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Solar wind
speed: 363.5 km/sec
density: 20.0 protons/cm3
Updated: Today at 1201 UT

X-ray Solar Flares
6-hr max: C4 1124 UT Apr09
24-hr: C4 1124 UT Apr09
Updated: Today at: 1205 UT
Daily Sun: 09 Apr 22

Strong flares are unlikely today. All of these sunspots have stable, quiet magnetic fields. Credit: SDO/HMI
Current Auroral Oval:

Planetary K-index
Now: Kp= 4 unsettled
24-hr max: Kp= 4 unsettled

Interplanetary Mag. Field
Btotal: 9.6 nT
Bz: -5.3 nT south

Updated: Today at 1201 UT
Coronal Holes: 09 Apr 22

Solar wind flowing from this equatorial coronal hole should reach Earth on April 11-12. Credit: SDO/AIA
WEAK IMPACT: Arriving a day later than expected, a CME grazed Earth's magnetic field on April 8th (0400 UT). It was a weak, glancing blow that almost escaped detection. The CME was hurled into space near the edge of the Earth-strike zone on April 3rd by a "canyon of fire" filament eruption. Its tardy arrival did not spark a geomagnetic storm.
Solar wind
speed: 521.4 km/sec
density: 7.8 protons/cm3
Updated: Today at 0540 UT

X-ray Solar Flares
6-hr max: C1 0521 UT Apr11
24-hr: C1 0521 UT Apr11
Updated: Today at: 0545 UT
Daily Sun: 11 Apr 22

Despite the recent strong performance of Solar Cycle 25, today's sun is almost blank. WIth no large sunspots to erupt, the chance of solar flares today is very low. Credit: SDO/HMI
Current Auroral Oval:

Planetary K-index
Now: Kp= 4 unsettled
24-hr max: Kp= 5 storm

Interplanetary Mag. Field
Btotal: 5.6 nT
Bz: -1.4 nT south
Updated: Today at 0540 UT
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Coronal Holes: 11 Apr 22

Solar wind flowing from this equatorial coronal hole should reach Earth on April 11-12. Credit: SDO/AIA
Solar wind
speed: 475.9 km/sec
density: 4.2 protons/cm3
Updated: Today at 0811 UT

X-ray Solar Flares
6-hr max: B2 0456 UT Apr13
24-hr: C1 1758 UT Apr12
Updated: Today at: 0815 UT
Daily Sun: 13 Apr 22


A new sunspot is emerging at the circled location. Credit: SDO/HMI
Current Auroral Oval:

Planetary K-index
Now: Kp= 3 quiet
24-hr max: Kp= 4 unsettled

Interplanetary Mag. Field
Btotal: 11.0 nT
Bz: -2.7 nT south
Updated: Today at 0810 UT
Coronal Holes: 13 Apr 22

Solar wind flowing from this equatorial coronal hole should reach Earth on April 16-17. Credit: SDO/AIA
FARSIDE EXPLOSION TARGETS MERCURY: A coronal mass ejection (CME) flew away from the farside of the sun during the late hours of April 11th. A new NASA model shows it is going to hit Mercury. Note the orange dot in this forecast animation.

https://www.spaceweather.com/images2022/12apr22/nasamodel_strip.gif

If the CME overwhelms Mercury's relatively weak magnetic field, it could scour material off the planet's surface creating a temporary atmosphere and adding material to Mercury's comet-like tail.

The farside of the sun has been active this week, with more than one significant CME. Helioseismic soundings of the farside reveal a large region of intense magnetism--probably a complex sunspot group. It will rotate over the sun's eastern limb about a week from now.
GEOMAGNETIC STORM WATCH (G2-CLASS): A CME is heading for Earth, propelled by the unexpected eruption of dead sunspot AR2987. NOAA forecasters say that G2-class geomagnetic storms are possible when the CME arrives midday on April 14th. During such storms, auroras can seen as far south as, e.g., New York and Idaho (geomagnetic latitude 55 degrees). https://spaceweatherarchive.files.wordpress.com/2022/04/s_explosion_crop2.gif?w=507&zoom=2
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Solar wind
speed: 428.3 km/sec
density: 5.5 protons/cm3
Updated: Today at 0544 UT

X-ray Solar Flares
6-hr max: B3 0545 UT Apr14
24-hr: B3 0545 UT Apr14
Updated: Today at: 0550 UT
Daily Sun: 14 Apr 22

All of these sunspots have stable, quiet magnetic fields. Strong flares today are unlikely. Credit: SDO/HMI
Current Auroral Oval:

Planetary K-index
Now: Kp= 3 quiet
24-hr max: Kp= 4 unsettled

Interplanetary Mag. Field
Btotal: 7.7 nT
Bz: -5.3 nT south
Updated: Today at 0544 UT
Coronal Holes: 14 Apr 22

Solar wind flowing from this equatorial coronal hole should reach Earth on April 17. Credit: SDO/AIA
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