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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: 451.0 km/sec
density: 5.1 protons/cm3
explanation | more data
Updated: Today at 2245 UT
X-ray Solar Flares
6-hr max: A0
2245 UT May02
24-hr: A0
0850 UT May02
explanation | more data
Updated: Today at: 2245 UT
Daily Sun: 02 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= 0 quiet
24-hr max: Kp= 4
unsettled
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: 4.6 nT
Bz: 2.4 nT south
explanation | more data
Updated: Today at 2245 UT
Coronal Holes:
A solar wind flowing from the indicated coronal hole should reach Earth on or about May 5th. Credit: SOHO Extreme UV Telescope
SPACE WEATHER
NOAA Forecasts
Updated at: 2008 May 02 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 02 2203 UTC
Mid-latitudes
0-24 hr
24-48 hr
ACTIVE
35 %
35 %
MINOR
10 %
10 %
SEVERE
05 %
05 %
High latitudes
0-24 hr
24-48 hr
ACTIVE
35 %
35 %
MINOR
20 %
20 %
SEVERE
10 %
10 %
What's up in Space
May 2, 2008
MOTHER'S DAY: Give your mom a truly heavenly gift on May 11th--a subscription to Space Weather PHONE!  

FLYBY ALERT: The International Space Station (ISS) is just beginning a 4-week series of bright flybys over Europe and North America. In early May, the ISS joins Jupiter and the stars of the Summer Triangle in a glittering pre-dawn sky. Later in the month, flybys shift to evening hours and the ISS will cross paths with Saturn, the Moon and Mars. US and Canadian readers, find out when to look using our new Simple Flybys tool. A worldwide version is coming soon; stay tuned.

SOLAR FILAMENT: Today, a dark magnetic filament is snaking over the sun's western limb, producing a beautiful 3D scene for amateur astronomers to photograph. It's "rather wonderful," says Pete Lawrence, who sends this snapshot from his backyard observatory in Selsey, UK:

Filaments are clouds of hydrogen held above the surface of the sun by magnetic fields. Backlit by the inferno below, they appear dark and cool, but that is an illusion. Like all things solar, filamentary clouds are bright and red-hot. We see this most clearly when a filament juts into the black of space beyond the sun's edge, as this one is doing in the left half of the photo.

In fact, this filament is about to go all the way over the edge, reclassifying itself from filament to prominence. If you have a solar telescope, train it on the western limb of the sun and watch the metamorphasis.

more images: from James Kevin Ty of Manila, the Philippines; from E. Signorelli and J. Stetson of South Portland, Maine; from Peter Paice of Belfast, Northern Ireland; from Malcolm Park of London, England, UK; from Maxim Usatov of Prague, the Czech Republic;

4D IONOSPHERE: The ionosphere is our planet's "final frontier." A realm of dancing auroras, radio-bending plasma bubbles and dangerous ultraviolet rays, it is the last wisp of Earth's atmosphere that astronauts leave behind when they enter space. And now it is 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. Get the full story from Science@NASA.


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 2, 2008 there were 947 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
2008 HD2
May 9
6.5 LD
19
40 m
2008 HR3
May 11
3.1 LD
17
50 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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