Subject: MM#009 Default Target" --><br>
<span id="date"><dfn>Date</dfn>: Wed, 21 Oct 2020 20:01:13 +0100</span><br /><br>
</address> <pre> </pre> Dear Collaborators,
<br />Solar activity is at a very low level. NOAA 12776 has decayed
slightly since the last message, once again losing spot area.
This region has now been confirmed as an alpha/H-type sunspot
group and has been flare-quiet since yesterday's B3.6 event.
Several A-class events and the largest flare of the period (a
B3.5 flare on 20-Oct-2020 at 22:58 UT) were produced by a weak
flux region in the North West quadrant that currently displays
a few small pores. Additional low B-class flares are possible
over the following 24-hour period as this region rotates up to
the North West limb.
<br />The approximate position of this region on 21-Oct-2020 at 18:00 UT is:
<br />N29W80 , ( 831&quot;, 452&quot; )
<br />See <a href="http://www.SolarMonitor.org">http://www.SolarMonitor.org</a> for images and
<a href="http://solar.physics.montana.edu/max_millennium/ops/observing.shtml">http://solar.physics.montana.edu/max_millennium/ops/observing.shtml</a>
for a description of the current Max Millennium Observing Plan. <br />Regards,
<br />Shaun Bloomfield (Northumbria University)
<span id="received"><dfn>Received on</dfn> Wed Oct 21 2020 - 13:01:26 MDT</span>
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