Space Weather Today pinned ยซSolar wind speed: 471.9 km/sec density: 11.57 protons/cm3 Updated: Today at 0312 UT X-ray Solar Flares 6-hr max: C8 0923 UT Jan16 24-hr: M1 1515 UT Jan15 Updated: Today at: 1515 UTยป
A CME IS COMING: Minor G1-class geomagnetic storms are possible on Jan. 19th when a CME is expected to graze Earth's magnetic field. The CME was hurled into space on Jan. 14th by a dramatic twisting eruption in the magnetic canopy of sunspot AR3182. High latitude sky watchers should be alert for auroras when the CME arrives.
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Solar wind
speed: 414.3 km/sec
density: 4.12 protons/cm3
Updated: Today at 0221 UT
X-ray Solar Flares
6-hr max: C2 1221 UT Jan17
24-hr: C9 0013 UT Jan17
Updated: Today at: 1425 UT
speed: 414.3 km/sec
density: 4.12 protons/cm3
Updated: Today at 0221 UT
X-ray Solar Flares
6-hr max: C2 1221 UT Jan17
24-hr: C9 0013 UT Jan17
Updated: Today at: 1425 UT
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Space Weather Today pinned ยซSolar wind speed: 414.3 km/sec density: 4.12 protons/cm3 Updated: Today at 0221 UT X-ray Solar Flares 6-hr max: C2 1221 UT Jan17 24-hr: C9 0013 UT Jan17 Updated: Today at: 1425 UTยป
Solar wind
speed: 434.4 km/sec
density: 8.05 protons/cm3
Updated: Today at 0222 UT
X-ray Solar Flares
6-hr max: M1 1035 UT Jan18
24-hr: M1 2329 UT Jan17
Updated: Today at: 1425 UT
speed: 434.4 km/sec
density: 8.05 protons/cm3
Updated: Today at 0222 UT
X-ray Solar Flares
6-hr max: M1 1035 UT Jan18
24-hr: M1 2329 UT Jan17
Updated: Today at: 1425 UT
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Space Weather Today pinned ยซSolar wind speed: 434.4 km/sec density: 8.05 protons/cm3 Updated: Today at 0222 UT X-ray Solar Flares 6-hr max: M1 1035 UT Jan18 24-hr: M1 2329 UT Jan17 Updated: Today at: 1425 UTยป
CME IMPACT SPARKS AURORAS: Arriving earlier than expected, a CME struck Earth's magnetic field on Jan. 17th around 2200 UT. Its arrival was signaled by an abrupt shift in the interplanetary magnetic field (IMF) near Earth. The impact sparked a brief outburst of Arctic auroras, which has since subsided. https://www.spaceweather.com/images2023/14jan23/two_cmes.gif
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Solar wind
speed: 367.7 km/sec
density: 2.45 protons/cm3
Updated: Today at 0247 UT
X-ray Solar Flares
6-hr max: M1 1012 UT Jan19
24-hr: M1 1012 UT Jan19
Updated: Today at: 1450 UT
speed: 367.7 km/sec
density: 2.45 protons/cm3
Updated: Today at 0247 UT
X-ray Solar Flares
6-hr max: M1 1012 UT Jan19
24-hr: M1 1012 UT Jan19
Updated: Today at: 1450 UT
CHANCE OF FLARES: NOAA forecasters say there is a 60% chance of M-class solar flares and a 15% chance of X-flares today. The most likely source is giant sunspot AR3190, which is directly facing Earth.
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Space Weather Today pinned ยซSolar wind speed: 367.7 km/sec density: 2.45 protons/cm3 Updated: Today at 0247 UT X-ray Solar Flares 6-hr max: M1 1012 UT Jan19 24-hr: M1 1012 UT Jan19 Updated: Today at: 1450 UTยป
Solar wind
speed: 392.7 km/sec
density: 1.37 protons/cm3
Updated: Today at 0217 UT
X-ray Solar Flares
6-hr max: C5 1407 UT Jan20
24-hr: C6 0152 UT Jan20
Updated: Today at: 1420 UT
speed: 392.7 km/sec
density: 1.37 protons/cm3
Updated: Today at 0217 UT
X-ray Solar Flares
6-hr max: C5 1407 UT Jan20
24-hr: C6 0152 UT Jan20
Updated: Today at: 1420 UT
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CHANCE OF FLARES: NOAA forecasters say there is a 60% chance of M-class solar flares and a 15% chance of X-flares today. The most likely source is giant sunspot AR3190, which is directly facing Earth.
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Solar wind
speed: 513.3 km/sec
density: 10.83 protons/cm3
Updated: Today at 0221 UT
X-ray Solar Flares
6-hr max: C6 0959 UT Jan23
24-hr: M1 1702 UT Jan22
Updated: Today at: 1425 UT
speed: 513.3 km/sec
density: 10.83 protons/cm3
Updated: Today at 0221 UT
X-ray Solar Flares
6-hr max: C6 0959 UT Jan23
24-hr: M1 1702 UT Jan22
Updated: Today at: 1425 UT
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Space Weather Today pinned ยซSolar wind speed: 513.3 km/sec density: 10.83 protons/cm3 Updated: Today at 0221 UT X-ray Solar Flares 6-hr max: C6 0959 UT Jan23 24-hr: M1 1702 UT Jan22 Updated: Today at: 1425 UTยป
CHANCE OF FLARES TODAY: NOAA forecasters say there is a 55% chance of M-class solar flares and a 10% chance of X-flares today, Jan. 23rd. The most likely flare-sites are sunspots AR3190 and AR3194, which have unstable 'delta-class' magnetic fields.
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