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Solar wind
speed: 288.3 km/sec
density: 2.3 protons/cm3
explanation | more data
Updated: Today at 2347 UT
X-ray Solar Flares
6-hr max: B9
1757 UT Mar17
24-hr: C2
0045 UT Mar17
explanation | more data
Updated: Today at: 2300 UT
Daily Sun: 17 Mar 14
None of these sunspots is strongly flaring. Solar activity is low. Credit: SDO/HMI
Sunspot number: 139
What is the sunspot number?
Updated 17 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
17 Mar 2014

The Radio Sun
10.7 cm flux: 136 sfu
explanation | more data
Updated 17 Mar 2014

Current Auroral Oval:
Switch to: Europe, USA, New Zealand, Antarctica
Credit: NOAA/POES
Planetary K-index
Now: Kp= 1 quiet
24-hr max: Kp= 1
quiet
explanation | more data
Interplanetary Mag. Field
Btotal: 4.0 nT
Bz: 1.6 nT south
explanation | more data
Updated: Today at 2347 UT
Coronal Holes: 17 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 17 2200 UTC
FLARE
0-24 hr
24-48 hr
CLASS M
35 %
35 %
CLASS X
05 %
05 %
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 17 2200 UTC
Mid-latitudes
0-24 hr
24-48 hr
ACTIVE
10 %
05 %
MINOR
01 %
01 %
SEVERE
01 %
01 %
High latitudes
0-24 hr
24-48 hr
ACTIVE
15 %
15 %
MINOR
20 %
15 %
SEVERE
20 %
05 %
 
Monday, Mar. 17, 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

GREEN SKIES ON ST. PATRICK'S DAY? NOAA forecasters estimate a 15% chance of polar geomagnetic storms on March 17th. That means the odds of green skies on St. Patrick's Day are low. Instead, look for shamrock colors here. Solar flare alerts: text, voice

SPACE WEATHER BALLOON--DOUBLE LAUNCH: Yesterday, the students of Earth to Sky Calculus launched a pair of research balloons into the stratosphere. One of the balloons carried an experimental Space Weather payload designed for rapid deployment during unexpected solar storms. Here it is, photographed in flight by the companion balloon:

The two balloons were about 18,000 feet above sea level when the photo was taken. One balloon photographing another in flight is a rare and possibly unique occurrence in the growing field of high-altitude ballooning. Congratulations to the students for breaking new ground in the air.

There was no solar storm yesterday. The test flight of the Rapid Response Space Weather Payload prepares the team for another day when a strong flare or geomagnetic storm takes forecasters by surprise. This fast-turnaround payload can be dispatched on a moment's notice to probe the stratosphere while the storm is underway. It includes a high-energy radiation sensor, a cryogenic thermometer, a GPS altimeter and other devices. Stay tuned for more data and images from the flight.

UPDATED--ERUPTING FILAMENT CREATES A 'CANYON OF FIRE': For days, amateur astronomers have been monitoring two long, dark filaments of magnetism snaking around the sun's southeastern limb. On March 16th, one of them became unstable and erupted. The resulting explosion split the sun's atmosphere, creating a "canyon of fire," shown here in a movie captured by the Solar Dynamics Observatory:

The glowing walls of the canyon are formed in a process closely related to that of arcade loops, which appear after many solar flares. The structure traces the original channel where the filament was suspended by magnetic forces above the stellar surface.

As erupting magnetic filaments often do, this one launched a coronal mass ejection (CME) into space. Update: The Solar and Heliospheric Observatory recorded a movie of the cloud expanding at 800 km/s (1.8 million mph). NOAA analysts say the CME is traveling south of the sun-Earth line and should not be geoeffective. Solar flare alerts: text, voice

Realtime Space Weather Photo Gallery


Realtime Aurora Photo Gallery


Realtime Mars 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. 17, 2014, the network reported 5 fireballs.
(5 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 17, 2014 there were potentially hazardous asteroids.
Recent & Upcoming Earth-asteroid encounters:
Asteroid
Date(UT)
Miss Distance
Size
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
36 m
2014 EY24
Mar 18
8.5 LD
70 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
2010 JO33
May 17
4 LD
43 m
2005 UK1
May 20
36.7 LD
1.1 km
1997 WS22
May 21
47.1 LD
1.5 km
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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