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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: 453.1 km/sec
density: 3.0 protons/cm3
explanation | more data
Updated: Today at 2246 UT
X-ray Solar Flares
6-hr max: A0
2245 UT May01
24-hr: A0
2245 UT May01
explanation | more data
Updated: Today at: 2245 UT
Daily Sun: 01 May 08
The sun is blank--no sunspots. Credit: SOHO/MDI
Sunspot number: 0
What is the sunspot number?
Updated 30 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: 8.1 nT
Bz: 7.7 nT south
explanation | more data
Updated: Today at 2247 UT
Coronal Holes:
A solar wind flowing from the indicated coronal hole hit Earth on April 30th and triggered a minor geomagnetic storm. Credit: SOHO Extreme UV Telescope
SPACE WEATHER
NOAA Forecasts
Updated at: 2008 May 01 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 May 01 2203 UTC
Mid-latitudes
0-24 hr
24-48 hr
ACTIVE
25 %
30 %
MINOR
05 %
10 %
SEVERE
01 %
05 %
High latitudes
0-24 hr
24-48 hr
ACTIVE
30 %
35 %
MINOR
10 %
15 %
SEVERE
01 %
05 %
What's up in Space
May 1, 2008
MOTHER'S DAY: Give your mom a truly heavenly gift on May 11th--a subscription to Space Weather PHONE!  

MUST-SEE FILAMENT: A dark magnetic filament is snaking over the sun's western limb today, producing a beautiful 3D scene for amateur astronomers to photograph. "It's spectacular," says Robert Arnold who sends this picture from the Isle of Sky, Scotland. If you have a solar telescope, take a look!

more images: from C. Keller and J. Stetson of South Portland, Maine; from Pete Lawrence of Selsey, West Sussex, UK; from Didier Favre of Brétigny sur Orge, France;

4D IONOSPHERE: The ionosphere is our planet's "final frontier." Stretching from 50 to 500 miles above Earth's surface, it is the last wisp of Earth's atmosphere that astronauts leave behind when they enter space. It is a realm of dancing auroras, radio-bending plasma bubbles and dangerous ultraviolet rays. And it is now on your home computer! (continued below)


Above: A screenshot of the 4D ionosphere

Yesterday, NASA-supported researchers at the Space Weather Workshop in Boulder, Colorado, unveiled a "4D" computer model for the general public. Download a few files and presto--you're flying through the ionosphere. The model shows the ionosphere as it is right now; it's a real-time display based on current solar activity and atmospheric conditions. This new tool can help ham radio operators plan their next DX transmissions, help pilots avoid polar radio blackouts, and help researchers see the effects of solar flares on Earth's atmosphere--and it's fun, too.

Find out how to start your own flight from Science@NASA.

GEOMAGNETIC STORM: "Where we live in Norway at 68o N latitude, the sky is too bright for auroras," reports Rob Stammes. At this time of year, the midnight sun spoils the show. "But I have another way of seeing the Northern Lights--on the paper of my magnetograph."

The squiggles on this plot, recorded by Stammes at the Polar Light Center in Lofoten, Norway, trace a geomagnetic storm on April 26th and 27th. "Red," he explains, "is the local magnetic field" swinging back and forth as a solar wind stream buffets Earth's magnetosphere. "Blue denotes electrical currents" flowing through the ground outside the instrument room, induced by the swinging motion of the overlying magnetic field.

Gusting solar wind, swinging magnetic fields, surging ground currents: that in a nutshell is a geomagnetic storm. If only the sky had been a little darker.

April 2008 Aurora Gallery
[Aurora Alerts] [Night-sky Cameras]

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 May 1, 2008 there were 946 potentially hazardous asteroids.
May 2008 Earth-asteroid encounters:
Asteroid
Date(UT)
Miss Distance
Mag.
Size
2008 HG
May 5
17 LD
18
90 m
2008 DE
May 9
17 LD
16
550 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 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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