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Solar wind
speed: 496.4 km/sec
density: 5.37 protons/cm3
more data: ACE, DSCOVR
Updated: Today at 0931 UT

X-ray Solar Flares
6-hr max: B3 0426 UT Jun01
24-hr: B5 1508 UT May31
explanation | more data
Updated: Today at: 0935 UT
Daily Sun: 01 Jun 22


A new sunspot is growing rapidly at the circled location. 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: 2.40 nT
Bz: -1.44 nT south
more data: ACE, DSCOVR
Updated: Today at 0931 UT
Coronal Holes: 01 Jun 22



There are no significant coronal holes on the Earthside of the sun. Credit: SDO/AIA
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EXPLODING COMET DEBRIS: Have you ever seen a piece of a comet explode? Francis Murphy did on Monday night in Thorndale, Pennsylvania:

https://spaceweathergallery.com/submissions/pics/f/Francis-Murphy-May_31st_2022_Meteor_Chart_1654037263.gif

The tau Herculid meteor shower was underway as debris from Comet 73P/Schwassmann-Wachmann 3 peppered the top of Earth's atmosphere. This piece of the broken comet disintegrated 90 km above above the ground, spreading its remains across the edge of space.

"The meteor's trail twisted and turned in high altitude winds," says Murphy. "It was the brightest of 10 to 15 tau Herculids we saw during a 3-hour observing session."

In Mormon Lake, Arizona, astronomer David Blanchard saw the same thing--twice. This video shows two tau Herculids disintegrating in a star field with satellites and airplanes whizzing by.
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FARSIDE SUNSPOTS: Right now, there are sunspots on the farside of the sun so big they are affecting the way the sun vibrates.

Helioseismologists have detected their echoes in the latest farside map from NASA's Solar Dynamics Observatory. Don't be surprised if we see CMEs billowing away from the farside of the sun in the days ahead.
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Solar wind
speed: 375.5 km/sec
density: 2.58 protons/cm3
more data: ACE, DSCOVR
Updated: Today at 0516 UT

X-ray Solar Flares
6-hr max: B7 0403 UT Jun02
24-hr: B8 1147 UT Jun01
explanation | more data
Updated: Today at: 0520 UT
Daily Sun: 01 Jun 22


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


Planetary K-index
Now: Kp= 1 quiet
24-hr max: Kp= 2 quiet
explanation | more data

Interplanetary Mag. Field
Btotal: 3.58 nT
Bz: -1.19 nT south
more data: ACE, DSCOVR
Updated: Today at 0516 UT
POSSIBLE WEAK CME IMPACT PREDICTED: Yesterday, a magnetic filament on the sun erupted (movie), hurling a faint CME into space. NOAA forecasters say it could hit Earth's magnetic field on June 5th or 6th. Even weak CME strikes can cause geomagnetic storms, so there is a chance of minor G1-class storms when the CME arrives.

https://www.spaceweather.com/images2022/01jun22/erupting_filament.gif
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Solar wind
speed: 333.4 km/sec
density: 3.23 protons/cm3
more data: ACE, DSCOVR
Updated: Today at 0716 UT

X-ray Solar Flares
6-hr max: B8 0248 UT Jun03
24-hr: B8 0248 UT Jun03
explanation | more data
Updated: Today at: 0720 UT
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Daily Sun: 03 Jun 22


Sunspot AR3027 has a reversed magnetic polarity. Credit: SDO/HMI
Current Auroral Oval:


Planetary K-index
Now: Kp= 1 quiet
24-hr max: Kp= 2 quiet
explanation | more data

Interplanetary Mag. Field
Btotal: 3.95 nT
Bz: -2.11 nT south
more data: ACE, DSCOVR
Updated: Today at 0717 UT
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Coronal Holes: 03 Jun 22



There are no significant coronal holes on the Earthside of the sun. Credit: SDO/AIA
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🚨CME NEAR-MISS POSSIBLE ON JUNE 5TH: A minor coronal mass ejection (CME) that left the sun on June 1st will pass close to Earth on June 5th, according to NOAA analysts. It might come close enough for a glancing blow. High latitude sky watchers should be alert for auroras when the CME arrives this weekend.
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Solar wind
speed: 295.9 km/sec
density: 6.49 protons/cm3
more data: ACE, DSCOVR
Updated: Today at 1040 UT

X-ray Solar Flares
6-hr max: B3 0748 UT Jun04
24-hr: B5 0126 UT Jun04
explanation | more data
Updated: Today at: 1045 UT
Daily Sun: 04 Jun 22



Sunspot AR3027 has a reversed magnetic polarity. Credit: SDO/HMI
Current Auroral Oval:

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

Interplanetary Mag. Field
Btotal: 3.73 nT
Bz: -1.04 nT south
more data: ACE, DSCOVR
Updated: Today at 1046 UT
Coronal Holes: 04 Jun 22



There are no significant coronal holes on the Earthside of the sun. Credit: SDO/AIA