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

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Science news and information about the Sun-Earth environment.

SPACE WEATHER
Current
Conditions

Solar Wind
speed: 381.4 km/s
density:
13.4 protons/cm3
explanation | more data
Updated: Today at 2245 UT


X-ray Solar Flares

6-hr max:
A3 1825 UT Sep27
24-hr: B1 0730 UT Sep27
explanation | more data
Updated: Today at 2245 UT

Daily Sun: 27 Sep '05

These sunspots pose no threat for strong solar flares. Credit: SOHO/MDI


Sunspot Number: 25
What is the sunspot number?
Updated: 26 Sep 2005

Far Side of the Sun

This holographic image reveals no sunspots on the far side of the sun. Image credit: SOHO/MDI

Interplanetary Mag. Field
Btotal: 1.0 nT
Bz:
0.7 nT south
explanation | more data
Updated: Today at 2246 UT

Coronal Holes:

A solar wind stream flowing from the indicated coronal hole might brush past Earth's magnetic field during the next 48 hours. Image 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 2005 Sep 26 2226 UTC
FLARE 0-24 hr 24-48 hr
CLASS M 05 % 05 %
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 2005 Sep 26 2226 UTC
Mid-latitudes
0-24 hr 24-48 hr
ACTIVE 25 % 25 %
MINOR 15 % 15 %
SEVERE 05 % 05 %

High latitudes
0-24 hr 24-48 hr
ACTIVE 30 % 35 %
MINOR 20 % 25 %
SEVERE 10 % 15 %

What's Up in Space -- 27 Sep 2005
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Did you miss the auroras of September? Next time get a phone alert: Sign up for SpaceWeather PHONE.

SOLAR PROMINENCE: Astronomers are monitoring a gigantic prominence on the sun--"the largest I've imaged in several years," says veteran astrophotographer Jack Newton. Two days ago it bent into an arch large enough for the whole planet Earth to slip through, as shown in this picture from Stefan Seip of Stuttgart, Germany:

Prominences are clouds of hot-glowing hydrogen gas held aloft by solar magnetic force fields. Big prominences like this one can last for many days before they collapse. If you have a safely-filtered telescope, check it out.

ICE HALOES: It might be warm where you're sitting now, but 5 to 10 km above your head, the atmosphere is freezing cold. Way up there, water vapor in clouds turns to ice, and when tiny ice-crystals catch rays from the sun ... wow! A beautiful light-show materializes, such as this display photographed on Sept. 20th by Patrick Bornet of Nièvre, France:

Click to view a labeled image.

"Unbelievably well aligned ice crystals made these halos," says atmospheric optics expert Les Cowley. "Plate-like crystals set more level than our dining tables made the sundogs and the colorful circumzenithal arc. Long pencil shape crystals aligned horizontally made the tangent arc and the rare supralateral arc. Only a few crystals tumbled to produce the weak circular 22-degree halo. Why are tiny crystals so well oriented? Gentle aerodynamic drag forces act on them as they drift slowly downwards inside high cirrus clouds."



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 are on a collision course with our planet, although astronomers are finding new ones all the time.

On 27 Sep 2005 there were 710 known Potentially
Hazardous Asteroids

August 2005 Earth-asteroid encounters
ASTEROID

 DATE (UT)

 MISS DISTANCE

 MAG.
1992 UY4

August 8

16 LD

 12
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. See also Snow Crystals.

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 --a gallery of up-to-date solar pictures from the National Solar Data Analysis Center at the Goddard Space Flight Center. See also the GOES-12 Solar X-ray Imager.

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

SOHO Farside Images of the Sun from SWAN and MDI.

The Latest SOHO Coronagraph Images -- from the Naval Research Lab

The Sun from Earth -- daily images of our star from the Big Bear Solar Observatory

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

Observable Comets -- from the Harvard Minor Planet Center.

What is the Interplanetary Magnetic Field? -- A lucid answer from the University of Michigan. See also the Anatomy of Earth's Magnetosphere.

Real-time Solar Wind Data -- from NASA's ACE spacecraft. How powerful are solar wind gusts? Read this story from Science@NASA.

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

Aurora Forecast --from the University of Alaska's Geophysical Institute

Daily Solar Flare and Sunspot Data -- from the NOAA Space Environment Center.

Lists of Coronal Mass Ejections -- from 1998 to 2001

What is an Iridium flare? See also Photographing Satellites by Brian Webb.

What is an Astronomical Unit, or AU?

Mirages: Mirages in Finland; An Introduction to Mirages;

NOAA Solar Flare and Sunspot Data: 1999; 2000; 2001; 2002; 2003; 2004; Jan-Mar., 2005;

Space Audio Streams: (University of Florida) 20 MHz radio emissions from Jupiter: #1, #2, #3, #4; (NASA/Marshall) INSPIRE: #1; (Stan Nelson of Roswell, New Mexico) meteor radar: #1, #2;

Recent International Astronomical Union Circulars

GLOSSARY | SPACE WEATHER TUTORIAL

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

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