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Solar wind
speed: 321.2 km/sec
density: 11.0 protons/cm3
explanation | more data
Updated: Today at 2346 UT
X-ray Solar Flares
6-hr max: M9
2234 UT Mar12
24-hr: M9
2234 UT Mar12
explanation | more data
Updated: Today at: 2300 UT
Daily Sun: 12 Mar 14
Sunspot AR2002 has a 'beta-gamma-delta' magnetic field that harbors energy for X-class solar flares. Credit: SDO/HMI
Sunspot number: 108
What is the sunspot number?
Updated 12 Mar 2014

Spotless Days
Current Stretch: 0 days
2014 total: 0 days (0%)
2013 total: 0 days (0%)
2012 total: 0 days (0%)
2011 total: 2 days (<1%)
2010 total: 51 days (14%)
2009 total: 260 days (71%)

Update
12 Mar 2014

The Radio Sun
10.7 cm flux: 152 sfu
explanation | more data
Updated 12 Mar 2014

Current Auroral Oval:
Switch to: Europe, USA, New Zealand, Antarctica
Credit: NOAA/POES
Planetary K-index
Now: Kp= 2 quiet
24-hr max: Kp= 2
quiet
explanation | more data
Interplanetary Mag. Field
Btotal: 7.4 nT
Bz: 7.3 nT south
explanation | more data
Updated: Today at 2346 UT
Coronal Holes: 12 Mar 14
There are no large coronal holes on the Earthside of the sun. Credit: SDO/AIA.

Spaceweather.com posts daily satellite images of noctilucent clouds (NLCs), which hover over Earth's poles at the edge of space. The data come from NASA's AIM spacecraft. The north polar "daisy" pictured below is a composite of near-realtime images from AIM assembled by researchers at the University of Colorado's Laboratory for Atmospheric and Space Physics (LASP).
Noctilucent Clouds
Switch view: Europe, USA, Asia, Polar
Updated at: 02-28-2014 16:55:02
SPACE WEATHER
NOAA Forecasts
Updated at: 2014 Mar 12 2200 UTC
FLARE
0-24 hr
24-48 hr
CLASS M
80 %
80 %
CLASS X
15 %
15 %
Geomagnetic Storms:
Probabilities for significant disturbances in Earth's magnetic field are given for three activity levels: active, minor storm, severe storm
Updated at: 2014 Mar 12 2200 UTC
Mid-latitudes
0-24 hr
24-48 hr
ACTIVE
05 %
05 %
MINOR
01 %
01 %
SEVERE
01 %
01 %
High latitudes
0-24 hr
24-48 hr
ACTIVE
15 %
15 %
MINOR
15 %
15 %
SEVERE
05 %
05 %
 
Wednesday, Mar. 12, 2014
What's up in space
 

When is the best time to see auroras? Where is the best place to go? And how do you photograph them? These questions and more are answered in a new book, Northern Lights - a Guide, by Pal Brekke & Fredrik Broms.

 
Northern Lights - a Guide

CHANCE OF FLARES: Sunspot AR2002 has been mostly quiet for the past 24 hours. Nevertheless, the Earth-facing active region has a'beta-gamma-delta' magnetic field tthat harbors ebergy for strong eruptions. NOAA forecasters estimate a 75% chance of M-class flares and a 15% chance of X-class flares on March 12th. Solar flare alerts: text, voice

BLACKOUT! This morning at 06:23 UT, NASA's Solar Dynamics Observatory (SDO) observed a sudden darkening of the sun's northwestern limb. A moment later the whole sun was gone. Scroll past the image to find out what happened:

Earth itself passed directly in front of the spacecraft, eclipsing the sun. This is SDO's spring eclipse season. Twice every year, around the time of the equinoxes, Earth can pass directly between the Sun and NASA's Solar Dynamics Observatory.

At the moment, SDO is near the midpoint of the season when the eclipses are longest and deepest. Once a day, Earth blocks the complete sun for more than an hour. That still allows almost 23 hours for monitoring solar activity, so not much action is missed. Eclipse season ends about a week from now. Between now and then, stay tuned for some rare blackouts. Solar flare alerts: text, voice

Realtime Space Weather Photo Gallery

FRIDAY IS PI DAY: Mark your calendar. This Friday, March 14th (3.14), is day. It's an occasion to celebrate one of the most compelling and mysterious constants of Nature. Pi appears in equations describing the orbits of planets, the colors of auroras, the structure of DNA. The value of is woven into the fabric of life, the universe and ... everything.

Humans have struggled to calculate for thousands of years. Divide the circumference of a circle by its diameter; the ratio is . Sounds simple, but the devil is in the digits. While the value of is finite (a smidgen more than 3), the decimal number is infinitely long:

3.1415926535897932384626433832795
02884197169399375105820974944592307
81640628620899862803482534211706...more

Supercomputers have succeeded in calculating more than 2700 billion digits and they're still crunching. The weirdest way to compute : throw needles at a table or frozen hot dogs on the floor. Party time!


Realtime Aurora Photo Gallery


Realtime Comet Photo Gallery


  All Sky Fireball Network

Every night, a network of NASA all-sky cameras scans the skies above the United States for meteoritic fireballs. Automated software maintained by NASA's Meteoroid Environment Office calculates their orbits, velocity, penetration depth in Earth's atmosphere and many other characteristics. Daily results are presented here on Spaceweather.com.

On Mar. 10, 2014, the network reported 3 fireballs.
(3 sporadics)

In this diagram of the inner solar system, all of the fireball orbits intersect at a single point--Earth. The orbits are color-coded by velocity, from slow (red) to fast (blue). [Larger image] [movies]

  Near Earth Asteroids
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 March 12, 2014 there were 1459 potentially hazardous asteroids.
Recent & Upcoming Earth-asteroid encounters:
Asteroid
Date(UT)
Miss Distance
Size
2014 EX24
Mar 9
0.7 LD
8 m
2014 CU13
Mar 11
8 LD
190 m
2014 EP12
Mar 14
2.9 LD
33 m
2014 EB25
Mar 14
2.7 LD
16 m
2014 DU22
Mar 14
7.9 LD
60 m
2014 EM
Mar 15
4.3 LD
37 m
2014 EY24
Mar 18
8.4 LD
81 m
2003 QQ47
Mar 26
49.9 LD
1.4 km
1995 SA
Apr 2
73.1 LD
1.6 km
2000 HD24
Apr 4
42.2 LD
1.3 km
2007 HB15
Apr 28
6.7 LD
12 m
Notes: LD means "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 Weather Prediction Center
  The official U.S. government space weather bureau
Atmospheric Optics
  The first place to look for information about sundogs, pillars, rainbows and related phenomena.
Solar Dynamics Observatory
  Researchers call it a "Hubble for the sun." SDO is the most advanced solar observatory ever.
STEREO
  3D views of the sun from NASA's Solar and Terrestrial Relations Observatory
Solar and Heliospheric Observatory
  Realtime and archival images of the Sun from SOHO.
Daily Sunspot Summaries
  from the NOAA Space Environment Center
Heliophysics
  the underlying science of space weather
Space Weather Alerts
   
  more links...
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