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

X-ray Solar Flares
6-hr max:
A0 1940 UT Apr08
24-hr: A0 1940 UT Apr08
explanation | more data
Updated: Today at 2245 UT

Daily Sun: 08 Apr '07

The sun is blank today--no sunspots. Credit: SOHO/MDI

Sunspot Number: 0
What is the sunspot number?
Updated: 07 Apr 2007

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: 16.6 nT
Bz:
2.9 nT south
explanation | more data
Updated: Today at 2246 UT

Coronal Holes:

A solar wind stream flowing from the indicated coronal hole could reach Earth late on April 9th or April 10th. 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 Apr 08 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 Apr 08 2203 UTC
Mid-latitudes
0-24 hr 24-48 hr
ACTIVE 30 % 20 %
MINOR 15 % 10 %
SEVERE 10 % 05 %

High latitudes
0-24 hr 24-48 hr
ACTIVE 35 % 25 %
MINOR 20 % 15 %
SEVERE 15 % 05 %

What's Up in Space -- 8 Apr 2007
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Did you miss last night's auroras? Next time get a wake-up call from Spaceweather PHONE.

AURORA WATCH: Sky watchers from Scandinavia to Alaska should be alert for auroras on April 10th. A solar wind stream is due to hit Earth, and the impact could cause high-latitude geomagnetic storms.

VENUS AND THE PLEIADES: The Goddess of Love is about to pay a visit to the Seven Sisters--or as an astronomer would say, Venus is moving into conjunction with the Pleiades. The planet and the star cluster will be side-by-side after dark on Wednesday, April 11th: finder chart.


Photo details: Canon EOS 20D, 135 mm, 100 ASA

Günther Strauch of Borken, Germany, snapped this picture of Venus approaching the Pleiades on April 4th. Venus was so bright it beamed right through the clouds, forming a lovely halo: image. "Very nice," he says. And the view will only improve in the nights ahead

What are the Pleiades? A cluster of baby stars. They formed barely 100 million years ago, during the age of dinosaurs on Earth, from a collapsing cloud of interstellar gas. The biggest and brightest are blue-white and about five times wider than our own sun. Because the brightest stars of the cluster form a little dipper shape in the sky, the Pleiades are often mistaken for the Little Dipper--but the two are not the same. The Little Dipper is another name for the constellation Ursa Minor, while the Pleiades are part of the constellation Taurus. Scanning the Pleiades with binoculars reveals dozens of stars invisible to the unaided eye. It's very pretty, so take a look!

MYSTERY IN THE CLOUDS: Seen through an ordinary backyard telescope, Venus seems bland. It's a featureless, cloud-covered orb about as interesting as a billiard ball. But if that same telescope is fitted with an ultraviolet filter, a mystery reveals itself. Venus' clouds are cross-crossed with fast-moving dark bands, shown here in a series of March 30th photos from Ed Lomeli of Sacramento, California:


Photo details: Celestron 9-inch telescope, DMK 21BF04, UV pass filter

The bands are the mystery. Some unknown substance within them strongly absorbs UV light, accounting for almost half of the solar energy trapped by Venus. Whatever is in there, it plays a big role in maintaining Venus' hellish climate; the average temperature on the surface is about 460° Celsius. Astronomers have been studying the bands since Mariner 10 spotted them in the 1970s, but decades later no one knows the identity of the "UV absorbers." Candidates range from gaseous chlorine and sulfur compounds to alien life using UV radiation as a source of energy. Maybe Venus Express, a European spacecraft orbiting Venus now, will solve the puzzle.

To photograph the bands, Lomelli used a 9-inch Celestron telescope, a 640x480 monochrome ccd camera, and a 1.25-inch Schuler photometric UV pass filter. "I also have the Baader UV pass filter, but the Schuler is a better performer," he advises.



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 8 Apr 2007 there were 855 known Potentially
Hazardous Asteroids

April 2007 Earth-asteroid encounters
ASTEROID

 DATE
(UT)

MISS DISTANCE

MAG.

 SIZE
2006 VV2

Mar. 31

8.8 LD

10

2 km
2007 FY20

Apr. 2

5.3 LD

19

50 m
2007 DS84

Apr. 14

16 LD

15

325 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

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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