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SpaceWeather.com -- News and information about meteor showers, solar flares, auroras, and near-Earth asteroids
SPACE WEATHER
Current conditions
Solar wind
speed: 476.0 km/sec
density: 0.9 protons/cm3
explanation | more data
Updated: Today at 2245 UT
X-ray Solar Flares
6-hr max: A3
1650 UT Apr26
24-hr: B3
1405 UT Apr26
explanation | more data
Updated: Today at: 2245 UT
Daily Sun: 26 Apr 08
The sun is blank--no sunspots. Credit: SOHO/MDI
Sunspot number: 0
What is the sunspot number?
Updated 25 Apr 2008
Far side of the Sun:
This holographic image reveals no sunspots on the farside of the sun. Image credit: SOHO/MDI
Planetary K-index
Now: Kp= 3 quiet
24-hr max: Kp= 3
quiet
explanation | more data
Current Auroral Oval:
Switch to: Europe, USA, New Zealand, Antarctica
Credit: NOAA/POES
What is the auroral oval?
Interplanetary Mag. Field
Btotal: 3.6 nT
Bz: 0.2 nT south
explanation | more data
Updated: Today at 2246 UT
Coronal Holes:
Earth is inside a solar wind stream flowing from the indicated coronal hole. Credit: SOHO Extreme UV Telescope
SPACE WEATHER
NOAA Forecasts
Updated at: 2008 Apr 26 2203 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: 2008 Apr 26 2203 UTC
Mid-latitudes
0-24 hr
24-48 hr
ACTIVE
10 %
10 %
MINOR
05 %
05 %
SEVERE
01 %
01 %
High latitudes
0-24 hr
24-48 hr
ACTIVE
10 %
10 %
MINOR
05 %
05 %
SEVERE
01 %
01 %
What's up in Space
April 26, 2008
FLYBY ALERT! Would you like a phone call when the International Space Station (ISS) is about to fly over your back yard? Sign up for Space Weather PHONE.  

SUNDAY MORNING WAKE-UP: Set your alarm for dawn. On Sunday morning, April 27th, Jupiter and the Moon will gather together for a lovely sunrise sky show. The two are so bright, they're visible even after the sky turns morning blue and all other stars and planets have faded away. Look out any south- or east-facing window and--presto!--you're wide awake, no coffee required. [sky map]

SOLAR ACTIVITY UPDATE: Today at 1405 UT, the sun unleashed a B3-class solar flare near one of the filaments described below. In the Netherlands, amateur astronomer Emiel Veldhuis was photographing the sun when the flare occured and he captured the explosion. The blast hurled a coronal mass ejection (CME, image) into space; it is too soon to say whether it is on an Earth-intercept trajectory. Stay tuned for updates.

SOLAR FILAMENTS: There's more to solar activity than sunspots. Consider today's sun, devoid of sunspots but criss-crossed with dark, writhing filaments like this one:

John Stetson and student B. Atkins took the picture from South Portland, Maine, on April 25th. "We saw lots of very nice solar activity that included a bright prominence, a number of active areas, and this large filament," says Stetson.

Solar filaments are long, sinuous clouds of hydrogen held above the surface of the sun by magnetic fields. They appear dark because they are cooler than the inferno below. For some reason--call it "solar weather"--the sun has broken out in a rash of filaments this weekend. At least half a dozen can be seen in backyard solar telescopes; if you have one, take a look.

more images: from Paulo Casquinha of Quinta do Anjo, Palmela - Portugal; from Malcolm Park of London, England, UK; from Stephen Ames of Hodegenville, KY; from Will Gater of Bristol, UK; from Patricia Cannaerts of Belgium; from Joel Bavais of Anvaing, Belgium;

END OF THE RAINBOW: At long last, Lorne Thompson of Las Vegas, Nevada, has found out what lies at the end of the rainbow. It's an outhouse:

You were expecting a pot of gold? "Potty of gold" is more like it.

Actually, there is no end to a rainbow. If the ground were removed, you would see that the rainbow makes a complete circle; this is called the "rainbow cone." Usually, less than half of the circle is visible because ground, hills and little blue buildings get in the way. To see more than half, go to the lofty perch of a mountaintop or an airplane. Voila!--no outhouse.

more images: from Steve Wainwright of South Wales UK; from Aslaug Ally of Ski, Norway; from Gary Shunk of Boulder, Colorado; from Grzegorz Willim of Jeleśnia, Polska; from Helmut Groell of Krefeld, Germany


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. [comment]
On April 26, 2008 there were 946 potentially hazardous asteroids.
April 2008 Earth-asteroid encounters:
Asteroid
Date(UT)
Miss Distance
Mag.
Size
2008 FH5
Apr. 2
7.6 LD
20
17 m
2001 QO142
Apr. 6
34 LD
17
685 m
2008 GF1
Apr. 7
0.8 LD
18
10 m
2005 BE2
Apr. 10
62 LD
18
1.0 km
2005 NB7
Apr. 17
16 LD
16
705 m
2008 FU6
Apr. 22
62 LD
16
1.4 km
2005 TB
Apr. 28
47 LD
18
1.3 km
2001 DQ8
Apr. 30
74 LD
17
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 Links
NOAA Space Weather Prediction Center
  The official U.S. government bureau for real-time monitoring of solar and geophysical events, research in solar-terrestrial physics, and forecasting solar and geophysical disturbances.
Atmospheric Optics
  The first place to look for information about sundogs, pillars, rainbows and related phenomena.
Solar and Heliospheric Observatory
  Realtime and archival images of the Sun from SOHO.
Daily Sunspot Summaries
  From the NOAA Space Environment Center
Current Solar Images
  from the National Solar Data Analysis Center
  more links...
©2008, SpaceWeather.com -- This site is penned daily by Dr. Tony Phillips.
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