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Solar wind
speed: 497.4 km/sec
density: 0.7 protons/cm3
explanation | more data
Updated: Today at 2351 UT
X-ray Solar Flares
6-hr max: B7
1654 UT Jun25
24-hr: M7
0816 UT Jun25
explanation | more data
Updated: Today at: 2300 UT
Daily Sun: 25 Jun 15
Sunspot AR2371 has a 'beta-gamma-delta' magnetic field that harbors energy for X-class solar flares. Credit: SDO/HMI

Sunspot number: 39
What is the sunspot number?
Updated 25 Jun 2015

Spotless Days
Current Stretch: 0 days
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 25 Jun 2015

The Radio Sun
10.7 cm flux: 110 sfu
explanation | more data
Updated 25 Jun 2015

Current Auroral Oval:
Switch to: Europe, USA, New Zealand, Antarctica
Credit: NOAA/Ovation
Planetary K-index
Now: Kp= 4 unsettled
24-hr max: Kp= 6
explanation | more data
Interplanetary Mag. Field
Btotal: 3.9 nT
Bz: 2.7 nT south
explanation | more data
Updated: Today at 2351 UT
Coronal Holes: 25 Jun 15

Solar wind flowing from the indicated coronal hole should reach Earth on June 28-29. Credit: SDO/AIA.
Noctilucent Clouds The northern season for NLCs is underway. NASA's AIM spacecraft spotted the first noctilucent clouds over the Arctic Circle on May 19th.
Switch view: Europe, USA, Asia, Polar
Updated at: 06-25-2015 16:55:02
NOAA Forecasts
Updated at: 2015 Jun 25 2200 UTC
0-24 hr
24-48 hr
60 %
60 %
20 %
20 %
Geomagnetic Storms:
Probabilities for significant disturbances in Earth's magnetic field are given for three activity levels: active, minor storm, severe storm
Updated at: 2015 Jun 25 2200 UTC
0-24 hr
24-48 hr
25 %
30 %
10 %
40 %
01 %
25 %
High latitudes
0-24 hr
24-48 hr
15 %
05 %
30 %
15 %
35 %
79 %
Thursday, Jun. 25, 2015
What's up in space

Learn to photograph Northern Lights like a pro. Sign up for Peter Rosen's Aurora Photo Courses in Abisko National Park, winner of the TripAdvisor Certificate of Excellence Award 2015.

Lapland tours

GEOMAGNETIC STORM IN CME'S WAKE: As expected, a CME hit Earth's magnetic field on June 24th. At first the impact had little effect, but now a G1-class geomagnetic storm is in progress as Earth passes through the CME's wake. High latitude sky watchers should remain alert for auroras. Aurora alerts: text or voice.

ANOTHER CME IS ON THE WAY: Since June 21st, four CMEs have hit Earth's magnetic field. A fifth is on the way. Sunspot AR2371 erupted again during the early hours of June 25th, producing an M7.9-class solar flare and a lopsided CME. The Solar and Heliospheric Observatory photograhed the storm cloud, which raced away from the sun faster than 2000 km/s (4.5 million mph):

The CME will probably sideswipe Earth's magnetic field on June 27th. NOAA computer models, due out later today, will refine the cloud's predicted arrival time and establish probabilities for geomagnetic storms. Stay tuned. Aurora alerts: text or voice.

THE SOLSTICE STORM: The current solar cycle has not been good to sky watchers. Years of weak solar activity have produced few widespread displays of the aurora boreais. The Solstice Storm of 2015 changed all that. A series of CMEs hit Earth's magnetic field on June 22nd, producing a severe G4-class geomagnetic storm. Northern Lights spilled across the Canadian border into more than 20 US states. Jason Brownlee sends this picture from Bend, Oregon:

"I photographed the auroras from the edge of Soda Creek in the Cascade Mountains," says Brownlee.

The lights descended even farther south than Oregon. Sky watchers saw auroras in the states of California, New Mexico, Colorado, Arizona, Texas, Georgia, Virginia and Arkansas--just to name a few. Browse the realtime aurora gallery for more sightings:

Realtime Aurora Photo Gallery

NOT A UFO: Many people who went outdoors to look for auroras on June 22nd saw auroras -- and something more. "We noticed a ghostly cloud-like object moving in an arc from the southeast to the northeast," says Lauri Kangas of Fort Frances, Ontario (Canada). "My wife commented that it was the closest thing she has seen to a UFO!" Kangas took this picture of the apparition:

David Jones of Lawrenceville, Georgia saw it, too. "At first I thought it was an airplane traveling south to north very slowly, but then I noticed it looked kind of fuzzy," he says. "As it continued traveling north, the star-like object clearly had a circle of mist or fog around it. I could also see smaller lights around the main one that appeared to twinkle."

This was not a UFO. Satellite expert Marco Langbroek explains: "On June 23 at 01:51:58 UT, the European Space Agency launched a Vega rocket with the Sentinel-2A satellite from Kourou, French Guyana. What [Kangas and others saw] is probably gases from the rocket's last engine burn."

The Sentinel-2 series of satellites is dedicated to observing Earth and its oceans. On June 22nd, in a reversal of roles, the people of Earth were observing Sentinel-2. Visit Langbroek's blog for more information.

Realtime Space Weather Photo Gallery

NEUTRONS IN THE STRATOSPHERE: For nearly two years, and the students of Earth to Sky Calculus have been using helium balloons to monitor X-rays and gamma-rays in the stratosphere. Their successful program has detected multiple radiation events in response to solar storms. On June 18th they added something new. For the first time, the group's Space Weather Payload included a bubble chamber for measuring neutrons. The device flew 109,012 feet above California's Sierra Nevada mountain range, then parachuted back to Earth, landing near Death Valley National Park. The results: Neutrons were detected.

Circled above are some of the bubbles that formed as neutrons passed through the chamber. By counting the bubbles, it is possible to estimate the total dose of neutron radiation absorbed during the 3 hour flight. The answer is 600 microRads (energy range 200 keV - 15 MeV). Interestingly, this is almost the same dose detected by onboard X-ray and gamma-ray sensors: 620 microRads (energy range 10 keV to 20 MeV). Lesson: if you only count X-rays and gamma-rays, then you are missing at least half of the radiation in the atmosphere. Neutrons matter, too.

Indeed, neutrons are a very important form of cosmic radiation, providing much of the biologically effective radiation dose at altitudes of interest to aviation and space tourism.  Low-energy neutrons also cause single-event upsets in aircraft avionics, especially devices that contain Boron 10. Adding a neutron sensor to the Space Weather Payload allows the students to monitor this type of radiation at altitudes ranging from ground level to 120,000 feet.

Realtime NLC Photo Gallery

Realtime Sprite 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

On Jun. 25, 2015, the network reported 4 fireballs.
(4 sporadics)

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 25, 2015 there were potentially hazardous asteroids.
Recent & Upcoming Earth-asteroid encounters:
Miss Distance
2015 KK57
Jun 23
8.3 LD
14 m
2015 MN11
Jun 24
12.5 LD
54 m
2015 MA54
Jun 25
6.8 LD
37 m
2005 VN5
Jul 7
12.6 LD
18 m
2015 HM10
Jul 7
1.1 LD
81 m
1994 AW1
Jul 15
25.3 LD
1.3 km
2011 UW158
Jul 19
6.4 LD
540 m
2013 BQ18
Jul 20
7.9 LD
38 m
1999 JD6
Jul 25
18.8 LD
1.6 km
2005 NZ6
Aug 6
76.5 LD
1.4 km
2005 JF21
Aug 16
20.1 LD
1.6 km
2004 BO41
Aug 31
57.3 LD
1.2 km
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.
  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.
  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
  the underlying science of space weather
Columbia Northern High School
  Web-based high school science course with free enrollment
  more links...
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