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

X-ray Solar Flares
6-hr max:
A0 2150 UT Apr07
24-hr: A0 1555 UT Apr07
explanation | more data
Updated: Today at 2245 UT

Daily Sun: 07 Apr '07

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

Sunspot Number: 0
What is the sunspot number?
Updated: 06 Apr 2007

Far Side of the Sun

This holographic image reveals one sunspot on the far side of the sun. Image credit: SOHO/MDI

Interplanetary Mag. Field
Btotal: 1.6 nT
Bz:
-0.0 nT
explanation | more data
Updated: Today at 2246 UT

Coronal Holes:

A solar wind stream flowing from the indicated coronal hole could reach Earth on April 9th. 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 07 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 07 2203 UTC
Mid-latitudes
0-24 hr 24-48 hr
ACTIVE 20 % 25 %
MINOR 05 % 15 %
SEVERE 01 % 10 %

High latitudes
0-24 hr 24-48 hr
ACTIVE 20 % 35 %
MINOR 10 % 20 %
SEVERE 05 % 15 %

What's Up in Space -- 7 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 9th and 10th. A solar wind stream is due to hit Earth, and the impact could cause high-latitude geomagnetic storms.

SOLAR ACTIVITY: A large tornado-shaped prominence is twisting over the northwestern limb of the sun. Eric Roel of Valle de Bravo, Mèxico, took this picture yesterday:

This prominence, essentially a magnetic vortex filled with glowing-hot hydrogen, towers about five Earth diameters over the surface of the sun. If you have a solar telescope, take a look!

more images: from Les Cowley of the UK; from Marko Vidovic of Stojnci, Slovenia; from P-M Hedén of Vallentuna, Sweden; from John Stetson of Falmouth, Maine; from Sally Russell of Southern England; from Emiel Veldhuis of Zwolle, the Netherlands; from Britta Suhre of Germany, NRW, Dortmund; from Pete Lawrence of Selsey, West Sussex, UK.

MYSTERY IN THE CLOUDS: Seen through an ordinary telescope, Venus looks a bit dull--it's a featureless, cloud-covered orb. But if that same telescope is fitted with an ultraviolet filter, a mystery reveals itself: Venus' clouds are cross-crossed with rapidly-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 ccd camera, 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 these bands since Mariner 10 first spotted them in the 1970s, but decades later no one knows the identity of the "UV absorbers." Maybe Venus Express, a European spacecraft orbiting Venus now, will eventually solve the mystery.

You can see Venus with your own eyes--indeed you can't miss it. It appears in the western sky at sunset glaring like a landing airplane. A backyard telescope reveals the point of light as a cloud-covered planet, and a UV filter reveals the mystery in the clouds. "I am using a 1.25-inch Schuler photometric UV pass filter. I also have the Baader UV pass filter, but the Schuler is a better performer," advises Lomeli.



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 7 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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