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Solar wind
speed: 438.8 km/sec
density: 5.3 protons/cm3
explanation | more data
Updated: Today at 2348 UT
X-ray Solar Flares
6-hr max: B3
1921 UT Jul26
24-hr: C1
1234 UT Jul26
explanation | more data
Updated: Today at: 2300 UT
Daily Sun: 26 Jul 15
Sunspots AR2389 and AR2390 pose a growing threat for minor C-class solar flares. Overall, solar activity remains low. Credit: SDO/HMI

Sunspot number: 41
What is the sunspot number?
Updated 26 Jul 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 26 Jul 2015

The Radio Sun
10.7 cm flux: 94 sfu
explanation | more data
Updated 26 Jul 2015

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
explanation | more data
Interplanetary Mag. Field
Btotal: 5.7 nT
Bz: 2.7 nT north
explanation | more data
Updated: Today at 2348 UT
Coronal Holes: 26 Jul 15

There are no large coronal holes on the Earthside of the sun. 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: 07-26-2015 16:55:03
NOAA Forecasts
Updated at: 2015 Jul 26 2200 UTC
0-24 hr
24-48 hr
05 %
05 %
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: 2015 Jul 26 2200 UTC
0-24 hr
24-48 hr
05 %
20 %
01 %
05 %
01 %
01 %
High latitudes
0-24 hr
24-48 hr
15 %
20 %
20 %
30 %
10 %
25 %
Sunday, Jul. 26, 2015
What's up in space

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Lapland tours

QUIET WITH A SLIGHT CHANCE OF FLARES: Solar activity is very low, and it is likely to remain so. There are only two sunspots on the Earthside of the sun; neither has the type of unstable magnetic field that harbors energy for strong explosions. NOAA forecasters put the odds of an M-class flare today at only 5%. Solar flare alerts: text or voice.

ALPHA CAPRICORNID METEOR SHOWER: Earth is passing through a stream of debris from Comet 169P/NEAT, source of the annual alpha Capricornid meteor shower. Last night (July 25-26), NASA's network of all-sky meteor cameras picked up 8 alpha Capricornid fireballs over the USA, including this one above Mount Hopkins, Arizona:

This is an annual shower, which peaks every year between the 25th and 30th of July. Peak rates are typically no higher than 5 to 10 meteors per hour.

Every year, however, the alpha Capricornids are improving. According to the research of meteor experts Peter Jenniskens and Jeremie Vaubaillon, the debris stream is slowly drifting across Earth's orbit, so that each year our planet passes a little closer to its heart. The bulk of the dust will not be in Earth's path until the 24th century. If their predictions are correct, the Alpha Capricornids will become a major annual storm in 2200 - 2400 A.D., one that will be "stronger than any current annual shower."

Until then, sky watchers should remain alert for a relatively small number of alpha Capricornid fireballs in the nights ahead. Observers in both hemispheres can see this minor but beautiful shower. The best time to look is during the hours around local midnight when the constellation Capricorn reaches its highest point in the southern sky.

Realtime Space Weather Photo Gallery

RADS ON A PLANE: Many people think that only astronauts have to worry about cosmic radiation. Not so. Regular air travelers are exposed to cosmic rays, too. This week,'s Dr. Tony Phillips and the students of Earth to Sky Calculus flew across the United States to conduct a transcontinental launch of space weather balloons. They took radiation sensors on board the plane to find out how many cosmic rays they would absorb during the flight. Here are the data they collected:

Radiation levels in the cabin of the Airbus 319 (Spirit Airlines FL640) tripled within ten minutes after takeoff, and were nearly 30 times ground level by the time the plane reached cruising altitude at 39,000 feet. Summing over the entire flight, the sensors measured about 1 mrem of radiation--similar to a dental x-ray. (Note: an earlier comparison to the annual dose of ground-level cosmic rays was incorrect.)

There was no solar storm in progress. The extra radiation was just a regular drizzle of cosmic rays reaching down to aviation altitudes. This radiation is ever-present and comes from supernovas, black holes, and other sources across the galaxy. Solar activity modulates the intensity of cosmic rays. Gusts of solar wind and CMEs can actually cause radiation levels to drop by sweeping aside cosmic rays near Earth. Periods of low solar activity, on the other hand, allow radiation levels to rise.

Solar activity is not the only variable: Radiation levels vary within the plane itself. Different-colored lines in the data plot, above, represent different locations inside the cabin. On this particular flight, dose rates were highest in First Class and lowest near the toilets in the rear. This gradient is not understood; presumably, it has something to do with the way the fuselage and fuel tanks interact with energetic particles. The altitude of the plane matters as well. When the cruising altitude increased about two hours into the flight, dose rates increased accordingly. All of these factors make radiation levels onboard airplanes unpredictable.

The radiation sensors are the same ones that Earth to Sky Calculus routinely flies onboard helium balloons to measure cosmic rays in the stratosphere. They 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.

Stay tuned for updates from the return flight.

Realtime NLC Photo Gallery

Realtime Aurora 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 Jul. 26, 2015, the network reported 26 fireballs.
(18 sporadics, 8 alpha Capricornids)

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 July 26, 2015 there were potentially hazardous asteroids.
Recent & Upcoming Earth-asteroid encounters:
Miss Distance
2011 UW158
Jul 19
6.4 LD
540 m
2013 BQ18
Jul 20
7.9 LD
38 m
2015 OQ21
Jul 24
1.5 LD
10 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
1991 CS
Sep 4
62.1 LD
1.4 km
2014 KS76
Sep 14
8.7 LD
22 m
2004 TR12
Sep 15
58.8 LD
1.0 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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