Solar wind
speed: 356.8 km/sec
density: 5.2 protons/cm3
explanation | more data
Updated: Today at 1003 UT
X-ray Solar Flares
6-hr max: B3
0313 UT Jul26
24-hr: B3
0313 UT Jul26
explanation | more data
Updated: Today at: 0900 UT
Daily Sun: 26 Jul 16
The sun is blank again--no sunspots. Credit: SDO/HMI

Sunspot number: 0
What is the sunspot number?
Updated 26 Jul 2016

Spotless Days
Current Stretch: 1 days
2016 total: 17 days (8%)
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 26 Jul 2016


The Radio Sun
10.7 cm flux: 74 sfu
explanation | more data
Updated 26 Jul 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= 4
unsettled
explanation | more data
Interplanetary Mag. Field
Btotal: 3.9 nT
Bz: 1.8 nT south
explanation | more data
Updated: Today at 1003 UT
Coronal Holes: 26 Jul 16

Solar wind flowing from the indicated coronal hole could reach Earth on July 29. 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: 07-24-2016 15:55:02
SPACE WEATHER
NOAA Forecasts
Updated at: 2016 Jul 25 2200 UTC
FLARE
0-24 hr
24-48 hr
CLASS M
10 %
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 Jul 25 2200 UTC
Mid-latitudes
0-24 hr
24-48 hr
ACTIVE
30 %
35 %
MINOR
15 %
15 %
SEVERE
01 %
01 %
High latitudes
0-24 hr
24-48 hr
ACTIVE
15 %
15 %
MINOR
30 %
30 %
SEVERE
45 %
45 %
 
Tuesday, Jul. 26, 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!

 

CHANCE OF STORMS TODAY: NOAA forecasters say there is a 45% chance of G1-class geomagnetic storms on July 26th when a high speed stream of solar wind is expected to hit Earth's magnetic field. The outskirts of a CME might deliver a glancing blow at about the same time. High-latitude sky watchers should be alert for auroras. Aurora alerts: text or voice

POLAR STRATOSPHERIC CLOUDS: The stratosphere is a relatively clear layer of Earth's atmosphere, almost always cloud-free. Almost always. Yesterday, researchers at Argentina's San Martín Base spotted a bank of fantastically colored clouds floating in the stratosphere above the Antarctic Peninsula:

"There were the biggest stratospheric clouds we've seen so far this year," says photographer "Marcelo," who is working at the Base this winter. "It was a colorful spectacle to begin the day."

These are called "Polar Stratospheric Clouds" (PSCs). They form in the lower stratosphere when temperatures drop to around minus 85º C. This explains why they are rare; even at the poles, such low temperatures are hard to achieve. High-altitude sunlight shining through tiny (~10µm) ice particles in PSCs produce bright iridescent colors by diffraction and interference. Once thought to be mere curiosities, some PSCs are now known to be associated with the destruction of ozone.

Apparitions of these clouds often persist for days. Stay tuned for more sightings from the frozen continent.

NEW ZEALAND LIGHT SHOW: "It is rare to see the Aurora Australis from Wellington, which is on the North Island of New Zealand," says photographer Jonathan Usher. "However, last night I noticed a glow far to the south that twinkled and moved." He took this picture from coastal Seatoun:

There was no geomagnetic storm when the lights appeared. The display was caused by "southward Bz." In other words, magnetic fields in the space around Earth pried open a crack in our planet's magnetosphere. Solar wind poured in to spark the Southern Lights.

Similar displays were recorded in Queenstown and Dunedin. It was a good night to be in New Zealand.

Realtime Aurora Photo Gallery

WHERE NO DUCK HAS GONE BEFORE: Yes, that really is a Vulcan rubber duck! The students of Earth to Sky Calculus flew the pointy-eared water bird to the stratosphere on July 19, 2016, as part of their ongoing program to monitor cosmic rays in the stratosphere. Here he is at the apex of the flight, 109,580 ft:

"Mr Squawk" hitchhiked on a helium balloon payload that carried an array of X-ray/gamma-ray sensors. By launching these sensors 3 or 4 times a month, the students have shown that cosmic rays are intensifying--a trend that affects mountain climbers, air travelers, high-altitude drones and astronauts on the International Space Station.

This research is crowd funded. Would you like to support it? Buy a duck! Edge of Space Vulcan Ducks are now available in the Earth to Sky Store.

Realtime Space Weather Photo Gallery


Realtime Noctilucent Cloud 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 Jul. 25, 2016, the network reported 15 fireballs.
(13 sporadics, 1 Southern delta Aquariid, 1 alpha Capricornid)

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 July 26, 2016 there were potentially hazardous asteroids.
Recent & Upcoming Earth-asteroid encounters:
Asteroid
Date(UT)
Miss Distance
Size
2016 NS
Jul 20
8.7 LD
34 m
2002 KL6
Jul 22
26.6 LD
1.4 km
2016 NJ39
Jul 22
11.5 LD
39 m
2011 BX18
Jul 25
52.7 LD
1.1 km
2016 NW15
Jul 26
13.7 LD
35 m
2016 NE39
Jul 26
6.7 LD
88 m
2016 NX22
Aug 2
12.9 LD
87 m
2005 OH3
Aug 3
5.8 LD
28 m
2000 DP107
Aug 12
66.5 LD
1.0 km
2004 BO41
Sep 7
38.9 LD
1.1 km
2015 KE
Sep 10
14.9 LD
23 m
2009 UG
Sep 30
7.3 LD
101 m
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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