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CO-ROTATING INTERACTION REGION: Geomagnetic storms (G1-class) are possible on April 29th when a co-rotating interaction region (CIR) is expected to hit Earth's magnetic field. CIRs are transition zones between fast- and slow-moving solar wind streams. They contain shock waves and compressed magnetic fields that do a good job sparking auroras. Aurora alerts: SMS Text

AFTERGLOW OF A GEOMAGNETIC STORM: An interplanetary shock wave hit Earth's magnetic field on April 27th. It wasn't a big one--just enough to spark an unexpected G1-class geomagnetic storm. Greg Ash photographed the afterglow from Duluth, Minnesota:

"It was really neat listening to the ice growl and shift while watching the auroras," says Ash. "A meteor streaked through the frame just as I was taking the picture."

The shock wave was probably a minor CME overlooked until it hit Earth. Right now the sun is crackling with solar flares, hurling multiple overlapping CMEs into space every day. A faint CME may have slipped through the net of NOAA analysts to deliver yesterday's surprise storm. This will happen increasingly often as Solar Cycle 25 intensifies.

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A NOCTILUCENT CLOUD OVER FLORIDA: Yesterday morning in Florida, Roger Menard went to the beach at sunrise to watch the Venus-Jupiter-Moon conjunction. "I also saw a noctilucent cloud (NLC)," he says. His cell phone captured the electric-blue cloud reaching toward the planetary trio:

"It is quite unusual to see a noctilucent cloud from as far south as Florida," says Menard.

He's right. But this was no ordinary noctilucent cloud. It was a "rocket cloud." Less than an hour earlier, SpaceX launched a Falcon 9 rocket from the Kennedy Space Center carrying four astronauts to the International Space Station. Ice crystals in the rocket's exhaust caught rays of sunlight in the upper atmosphere, producing the unusual NLC.

The noctilucent cloud is gone now, but the conjunction is still underway. Venus and Jupiter are converging for a close encounter on Saturday, April 30th. Set your alarm and enjoy the show. Sky maps: April 28, 29, 30, May 1.

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  All Sky Fireball Network
Every night, a network of NASA all-sky cameras scans the skies above the United States for meteoritic fireballs. Automated software maintained by NASA's Meteoroid Environment Office calculates their orbits, velocity, penetration depth in Earth's atmosphere and many other characteristics. Daily results are presented here on Spaceweather.com.

On Apr 27, 2022, the network reported 6 fireballs.
(5 sporadics, 1 beta Pegasid)

In this diagram of the inner solar system, all of the fireball orbits intersect at a single point--Earth. The orbits are color-coded by velocity, from slow (red) to fast (blue). [Larger image] [movies]

  Near Earth Asteroids
Potentially Hazardous Asteroids (PHAs) are space rocks larger than approximately 100m that can come closer to Earth than 0.05 AU. None of the known PHAs is on a collision course with our planet, although astronomers are finding new ones all the time.
On April 28, 2022 there were 2276 potentially hazardous asteroids.
Recent & Upcoming Earth-asteroid encounters:
Asteroid
Date(UT)
Miss Distance
Velocity (km/s)
Diameter (m)
2022 GU3
2022-Apr-22
4.6 LD
8.7
25
2017 UR2
2022-Apr-22
19.4 LD
9.3
10
2022 HL1
2022-Apr-23
13.9 LD
12.9
30
2022 HQ
2022-Apr-23
8.7 LD
7
13
2022 HD
2022-Apr-24
3.7 LD
7.4
13
2022 HH1
2022-Apr-24
7.2 LD
5.2
11
2022 HA1
2022-Apr-24
17 LD
8.8
42
2020 VN1
2022-Apr-25
19.3 LD
2.3
9
2022 HB2
2022-Apr-25
2.2 LD
8.1
13
2022 HK1
2022-Apr-25
4.4 LD
5.7
7
2022 HS1
2022-Apr-25
4.4 LD
5.8
12
2022 HB1
2022-Apr-26
0.5 LD
14.1
12
418135
2022-Apr-28
8.5 LD
10.4
466
2022 HX1
2022-Apr-30
6.5 LD
11.8
15
2022 HS
2022-May-01
6.7 LD
5.7
20
2017 XO2
2022-May-01
18.8 LD
12.4
125
2022 HA2
2022-May-02
12.1 LD
12.9
38
2022 HW
2022-May-02
16.1 LD
16.1
47
2022 HW1
2022-May-03
9.9 LD
7.7
20
2022 HR1
2022-May-03
5.1 LD
13.3
23
2017 HG1
2022-May-04
18.2 LD
6
11
2022 HF1
2022-May-08
8.8 LD
17.1
62
467460
2022-May-09
14.9 LD
11.3
513
2019 JE
2022-May-11
4.9 LD
7.2
20
2012 UX68
2022-May-15
2.8 LD
8.2
54
388945
2022-May-15
15 LD
8.2
290
2013 UX
2022-May-17
16.8 LD
16.3
141
2021 WY
2022-May-18
16.9 LD
9
65
2022 HD1
2022-May-20
15.3 LD
6.8
60
7335
2022-May-27
10.5 LD
13.1
1058
2021 KO2
2022-May-30
3.1 LD
14.8
9
2020 DA4
2022-Jun-01
5.5 LD
8.9
26
2021 GT2
2022-Jun-06
9.5 LD
7.5
50
2018 LU2
2022-Jun-09
14.8 LD
10.7
16
2006 XW4
2022-Jun-12
5.9 LD
7.3
49
2022 GU6
2022-Jun-12
3.2 LD
8.4
86
Notes: LD means "Lunar Distance." 1 LD = 384,401 km, the distance between Earth and the Moon. 1 LD also equals 0.00256 AU. MAG is the visual magnitude of the asteroid on the date of closest approach.
  Cosmic Rays in the Atmosphere

SPACE WEATHER BALLOON DATA: Almost once a week, Spaceweather.com and the students of Earth to Sky Calculus fly space weather balloons to the stratosphere over California. These balloons are equipped with sensors that detect secondary cosmic rays, a form of radiation from space that can penetrate all the way down to Earth's surface. Our monitoring program has been underway without interruption for 7 years, resulting in a unique dataset of in situ atmospheric measurements.

Latest results (Nov. 2021): Our balloons have just measured a sudden drop in atmospheric radiation. It happened during the strong geomagnetic storms of Nov. 3-4, 2021. Here are the data:

This is called a "Forbush decrease," named after American physicist Scott Forbush who studied cosmic rays in the early 20th century.  It happens when a CME from the sun sweeps past Earth and literally pushes cosmic rays away from our planet. Radiation from deep space that would normally pepper Earth's upper atmosphere is briefly wiped out.

We have measured Forbush decreases before. For example, here's one from Sept. 2014. The Forbush Decrease of Nov. 3-4, 2021, was the deepest in the history of our 7-year atmospheric monitoring program. Radiation levels in the stratosphere over California dropped nearly 20%, more than doubling the previous record from our dataset. 

En route to the stratosphere, our sensors also pass through aviation altitudes, so we can sample radiation where planes fly. This plot shows how the Forbush decrease was restricted to the stratosphere; it did not affect lower levels of the atmosphere:

The dose rates shown above are expressed as multiples of sea level. For instance, we see that boarding a plane that flies at 25,000 feet exposes passengers to dose rates ~10x higher than sea level. At 40,000 feet, the multiplier is closer to 50x. The higher you fly, the more radiation you will absorb.

.Who cares? Cosmic rays are a surprisingly "down to Earth" form of space weather. They can seed clouds, trigger lightning, and penetrate commercial airplanes. According to a study from the Harvard T.H. Chan school of public health, crews of aircraft have higher rates of cancer than the general population. The researchers listed cosmic rays, irregular sleep habits, and chemical contaminants as leading risk factors. Somewhat more controversial studies (#1, #2, #3, #4) link cosmic rays with cardiac arrhythmias and sudden cardiac death.

.Technical notes: The radiation sensors onboard our helium balloons detect X-rays and gamma-rays in the energy range 10 keV to 20 MeV. These energies span the range of medical X-ray machines and airport security scanners.

Data points in the first graph ("Stratospheric Radiation") correspond to the peak of the Regener-Pfotzer maximum, which lies about 67,000 feet above central California. When cosmic rays crash into Earth's atmosphere, they produce a spray of secondary particles that is most intense at the entrance to the stratosphere. Physicists Eric Regener and Georg Pfotzer discovered the maximum using balloons in the 1930s and it is what we are measuring today.

  Essential web links
NOAA Space Weather Prediction Center
  The official U.S. government space weather bureau
Atmospheric Optics
  The first place to look for information about sundogs, pillars, rainbows and related phenomena.
Solar Dynamics Observatory
  Researchers call it a "Hubble for the sun." SDO is the most advanced solar observatory ever.
STEREO
  3D views of the sun from NASA's Solar and Terrestrial Relations Observatory
Solar and Heliospheric Observatory
  Realtime and archival images of the Sun from SOHO.
SolarMonitor.org
  information about sunspots based on the latest NOAA/USAF Active Region Summary
Daily Sunspot Summaries
  from the NOAA Space Environment Center
NOAA 27-Day Space Weather Forecasts
  fun to read, but should be taken with a grain of salt! Forecasts looking ahead more than a few days are often wrong.
Aurora 30 min forecast
  from the NOAA Space Environment Center
Live Aurora Webcam
  from Lights over Lapland
Heliophysics
  the underlying science of space weather

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Unexpected Storm Observed
April 27, 2022 @ 18:00 UTC
An unexpected geomagnetic storm today as the Bz component of the interplanetary magnetic field (IMF) decided to tip south. Minor (G1) conditions observed at 14:02 UTC. High latitude sky watchers should be alert for aurora once it is dark outside.

A minor (G1) geomagnetic storm watch was officially added beginning April 29th. A coronal hole solar wind stream is expected to reach Earth and could be responsible for displays of aurora at higher latitudes. High latitude sky watchers should be alert within the next 48-72 hours. Image below showing coronal hole #78 by SDO/HMI.

Geomagnetic Storm Watch
April 27, 2022 @ 01:20 UTC

Three Days of Coronal Mass Ejections
April 28, 2022 @ 14:20 UTC
How many coronal mass ejections have been observed over the past 3 days? Well... the answer is in the video below.

It appears that most of these plasma eruptions are farsided or off the limbs and not directed towards Earth. Sooner or later, we will be in the path. For now we wait. Composite video by LASCO C2/C3.

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