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<p class="MsoNormal"><span style="font-family:"Times New Roman",serif;color:black">Dear Colleagues,<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">We would like to invite you to submit an abstract to the <b>ST3.2 session in Ionosphere and Thermosphere</b> program group to be held at the EGU General Assembly 2022, April 3-8 in Vienna, Austria.<span class="apple-converted-space"> <o:p></o:p></span></span></p>
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<p class="MsoNormal"><span class="apple-converted-space"><span style="font-family:"Times New Roman",serif;color:black">Note that the abstract deadline has been extended to Jan 14.<o:p></o:p></span></span></p>
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<b><span style="font-family:"Times New Roman",serif;color:black">Abstract submission:<span class="apple-converted-space"> </span></span></b><span style="font-family:"Times New Roman",serif;color:black"><a href="https://meetingorganizer.copernicus.org/EGU22/session/43637" title="https://meetingorganizer.copernicus.org/EGU22/session/43637">https://meetingorganizer.copernicus.org/EGU22/session/43637</a></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">ST4.2 - 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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<u><span style="font-family:"Times New Roman",serif;color:black">Session details</span></u><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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<i><span style="font-family:"Times New Roman",serif;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 class="apple-converted-space"> </span></span></i><span style="color:black"><o:p></o:p></span></p>
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<span style="font-family:"Times New Roman",serif;color:black">We look forward to receiving your contributions and thank you very much for your attention.<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">Sincerely yours, session conveners,<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">Chao Xiong,<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">Lucilla Alfonsi,<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">Jens Berdermann,<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">Yaqi Jin,<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">Jeffrey Klenzing</span><span style="color:black"><o:p></o:p></span></p>
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