The Royal Observatory at Belgium has issued its latest report:
COMMENT: The solar activity has been quiet over the past 24 hours. The
X-ray flux was below C-level. The sunspot (Catania sunspot group 9, NOAA
Active region 2734) remained stable and continued to show mild activity
with few A and small B-class flares. Solar activity is expected to remain
at low levels with a very small chance of C-class flare.No Earth directed Coronal Mass Ejection has been observed. The greater than
10 MeV solar protons flux remained at nominal levels over the past 24 hours
and is expected to remain so.The solar wind parameters are currently slightly enhanced due to several
small patchy equatorial coronal holes (negative polarity) that have now
rotated into the west hemisphere. During the last 24-hour, the solar wind
speed was about 500 km/s at the beginning of the period and then decreased
to about 400 km/s. The total interplanetary magnetic field strength ranged
between 5 nT and 8 nT. The Bz component fluctuated between -4 nT and 6.5
nT. Another small patchy equatorial coronal hole (negative polarity) is
currently facing Earth. The slightly enhanced solar wind parameters are
expected to persist for more days, due to all those small patchy equatorial
coronal holes on the surface of the Sun.The geomagnetic conditions were quiet to unsettle over the past 24 hours,
with K-index (Dourbes) ranging from 1 and 3, and Kp (NOAA) ranging from 1
and 2. In response to the slightly enhanced interplanetary magnetic field
and possible prolonged period of southward directed Bz component, the
geomagnetic conditions are expected to remain quiet to unsettle.TODAY'S ESTIMATED ISN : 017, BASED ON 15 STATIONS.
NOAA's flux chart shows that the solar activity remains in the lowest A basement.
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