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SpaceWeather.com -- News and information about meteor showers, solar flares, auroras, and near-Earth asteroids
 
Solar wind
speed: 574.0 km/sec
density: 0.1 protons/cm3
explanation | more data
Updated: Today at 2350 UT
X-ray Solar Flares
6-hr max: C1
2113 UT Feb18
24-hr: C7
0158 UT Feb18
explanation | more data
Updated: Today at: 2300 UT
Daily Sun: 18 Feb 16
Solar activity is waning as sunspot AR2497 disappears over the sun's western limb. Credit: SDO/HMI

Sunspot number: 60
What is the sunspot number?
Updated 18 Feb 2016

Spotless Days
Current Stretch: 0 days
2016 total: 0 days (0%)
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 18 Feb 2016


The Radio Sun
10.7 cm flux: 100 sfu
explanation | more data
Updated 18 Feb 2016

Current Auroral Oval:
Switch to: Europe, USA, New Zealand, Antarctica
Credit: NOAA/Ovation
Planetary K-index
Now: Kp= 5 storm
24-hr max: Kp= 5
storm
explanation | more data
Interplanetary Mag. Field
Btotal: 3.7 nT
Bz: 0.3 nT south
explanation | more data
Updated: Today at 2352 UT
Coronal Holes: 18 Feb 16

Earth is inside a stream of solar wind flowing from this southern coronal hole. Credit: SDO/AIA.
Noctilucent Clouds The southern season for noctilucent clouds began on Dec. 13, 2015. It is expected to end in late February 2016.
Switch view: Ross Ice Shelf, Antarctic Peninsula, East Antarctica, Polar
Updated at: 02-12-2016 16:55:02
SPACE WEATHER
NOAA Forecasts
Updated at: 2016 Feb 18 2200 UTC
FLARE
0-24 hr
24-48 hr
CLASS M
01 %
01 %
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: 2016 Feb 18 2200 UTC
Mid-latitudes
0-24 hr
24-48 hr
ACTIVE
40 %
25 %
MINOR
20 %
05 %
SEVERE
01 %
01 %
High latitudes
0-24 hr
24-48 hr
ACTIVE
10 %
15 %
MINOR
25 %
30 %
SEVERE
50 %
30 %
 
Thursday, Feb. 18, 2016
What's up in space
 

Marianne's Heaven On Earth Aurora Chaser Tours Chasethelighttours.co.uk invites you to join them in their quest to find and photograph the Aurora Borealis. Experience the winter wonderland in the Tromsø Area.

 
Chase the Light Tours

SUBSIDING CHANCE OF FLARES: Solar activity is returning to very low levels as active sunspot AR2497 rotates over the sun's western limb. NOAA forecasters are lowering the odds of an M-class solar flare from 30% today to only 1% on Feb. 19th. Stay tuned for quiet. Solar flare alerts: text or voice

SOLAR WIND SPARKS AURORAS: For the second day in a row, a high-speed stream of solar wind is buffeting Earth's magnetic field. Last night, Feb. 17th, Northern Lights spilled across the Canadian border into Minnesota, where Travis Novitsky took this picture:

"While last night's activity was not exactly mind blowing, it was very beautiful with a soft green arc along the northern horizon," says Novitsky. "I snowshoed to a location in the Superior National Forest in order to frame the trees against the sky with auroras behind them. It turned out to be a great spot to photograph the lights. I can't wait to go back during a more powerful storm!"

More auroras are in the offing. NOAA forecasters estimate a 50% chance of G1-class geomagnetic storms on Feb. 18th as the solar wind continues to blow. Aurora alerts: text or voice

Realtime Aurora Photo Gallery

RED RAINBOW: Rainbows are normally red, yellow, green and blue--in short, all the colors of a rainbow. But the towering rainbow Jan Koeman photographed from Kloetinge, the Netherlands, on Feb. 18th was simply red:

"I have never seen such a rainbow before," says Koeman. "It appeared just a few minutes after a red sunrise."

What made the rainbow red? Simply, it was the red sunrise. All of the other colors of the rainbow had been scattered away by air molecules and dust particles in front of the low-hanging sun.

Koeman notes another puzzle: Rainbows require raindrops, "but it was not raining at all!" he says. Atmospheric optics expert Les Cowley thinks the raindrops were there, in the distance. "There could be rain on the horizon or virga. Virga is cloud precipitation that does not reach the ground," says Cowley.

Realtime Spaceweather 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 Feb. 18, 2016, the network reported 12 fireballs.
(12 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 February 18, 2016 there were potentially hazardous asteroids.
Recent & Upcoming Earth-asteroid encounters:
Asteroid
Date(UT)
Miss Distance
Size
2016 BE
Feb 1
5.9 LD
86 m
2016 BA15
Feb 1
2.9 LD
19 m
2015 XA379
Feb 7
8.1 LD
38 m
2016 BQ
Feb 7
11.1 LD
21 m
2014 QD364
Feb 7
14 LD
16 m
2013 VA10
Feb 8
12.5 LD
165 m
2016 BQ15
Feb 8
8.5 LD
44 m
2014 EK24
Feb 14
13.8 LD
94 m
2010 LJ14
Feb 16
68.5 LD
1.2 km
1999 YK5
Feb 19
51.7 LD
2.0 km
2010 WD1
Feb 22
12.3 LD
22 m
1991 CS
Feb 23
65.5 LD
1.4 km
2011 EH17
Mar 1
11.1 LD
52 m
2013 TX68
Mar 5
0.044 LD
30 m
2001 PL9
Mar 9
77.6 LD
1.2 km
2010 FX9
Mar 19
6.9 LD
62 m
252P/LINEAR
Mar 21
13.9 LD
0 m
2016 BA14
Mar 22
9.2 LD
540 m
1993 VA
Mar 23
59.6 LD
1.6 km
2001 XD
Mar 28
64.5 LD
1.0 km
2016 BC14
Mar 29
9.9 LD
280 m
2002 AJ29
Apr 6
55.2 LD
1.5 km
2002 EB3
Apr 8
55.6 LD
1.2 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.
  Cosmic Rays in the Atmosphere
Situation Report -- Oct. 30, 2015 Stratospheric Radiation (+37o N)
Cosmic ray levels are elevated (+6.1% above the Space Age median). The trend is flat. Cosmic ray levels have increased +0% in the past month.
Sept. 06: 4.14 uSv/hr (414 uRad/hr)
Sept. 12: 4.09 uSv/hr (409 uRad/hr)
Sept. 23: 4.12 uSv/hr (412 uRad/hr)
Sept. 25: 4.16 uSv/hr (416 uRad/hr)
Sept. 27: 4.13 uSv/hr (413 uRad/hr)
Oct. 11: 4.02 uSv/hr (402 uRad/hr)
Oct. 22: 4.11 uSv/hr (411 uRad/hr)
These measurements are based on regular space weather balloon flights: learn more.

Approximately once a week, Spaceweather.com and the students of Earth to Sky Calculus fly "space weather balloons" to the stratosphere over California. These balloons are equipped with radiation sensors that detect cosmic rays, a surprisingly "down to Earth" form of space weather. Cosmic rays can seed clouds, trigger lightning, and penetrate commercial airplanes. Our measurements show that someone flying back and forth across the continental USA, just once, can absorb as much ionizing radiation as 2 to 5 dental X-rays. For example, here is the data from a flight on Oct. 22, 2015:

Radiation levels peak at the entrance to the stratosphere in a broad region called the "Pfotzer Maximum." This peak is named after physicist George Pfotzer who discovered it using balloons and Geiger tubes in the 1930s. Radiation levels there are more than 80x sea level.

Note that the bottom of the Pfotzer Maximim is near 55,000 ft. This means that some high-flying aircraft are not far from the zone of maximum radiation. Indeed, according to the Oct 22th measurements, a plane flying at 45,000 feet is exposed to 2.79 uSv/hr. At that rate, a passenger would absorb about one dental X-ray's worth of radiation in about 5 hours.

The radiation sensors onboard our helium balloons detect X-rays and gamma-rays in the energy range 10 keV to 20 MeV. These energies span the range of medical X-ray machines and airport security scanners.

  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
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