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<span
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Colleagues,</span></p>
<p
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<span
style="font-family: "Segoe UI", "Segoe UI Web (West European)", -apple-system, BlinkMacSystemFont, Roboto, "Helvetica Neue", sans-serif; font-size: 15px; color: rgb(14, 16, 26); background-color: initial;"><br>
</span></p>
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<span
style="font-family: "Segoe UI", "Segoe UI Web (West European)", -apple-system, BlinkMacSystemFont, Roboto, "Helvetica Neue", sans-serif; font-size: 15px; color: rgb(14, 16, 26); background-color: initial;">We
invite you to contribute by submitting an abstract to the <b>EGU25
(EGU General Assembly) session</b></span></p>
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<span
style="font-family: "Segoe UI", "Segoe UI Web (West European)", -apple-system, BlinkMacSystemFont, Roboto, "Helvetica Neue", sans-serif; font-size: 15px; color: rgb(14, 16, 26); background-color: initial;"><b>EMRP2.5 "LEO
satellites for Exploring Earth’s Magnetic Field and
Ionospheric/Thermospheric Environment"</b></span></p>
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<span
style="font-family: "Segoe UI", "Segoe UI Web (West European)", -apple-system, BlinkMacSystemFont, Roboto, "Helvetica Neue", sans-serif; font-size: 15px; color: rgb(14, 16, 26); background-color: initial;">scheduled
for
<b>27 April–2 May 2025, Vienna</b>, Austria.</span></p>
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<span
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</span></p>
<p
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<span
style="font-family: "Segoe UI", "Segoe UI Web (West European)", -apple-system, BlinkMacSystemFont, Roboto, "Helvetica Neue", sans-serif; font-size: 15px; color: rgb(14, 16, 26); background-color: initial;">The
<b>abstract submission deadline</b> is Wednesday, <b>15 January</b> 2025,
at <b>13:00 CET</b>. <br>
</span></p>
<p
style="text-align: left; text-indent: 0px; background-color: initial; margin-top: 0pt; margin-bottom: 0pt;"><span
style="font-family: "Segoe UI", "Segoe UI Web (West European)", -apple-system, BlinkMacSystemFont, Roboto, "Helvetica Neue", sans-serif; font-size: 15px; color: rgb(14, 16, 26); background-color: initial;"><b>Session
Link</b>:
<a class="moz-txt-link-freetext" href="https://meetingorganizer.copernicus.org/EGU25/session/51729">https://meetingorganizer.copernicus.org/EGU25/session/51729</a><br>
</span></p>
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<span
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submission Link</b>:
<a
href="https://meetingorganizer.copernicus.org/EGU25/abstractsubmission/51729"
id="LPlnk299138" style="margin-top: 0px; margin-bottom: 0px;"
class="moz-txt-link-freetext">
https://meetingorganizer.copernicus.org/EGU25/abstractsubmission/51729</a></span></p>
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<span
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</span></p>
<p
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<span
style="font-family: "Segoe UI", "Segoe UI Web (West European)", -apple-system, BlinkMacSystemFont, Roboto, "Helvetica Neue", sans-serif; font-size: 15px; color: rgb(14, 16, 26); background-color: rgb(255, 255, 255);"><b>EMRP2.5</b></span><span
style="font-family: "Segoe UI", "Segoe UI Web (West European)", -apple-system, BlinkMacSystemFont, Roboto, "Helvetica Neue", sans-serif; font-size: 15px; color: rgb(14, 16, 26); background-color: initial;"><b>session
summary:</b></span></p>
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<span
style="font-family: "Segoe UI", "Segoe UI Web (West European)", -apple-system, BlinkMacSystemFont, Roboto, "Helvetica Neue", sans-serif; font-size: 15px; color: rgb(14, 16, 26); background-color: initial;"><i>Launched
in November 2013, the ESA Earth Explorer Swarm satellite trio
has provided, for one solar cycle, continuous accurate
measurements of the magnetic field, accompanied by plasma and
electric field measurements, precise navigation, and
accelerometer observations.<br>
The polar-orbiting Swarm satellites are augmented with
absolute magnetic scalar and vector data from the
low-inclination Macau Science Satellite 1 (MSS-1, since May
2023, 41° inclination, covering all Local Times within 2
months) and with absolute scalar field measurements from the
CSES satellite (since 2018, fixed 02/14 LT near-polar orbit)
which significantly extend the data coverage in space and
time.<br>
In addition, the ESA Scout NanoMagSat constellation consisting
of one near-polar and two 60° inclination satellites, is now
also in the pipeline, with a sequence of launches planned to
start at the end of 2027 for full operation in 2028. It will
acquire absolute vector magnetic data at 1 Hz, very low noise
scalar and vector magnetic field data at 2 kHz, electron
density data at 2 kHz and electron temperature data at 1 Hz.
It will also acquire navigation data, enabling top-side TEC
retrieval, and collect ionospheric radio-occultation profiles.<br>
<br>
This session invites contributions on investigations in
geomagnetism, ionospheric and thermospheric sciences related
to Earth and near-Earth processes, with focus on existing and
planned Low-Earth-Orbiting satellites. Combined analyses of
satellite- and ground-based or model data are welcome.</i></span></p>
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<span style="background-color: initial;"><br>
</span></div>
<p
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<span
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look forward to your valuable contributions and appreciate your
attention and interest.</span></p>
<p
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<span
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</span></p>
<p class="elementToProof"
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<span
style="font-family: "Segoe UI", "Segoe UI Web (West European)", -apple-system, BlinkMacSystemFont, Roboto, "Helvetica Neue", sans-serif; font-size: 15px; color: rgb(14, 16, 26); background-color: initial;">Sincerely
yours,<br>
the session conveners<br>
Martin Fillion, Jose van den IJssel, Claudia Stolle, and Nils
Olsen</span></p>
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