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Solar wind
speed: 356.6 km/sec
density: 6.4 protons/cm3
explanation | more data
Updated: Today at 2346 UT
X-ray Solar Flares
6-hr max: C5
1839 UT Jul09
24-hr: M1
0026 UT Jul09
explanation | more data
Updated: Today at: 2300 UT
Daily Sun: 09 Jul 14
Big sunspots AR2108 and AR2109 have "delta-class" magnetic fields that harbor energy for X-class solar flares. Sunspot AR2113 poses a threat for M-class flares. Credit: SDO/HMI
Sunspot number: 209
What is the sunspot number?
Updated 09 Jul 2014

Spotless Days
Current Stretch: 0 days
2014 total: 0 days (0%)
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%)

09 Jul 2014

The Radio Sun
10.7 cm flux: 201 sfu
explanation | more data
Updated 09 Jul 2014

Current Auroral Oval:
Switch to: Europe, USA, New Zealand, Antarctica
Planetary K-index
Now: Kp= 2 quiet
24-hr max: Kp= 2
explanation | more data
Interplanetary Mag. Field
Btotal: 6.9 nT
Bz: 4.4 nT south
explanation | more data
Updated: Today at 2347 UT
Coronal Holes: 09 Jul 14
A stream of solar wind flowing from this minor coronal hole should reach Earth on July 9-10..Credit: SDO/AIA. posts daily satellite images of noctilucent clouds (NLCs), which hover over Earth's poles at the edge of space. The data come from NASA's AIM spacecraft. The north polar "daisy" pictured below is a composite of near-realtime images from AIM assembled by researchers at the University of Colorado's Laboratory for Atmospheric and Space Physics (LASP).
Noctilucent Clouds
Switch view: Europe, USA, Asia, Polar
Updated at: 07-09-2014 14:55:05
NOAA Forecasts
Updated at: 2014 Jul 09 2200 UTC
0-24 hr
24-48 hr
70 %
70 %
15 %
15 %
Geomagnetic Storms:
Probabilities for significant disturbances in Earth's magnetic field are given for three activity levels: active, minor storm, severe storm
Updated at: 2014 Jul 09 2200 UTC
0-24 hr
24-48 hr
10 %
10 %
01 %
01 %
01 %
01 %
High latitudes
0-24 hr
24-48 hr
15 %
15 %
20 %
20 %
10 %
10 %
Wednesday, Jul. 9, 2014
What's up in space

When is the best time to see auroras? Where is the best place to go? And how do you photograph them? These questions and more are answered in a new book, Northern Lights - a Guide, by Pal Brekke & Fredrik Broms.

Northern Lights - a Guide

HELIOPHYSICS SUMMER SCHOOL: The 2014 Heliophysics Summer School is underway in Boulder, CO, and Dr. Tony Phillips (@spaceweatherman) is tweeting from the classroom. Follow the lectures on Twitter using the hashtag #helioschool.

RADIO STATIC FROM THE SUN: The M6-flare of July 8th, described below, had a noisy side-effect. It caused a roar of static to issue from the loudspeakers of shortwave radios on Earth. In New Mexico, amateur radio astronomer Thomas Ashcraft recorded the sounds:

"The M6.5 flare yesterday generated a complex mix of Type II and Type IV solar radio emissions," says Ashcraft. "This two minute audio sample, recorded in stereo at the frequencies of 23 MHz and 21 MHz, captures the dynamic character of the bursts."

Radio bursts such as these are sparked by shock waves moving through the sun's atmosphere. Set in motion by flares, these shock waves excite plasma instabilitties that emit static-y radio waves. Becase there are a whole variety of plasma instabilites, there is a corresponding variety of radio burst types. Ashcraft recorded two: Type II and Type IV. More examples may be found here.

SOLAR FLARE ERUPTS FROM UNEXPECTED SOURCE: Yesterday, July 8th, Earth-orbiting satellites detected a strong M6-class solar flare. NASA's Solar Dynamics Observatory recorded the extreme ultraviolet flash:

X-ray and UV radiation from the flare sent waves of ionization coursing through Earth's upper atmosphere. This briefly disturbed the propagation of shortwave radio transmissions around the dayside of our planet, especially over Europe and North America. Conditions have since returned to normal.

The flare came as little surprise. A phalanx of large sunspots is crossing the solar disk, and forecasters have been predicting an explosion for more than a week. However, the source of the flare was unexpected. It came from a minor and seemingly harmless sunspot named AR2113. Appearances notwithstanding, AR2113 has a 'beta-gamma' magnetic field that harbors energy for M-class solar flares.

With this flare, AR2113 joins two other sunspots capable of potent activity: AR2108 and AR2109. NOAA forecasters estimate a 75% chance of M-flares and a 20% chance of X-flares on July 9th. Solar flare alerts: text, voice

Realtime Space Weather Photo Gallery

SPOTTY SUNRISE: Astrophotographers around the world are snapping pictures of this week's large sunspots. "After taking some sunspot images yesterday afternoon, I was thinking that it would be nice to capture the spotty Sun at sunrise," says Stephen Mudge of Brisbane, Australia. "And then I thought it would be even nicer if that sunrise was behind the city buildings. So after a bit of time studying Stellarium and looking at maps, and then a quick reconnaissance drive, I settled on Green Hill Reservoir as a suitable location for a photo shoot." This was the result

"I got up there just as dawn started and took some panoramas of the city. Then, with the camera still in position on the tripod, I added a Baader solar filter and captured the rising sun with exposures every 3.5 minutes," explains Mudge. "I managed to pick the location perfectly (with the Sun rising right in the middle of the city), and the weather cooperated beautifully, so I'm pretty happy with the result!"

Who knew sunspots could be a muse for creative photography? Check the realtime photo gallery for more examples.

ELECTRIC-BLUE SUNRISE: Yesterday morning in Russia, the sunrise was electric-blue. Bright bands of noctilucent clouds zig-zagged like lightning across the twilight sky, continuing a two-day display that has delighted observers across northern Europe. Michael Zavyalov sends this picture taken July 8th from the city of Yaroslavl:

"Another night with bright noctilucent clouds (NLCs) in Yaroslavl!" says Zavyalov. "We could even see their reflection in the water."

NLCs are Earth's highest clouds. Seeded by "meteor smoke," they form at the edge of space 83 km above Earth's surface. When sunlight hits the tiny ice crystals that make up these clouds, they glow electric blue.

In the northern hemisphere, July is the best month to see them. NLCs appear during summer because that is when water molecules are wafted up from the lower atmosphere to mix with the meteor smoke. That is also, ironically, when the upper atmosphere is coldest, allowing the ice crystals of NLCs to form.

The natural habitat of noctilucent clouds is the Arctic Circle. In recent years, however, they have spread to lower latitudes with sightings as far south as Utah and Colorado. This will likely happen in 2014 as well. Observing tips: Look west 30 to 60 minutes after sunset when the Sun has dipped 6o to 16o below the horizon. If you see blue-white tendrils zig-zagging across the sky, you may have spotted a noctilucent cloud.

Realtime NLC Photo Gallery

Realtime Comet Photo Gallery

Realtime Aurora 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. 9, 2014, the network reported 26 fireballs.
( 26 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 July 9, 2014 there were 1489 potentially hazardous asteroids.
Recent & Upcoming Earth-asteroid encounters:
Miss Distance
2014 MJ26
Jul 2
9.7 LD
47 m
2013 AG69
Jul 8
2.7 LD
15 m
2014 MF6
Jul 9
9.1 LD
305 m
2011 PU1
Jul 17
7.9 LD
43 m
2002 JN97
Aug 2
61.4 LD
2.0 km
2001 RZ11
Aug 17
34.2 LD
2.2 km
2013 WT67
Aug 17
16.1 LD
1.1 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
Space Weather Alerts
  more links...
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