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Solar wind
speed: 298.7 km/sec
density: 6.0 protons/cm3
explanation | more data
Updated: Today at 2346 UT
X-ray Solar Flares
6-hr max: C1
2208 UT Dec27
24-hr: C4
1213 UT Dec27
explanation | more data
Updated: Today at: 2300 UT
Daily Sun: 27 Dec 13
Sunspots AR1934 and AR1936 have 'beta-gamma' magnetic fields that harbor energy for M-class solar flares. Credit: SDO/HMI
Sunspot number: 96
What is the sunspot number?
Updated 27 Dec 2013

Spotless Days
Current Stretch: 0 days
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%)
Since 2004: 821 days
Typical Solar Min: 486 days

Update
27 Dec 2013

The Radio Sun
10.7 cm flux: 125 sfu
explanation | more data
Updated 27 Dec 2013

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: 3.1 nT
Bz: 2.9 nT south
explanation | more data
Updated: Today at 2347 UT
Coronal Holes: 27 Dec 13
Solar wind flowing from the indicated coronal hole could reach Earth on Jan 2-3. 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: 12-27-2013 10:55:02
SPACE WEATHER
NOAA Forecasts
Updated at: 2013 Dec 27 2200 UTC
FLARE
0-24 hr
24-48 hr
CLASS M
25 %
25 %
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: 2013 Dec 27 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 %
 
Friday, Dec. 27, 2013
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

(ALMOST NO) CHANCE OF FLARES: Two sunspots facing Earth (AR1934 and AR1936) have 'beta-gamma' magnetic fields that harbor energy for strong flares. Both sunspots have been quiet for days, however, and they show no signs of an imminent eruption. This has prompted NOAA forecasters to place low odds on flares today: a 25% chance of M-flares and a 1% chance X-flares. Solar flare alerts: text, voice.

RADIO STORMS ON JUPITER: This week, there was a storm on Jupiter--a radio storm. Amateur radio astronomer Thomas Ashcraft recorded the event on Dec. 23rd using a shortwave radio telescope located in New Mexico. Click on the image to hear the whooshing, crackling, popping sounds that emerged from his telescope's loudspeaker:

"Although few were aware of it, Earth was bathed in Jovian radio beams for an hour and half," says Ashcraft. "The audio recording captures the sounds I heard during one minute around 09:30 UT."

Jupiter's radio storms are caused by natural radio lasers in the planet's magnetosphere that sweep past Earth as Jupiter rotates. Electrical currents flowing between Jupiter's upper atmosphere and the volcanic moon Io can boost these emissions to power levels easily detected by ham radio antennas on Earth. Jovian "S-bursts" (short bursts) and "L-bursts" (long bursts) mimic the sounds of woodpeckers, whales, and waves crashing on the beach. Here are a few audio samples: S-bursts, S-bursts (slowed down 128:1), L-Bursts

Now is a good time to listen to Jupiter's radio storms. The distance between Earth and Jupiter is decreasing as the giant planet approaches opposition on Jan. 5th; and the closer Jupiter comes, the louder it gets. Jupiter is a bit like a lighthouse. It is possible to predict when the planet's most intense radio beams will sweep past Earth. The next storm is due on Dec. 30th between 10:00 and 11:00 UT. NASA's Radio Jove Project explains how to build your own receiver.

Realtime Space Weather Photo Gallery

SOLAR WIND STREAM MISSES EARTH: A stream of solar wind expected to hit Earth's magnetic field on Dec. 26-27 has apparently missed, sailing mostly north of our planet. As a result, Earth's magnetic field is quiet and the polar auroral oval is dim. Another solar wind stream is coming, though, and it will likely reach Earth on Jan. 2-3, producing the first auroras of New Year. Arctic sky watchers could see something like this:

Nancy Dean of Sterling, Alaska, took the picture on Dec. 26th. "It was about 1:30 in the morning and -20 degrees outside when I got this photo," she says. At the time, the interplanetary magnetic (IMF) field near Earth had turned south, opening a crack in our planet's magnetosphere. Solar wind poured in and fueled the display. Aurora alerts: text, voice.

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 Dec. 27, 2013, the network reported 16 fireballs.
(13 sporadics, 2 December Leonis Minorids, 1 December Hydrid)

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]

On Dec. 26, 2013, the network reported 24 fireballs.
(21 sporadics, 3 December Leonis Minorids)

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 December 27, 2013 there were 1448 potentially hazardous asteroids.
Recent & Upcoming Earth-asteroid encounters:
Asteroid
Date(UT)
Miss Distance
Size
2013 YQ2
Dec 21
4.2 LD
86 m
2013 YB
Dec 23
0.07 LD
2 m
2011 YD29
Dec 28
6.1 LD
24 m
2013 YL2
Jan 3
3.6 LD
109 m
2007 SJ
Jan 21
18.9 LD
1.9 km
2012 BX34
Jan 28
9.6 LD
13 m
2006 DP14
Feb 10
6.2 LD
730 m
2000 EM26
Feb 18
8.8 LD
195 m
2000 EE14
Mar 6
64.6 LD
1.8 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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