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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: 537.1 km/sec
density: 0.8 protons/cm3
explanation | more data
Updated: Today at 2240 UT
X-ray Solar Flares
6-hr max: A0
2245 UT Oct03
24-hr: A0
2245 UT Oct03
explanation | more data
Updated: Today at: 2245 UT
Daily Sun: 03 Oct 07
Sunspot 971 is almost invisibly small, but it is there. Credit: SOHO/MDI
Sunspot number: 0
What is the sunspot number?
Updated 02 Oct 2007
Far side of the Sun:
This holographic image reveals no large sunspots on the far side of the sun. Image credit: SOHO/MDI
Planetary K-index
Now: Kp= 3 quiet
24-hr max: Kp= 4
unsettled
explanation | more data
Current Auroral Oval:

Switch to: Europe, USA, New Zealand, Antarctica
Credit: NOAA/POES
Updated: 2007 Oct 03 2146 UT
What is the auroral oval?
Interplanetary Mag. Field
Btotal: 4.7 nT
Bz: 0.4 nT north
explanation | more data
Updated: Today at 2246 UT
Coronal Holes:
There are no large coronal holes on the sun today. Credit: Hinode X-tray Telescope
SPACE WEATHER
NOAA Forecasts
Updated at: 2007 Oct 03 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: 2007 Oct 03 2203 UTC
Mid-latitudes
0-24 hr
24-48 hr
ACTIVE
25 %
10 %
MINOR
10 %
05 %
SEVERE
01 %
01 %
High latitudes
0-24 hr
24-48 hr
ACTIVE
30 %
25 %
MINOR
15 %
10 %
SEVERE
05 %
01 %

What's up in Space
October 3, 2007
Where's Saturn? Is that a UFO--or the ISS? What's the name of that star? Get the answers from mySKY--a fun new astronomy helper from Meade. .

PROMINENCE ALERT: Got a solar telescope? Point it at the sun. Two large and active prominences have jumped up and are putting on a good show for onlookers: image.

more images: from Maxim Usatov of Dniepropetrovsk, Ukraine; from Pascal Paquereau of Mouzeuil-Saint-Martin, Vendée, France.

AURORA BURST: Last night, for no apparent reason, the sky over Baffin Island, Canada, erupted in green. "I had just come back from walking my dog when the night sky suddenly burst into light," reports Claus Vogel. "The display was dazzling." He grabbed his Nikon D200 and snapped this photo:

Researchers call this kind of outburst an "auroral substorm." First recognized in the early 1960s by a young Japanese physicist named Shun-ichi Akasofu, auroral substorms have been studied for almost 50 years, yet to this day they are neither predictable nor fully understood.

To solve the mystery, NASA has deployed a swarm of five spacecraft named THEMIS dedicated to the study of substorms. The probes are gathering data now--indeed, they may have observed the Baffin Island outburst pictured above--and mission scientists are reportedly learning a lot. We await the answers and, meanwhile, enjoy the show.

September 2007 Aurora Gallery
[August 2007 Aurora Gallery] [Aurora Alerts]

MICRO-SUNSPOT: Sunspots can grow so big they dwarf the planet Jupiter. But have you ever wondered, how small can they shrink? Yesterday, Japan's Hinode spacecraft photographed dwindling sunspot 971 revealing two dark cores each smaller than the United States:

Technically, these are called pores--sunspots so small they do not even contribute to the sunspot number. (The sunspot number when Hinode took the picture was officially zero.) With its sub-arcsecond resolution (0.2"), Hinode's solar telescope is powerful enough to see these small features on a routine basis.

The bumpy lumps surrounding the pores are called granules, They are California-sized blobs of sun rising and falling like water boiling on a hot stove. Indeed, the surface of the sun is boiling because it sits on top of a 15-million degree nuclear furnace. Conventional wisdom says sunspots never shrink any smaller than granules. Is this true? Hinode is just beginning to explore the sun in high resolution. Whether conventional wisdom survives the scrutiny remains to be seen.

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 October 3, 2007 there were 888 potentially hazardous asteroids.
Sept. 2007 Earth-asteroid encounters:
Asteroid
Date(UT)
Miss Distance
Mag.
Size
2007 RF1
Sep. 2
8.5 LD
18
26 m
2007 RS1
Sep. 5
0.2 LD
17
3 m
2007 RJ1
Sep. 16
2.5 LD
16
40 m
2007 RC20
Sep. 20
5.1 LD
19
22 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 Environment 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...
©2007, SpaceWeather.com -- This site is penned daily by Dr. Tony Phillips.
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