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SpaceWeather.com -- News and information about meteor showers, solar flares, auroras, and near-Earth asteroids

SpaceWeather.com
Science news and information about the Sun-Earth environment.

SPACE WEATHER
Current
Conditions

Solar Wind
speed: 651.4 km/s
density:
1.1 protons/cm3
explanation | more data
Updated: Today at 2246 UT

X-ray Solar Flares
6-hr max:
A2 1740 UT Jan18
24-hr: B1 0200 UT Jan18
explanation | more data
Updated: Today at 2245 UT

Daily Sun: 18 Jan '07

Sunspot 938 poses no threat for strong solar flares. Credit:
SOHO/MDI

Sunspot Number: 17
What is the sunspot number?
Updated: 17 Jan 2007

Far Side of the Sun

This holographic image reveals one possible sunspot group on the far side of the sun. Image credit: SOHO/MDI

Interplanetary Mag. Field
Btotal: 4.5 nT
Bz:
2.7 nT north
explanation | more data
Updated: Today at 2247 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

Solar Flares: Probabilities for a medium-sized (M-class) or a major (X-class) solar flare during the next 24/48 hours are tabulated below.
Updated at 2007 Jan 18 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 Jan 18 2203 UTC
Mid-latitudes
0-24 hr 24-48 hr
ACTIVE 20 % 15 %
MINOR 10 % 05 %
SEVERE 05 % 01 %

High latitudes
0-24 hr 24-48 hr
ACTIVE 30 % 25 %
MINOR 15 % 15 %
SEVERE 10 % 05 %

What's Up in Space -- 18 Jan 2007
Subscribe to Space Weather News

Did you sleep through the auroras of Dec. 14th? Next time get a wake-up call: Spaceweather PHONE.

WISCONSIN AURORAS: Last night the sky turned green over Chippewa Falls, Wisconsin. "The auroras were faint, but it was a beautiful scene," says photographer Tony Wilder. The cause of the display: a solar wind stream is buffeting Earth's magnetic field. High-latitude sky watchers should remain alert for more auroras tonight

GREAT COMET: "Here in Argentina, Comet McNaught is a real hit. It's a wonderful sight after sunset," reports Mariano Ribas of Buenos Aires. "The comet's magnitude is around -3, and its bright and curved tail is easy to see with the naked eye: image."

The comet is widely visible from all parts of the Southern Hemisphere. This Jan. 17th photo comes from Kevin Crause of Mossel Bay, South Africa:


Photo details: Nikon D2X, 120mm lens, f/5.3, 9sec, ISO 200

Comet McNaught Photo Gallery
[finder chart] [ephemeris] [orbit] [comet binoculars]

Look at the photo, above: McNaught's dusty tail is curved. Why? Because it traces the comet's curved orbit. The tail curves so much that it actually leads all the way back to the northern hemisphere where it can be seen glowing very faintly in the western sky after sundown.

Amateur astronomer Paul Robinson first spotted it on Jan. 16th from Boulder, Colorado: diagram. "The tail is very faint and resembles a pale aurora borealis," he says. One night later, Dan Laszlo of the Northern Colorado Astronomical Society took this picture:


Photo details: Canon 20D, ISO 1600, f/4, 17mm lens, 20 seconds

"As Paul Robinson described, the multiple streamers looked like faint auroral rays," says Laszlo. "The tail was visible in binoculars when Venus set."

These are extraordinary observations and astronomers elsewhere are encouraged to confirm them. "Find the darkest sky you can," Laszlo advises, "and look west between one and two hours after sunset. A site where you can see zodiacal light would be best." Try it!



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 18 Jan 2007 there were 832 known Potentially
Hazardous Asteroids

Jan 2007 Earth-asteroid encounters
ASTEROID

 DATE
(UT)

MISS DISTANCE

MAG.

 SIZE
2006 UQ17

Jan. 2

11 LD

16

175 m
1991 VK

Jan. 21

26 LD

15

2.0 km
5011 Ptah

Jan. 21

77 LD

15

1.6 km
2006 CJ

Jan. 31

10 LD

~16

385 m
2006 AM4

Feb. 1

5.2 LD

16

180 m
Notes: LD is a "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 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. (European Mirror Site)

Daily Sunspot Summaries -- from the NOAA Space Environment Center.

Current Solar Images -- from the National Solar Data Analysis Center

X-ray images of the Sun: GOES-12 and GOES-13

Recent Solar Events -- a summary of current solar conditions from lmsal.com.

What is the Magnetosphere?

The Lion Roars -- visit this site to find out what the magnetosphere sounds like.

List of Potentially Hazardous Asteroids -- from the Harvard Minor Planet Center.

Observable Comets -- from the Harvard Minor Planet Center.

Real-time Solar Wind Data -- from NASA's ACE spacecraft.

How powerful are solar wind gusts? Not very! Read this story from Science@NASA.

More Real-time Solar Wind Data -- from the Solar and Heliospheric Observatory Proton Monitor.

Lists of Coronal Mass Ejections -- from 1996 to 2006

Mirages: Mirages in Finland; An Introduction to Mirages;

NOAA Solar Flare and Sunspot Data: 1994, 1995, 1996, 1997, 1998, 1999; 2000; 2001; 2002; 2003; 2004; 2005; Jan-Mar 2006; Apr-Jun 2006; Jul-Sep 2006; Oct-Dec 2006.

This site is penned daily by Dr. Tony Phillips: email


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