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Solar wind
speed: 356.9 km/sec
density: 2.2 protons/cm3
explanation | more data
Updated: Today at 2347 UT
X-ray Solar Flares
6-hr max: C1
2213 UT Apr14
24-hr: C7
0438 UT Apr14
explanation | more data
Updated: Today at: 2300 UT
Daily Sun: 14 Apr 14
Earth-facing sunspots AR2034 and AR2035 have 'beta-gamma' magnetic fields that harbor energy for M-class solar flares. Credit: SDO/HMI
Sunspot number: 95
What is the sunspot number?
Updated 14 Apr 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
14 Apr 2014

The Radio Sun
10.7 cm flux: 137 sfu
explanation | more data
Updated 14 Apr 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= 3
quiet
explanation | more data
Interplanetary Mag. Field
Btotal: 3.1 nT
Bz: 0.6 nT south
explanation | more data
Updated: Today at 2346 UT
Coronal Holes: 14 Apr 14
There are no large equatorial 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 Apr 14 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 Apr 14 2200 UTC
Mid-latitudes
0-24 hr
24-48 hr
ACTIVE
25 %
05 %
MINOR
10 %
01 %
SEVERE
01 %
01 %
High latitudes
0-24 hr
24-48 hr
ACTIVE
15 %
15 %
MINOR
25 %
15 %
SEVERE
35 %
05 %
 
Monday, Apr. 14, 2014
What's up in space
 

On April 15th there will be a total eclipse of the Moon. Got clouds? No problem. The event will be broadcast live on the web by the Coca-Cola Science Center.

 
2014 Lunar Eclipse Live

A NEW MOON NAMED 'PEGGY': NASA's Cassini spacecraft has photographed a small icy object forming at the edge of Saturn's rings. Informally named "Peggy," it may be a new moon caught in the act of genesis. Get the full story from Science@NASA.

LUNAR ECLIPSE, TUESDAY MORNING: The mainstream media is abuzz with reports of a "blood moon" on Tuesday morning. The scientific term is "lunar eclipse." On April 15th at 6 minutes past midnight Pacific Time (3:06 a.m Eastern Time), the Moon will enter the sunset-colored colored shadow of Earth, producing a total eclipse of the Moon:


Above: A total lunar eclipse on Dec. 21, 2010. Photo credit: Gary A. Becker

The color of Earth's shadow, and thus the color of the eclipsed Moon, depends substantially on the amount of volcanic ash and other aerosols floating in the stratosphere. According to atmospheric sciences professor Richard Keen of the University of Colorado, the stratosphere is clear. This means the eclipse will be not "blood red," but rather bright orange.

See for yourself. The event will be visible from Australia, New Zealand, and all of the Americas: visibility map. It's so bright, even observers in light-polluted cities will have no trouble enjoying the show. Got clouds? No problem. The event will be broadcast live on the web by the Coca-Cola Science Center at Columbus State University in Georgia.

For more information about the eclipse, get the full story and a video from Science@NASA.

Realtime Eclipse Photo Gallery

NASA SPACECRAFT vs. THE LUNAR ECLIPSE: NASA's LADEE spacecraft, now orbiting the Moon on a mission to study the lunar atmosphere, might not survive the lunar eclipse. "LADEE wasn't designed to go through a long eclipse and keep things running," says Richard Elphic, the project scientist for LADEE at NASA Ames.

The spacecraft is solar powered, and it uses battery-driven heaters to keep itself warm. LADEE regularly experiences periods of low-to-no sunlight for 45 minutes when it passes over the nightside of the Moon. During the eclipse, the "shadow time" will last as much as 4 hours.

"Even dipping into the penumbra (the outskirts of Earth's shadow) means we lose power generation, and for the full Earth umbra (the dark core of Earth's shadow) there's no solar array generation at all," continues Elphic. "So we'll be running on battery, with no array generation, and using heaters more than usual to keep things warm."

"There are some areas of the spacecraft that will not be warmed up by heaters – part of LADEE's propulsion system, for example.  So it is possible these might freeze and never warm up sufficiently again.  We won't know until after eclipse and we get housekeeping and state of health data," says Elphic.

And now for the good news. "Our in flight data show that power and thermal are behaving better than predicted, because of the built in margins, so we expect the spacecraft to survive just fine," reports Butler Hine, the LADEE Project Manager at Ames. "The unheated portions of the propulsion system are mainly what we will be watching for any freezing."

Regardless of how LADEE emerges from the eclipse, the mission is near its end. NASA's plans to crash LADEE into the lunar surface as part of a "skimming" maneuver that will allow the spacecraft to sample the Moon's near-surface atmosphere. "We have already used our extra fuel for the one month extension we are in now," concludes Hine. "Even if we survive the eclipse we will impact as planned. We do get an extra week of science data if we survive the eclipse, however."

Stay tuned for updates from LADEE.

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 Apr. 13, 2014, the network reported 6 fireballs.
(6 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 April 14, 2014 there were 1466 potentially hazardous asteroids.
Recent & Upcoming Earth-asteroid encounters:
Asteroid
Date(UT)
Miss Distance
Size
2014 GQ45
Apr 10
8.2 LD
33 m
2007 TV18
Apr 18
7.4 LD
88 m
2014 GG49
Apr 19
3.9 LD
31 m
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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