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Solar wind
speed: 612.1 km/sec
density: 0.7 protons/cm3
explanation | more data
Updated: Today at 2345 UT
X-ray Solar Flares
6-hr max: C1
2147 UT May26
24-hr: C3
0958 UT May26
explanation | more data
Updated: Today at: 2300 UT
Daily Sun: 26 May 13
Sunspot AR1756 has a 'beta-gamma' magnetic field that harbors energy for M-class solar flares. Credit: SDO/HMI
Sunspot number: 107
What is the sunspot number?
Updated 26 May 2013

Spotless Days
Current Stretch: 0 days
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%)
Since 2004: 821 days
Typical Solar Min: 486 days

Update
26 May 2013

The Radio Sun
10.7 cm flux: 121 sfu
explanation | more data
Updated 26 May 2013

Current Auroral Oval:
Switch to: Europe, USA, New Zealand, Antarctica
Credit: NOAA/POES
Planetary K-index
Now: Kp= 3 quiet
24-hr max: Kp= 4
unsettled
explanation | more data
Interplanetary Mag. Field
Btotal: 4.3 nT
Bz: 0.3 nT north
explanation | more data
Updated: Today at 2346 UT
Coronal Holes: 26 May 13
Solar wind flowing from this coronal hole could brush past Earth's magnetic field on May 27-28. Credit: SDO/AIA.

NEW: Spaceweather.com is now posting 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: 05-25-2013 14:55:02
SPACE WEATHER
NOAA Forecasts
Updated at: 2013 May 26 2200 UTC
FLARE
0-24 hr
24-48 hr
CLASS M
25 %
25 %
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: 2013 May 26 2200 UTC
Mid-latitudes
0-24 hr
24-48 hr
ACTIVE
20 %
10 %
MINOR
05 %
01 %
SEVERE
01 %
01 %
High latitudes
0-24 hr
24-48 hr
ACTIVE
15 %
15 %
MINOR
25 %
20 %
SEVERE
25 %
20 %
 
Sunday, May. 26, 2013
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

SOLAR WIND STORM: Solar wind is blowing around Earth faster than 600 km/s (1.3 million mph) as our planet moves through the wake of a CME that struck on May 24th. This is causing geomagnetic unrest around the poles. Aurora sightings have been few, however, because of the competing glare of the full Moon. Aurora alerts: text, voice.

SUNSET PLANET SHOW: When the sun goes down tonight, step outside and look west. Venus, Jupiter and Mercury have converged to form a bright triangle in the sunset sky. Richard Sears sends this picture from Atwater, California:

"I took the picture on May 25th," says Sears. "What a way to end the day!"

Tonight will be even better. On Sunday, May 26th, the planets fit within a tightening circle less than 3o wide. There won't be another triple conjunction like this until October 2015, so don't miss it! NASA: video, full story.

Realtime Planet Photo Gallery

BACTERIA FLY INTO RADIATION STORM: Three days ago, high school students in Bishop, California, using a suborbital helium balloon launched a petri dish full of extreme-loving halobacteria into the strongest radiation storm of the year. They wanted to know how the extremophiles would fare when peppered with protons at the edge of space. Here is a picture of the sample 108,000 feet above Earth's surface:

The radiation storm was sparked by an M5-class solar flare on May 22nd. Students launched their microbes in the immediate aftermath of the flare when the highest energy protons (E > 100 MeV) were peaking in intensity. In addition to solar protons, the bacteria experienced air pressures only 1% that of sea level on the Earth below, temperatures as low as -65 C, and 70 mph winds. A student recovery team collected the payload from a remote desert in Nevada on May 23rd. Now they are culturing the bacteria to see if they survived.

The students, who call themselves Earth to Sky Calculus, have been launching research balloons for more than two years. Their projects include studies of high-altitude biology, measurements of the effects of solar flares on the ozone layer, and stratospheric photography of meteor showers.

How do they afford all this? To fund their activities, they have started a business called "Edge of Space Advertising." For a fee, they'll fly your banner, card, cow, running shoes, president or other object to the edge of space and send you the video. Contact Earth to Sky Calculus mentor Dr. Tony Phillips for details.

Realtime Space Weather Photo Gallery


Realtime Aurora Photo Gallery


Realtime Comet Photo Gallery


Realtime Noctilucent Cloud Photo Gallery
[previous years: 2003, 2004, 2005, 2006, 2007, 2008, 2009, 2011]

  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 May 26, 2013 there were potentially hazardous asteroids.
Recent & Upcoming Earth-asteroid encounters:
Asteroid
Date(UT)
Miss Distance
Size
2013 KB
May 22
3.2 LD
16 m
2013 KS1
May 22
4.8 LD
19 m
2004 BV102
May 25
69.9 LD
1.4 km
1998 QE2
May 31
15.2 LD
1.6 km
2009 FE
Jun 4
9.6 LD
230 m
2000 FM10
Jun 5
50.3 LD
1.3 km
2002 KL3
Jun 6
66.4 LD
1.1 km
1999 WC2
Jun 12
39.2 LD
1.9 km
2006 RO36
Jun 18
70.9 LD
1.2 km
2001 PJ9
Jul 17
29.2 LD
1.1 km
2006 BL8
Jul 26
9.3 LD
48 m
2003 DZ15
Jul 29
7.6 LD
153 m
2005 WK4
Aug 9
8.1 LD
420 m
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.
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
Heliophysics
  the underlying science of space weather
Space Weather Alerts
   
  more links...
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