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Solar wind
speed: 523.5 km/sec
density: 3.2 protons/cm3
explanation | more data
Updated: Today at 2351 UT
X-ray Solar Flares
6-hr max: C2
2117 UT Jun16
24-hr: C2
0406 UT Jun16
explanation | more data
Updated: Today at: 2300 UT
Daily Sun: 16 Jun 15
The magnetic field of sunspot AR2367 has simplified, and it no longer poses a threat for strong flares. Credit: SDO/HMI

Sunspot number: 107
What is the sunspot number?
Updated 16 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 16 Jun 2015


The Radio Sun
10.7 cm flux: 135 sfu
explanation | more data
Updated 16 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= 3
quiet
explanation | more data
Interplanetary Mag. Field
Btotal: 7.1 nT
Bz: 5.4 nT north
explanation | more data
Updated: Today at 2350 UT
Coronal Holes: 16 Jun 15

There are no large coronal holes on the Earthside of the sun. 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: 06-15-2015 16:55:02
SPACE WEATHER
NOAA Forecasts
Updated at: 2015 Jun 16 2200 UTC
FLARE
0-24 hr
24-48 hr
CLASS M
30 %
25 %
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: 2015 Jun 16 2200 UTC
Mid-latitudes
0-24 hr
24-48 hr
ACTIVE
20 %
10 %
MINOR
05 %
01 %
SEVERE
01 %
01 %
High latitudes
0-24 hr
24-48 hr
ACTIVE
15 %
20 %
MINOR
30 %
20 %
SEVERE
25 %
10 %
 
Tuesday, Jun. 16, 2015
What's up in space
 

Learn to photograph Northern Lights like a pro. Sign up for Peter Rosen's Aurora Photo Courses in Abisko National Park, winner of the TripAdvisor Certificate of Excellence Award 2015.

 
Lapland tours

QUIET SUN: Solar activity is low ... again. Continuing a trend that began in early May, the sun is mostly quiet with little chance of a significant flare on June 16th. NOAA forecasters put the odds of an X-class explosion at no more than 5%. Solar flare alerts: text, voice

ANTARCTIC AURORAS: With the approach of southern winter, night is falling across Antarctica. The night sky, however, is anything but dark. "On June 11th, the South Pole lit up with one of the best displays of auroras anyone has seen in years," reports Liz Widen, a science engineer wintering over at McMurdo Station. "The show lasted more an hour."

"They were extremely vivid and active," says Widen. "It was hard to keep taking photos, however, with a wind chill of -45 C."

More southern lights could be in the offing. NOAA forecasters estimate a 60% chance of polar geomagnetic storms on June 16th as Earth exits a high-speed solar wind stream. Aurora alerts: text, voice

Realtime Aurora Photo Gallery

POLLEN CORONAS: It begins with a sneeze. Pollen floating through the air tickles your nose, and your body responds by expelling the allergen. Gesundheit! When the paroxysm subsides, look up at the sky. The same pollen that makes you sneeze can also make beautiful coronas around the sun, like this one photographed on June 15th by Vesa Vauhkonen of Rautalampi, Finland :

"Pine is strongly flowering now in the middle Finland, and the coronas have been quite impressive over the past few days," says Vauhkonen. "But less impressive is the penetration of pollen everywhere--especially in the eyes and noses of people and animals. "

Atmospheric optics expert Les Cowley explains the phenonenon: "Coronas are produced when light waves scatter from the outsides of small particles. Tiny droplets of water in clouds make most coronas, but opaque equal-sized pollen grains do even better. They make small but very colorful multi-ringed coronas."

"Unlike water droplets, pollens are non-spherical--and this adds to their magic," he continues. "Many have air sacs to help carry them in the wind. These align the grains to give beautiful elliptical coronas with bright spots." This is why Vauhkonen's pollen corona looks the way it does.

As northern spring turns into summer, pollen coronas become increasingly common. Look for them the next time your nose feels a tickle.

MAMMATUS CLOUDS: On June 8th, during a gap between storms, a remarkable cloud formation appeared over Munster, Indiana. "I have never seen anything like it," says Cassandra Sotos, who photographed the apparition:

These are called "mammatus clouds." Named for their resemblance to a cow's underbelly, they sometimes appear at the end of severe thunderstorms when the thundercloud is breaking up. They are interesting in part because they're formed by sinking air. (Most clouds are formed by rising air.) Contrary to myth, however, they don't continue sinking downward to form tornadoes.

"The upside down convection was stunning," says Sotos.

Researchers have called mammatus clouds an "intriguing enigma," because their inner workings are not fully understood. The clouds are fairly common but often go unnoticed because potential observers have been chased indoors by the rain. If you are one of them, go back outside when the downpour stops; you could witness a beautiful mystery in the sky.

Realtime Space Weather Photo Gallery


Realtime NLC Photo Gallery


Realtime Aurora Photo Gallery


Realtime Sprite 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. 16, 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 16, 2015 there were potentially hazardous asteroids.
Recent & Upcoming Earth-asteroid encounters:
Asteroid
Date(UT)
Miss Distance
Size
2012 XB112
Jun 11
10.1 LD
2 m
2015 LF21
Jun 11
3.2 LD
28 m
1566 Icarus
Jun 16
21 LD
1.0 km
2015 MA
Jun 17
1.7 LD
22 m
2015 LK
Jun 17
7.8 LD
36 m
2015 LG
Jun 18
8.8 LD
54 m
2015 LQ21
Jun 18
12.9 LD
65 m
2015 LR21
Jun 20
2.5 LD
23 m
2015 KK57
Jun 23
8.3 LD
14 m
2005 VN5
Jul 7
12.6 LD
18 m
2015 HM10
Jul 7
1.1 LD
81 m
1994 AW1
Jul 15
25.3 LD
1.3 km
2011 UW158
Jul 19
6.4 LD
540 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
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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