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SpaceWeather.com -- News and information about meteor showers, solar flares, auroras, and near-Earth asteroids
 
Solar wind
speed: 421.2 km/sec
density: 1.2 protons/cm3
explanation | more data
Updated: Today at 2352 UT
X-ray Solar Flares
6-hr max: B1
1719 UT Jun20
24-hr: B9
0300 UT Jun20
explanation | more data
Updated: Today at: 2300 UT
Daily Sun: 20 Jun 16
None of these sunspots poses a threat for strong flares. Solar activity remains low. Credit: SDO/HMI

Sunspot number: 48
What is the sunspot number?
Updated 20 Jun 2016

Spotless Days
Current Stretch: 0 days
2016 total: 4 days (1%)
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 20 Jun 2016


The Radio Sun
10.7 cm flux: 84 sfu
explanation | more data
Updated 20 Jun 2016

Current Auroral Oval:
Switch to: Europe, USA, New Zealand, Antarctica
Credit: NOAA/Ovation
Planetary K-index
Now: Kp= 1 quiet
24-hr max: Kp= 1
quiet
explanation | more data
Interplanetary Mag. Field
Btotal: 4.3 nT
Bz: 0.5 nT north
explanation | more data
Updated: Today at 2352 UT
Coronal Holes: 20 Jun 16
Solar wind flowing from the indicated coronal hole should reach Earth on ~June 23rd. Credit: SDO/AIA.
Noctilucent Clouds Images from NASA's AIM spacecraft are once again appearing on Spaceweather.com. Check back daily for space-based sightings of noctilucent clouds.
Switch view: Europe, USA, Asia, Polar
Updated at: 06-20-2016 22:55:02
SPACE WEATHER
NOAA Forecasts
Updated at: 2016 Jun 20 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 Jun 20 2200 UTC
Mid-latitudes
0-24 hr
24-48 hr
ACTIVE
10 %
10 %
MINOR
01 %
01 %
SEVERE
01 %
01 %
High latitudes
0-24 hr
24-48 hr
ACTIVE
15 %
15 %
MINOR
15 %
10 %
SEVERE
10 %
10 %
 
Monday, Jun. 20, 2016
What's up in space
       
 

It's waiting for you: The most successful Aurora Photo Tour on Earth! 100% success rate 4 years in a row and winner of the TripAdvisor Certificate of Excellence Award. Join LapplandMedia's aurora tours in Abisko, Swedish Lapland!

 

SOLSTICE FULL MOON: It's a coincidence: Tonight's full Moon falls on the solstice, June 20th, the longest day of the year in the northern hemisphere. That means the next 24 hours will be the brightest of the year--a long day of sunlight followed by a short but glowing night of full moonlight. Got photos? Submit them here.

ELECTRIC BLUE SUNSETS: Northern summer has begun. That means it's time for picnics, hot dogs, dips in the pool, and ... oh yes ... electric blue sunsets. Summer is the season for noctilucent clouds (NLCs), and reports of their telltale blue ripples are pouring in from Canada, Alaska and many countries in Europe. Marek Nikodem sends this picture from Żnin Lake, near Szubin, Poland:

"Last night, I watched a fantastic display of NLCs," says Nikodem. "Before midnight the clouds were low on the horizon. After midnight a great complex sprung up, as wide as 100 degrees. It was absolutely beautiful."

Noctilucent clouds are a true space weather phenomenon. They assemble at the edge of space, ~83 km above Earth's surface, when diaphanous wisps of water vapor wrap themselves around meteoroids to form tiny ice crystals. Long ago, they were confined to Arctic latitudes. As a result of climate change, they are now brightening and spreading, with sightings in recent years as far south as Colorado and Utah.

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 Noctilucent Cloud Photo Gallery

POLAR STRATOSPHERIC CLOUDS: Bright colors have appeared in the skies over Antarctica--but it's not the aurora australis. Instead, pastel stratospheric clouds are floating over the frozen continent. B. Sudarsan Patro photographed the apparition on June 17th from the Bharati Indian Base Station:

"The clouds were absolutely stunning," says Patro. "It was really surprising and a new experience for all of us."

Atmospheric optics expert Les Cowley says "Bharati Station at 70 degrees south is just the place to get these wonderful filmy Polar Stratospheric Clouds (PSCs).  Floating 9 to 16 miles high, they need stunningly-cold temperatures below -85 Celsius to form."

Sunlight shining through tiny ice particles ~10µm across produce the characteristic bright iridescent colors of PSCs by diffraction and interference. "More familiar tropospheric clouds can also shine with iridescent colours," says Cowley, "but never as vividly or memorably as PSCs.  This page helps distinguish the two."

Realtime Space Weather Photo Gallery

Realtime Sprite Photo Gallery


Realtime Aurora 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 Jun. 20, 2016, the network reported 2 fireballs.
(2 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 20, 2016 there were 1707 potentially hazardous asteroids.
Recent & Upcoming Earth-asteroid encounters:
Asteroid
Date(UT)
Miss Distance
Size
2016 LK49
Jun 16
3.2 LD
28 m
2016 LY8
Jun 18
13.4 LD
102 m
2016 MA
Jun 19
2.6 LD
15 m
2009 CV
Jun 20
12.4 LD
60 m
2010 NY65
Jun 24
10.7 LD
215 m
2002 KL6
Jul 22
26.6 LD
1.4 km
2011 BX18
Jul 25
52.7 LD
1.1 km
2005 OH3
Aug 3
5.8 LD
28 m
2000 DP107
Aug 12
66.5 LD
1.0 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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