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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: 489.8 km/s
density:
3.7 protons/cm3
explanation | more data
Updated: Today at 2255 UT

X-ray Solar Flares

6-hr max:
C8 2245 UT May02
24-hr: C8 2245 UT May02
explanation | more data
Updated: Today at 2245 UT

Daily Sun: 02 May '05

Sunspot 756 poses a threat for M-class solar flares. Credit: SOHO/MDI


Sunspot Number: 61
What is the sunspot number?
Updated: 01 May 2005

Far Side of the Sun

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

Interplanetary Mag. Field
Btotal: 3.8 nT
Bz:
0.3 nT south
explanation | more data
Updated: Today at 2256 UT

Coronal Holes:

Earth is inside a solar wind stream flowing from the indicated coronal hole. Image credit: SOHO Extreme Ultraviolet 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 May 01 2204 UTC
FLARE 0-24 hr 24-48 hr
CLASS M 30 % 30 %
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 May 01 2204 UTC
Mid-latitudes
0-24 hr 24-48 hr
ACTIVE 30 % 20 %
MINOR 15 % 10 %
SEVERE 05 % 01 %

High latitudes
0-24 hr 24-48 hr
ACTIVE 35 % 25 %
MINOR 15 % 10 %
SEVERE 10 % 05 %

What's Up in Space -- 2 May 2005
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WEEKEND AURORAS: In Alaska, this weekend, the auroras were so bright they shined through the twilight glow of the midnight sun. "It was spectacular," says Joseph Hall who took this picture near Fairbanks at two o'clock in the morning on May 1st:

The display was sparked by a solar wind stream buffeting Earth's magnetic field. Earth is exiting the stream now and the chance of more auroras tonight is low.

BIG SUNSPOT: More than four years after solar maximum, the sun continues to produce big sunspots. One is transiting the solar disk today: sunspot 756. It's about five times wider than Earth and poses a threat for M-class solar flares. (continued below)


Sunspot 756, April 25th - May 1st. Credit: SOHO.

Sunspot 756 is big enough to see with the naked eye, but do not stare at the blinding sun. Try building a safe solar projector instead.

"In the age of the pixel," says Gandini Elena of Caprino Bergamasco, Italy, "I made this image of sunspot 756 using only a pencil--just like Galileo."

more images: from Sylvain Weiller of St Rémy lès Chevreuse, France; from Enrico Perissinotto of Premariacco (Udine) Italy; from Francis Adelving near Grenoble, France; from Rijk-Jan Koppejan of Middelburg, The Netherlands; from Jim Adams of Rochester, New York; from Jack Newton in British Columbia, Canada; from Andreas Murner of Lake Chiemsee, Bavaria, Germany; from Joel Bavais of Ath, Belgium; from Pavol Rapavy of Rimavska Sobota, Slovakia; from Jérôme Grenier of Paris, France; from Dan Schechter of Long Beach, CA;

BONUS: April 24th Lunar Eclipse Gallery



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 2 May 2005 there were 681 known Potentially
Hazardous Asteroids

April 2005 Earth-asteroid encounters
ASTEROID

 DATE (UT)

 MISS DISTANCE

 MAG.
2005 EU2

Apr. 5

6.2 LD

 18
2005 EE169

Apr. 6

5.9 LD

 18
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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