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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: 413.2 km/s
density:
4.0 protons/cm3
explanation | more data
Updated: Today at 2245 UT


X-ray Solar Flares

6-hr max:
B2 1810 UT Oct12
24-hr: C1 0540 UT Oct12
explanation | more data
Updated: Today at 2245 UT

Daily Sun: 12 Oct '05

Once-mighty sunspot 798 is transiting the Earth-facing side of the sun again. This time, however, the spot is no more than a scattered group of barely-visible 'sun-specks.' Click here for a closer look. Credit: SOHO/MDI


Sunspot Number: 25
What is the sunspot number?
Updated: 11 Oct 2005

Far Side of the Sun

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

Interplanetary Mag. Field
Btotal: 3.4 nT
Bz:
2.9 nT north
explanation | more data
Updated: Today at 2246 UT

Coronal Holes:

A solar wind stream flowing from the indicated coronal hole might buffet Earth's magnetic field briefly on Oct. 14th. 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 Oct 11 2214 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 2005 Oct 11 2214 UTC
Mid-latitudes
0-24 hr 24-48 hr
ACTIVE 15 % 15 %
MINOR 01 % 01 %
SEVERE 01 % 01 %

High latitudes
0-24 hr 24-48 hr
ACTIVE 20 % 20 %
MINOR 05 % 05 %
SEVERE 01 % 01 %

What's Up in Space -- 12 Oct 2005
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QUIET SUN: Solar activity is very low. Solar flares and auroras are unlikely this week.

FEAR AND PANIC: The two moons of Mars, Phobos and Deimos (Greek for Fear and Panic), are easy to overlook. They're tiny, less than 22 km wide, dim and rarely seen through a telescope. Mars itself shines 242,000 times brighter than Phobos and 741,000 times brighter than Deimos. The two moons get lost in the glare.

Nevertheless, it is possible, with effort, to photograph Phobos and Deimos. Steve Bodin of Mattawa, Washington, did it on October 10th:

"This is a composite of two exposures: a short exposure for Mars and a longer one to capture the faint moons," says Bodin, who used a 16-inch telescope and a color video camera. "Note the two 12th-magnitude stars visible to the upper right of Mars."

DANCING PROMINENCE: Who says solar activity is low? This morning in Germany, Stefan Seip photographed a solar prominence, and he swears he saw a dancer among the fiery plumes:

Staring at prominences on the sun is a bit like staring at clouds on Earth: with enough imagination, you can see all sorts of fantastic shapes. In fact, solar prominences are clouds. Unlike Earth-clouds, however, which tend to be cold and watery, solar clouds are hot and made mostly of hydrogen. This cloudy prominence will likely persist for another day or so. What shape will it be tomorrow?

more images: from Andreas Murner of Lake Chiemsee, Bavaria, Germany;



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 12 Oct 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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