIiLCJBTiI6Ik1haWwiLCJXVCI6Mn0%3D%7C1000&sdata=ksfeYpOKCbiGZaSHdD81EoXODe1SG8%2BV6HhQFWcU5xA%3D&reserved=0"><span style="color:#0563C1">https://egu21.eu/about/provisional_format_of_egu21.html</span></a><span class="apple-converted-space"> </span></span><span style="font-family:"Times New Roman",serif;color:black"> <span class="apple-converted-space"> </span></span><span style="color:black"><o:p></o:p></span></p>
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<span style="font-family:"Times New Roman",serif;color:black">The full session description is below.</span><span style="color:black"><o:p></o:p></span></p>
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<b><span style="font-family:"Times New Roman",serif;color:black">The abstract submission deadline is 13 January 2021, 13:00 CET.</span></b><span style="color:black"><o:p></o:p></span></p>
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<span style="font-size:11.5pt;font-family:"Times New Roman",serif;color:black">Best regards,</span><span style="color:black"><o:p></o:p></span></p>
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<span style="font-size:11.5pt;font-family:"Times New Roman",serif;color:black">-Jeff</span><span style="color:black"><o:p></o:p></span></p>
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<b><span style="font-size:11.5pt;font-family:"Helvetica Neue";color:black"> </span></b><span style="color:black"><o:p></o:p></span></p>
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<b><span style="font-size:11.5pt;font-family:"Helvetica Neue";color:black">Towards better understanding of the ionospheric plasma irregularities and scintillations</span></b><span style="color:black"><o:p></o:p></span></p>
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<span style="font-size:11.5pt;font-family:"Helvetica Neue";color:black">Convener: Chao Xiong <span class="gmail-m-505564257379987799d-none">| </span>Co-conveners: Lucilla Alfonsi, Jens Berdermann, Yaqi Jin, Jeffrey Klenzing</span><span style="color:black"><o:p></o:p></span></p>
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<span style="font-size:11.5pt;font-family:"Helvetica Neue";color:black"> </span><span style="color:black"><o:p></o:p></span></p>
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<span style="font-size:11.5pt;font-family:"Helvetica Neue";color:black"><a href="https://gcc02.safelinks.protection.outlook.com/?url=https%3A%2F%2Fmeetingorganizer.copernicus.org%2FEGU21%2Fabstractsubmission%2F40166&data=04%7C01%7Cjeffrey.klenzing%40nasa.gov%7C4feb48fb43774bba029a08d8957f61f2%7C7005d45845be48ae8140d43da96dd17b%7C0%7C0%7C637423721618921246%7CUnknown%7CTWFpbGZsb3d8eyJWIjoiMC4wLjAwMDAiLCJQIjoiV2luMzIiLCJBTiI6Ik1haWwiLCJXVCI6Mn0%3D%7C1000&sdata=OaImTnZf2wLyMNL5cz7jxGKvFC7DnjIEGxAtxQUZs8Y%3D&reserved=0" target="_blank" title="Original URL:
https://meetingorganizer.copernicus.org/EGU21/abstractsubmission/40166
Click to follow link."><span style="color:#0563C1">Abstract
submission</span></a></span><span style="color:black"><o:p></o:p></span></p>
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<span style="font-size:11.5pt;font-family:"Helvetica Neue";color:black"> </span><span style="font-family:"-webkit-standard",serif"><o:p></o:p></span></p>
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<span style="font-size:11.5pt;font-family:"Helvetica Neue";color:black">Plasma density irregularities can occur at all latitudes in the Earth’s ionosphere. However, the onset and evolution of these irregularities as well as their influence on the radio wave
signals continue to be unsolved scientific questions. The various proposed generation mechanisms, including instability growth rates and seeding processes, are strongly coupled to the neutral atmosphere and magnetospheric dynamics, making the forecasting of
ionospheric irregularities much more challenging. Recent observations from ground- and space-based measurements, as well as new innovative data analysis and modeling techniques, e.g., data assimilation and machine learning, have the potential to advance our
understanding of the ionospheric irregularities. Studies that focus on the observation, modeling and prediction of plasma irregularities of different scales are welcome at this session. The mitigation of negative effects and recent developments to forecast
scintillation effects on Global Navigation Satellite or other communication systems are also of high interest.</span><span style="font-family:"-webkit-standard",serif;color:black"><o:p></o:p></span></p>
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