Solar wind
speed: 365.8 km/sec
density: 6.5 protons/cm3
more data: ACE, DSCOVR
Updated: Today at 0641 UT
X-ray Solar Flares
6-hr max: B1
0103 UT Feb27
24-hr: B1
0103 UT Feb27
explanation | more data
Updated: Today at: 0600 UT
Daily Sun: 26 Feb 17
The magnetic field of sunspot AR2638 is decaying, and it no longer harbors energy for M-class solar flares. Credit: SDO/HMI

Sunspot number: 35
What is the sunspot number?
Updated 26 Feb 2017

Spotless Days
Current Stretch: 0 days
2017 total: 11 days (21%)
2016 total: 32 days (9%)
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 Feb 2017


The Radio Sun
10.7 cm flux: 80 sfu
explanation | more data
Updated 26 Feb 2017

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: 5.2 nT
Bz: -2.1 nT north
more data: ACE, DSCOVR
Updated: Today at 0642 UT
Coronal Holes: 26 Feb 17

Solar wind flowing from the indicated coronal hole should reach Earth on Feb. 28-March 1. Credit: NASA/SDO.
Noctilucent Clouds The southern season for noctilucent clouds began on Nov. 17, 2016. Come back to this spot every day to see the "daily daisy" from NASA's AIM spacecraft, which is monitoring the dance of electric-blue around the Antarctic Circle.
Switch view: Ross Ice Shelf, Antarctic Peninsula, East Antarctica, Polar
Updated at: 02-24-2017 17:55:02
SPACE WEATHER
NOAA Forecasts
Updated at: 2017 Feb 26 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: 2017 Feb 26 2200 UTC
Mid-latitudes
0-24 hr
24-48 hr
ACTIVE
10 %
25 %
MINOR
01 %
10 %
SEVERE
01 %
01 %
High latitudes
0-24 hr
24-48 hr
ACTIVE
15 %
15 %
MINOR
20 %
30 %
SEVERE
10 %
40 %
 
Monday, Feb. 27, 2017
What's up in space
       
 

Directly under the Arctic Circle! Marianne's Arctic Xpress in Tromsø offers fjord, whale and wildlife tours by day, aurora tours by night. Book Now for out of this world day and night adventures.

 

CHANCE OF STORMS: NOAA forecasters estimate a 40% chance of polar geomagnetic storms late on Feb. 28th when the leading edge of a solar wind stream hits Earth's magnetic field.  Arctic sky watchers should be alert for auroras as the month of March begins. Free: Aurora alerts.

SOUTHERN HEMISPHERE SOLAR ECLIPSE: This morning in Santiago, Chile, the Moon passed in front of the sun, off-center, transforming the solar disk into a crescent.  At first it seemed that no one would see it. "The clouds had no mercy," reports Patricio Leon, "but eventually a small clearing revealed the eclipse." He took this picture at 14:03 UT when the sun was 49% covered:

The eclipse was also visible in Brazil. Edson Luiz Duffeck Karlson of São José dos Pinhais, Paraná, saw it a bit differently, though. Instead of watching the event unfold overhead, he set up a simple pinhole projector and used it to cast an image of the crescent sun onto a painting in his home.

"The clouds, in this case, are brushstrokes of oil," he says. "I painted them myself."

This eclipse was special. In a narrow corridor cutting across the southern reaches of Chile and Argentina, and stretching across the Atlantic to Angola, the Democratic Republic of the Congo, and Zambia in Africa, the Moon crossed the sun dead-center. Yet it only covered 99% of the solar disk. This allowed a fiery ring of solar plasma to circumscribe the mountainous limb of the Moon--like this.

Did anyone see the "ring of fire"? Stay tuned for sightings.

Realtime Solar Eclipse Photo Gallery

ARCTIC SPACE REINDEER: The students of Earth to Sky Calculus are about to travel inside the Arctic Circle (Abisko, Sweden) for their first polar space weather balloon launch. To raise money for the trip, on Feb. 23rd they flew a payload-full of Arctic reindeer pendants to the edge of space:

You can have one for $129.95. Each glittering pendant comes with a greeting card showing the jewelry in flight and certifying that it has been to the stratosphere and back again. These pendants make great Birthday and Mother's Day gifts.

Bonus: Would you like your pendant to be flown over the Arctic as well? Make a note to that effect in the COMMENTS box at checkout, and we will take your pendent to Sweden for a second trip to the stratosphere.

Realtime Space Weather Photo Gallery

AURORA ROCKET LAUNCH: On Feb. 22nd, shortly after midnight, bright green auroras erupted over Alaska's Poker Flat Research Range. Researchers from Dartmouth College promptly launched a rocket into the glowing maelstrom. Photographer Marketa Murray of Fairbanks captured the event in a perfectly-timed self-portrait:

"We tuned into the Poker Flat Research Range radio for a heads-up that the rocket was about to launch," explains Murray. "The picture shows both stages of the Black Brant IX sounding rocket burning for the ionosphere."

The goal of the mission, named ISINGLASS (Ionospheric Structuring: In Situ and Groundbased Low Altitude Studies) is to decipher the mysterious shapes of the aurora borealis. Some auroras look like flames, others like swirls, ripples or curtains. The rocket was designed to scatter an array of sensors into the auroral zone, mapping the particles and fields underlying these forms.

"Auroras are the last step of a chain of processes connecting the solar wind to the atmosphere," says Dr. Kristina Lynch of Dartmouth, the mission's principal investigator. "We are seeking to understand what structure in these visible signatures can tell us about the electrodynamics of processes higher up."

"It was a beautiful launch with an extensive set of collaborative ground based data, and will make a great study," she says.

Ultimately, the results could allow researchers to look up at the sky and, based on little more than the shapes they see, predict conditions at the edge of space. Was the mission a success? Stay tuned for updates from the launch team.

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 Feb. 26, 2017, the network reported 5 fireballs.
(5 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 27, 2017 there were 1775 potentially hazardous asteroids.
Recent & Upcoming Earth-asteroid encounters:
Asteroid
Date(UT)
Miss Distance
Size
2017 DR34
Feb 25
0.6 LD
7 m
2017 DX35
Feb 25
13.3 LD
17 m
2017 DV36
Feb 27
1 LD
12 m
2017 DS34
Feb 27
7.1 LD
31 m
2017 BM123
Feb 27
12.4 LD
79 m
2017 DJ16
Feb 28
4.1 LD
30 m
2012 DR32
Mar 2
4.7 LD
52 m
2017 DV35
Mar 8
9.6 LD
15 m
2017 DR35
Mar 9
11.8 LD
26 m
2017 DA36
Mar 10
4 LD
46 m
1998 SL36
Mar 16
8.3 LD
390 m
2015 TC25
Mar 26
7.6 LD
6 m
2003 BD44
Apr 18
21.7 LD
1.9 km
2014 JO25
Apr 19
4.6 LD
1.0 km
1999 CU3
Apr 19
63.7 LD
1.9 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

Readers, thank you for your patience while we continue to develop this new section of Spaceweather.com. We've been working to streamline our data reduction, allowing us to post results from balloon flights much more rapidly, and we have developed a new data product, shown here:

This plot displays radiation measurements not only in the stratosphere, but also at aviation altitudes. Dose rates are expessed as multiples of sea level. For instance, we see that boarding a plane that flies at 25,000 feet exposes passengers to dose rates ~10x higher than sea level. At 40,000 feet, the multiplier is closer to 50x. These measurements are made by our usual cosmic ray payload as it passes through aviation altitudes en route to the stratosphere over California.

What is this all about? 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. Furthermore, there are studies ( #1, #2, #3, #4) linking cosmic rays with cardiac arrhythmias and sudden cardiac death in the general population. Our latest measurements show that cosmic rays are intensifying, with an increase of more than 12% since 2015:


Why are cosmic rays intensifying? The main reason is the sun. Solar storm clouds such as coronal mass ejections (CMEs) sweep aside cosmic rays when they pass by Earth. During Solar Maximum, CMEs are abundant and cosmic rays are held at bay. Now, however, the solar cycle is swinging toward Solar Minimum, allowing cosmic rays to return. Another reason could be the weakening of Earth's magnetic field, which helps protect us from deep-space radiation.

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.

The data points in the graph above correspond to the peak of the Reneger-Pfotzer maximum, which lies about 67,000 feet above central California. When cosmic rays crash into Earth's atmosphere, they produce a spray of secondary particles that is most intense at the entrance to the stratosphere. Physicists Eric Reneger and Georg Pfotzer discovered the maximum using balloons in the 1930s and it is what we are measuring today.

  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
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NOAA 27-Day Space Weather Forecasts
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Aurora 30 min forecast
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