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SpaceWeather.com -- News and information about meteor showers, solar flares, auroras, and near-Earth asteroids
 
Solar wind
speed: 551.9 km/sec
density: 7.4 protons/cm3
more data: ACE, DSCOVR
Updated: Today at 2350 UT
X-ray Solar Flares
6-hr max: A8
2218 UT Jun17
24-hr: B1
0257 UT Jun17
explanation | more data
Updated: Today at: 2300 UT
Daily Sun: 17 Jun 17
The magnetic field of sunspot AR2663 has decayed and it no longer poses a threat for strong solar flares. Credit: SDO/HMI

Sunspot number: 28
What is the sunspot number?
Updated 17 Jun 2017

Spotless Days
Current Stretch: 0 days
2017 total: 42 days (25%)
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 17 Jun 2017


The Radio Sun
10.7 cm flux: 74 sfu
explanation | more data
Updated 17 Jun 2017

Current Auroral Oval:
Switch to: Europe, USA, New Zealand, Antarctica
Credit: NOAA/Ovation
Planetary K-index
Now: Kp= 4 unsettled
24-hr max: Kp= 4
unsettled
explanation | more data
Interplanetary Mag. Field
Btotal: 6.6 nT
Bz: -1.7 nT south
more data: ACE, DSCOVR
Updated: Today at 2349 UT
Coronal Holes: 17 Jun 17

Earth is inside a stream of solar wind flowing from the indicated coronal hole. Credit: NASA/SDO.
Noctilucent Clouds NASA's AIM spacecraft, which monitors NLCs from space, recent moved into a new orbit around Earth. Daily data are currently unavailable while the spacecraft's pointing settles. Polar images should resume in early June. Stay tuned!
Switch view: Ross Ice Shelf, Antarctic Peninsula, East Antarctica, Polar
Updated at: 02-24-2017 17:55:02
SPACE WEATHER
NOAA Forecasts
Updated at: 2017 Jun 17 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: 2017 Jun 17 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
05 %
10 %
 
Saturday, Jun. 17, 2017
What's up in space
       
 

Lights Over lapland is excited to announce that Autumn Aurora Adventures are available for immediate booking! Reserve your adventure of a lifetime in Abisko National Park, Sweden today!

 

FATHER'S DAY ROCKET LAUNCH: On June 18th, NASA will try for the 8th time to launch a sounding rocket from Wallops Flight Facility in Virginia, creating a colorful display of artificial clouds high above the eastern seaboard of the USA. Previous launches have been aborted because of, e.g., high winds, clouds, and boats in the hazard area. The launch window is from 9:05 to 9:20 pm Eastern Time.  Blue-green and red vapors may be visible from New York to North Carolina between 4 and 5.5 minutes after launch. Free: Aurora Alerts

RETURN OF THE NOCTILUCENT CLOUDS: A mesospheric heat wave that wiped out noctilucent clouds (NLCs) in early June is subsiding. As temperatures drop 83 km above Earth's surface, summertime wisps of water vapor are rapidly crystallizing around specks of meteor smoke with visible results. The NLCs are back. Allan Trow photographed their silvery tendrils over Anglesey, N. Wales, UK, on June 16th:

"The clouds were so expansive, I had to stitch two images together to capture the complete display," says Trow.

This is an unusually late start to the summer season for NLCs, and no one can say for sure what will happen next. However, researchers working with NASA's AIM spacecraft, which studies NLCs from Earth orbit, believe the clouds will quickly intensify as the 2nd half of June unfolds.

When noctilucent clouds first appeared in the 19th century, you had to travel to Arctic latitudes to see them. In recent years, however, they have intensified and spread with sightings as far south as Colorado and Kansas--a development that might be related to climate change. Observing tips: Look west 30 to 60 minutes after sunset when the sun has dipped ~10 degrees below the horizon. If you see luminous blue-white tendrils spreading across the sky, you may have spotted a noctilucent cloud.

Realtime Noctilucent Cloud Photo Gallery

FATHER'S DAY AT THE EDGE OF SPACE: On June 10th, the students of Earth to Sky Calculus flew a cosmic ray balloon to the edge of space, collecting another data point for their atmospheric radiation monitoring program. To support the flight, Spaceweather.com reader Caryl Anne Crowne bought her husband Erick a Father's Day gift.  She sent his picture to the stratosphere:

Pictured alongside Erick is their newborn daughter Vayda. She will receive the bunny! "I'm really excited to share this with Erick  for his first Father's Day!" says Caryl Anne, who will also be giving him a complete 2 hour HD video of the flight.

Readers, if you would like to support our student research program and send your own picture to the stratosphere, you can buy a Ticket to Space discounted for Father's Day.  In fact, there's still time to give it as a Father's Day gift because we can email the certificate to you on June 18th. 

Happy Father's Day, Erick!

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

POLAR MESOSPHERIC SUMMERTIME ECHOES: High above the Arctic Circle in Lofoten, Norway,  researcher Rob Stammes cannot see noctilucent clouds through the glare of the midnight sun.  Nevertheless, he knew they had returned. How? He heard them! "On June 15th, my VHF radio system recorded polar mesospheric summertime echoes (PMSEs)--a sign of noctilucent cloud activity," he explains.


PMSEs are terrestrial radio stations reflected from an altitude of 80 km to 90 km. That part of Earth's upper atmosphere is the mesosphere--the same place noctilucent clouds are found. The exact cause of PMSEs is not yet known; theorists have proposed explanations ranging from steep electron density gradients and "dressed aerosols" to gravity waves and turbulence. The echoes are often accompanied by visible NLCs.

"I normally use my VHF receiving system for signals from auroras and meteors," says Stammes. But there were no meteor showers or geomagnetic storms in progress at the time. "This event was much more like a PMSE, which I have detected many times in previous seasons."

He detected another episode of radio echoes on June 16th--confirming what is now obvious to the naked eye for many northern sky watchers: NLC season is finally underway. Stay tuned for more PMSEs.

Realtime Space Weather Photo Gallery

Realtime Aurora Photo Gallery


Realtime Comet 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 Jun. 17, 2017, the network reported 12 fireballs.
(11 sporadics, 1 Northern June Aquilid)

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 June 17, 2017 there were 1803 potentially hazardous asteroids.
Recent & Upcoming Earth-asteroid encounters:
Asteroid
Date(UT)
Miss Distance
Velocity (km/s)
Diameter (m)
2017 LE1
2017-Jun-15
20 LD
6.4
25
2010 VB1
2017-Jun-16
10.3 LD
8.3
81
2017 LX
2017-Jun-16
2.8 LD
20
20
2017 LV
2017-Jun-18
6.8 LD
10.7
21
471984
2017-Jun-18
19.1 LD
7.7
102
2017 LW
2017-Jun-20
15.7 LD
3.5
28
441987
2017-Jun-24
7.9 LD
12.7
178
2017 BS5
2017-Jul-23
3.1 LD
5.8
54
2014 OA339
2017-Aug-13
12.3 LD
10
47
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
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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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