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SpaceWeather.com -- News and information about meteor showers, solar flares, auroras, and near-Earth asteroids
 
Solar wind
speed: 391.8 km/sec
density: 2.6 protons/cm3
more data: ACE, DSCOVR
Updated: Today at 2346 UT
X-ray Solar Flares
6-hr max: B1
1843 UT Apr23
24-hr: B1
1843 UT Apr23
explanation | more data
Updated: Today at: 2300 UT
Daily Sun: 23 Apr 18
Sunspot AR2706 has a stable magnetic field that poses no threat for strong solar flares. Credit: SDO/HMI

Sunspot number: 20
What is the sunspot number?
Updated 23 Apr 2018

Spotless Days
Current Stretch: 0 days
2018 total: 67 days (60%)
2017 total: 104 days (28%)
2016 total: 32 days (9%)
2015 total: 0 days (0%)

2014 total: 1 day (<1%)
2013 total: 0 days (0%)
2012 total: 0 days (0%)
2011 total: 2 days (<1%)
2010 total: 51 days (14%)
2009 total: 260 days (71%)

Updated 23 Apr 2018


The Radio Sun
10.7 cm flux: 76 sfu
explanation | more data
Updated 23 Apr 2018

Current Auroral Oval:
Switch to: Europe, USA, New Zealand, Antarctica
Credit: NOAA/Ovation
Planetary K-index
Now: Kp= 2 quiet
24-hr max: Kp= 3
quiet
explanation | more data
Interplanetary Mag. Field
Btotal: 3.6 nT
Bz: 0.7 nT north
more data: ACE, DSCOVR
Updated: Today at 2347 UT
Coronal Holes: 23 Apr 18

Solar wind flowing from this northern cornal hole might graze Earth's magnetic field on April 25th or 26th. Credit: SDO/AIA
Noctilucent Clouds Our connection with NASA's AIM spacecraft has been restored! New images from AIM show that the southern season for noctilucent clouds (NLCs) is underway. Come back to this spot every day to see AIM's "daily daisy," which reveals the dance of electric-blue NLCs around the Antarctic Circle..
Switch view: Ross Ice Shelf, Antarctic Peninsula, East Antarctica, Polar
Updated at: 02-07-2018 17:55:05
SPACE WEATHER
NOAA Forecasts
Updated at: 2018 Apr 23 2200 UTC
FLARE
0-24 hr
24-48 hr
CLASS M
01 %
01 %
CLASS X
01 %
01 %
Geomagnetic Storms:
Probabilities for significant disturbances in Earth's magnetic field are given for three activity levels: active, minor storm, severe storm
Updated at: 2018 Apr 23 2200 UTC
Mid-latitudes
0-24 hr
24-48 hr
ACTIVE
10 %
10 %
MINOR
01 %
01 %
SEVERE
01 %
01 %
High latitudes
0-24 hr
24-48 hr
ACTIVE
15 %
15 %
MINOR
15 %
15 %
SEVERE
10 %
10 %
 
Monday, Apr. 23, 2018
What's up in space
       
 

Lights Over Lapland is excited to announce that our aurora webcam will be up and running 365 days per year! You can now enjoy watching the Midnight Sun and all of the other drama in the sky above Abisko National Park, Sweden here.

 

SOLAR MINIMUM SUNSPOT: Solar minimum is approaching and, as a result, sunspot numbers are crashing toward zero. Nevertheless, there is a relatively large spot on the sun today. AR2706 has a primary core almost twice as wide as Earth, making it an easy target for backyard solar telescopes. So far AR2706 has produced no flares--a lassitude typical of solar minimum sunspots. Free: Aurora Alerts

THE MYSTERY OF LAST FRIDAY'S AURORAS: Before sunrise on Friday, April 20th, Northern Lights spilled across the Canadian border into almost a dozen US states. The unexpected display was seen from Washington to Maine, with sightings as far south as Illinois and Indiana. "The lights danced from sunrise to sunset," reports eyewitness Thomas Spence, who sends this picture from the Superior National Forest  in the Arrowhead Region of Minnesota:

The display was sparked by an interplanetary shock wave that hit Earth's magnetic field during the waning minutes of April 19th. Interplanetary shock waves are supersonic disturbances in the solar wind, causing sudden discontinuities in the speed, temperature, and density of gaseous material blowing around our planet. During periods of high solar activity, these shocks are routinely delivered to Earth by coronal mass ejections (CMEs)--that is, big explosions on the sun.

And therein lies the mystery.

There was no big explosion on the sun last week. So what caused the shock wave? No one knows. Despite the fact that there are multiple satellites keeping an eye on the sun 24/7, we missed something. The stealthy disturbance left the surface of the sun and traveled across the sun-Earth divide, unseen and undetected for several days, before it hit, sparking a moderately strong G2-class geomagnetic storm attended by strangely colored, widespread auroras. Surprises are still possible in space weather, after all.

Realtime Aurora Photo Gallery

MOTHER'S DAY IS JUST 3 WEEKS AWAY: Nothing says "I love you" like a heart-shaped pendant from the edge of space. On March 18, 2018, the students of Earth to Sky Calculus launched an array of cosmic ray sensors to the stratosphere onboard a helium balloon. This Mother's Day gift went along for the ride:

You can have it for $199.95. The students are selling these sterling silver pendants as a fund-raiser for their cosmic ray monitoring program. All proceeds support atmospheric radiation measurements and hands-on STEM education.

Each pendant comes with a greeting card showing the jewelry in flight and telling the story of its journey to the stratosphere and back again. Mom-satisfaction guaranteed.

Far Out Gifts: Earth to Sky Store
All proceeds support hands-on STEM education

VOLCANIC SUNDOGS: Sundogs are common. The rainbow-colored splashes of light frequently appear on either side of the sun when sunbeams lance through icy cirrus clouds. On April 20th, Daryl Peterson of Anchorage, Alaska, witnessed an uncommon type of sundog. "They were volcanic," he says. Take a look at his photo, then scroll down for an explanation:

"From my location in Anchorage, I can easily see three active volcanoes in the ring of fire group that begins just 90 miles from here, across the Cook Inlet," says Pederson. "On April 20th I was scouting locations that would make great foregrounds for Northern Lights photography. For the first time in a long time I could see activity from all three volcanoes. Just before sunset an intense sundog formed from the steam that had been pumping out of the Mount Spurr stratovolcano."

The steamy exhaust was freezing in the cold Alaska air, forming the ice crystals required for sundog formation. "These rare sundogs were made even more impressive by their reflection on the water," says Pederson.

Realtime Space Weather Photo Gallery

  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. 23, 2018, the network reported 26 fireballs.
(19 sporadics, 6 April Lyrids, 1 eta Aquariid)

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 23, 2018 there were 1907 potentially hazardous asteroids.
Recent & Upcoming Earth-asteroid encounters:
Asteroid
Date(UT)
Miss Distance
Velocity (km/s)
Diameter (m)
2018 HU
2018-Apr-18
8 LD
9.7
27
2018 HC1
2018-Apr-19
1.2 LD
15.5
16
2018 HS
2018-Apr-20
5.1 LD
18.9
35
2018 GS3
2018-Apr-20
8.5 LD
19.8
24
2016 JP
2018-Apr-20
12 LD
12.7
214
2018 HT
2018-Apr-21
7.1 LD
7.6
15
2018 GR1
2018-Apr-21
18.3 LD
16.4
52
2018 HN
2018-Apr-21
8 LD
9.8
37
2018 HV
2018-Apr-22
0.4 LD
16
6
2018 GG4
2018-Apr-23
9.8 LD
14.9
20
2012 XL16
2018-Apr-23
15.8 LD
6.1
28
2018 GH
2018-Apr-25
14.6 LD
10.7
89
2018 HP
2018-Apr-26
11.6 LD
10.3
20
2018 GH5
2018-Apr-27
12.2 LD
12.7
32
2018 GB2
2018-Apr-27
17.1 LD
14.6
92
2013 US3
2018-Apr-29
10.1 LD
7.7
214
2018 GO4
2018-Apr-29
11.8 LD
8.6
46
2018 GY1
2018-Apr-29
13.2 LD
16.7
141
2018 FV4
2018-Apr-29
17.7 LD
6.5
59
2002 JR100
2018-Apr-29
10.8 LD
7.7
49
2018 HB1
2018-May-02
10.2 LD
9.2
39
1999 FN19
2018-May-07
9.7 LD
5.7
118
2016 JQ5
2018-May-08
6.3 LD
10.4
9
388945
2018-May-09
6.5 LD
9
295
2018 GR2
2018-May-11
13.4 LD
9.8
109
1999 LK1
2018-May-15
13.3 LD
10
141
2018 GL1
2018-May-18
14.3 LD
5.2
67
68347
2018-May-29
9.5 LD
13.3
389
2013 LE7
2018-May-31
17.8 LD
1.7
12
2018 EJ4
2018-Jun-10
5.6 LD
6.2
195
2015 DP155
2018-Jun-11
9 LD
4.4
170
2017 YE5
2018-Jun-21
15.6 LD
15.5
513
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

Readers, thank you for your patience while we continue to develop this new section of Spaceweather.com. We've been working to streamline our data reduction, allowing us to post results from balloon flights much more rapidly, and we have developed a new data product, shown here:

This plot displays radiation measurements not only in the stratosphere, but also at aviation altitudes. Dose rates are expessed 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. These measurements are made by our usual cosmic ray payload as it passes through aviation altitudes en route to the stratosphere over California.

What is this all about? Approximately 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 radiation sensors that detect cosmic rays, a surprisingly "down to Earth" form of space weather. Cosmic rays can seed clouds, trigger lightning, and penetrate commercial airplanes. Furthermore, there are studies ( #1, #2, #3, #4) linking cosmic rays with cardiac arrhythmias and sudden cardiac death in the general population. Our latest measurements show that cosmic rays are intensifying, with an increase of more than 13% since 2015:


Why are cosmic rays intensifying? The main reason is the sun. Solar storm clouds such as coronal mass ejections (CMEs) sweep aside cosmic rays when they pass by Earth. During Solar Maximum, CMEs are abundant and cosmic rays are held at bay. Now, however, the solar cycle is swinging toward Solar Minimum, allowing cosmic rays to return. Another reason could be the weakening of Earth's magnetic field, which helps protect us from deep-space radiation.

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.

The data points in the graph above correspond to the peak of the Reneger-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 Reneger 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.
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
Heliophysics
  the underlying science of space weather
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