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Solar wind
speed: 577.8 km/sec
density: 3.0 protons/cm3
explanation | more data
Updated: Today at 2347 UT
X-ray Solar Flares
6-hr max: C2
2217 UT Jun21
24-hr: M2
0316 UT Jun21
explanation | more data
Updated: Today at: 2300 UT
Daily Sun: 21 Jun 13
Sunspots AR1775 and 1777 pose a threat for M-class solar flares. Credit: SDO/HMI
Sunspot number: 128
What is the sunspot number?
Updated 21 Jun 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
21 Jun 2013

The Radio Sun
10.7 cm flux: 128 sfu
explanation | more data
Updated 21 Jun 2013

Current Auroral Oval:
Switch to: Europe, USA, New Zealand, Antarctica
Credit: NOAA/POES
Planetary K-index
Now: Kp= 3 quiet
24-hr max: Kp= 4
unsettled
explanation | more data
Interplanetary Mag. Field
Btotal: 7.6 nT
Bz: 6 nT south
explanation | more data
Updated: Today at 2347 UT
Coronal Holes: 21 Jun 13
Solar wind flowing from this coronal hole could brush against Earth's magnetic field on June 22-24. Credit: SDO/AIA.

NEW: 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: 06-21-2013 15:45:01
SPACE WEATHER
NOAA Forecasts
Updated at: 2013 Jun 21 2200 UTC
FLARE
0-24 hr
24-48 hr
CLASS M
30 %
30 %
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: 2013 Jun 21 2200 UTC
Mid-latitudes
0-24 hr
24-48 hr
ACTIVE
30 %
20 %
MINOR
10 %
05 %
SEVERE
01 %
01 %
High latitudes
0-24 hr
24-48 hr
ACTIVE
15 %
15 %
MINOR
25 %
25 %
SEVERE
40 %
25 %
 
Friday, Jun. 21, 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

SUMMER SOLSTICE: Today is the first day of northern summer. At 1:04 a.m. EDT on June 21st, the sun reached its highest point on the celestial sphere (declination = +23.5o) marking the start of summer in the northern hemisphere, and winter in the south. Happy solstice!

SOLSTICE SOLAR FLARE: This morning, June 21st at 03:16 UT, the sun itself marked the solstice with an M2-class solar flare from sunspot AR1777. NASA's Solar Dynamics Observatory photographed the extreme ultraviolet flash and a plume of material flying out of the blast site:

As sunspots go, AR1777 is neither large nor apparently menacing, yet it has been crackling with flares for days. Before it rotated over the sun's eastern limb on June 20th, it unleashed a series of farside flares and CMEs. Today's explosion was not Earth directed, but future explosions could be as the sun's rotation continues to turn AR1777 toward our planet. NOAA forecasters estimate a 30% chance of M-flares and a 5% chance of X-flares during the next 24 hours. Solar flare alerts: text, voice.

Realtime Space Weather Photo Gallery

CHINESE SPACE STATION CROSSES THE SUN: Earlier this week in the sunny skies above the south of France, China's experimental Tiangong-1 space station flew directly in front of the sun. Using a filtered 6-inch telescope, astrophotographer Thierry Legault recorded the station's silhouette alongside big sunspot AR1775:

"I recorded two transits--one on June 16 and another on June 17th," says Legault. "They show the Tiangong-1 with 3 taikonauts inside."

Most readers are familiar with the 450-ton International Space Station. Fewer, perhaps, know about China's 8.5-ton Tiangong-1 (Heavenly Palace-1). It was launched in Sept. 2011 to establish a foothold in Earth orbit for China's fledgling space program. Tiangong-1 was briefly boarded by taikonauts (Chinese astronauts) in June 2012, and a second group is onboard now. Three Taikonauts arrived on June 13, 2013, on a 15-day mission to practice rendevous and docking maneuvers and to gain experience living in space. Their expedition is attracting little attention in Western press, but it is being widely followed in China. Earlier this week, more than 60 million students and teachers at 80,000 Chinese schools watched a live lecture by the crew of the Tiangong-1.

According to some reports, the Tiangong-1 will be de-orbited in late 2013 to make way for more advanced experimental stations, Tiangong-2 and Tiangong-3 in the years ahead. Ultimately, China hopes to place an Mir-class station in orbit by 2020.

See the Tiangong-1 before it goes! Spaceweather's Simple Flybys app turns your smartphone into a field-tested space station tracker. It works for both the ISS and the Tiangong-1.

SIX MONTHS IN A BEER CAN: The summer solstice has arrived, and in the Netherlands that means it's time to open up beer cans around the Philippus Lansbergen Observatory in Middleberg. It's not what you think! There's no beer inside, only photo paper. Every year, astronomers at the observatory help members of the public make beer-can solargraphs to record the motion of the sun across the sky. Yesterday, after six months in the field, the solargraphs were opened, and this is what they revealed:

"This shows the movement of the Sun with 1 single shot of 6 months exposure time," explains Jan Koeman of the Philippus Lansbergen Observatory. "We deployed the beer-can solargraphs in December and opened them yesterday."

The lowest arcs were traced by the winter sun of Dec. 2012. The highest arc was made by the sun yesterday on the eve of the 2013 summer solstice. Occasional gaps are caused by clouds.

"It seems the sun has been shining a lot the last 6 months," notes Koeman. "This does not match with the general view of cloudy weather in the Netherlands!"

6-month Solargraph How-to Guides: #1, #2, #3


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


Realtime Aurora Photo Gallery


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 June 21, 2013 there were potentially hazardous asteroids.
Recent & Upcoming Earth-asteroid encounters:
Asteroid
Date(UT)
Miss Distance
Size
2006 RO36
Jun 18
70.9 LD
1.2 km
2001 PJ9
Jul 17
29.2 LD
1.1 km
2006 BL8
Jul 26
9.3 LD
48 m
2003 DZ15
Jul 29
7.6 LD
153 m
2005 WK4
Aug 9
8.1 LD
420 m
1999 CF9
Aug 23
24.7 LD
1.1 km
2002 JR9
Aug 31
63.5 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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