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Solar wind
speed: 452.3 km/sec
density: 1.6 protons/cm3
explanation | more data
Updated: Today at 2347 UT
X-ray Solar Flares
6-hr max: C1
2135 UT Sep04
24-hr: C3
0428 UT Sep04
explanation | more data
Updated: Today at: 2300 UT
Daily Sun: 04 Sep 13
AR1837 is crackling with low-level C-flares. Otherwise, the Earthside of the sun is quiet. Credit: SDO/HMI
Sunspot number: 74
What is the sunspot number?
Updated 04 Sep 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
04 Sep 2013

The Radio Sun
10.7 cm flux: 106 sfu
explanation | more data
Updated 04 Sep 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: 4.4 nT
Bz: 2.8 nT north
explanation | more data
Updated: Today at 2347 UT
Coronal Holes: 04 Sep 13
Solar wind flowing from the indicated coronal hole should reach Earth on Sept. 5-6. Credit: SDO/AIA.

Spaceweather.com is now posting 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: 09-02-2013 11:55:02
SPACE WEATHER
NOAA Forecasts
Updated at: 2013 Sep 04 2200 UTC
FLARE
0-24 hr
24-48 hr
CLASS M
05 %
05 %
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 Sep 04 2200 UTC
Mid-latitudes
0-24 hr
24-48 hr
ACTIVE
15 %
15 %
MINOR
05 %
05 %
SEVERE
01 %
01 %
High latitudes
0-24 hr
24-48 hr
ACTIVE
15 %
15 %
MINOR
25 %
25 %
SEVERE
25 %
25 %
 
Wednesday, Sep. 4, 2013
What's up in space
 

They came from outer space--and you can have one! Genuine meteorites are now on sale in the Space Weather Store.

 
Own your own meteorite

QUIET SUNSPOTS: All of the sunspots on the Earthside of the sun are stable and quiet. NOAA forecasters estimate a slight 5% chance of M-class solar flares and no more than a 1% chance of X-class flares on Sept. 4th. Solar flare alerts: text, voice.

SOLAR ECLIPSE: Twice every year, around the time of the equinoxes, Earth can pass directly between the Sun and NASA's Solar Dynamics Observatory (SDO), producing a series of beautiful eclipses from the point of view of the spacecraft. SDO's autumnal eclipse season began this week, producing a partial blackout of the sun:

During the eclipse, which was centered around 0658 UT on Sept. 2nd, Earth covered about half of the sun. Because these eclipses typically last for only minutes each day (maximum=72 minutes), there is still plenty of uninterrupted time for SDO to monitor activity on the sun. The ongoing eclipse season will end on Sept. 25th. Between now and then, stay tuned for some rare blackouts.

Realtime Space Weather Photo Gallery

ACTIVE PROMINENCE: The face of the sun may be quiet, but the edge is surging with activity. "A fantastic prominence is forming on the solar limb," reports amateur astronomer Sergio Castillo of Inglewood, California. "It is so bright, it caught my eye right away." This is how it looked through his backyard solar telescope:

"This prom is for sure making up for the absence of flares on the sun this week," he adds.

Prominences are clouds of hot-glowing plasma held above the sun's surface by magnetic fields. Observing from the Sorbas area of southern Spain, amateur astronomer Andy Devey has video-recorded a strong vortex motion in this prominence. If the spinning motion destabilizes the underlying magnetic field and the prominence collapses, the result could be a Hyder flare. Solar astronomers are encouraged to monitor developments. Solar flare alerts: text, voice.

Realtime Space Weather Photo Gallery

ARCTIC LIGHTS: "Last night (Sept. 2) we had a spectacular sunset," reports photographer Frank Olsen, "but the auroras were even better." This is what the end of the day looked like from Olsen's photo-site on Andøya island, Norway:

The source of the display was a minor solar wind stream buffeting Earth's magnetic field--not hard enough to trigger a full-fledged geomagnetic storm, but enough to spark auroras visible against the darkening late-summer sky.

More lights could be in the offing. NOAA forecasters estimate a 25% chance of polar geomagnetic storms on Sept. 5-6 when a solar wind stream is expected to hit Earth's magnetic field. Aurora alerts: text, voice.

Realtime Aurora Photo Gallery

SWx EXPERIMENT IN RIPLEY'S BELIEVE IT OR NOT: In March 2012, a group of high school students in Bishop, California, used a helium balloon to launch a pair of medical radiation badges to the edge of space. The goal of their experiment was to measure high-altitude radiation levels during a solar proton storm, which was underway at the time of the flight. Usually such experiments are published in academic journals, but this time Ripley's Believe it or Not! took an interest. Why? Because the students pinned the radiation badges to a rubber chicken:

Camilla the Rubber Chicken, formerly of NASA, crewed the suborbital capsule and wore the radiation badges on a hand-knit spacesuit. She reached an altitude of 128,000 feet, withstanding temperatures as low as -63o C and air pressures as little as 1% sea level during the nearly three hour flight. More information about the flight may be found on page 235 of Dare to Look!, Ripley's latest hardbound volume available from RipleyBooks.com. (Note: The same picture was selected by Time magazine as one of the most surprising photos of 2012.)

The students, who call themselves Earth to Sky Calculus, are still doing space weather research. Recent and ongoing experiments include payloads to measure the effect of solar flares on the ozone layer and to assess the ability of microbes to withstand radiation storms. You can follow their activities on Facebook and Twitter.


Realtime Noctilucent Cloud Photo Gallery
[previous years: 2003, 2004, 2005, 2006, 2007, 2008, 2009, 2011]


Realtime Comet Photo Gallery

  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 September 4, 2013 there were potentially hazardous asteroids.
Recent & Upcoming Earth-asteroid encounters:
Asteroid
Date(UT)
Miss Distance
Size
2013 RO5
Sep 1
8.3 LD
47 m
2013 RG
Sep 3
0.6 LD
6 m
2013 RZ5
Sep 4
1.1 LD
10 m
2013 QE16
Sep 5
8.2 LD
22 m
2013 RQ5
Sep 6
4.8 LD
27 m
2000 DK79
Nov 10
49.1 LD
3.2 km
2011 JY1
Nov 13
8.2 LD
57 m
2001 AV43
Nov 18
2.9 LD
58 m
2010 CL19
Nov 25
37.6 LD
1.3 km
2013 NJ
Nov 26
2.5 LD
180 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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