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Solar wind
speed: 459.3 km/sec
density: 1.9 protons/cm3
explanation | more data
Updated: Today at 2346 UT
X-ray Solar Flares
6-hr max: B8
2113 UT Mar25
24-hr: C1
0529 UT Mar25
explanation | more data
Updated: Today at: 2300 UT
Daily Sun: 25 Mar 14
Sunspot AR2010 has a 'beta-gamma-delta' magnetic field that harbor energy for X-class solar flares. Credit: SDO/HMI
Sunspot number: 132
What is the sunspot number?
Updated 25 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
25 Mar 2014

The Radio Sun
10.7 cm flux: 159 sfu
explanation | more data
Updated 25 Mar 2014

Current Auroral Oval:
Switch to: Europe, USA, New Zealand, Antarctica
Credit: NOAA/POES
Planetary K-index
Now: Kp= 3 quiet
24-hr max: Kp= 3
quiet
explanation | more data
Interplanetary Mag. Field
Btotal: 9.3 nT
Bz: 6.9 nT north
explanation | more data
Updated: Today at 2035 UT
Coronal Holes: 25 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 25 2200 UTC
FLARE
0-24 hr
24-48 hr
CLASS M
35 %
35 %
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: 2014 Mar 25 2200 UTC
Mid-latitudes
0-24 hr
24-48 hr
ACTIVE
30 %
05 %
MINOR
10 %
01 %
SEVERE
01 %
01 %
High latitudes
0-24 hr
24-48 hr
ACTIVE
15 %
15 %
MINOR
30 %
15 %
SEVERE
40 %
05 %
 
Tuesday, Mar. 25, 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

CME IMPACT: A CME hit Earth's magnetic field on March 25th at approximately 19:45 UT (12:45 pm PDT). Minor to moderate geomagnetic storms are possible in the hours ahead. High-latitude sky watchers should be alert for auroras after nightfall. Aurora alerts: text, voice

OBJECT AT THE EDGE OF SPACE: On March 16th, a strangely-shaped object was photographed 92,000 feet above Earth's surface. Can you guess what it is? Scrutinize the image, then scroll down for the answer:

It's a tangled wad of natural rubber, the remains of a suborbital helium research balloon that popped approximately 2 seconds before the photo was taken. Regular readers might have already guessed that the picture was taken by the Space Weather Rapid Response (SWxRR) Payload launched to the stratosphere on March 16th by the students of Earth to Sky Calculus. This is just one of many spectacular pictures captured during the two-hour flight to the edge of space.

SWxRR is an experimental payload that can be launched to the edge of space with minimal delay in response to fast-developing or unexpected space weather events. It contains cameras, a cryogenic thermometer, a GPS altimeter, and a 10.0 KeV to 20.0 MeV radiation counter to measure the effect of solar storms on Earth's upper atmosphere. Ultimately, as techniques are improved, we hope to be able to sample the radiation content of the atmosphere and report results to readers while storms are in progress. Data from the March 16th flight are being analyzed now. Stay tuned for updates.

Realtime Space Weather Photo Gallery

ACTIVE SUNSPOTS: Earth is looking down the double barrel of two potentially active sunspots: AR2010 and AR2014 have complex magnetic fields that harbor energy for strong eruptions, and both have grown since the week began. Click to view a movie of their development from NASA's Solar Dynamics Observatory:

The CME expected to sideswipe Earth later today was propelled toward us by a C-flare from sunspot AR2014 on March 23rd. Otherwise the two sunspots have been mostly quiet. Is it the calm before the storm? NOAA forecasters estimate a 45% chance of M-class flares and a 5% chance of X-flares on March 25th.. Solar flare alerts: text, voice

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. 22, 2014, the network reported 2 fireballs.
(2 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 25, 2014 there were 1462 potentially hazardous asteroids.
Recent & Upcoming Earth-asteroid encounters:
Asteroid
Date(UT)
Miss Distance
Size
2014 FB7
Mar 21
3.1 LD
14 m
2014 FZ
Mar 25
7.5 LD
18 m
2014 FD
Mar 25
4.5 LD
36 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
2002 JC
May 24
48.7 LD
1.4 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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