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FARSIDE SUNSPOTS: Today, there are 8 sunspot groups on the solar disk--the most in years. Get ready for two more. NASA's STEREO-A spacecraft is monitoring a pair of extreme ultraviolet hotspots behind the sun's eastern limb. It is probably the glow of two more sunspot groups. The active regions will rotate into view by mid-week.
Solar wind
speed: 493.7 km/sec
density: 7.29 protons/cm3
more data: ACE, DSCOVR
Updated: Today at 0132 UT

X-ray Solar Flares
6-hr max: C2 0823 UT May18
24-hr: C4 1626 UT May17
explanation | more data
Updated: Today at: 1335 UT
Daily Sun: 18 May 22


Sunspot AR3014 has a 'beta-gamma' magnetic field that poses a threat for strong M-class solar flares. Credit: SDO/HMI
Current Auroral Oval:

Planetary K-index
Now: Kp= 2 quiet
24-hr max: Kp= 3 quiet
explanation | more data

Interplanetary Mag. Field
Btotal: 5.74 nT
Bz: -1.03 nT south
more data: ACE, DSCOVR
Updated: Today at 0132 UT
Coronal Holes: 18 May 22



Solar wind flowing from this coronal hole should reach Earth on May 20-21. Credit: SDO/AIA
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DOUBLE TROUBLE: Since yesterday, big sunspot AR3014 has doubled in size. This 24-hour movie from NASA's Solar Dynamics Observatory shows the sunspot's rapid growth. AR3014 has a 'beta-gamma' magnetic field that harbors energy for strong M-class solar flares. https://www.spaceweather.com/images2022/18may22/double_anim_strip.gif
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TOTAL ECLIPSE OF THE MOON: There's something magic about the darkness that falls during a lunar eclipse. The nightscape should be flooded with moonlight. Instead, the stars pop out. On May 15th, Brad Goldpaint photographed the phenomenon from Farmington, New Mexico.

Source: https://spaceweathergallery.com/indiv_upload.php?upload_id=184898
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Solar wind
speed: 551.3 km/sec
density: 1.80 protons/cm3
more data: ACE, DSCOVR
Updated: Today at 1122 UT

X-ray Solar Flares
6-hr max: M5 0719 UT May19
24-hr: M5 0719 UT May19
explanation | more data
Updated: Today at: 1125 UT
Daily Sun: 19 May 22


Sunspot AR3014 has a 'beta-gamma-delta' magnetic field that poses a threat for X-class solar flares. Credit: SDO/HMI
Current Auroral Oval:

Planetary K-index
Now: Kp= 3 quiet
24-hr max: Kp= 3 quiet
explanation | more data

Interplanetary Mag. Field
Btotal: 4.62 nT
Bz: 4.45 nT north
more data: ACE, DSCOVR
Updated: Today at 1122 UT
Coronal Holes: 19 May 22



Solar wind flowing from this coronal hole should reach Earth on May 21st. Credit: SDO/AIA
INCREASING CHANCE OF FLARES: Big sunspot AR3014 has an unstable 'beta-gamma-delta' magnetic field that harbors energy for strong explosions. NOAA forecasters estimate a 35% chance of M-class solar flares and a 15% chance of X-flares on May 19th. Any eruptions will be geoeffective because the sunspot is directly facing Earth.
Solar wind
speed: 540.4 km/sec
density: 9.96 protons/cm3
more data: ACE, DSCOVR
Updated: Today at 0635 UT

X-ray Solar Flares
6-hr max: C1 0043 UT May20
24-hr: M5 0719 UT May19
explanation | more data
Updated: Today at: 0640 UT
Daily Sun: 20 May 22

Sunspot AR3014 has a 'beta-gamma-delta' magnetic field that poses a threat for X-class solar flares. Credit: SDO/HMI
Current Auroral Oval:

Planetary K-index
Now: Kp= 3 quiet
24-hr max: Kp= 3 quiet
explanation | more data

Interplanetary Mag. Field
Btotal: 5.44 nT
Bz: 0.67 nT north
more data: ACE, DSCOVR
Updated: Today at 0635 UT
Coronal Holes: 20 May 22



Earth is entering a stream of solar wind flowing from the indicated coronal hole. Credit: SDO/AIA
OLD VENUS PROBE TO CRASH INTO EARTH: In March 1972, Russia launched a spacecraft to Venus. The Venera probe (since renamed "Kosmos 482") never made it out of Earth orbit. A new analysis by Dr. Marco Langbroek suggests that orbital decay is bringing the old probe back to Earth. "This is a lander built to withstand atmospheric reentry [on Venus]," notes Langbroek, so it "will make for an interesting reentry sometime between 2024 and 2026."

Read: https://www.thespacereview.com/article/4384/1
ACTIVE SUNSPOT: A storm is swirling around sunspot AR3014. This morning in Romania, astronomer Maximilian Teodorescu made a 45 minute movie of the sun's atmosphere above the huge sunspot. It is literally seething.

https://www.spaceweather.com/images2022/19may22/seething_strip_opt.gif

"I caught a pretty big M-class solar flare," says Teodorescu. In addition, dark filaments of magnetism can be seen snaking through the region as lesser flares illuminate the interstices. The tumult overlies of the biggest sunspots of Solar Cycle 25 with an unstable 'beta-gamma-delta' magnetic field that harbors energy for powerful X-flares.
Solar wind
speed: 517.4 km/sec
density: 8.72 protons/cm3
Updated: Today at 1027 UT

X-ray Solar Flares
6-hr max: C3 0847 UT May23
24-hr: C4 2340 UT May22
Updated: Today at: 1030 UT