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


X-ray Solar Flares

6-hr max:
A2 2100 UT Mar17
24-hr: A2 0555 UT Mar17
explanation | more data
Updated: Today at 2245 UT

Daily Sun: 17 Mar '06

Tiny sunspots 860 and 861 pose no threat for strong solar flares. Photo credit: SOHO/MDI


Sunspot Number: 22
What is the sunspot number?
Updated: 16 Mar 2006

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: 3.5 nT
Bz:
3.0 nT north
explanation | more data
Updated: Today at 2246 UT

Coronal Holes:

SOHO ultraviolet images of the sun are temporarily unavailable. Why? The telescope's CCD camera is being baked out.


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 2006 Mar 17 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 2006 Mar 17 2203 UTC
Mid-latitudes
0-24 hr 24-48 hr
ACTIVE 10 % 30 %
MINOR 01 % 10 %
SEVERE 01 % 05 %

High latitudes
0-24 hr 24-48 hr
ACTIVE 25 % 40 %
MINOR 05 % 25 %
SEVERE 01 % 10 %

What's Up in Space -- 17 Mar 2006
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QUIET SUN: There are only a few small spots on the sun today, and neither poses a threat for flares. That means solar activity is low. Or is it? Continued below...

ACTIVE SUN: "Today is a nice day for sungazing," says Greg Piepol of Rockville, Maryland, who photographed at least five prominences dancing along the limb of the sun on March 16th:


The sun on March 16th, as seen through a Coronado telescope.

Although they resemble flames, prominences are not fire. They are clouds of hot gas held aloft by magnetic force fields. And because prominences do not depend on sunspots for their magnetism, they are visible even during the lowest ebb of the sunspot cycle--like now.

more images: from John Stetson of Falmouth, Maine; from Mike Strieber of Newport News, Virginia; from Gary Palmer of Los Angeles, California; from Peter Paice of Belfast, Northern Ireland;

SATURN'S RINGS: Saturn's rings are vanishing! No need to panic, it's happened before. As Saturn goes around the sun, it occasionally turns its rings edge-on to Earth. Because the rings are so thin, they disappear when viewed through a small telescope.

The next "ring plane crossing" isn't due until 2009. Already, though, we can see the process at work. Witness this 3-year animation assembled by Alan Friedman from pictures he has taken from his backyard in Buffalo, New York, between 2004 and 2006:


Animation credit: Alan Friedman and Richard Bosman

In the years ahead, Saturn's rings will become thinner and thinner until, on Sept. 4, 2009, they will briefly disappear. When this happened to Galileo in 1612, he temporarily abandoned his study of the planet. Big mistake: ring plane crossings are good times to discover new moons and faint outer rings.



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 17 Mar 2006 there were 773 known Potentially
Hazardous Asteroids

March 2006 Earth-asteroid encounters
ASTEROID

 DATE
(UT)

MISS DISTANCE

MAG.

 SIZE
(meters)
2000 PN9

March 6

7.9 LD

12

~2 km
2006 EH1

March 7

2.0 LD

18

~20 m
2006 EC

March 8

0.7 LD

16

~19 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. 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

Daily images from the sun -- 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.

Lists of Coronal Mass Ejections -- from 1998 to 2001

Mirages: Mirages in Finland; An Introduction to Mirages;

NOAA Solar Flare and Sunspot Data: 1996, 1997, 1998, 1999; 2000; 2001; 2002; 2003; 2004; 2005; Jan-Mar 2006;

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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