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Solar wind
speed: 400.5 km/sec
density: 11.8 protons/cm3
explanation | more data
Updated: Today at 2351 UT
X-ray Solar Flares
6-hr max: C1
1800 UT Jun07
24-hr: C1
1037 UT Jun07
explanation | more data
Updated: Today at: 2300 UT
Daily Sun: 07 Jun 15
Sunspot AR2361 is crackling with C-class solar flares. Credit: SDO/HMI

Sunspot number: 129
What is the sunspot number?
Updated 07 Jun 2015

Spotless Days
Current Stretch: 0 days
2015 total: 0 days (0%)

2014 total: 1 day (<1%)
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%)

Updated 07 Jun 2015


The Radio Sun
10.7 cm flux: 133 sfu
explanation | more data
Updated 07 Jun 2015

Current Auroral Oval:
Switch to: Europe, USA, New Zealand, Antarctica
Credit: NOAA/Ovation
Planetary K-index
Now: Kp= 2 quiet
24-hr max: Kp= 2
quiet
explanation | more data
Interplanetary Mag. Field
Btotal: 16.7 nT
Bz: 9.4 nT south
explanation | more data
Updated: Today at 2350 UT
Coronal Holes: 07 Jun 15

Solar wind flowing from this minor coronal hole could reach Earth on June 9-10. Credit: SDO/AIA.
Noctilucent Clouds The northern season for NLCs is underway. NASA's AIM spacecraft spotted the first noctilucent clouds over the Arctic Circle on May 19th.
Switch view: Europe, USA, Asia, Polar
Updated at: 06-07-2015 21:55:03
SPACE WEATHER
NOAA Forecasts
Updated at: 2015 Jun 07 2200 UTC
FLARE
0-24 hr
24-48 hr
CLASS M
20 %
20 %
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: 2015 Jun 07 2200 UTC
Mid-latitudes
0-24 hr
24-48 hr
ACTIVE
35 %
35 %
MINOR
15 %
20 %
SEVERE
01 %
01 %
High latitudes
0-24 hr
24-48 hr
ACTIVE
15 %
10 %
MINOR
30 %
25 %
SEVERE
45 %
50 %
 
Sunday, Jun. 7, 2015
What's up in space
 

Come to Tromsø and share Marianne's passion for rural photography: Chasethelighttours.co.uk invites you to experience "Heaven on Earth" with an aurora, fjord, fishing, whale watching, photography or sightseeing tour.

 
Chase the Light Tours

CO-ROTATING INTERACTION REGION: NOAA forecasters estimate a 45% chance of polar geomagnetic storms on June 8th when a co-rotating interaction region (CIR) is expected to hit Earth's magnetic field. CIRs are transition zones between fast- and slow-moving solar wind streams. Solar wind plasma piles up in these regions, producing density gradients and shock waves that do a good job of sparking auroras. Aurora alerts: text, voice

WEEKEND NOCTILUCENT CLOUDS: All weekend long, ripples of electric-blue have criss-crossed the evening skies of northern Europe. Saturday night in Estonia, for instance, looked like this:

"Using my Pentax K-30 digital camera, I created a panoramic image of the display," says photographer Jüri Voit. "It was widespread and beautiful."

Summer is the season for noctilucent clouds (NLCs). They form at the edge of space, 82 km above Earth's surface, when diaphanous wisps of water vapor wrap themselves around meteoroids to form tiny ice crystals. The crystals are so tiny that they scatter blue light--hence the clouds' electric-blue color. Why summer? Ironically, that is the only time the upper atmosphere is cold enough for these icy clouds to form.

Noctilucent clouds first appeared in the 19th century after the eruption of super-volcano Krakatoa. At the time, people thought NLCs were caused by the eruption, but long after Krakatoa's ash settled, the clouds remained. In recent years, NLCs have intensified and spread with summer sightings as far south as Utah and Colorado. This could be a sign of increasing greenhouse gases in Earth's atmosphere.

Observing tips: Look west 30 to 60 minutes after sunset when the sun has dipped 6o to 16o below the horizon. If you see luminous blue-white tendrils spreading across the sky, you may have spotted a noctilucent cloud.

Realtime NLC Photo Gallery

NOT A RAINBOW: At this time of year, a colorful arc often appears in the noontime sky. It looks like a rainbow, but it's not. "We saw one during Saturday's June Bug parade in Baldwin, Wisconsin," reports Craig Braymen. "This picture barely does it justice."

Braymen witnessed a circumhorizon arc--a rainbow-colored band of light caused by the sun shining through plate-shaped ice crystals in cirrus clouds. Summer is the season for circumhorizontal arcs because they appear only when the sun is high in the sky--more than 58o above the horizon. The arc's enormous size and pure spectral colors make it one of the most beautiful of all ice halos.

At medium latitudes, like much of the USA, the arc is not rare.Typically, it can be seen several times each summer. In contrast, further north in much of Europe the circumhorizon arc is a rarity and impossible to see north of Copenhagen. See the charts in Les Cowley's web page 'How rare?' for the visibility at your location.

Realtime Space Weather Photo Gallery


Realtime Sprite Photo Gallery


Realtime Meteor Photo Gallery


Realtime Aurora 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 Jun. 7, 2015, the network reported 14 fireballs.
(14 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 June 7, 2015 there were potentially hazardous asteroids.
Recent & Upcoming Earth-asteroid encounters:
Asteroid
Date(UT)
Miss Distance
Size
2015 KM57
Jun 3
6.6 LD
35 m
2005 XL80
Jun 4
38.1 LD
1.0 km
2015 KA122
Jun 6
3.3 LD
95 m
2015 KU121
Jun 7
7.5 LD
115 m
2012 XB112
Jun 11
10.1 LD
2 m
2015 KK57
Jun 23
8.3 LD
13 m
2005 VN5
Jul 7
12.6 LD
18 m
2015 HM10
Jul 7
1.1 LD
73 m
1994 AW1
Jul 15
25.3 LD
1.4 km
2011 UW158
Jul 19
6.4 LD
565 m
2013 BQ18
Jul 20
7.9 LD
38 m
1999 JD6
Jul 25
18.8 LD
1.6 km
2005 NZ6
Aug 6
76.5 LD
1.4 km
2005 JF21
Aug 16
20.1 LD
1.6 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
Columbia Northern High School
  Web-based high school science course with free enrollment
  more links...
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