Solar wind
speed: 718.0 km/sec
density: 3.7 protons/cm3
more data: ACE, DSCOVR
Updated: Today at 2030 UT
X-ray Solar Flares
6-hr max: B2
1801 UT Mar30
24-hr: B3
0012 UT Mar30
explanation | more data
Updated: Today at: 1959 UT
Daily Sun: 30 Mar 17
The magnetic field of sunspot AR2645 has decayed since yesterday, and it no longer poses a threat for M-class solar flares. Credit: SDO/HMI

Sunspot number: 53
What is the sunspot number?
Updated 30 Mar 2017

Spotless Days
Current Stretch: 0 days
2017 total: 27 days (30%)
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 30 Mar 2017


The Radio Sun
10.7 cm flux: 83 sfu
explanation | more data
Updated 30 Mar 2017

Current Auroral Oval:
Switch to: Europe, USA, New Zealand, Antarctica
Credit: NOAA/Ovation
Planetary K-index
Now: Kp= 4 unsettled
24-hr max: Kp= 5
storm
explanation | more data
Interplanetary Mag. Field
Btotal: 4.7 nT
Bz: -2.5 nT south
more data: ACE, DSCOVR
Updated: Today at 2029 UT
Coronal Holes: 30 Mar 17

Earth is inside a stream of solar wind flowing the indicated coronal hole. 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 Mar 29 2200 UTC
FLARE
0-24 hr
24-48 hr
CLASS M
10 %
10 %
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 Mar 29 2200 UTC
Mid-latitudes
0-24 hr
24-48 hr
ACTIVE
35 %
30 %
MINOR
20 %
20 %
SEVERE
05 %
05 %
High latitudes
0-24 hr
24-48 hr
ACTIVE
15 %
15 %
MINOR
20 %
15 %
SEVERE
25 %
15 %
 
Thursday, Mar. 30, 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. Email Marianne for bookings and availability.

 

SOLAR WIND STREAM SPARKS AURORAS: For the 4th day in a row, Earth is inside a stream of solar wind flowing from canyon-shaped hole in the sun's atmosphere. The gaseous material is pressing against Earth's magnetic field with speeds exceeding 600 km/s, sparking intermittent auroras around both poles. [photo gallery] [aurora alerts]

APRIL 1ST COMET FLYBY: Green comet 41P/Tuttle-Giacobini-Kresak is flying over Earth's North Pole this week where sky watchers can find it all night long not far from the bowl of the Big Dipper. At closest approach on April 1st it will be just 21 million km from Earth--an easy target for backyard telescopes and almost visible to the naked eye. Amateur astronomer Yasushi Aoshima sends this picture of the approaching comet from Fukushima, Japan:

"On March 22nd I caught 41P 'eating' M108, the Surfboard Galaxy," says Aoshima. "The comet's green atmosphere appeared to swallow the distant spiral galaxy as it exited Ursa Major."

Why green? Like many comets, 41P has a verdant hue because its atmosphere contains diatomic carbon (C2)--a substance that glows green in the near vacuum of space.

Comet 41P is not only approaching Earth, but also the sun. April 12th is the date of perihelion (minimum distance from the sun). This means we are catching the comet just as solar heating is furiously searing its icy core. The green atmosphere should be well puffed up by streamers of vaporizing gas. Optimistic estimates of the comet's brightness place it at magnitude +6, near the lower limit of naked-eye visibility.

This is not a Great Comet, but it should be a good one. The best time to observe is during the dark hours before sunrise when the green fuzzball is high in the northern sky. If you have a GOTO telescope, you can point it using an ephemeris from the Minor Planet Center. These sky maps show approximately where to look: March 31, April 1, 2.

Realtime Comet Photo Gallery

TOUCHING THE EDGE OF SPACE: On March 10, 2017, the students of Earth to Sky Calculus launched a space weather balloon from the frozen surface of Lake Tornetrask 250 km inside the Arctic Circle. A payload-full of reindeer pendants hitched a ride 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 telling the story of its journey 97,000 feet above the Lapland of Northern Sweden. They make great Birthday and Mother's Day gifts.

More far-out gifts may be found in the Earth to Sky store. All proceeds support STEM education and our atmospheric cosmic ray monitoring program. 

'DIAMOND DUST' ICE HALOS: Northern Spring has arrived--but it is still cold above the Arctic Circle in Alaska. On March 27th, ice crystals filled the air of the Coleville River Delta on the state's north coast. When sunlight hit the glittering atmosphere, this is what happened:

"An incredible network of ice halos surrounded the sun," says photographer James Helmericks. "It started around 12:30 pm with an ordinary 22 degree halo and some sundogs. As the sun sank lower into the afternoon sky, many other halos appeared, including a 360 degree parhelic circle, a bright circumzenithal arc, a 46 degree halo, and more." (Readers can go halo-hunting in this picture using a finder-chart from the South Pole.)

The variety and sharpness of this halo display is a sign that the sun was shining through "diamond dust"--jewel-like ice crystals of exceptional purity that form in cold polar environments. Indeed, a close look at Helmericks' picture shows specks of light in the air. Those are the glittering crystals of diamond dust which make these halos so beautiful.

Realtime Space Weather Photo Gallery

SUNSPOT SUNSET: Sunspots AR2644 and AR2645 have grown so large that some sky watchers are noticing them as blemishes on the setting sun. Yesterday evening in Girona, Spain, photographer Mohamad Soltanolkotabi went outside to look at the crescent Moon and, when he faced west, captured the sunspots instead:

"The sun was dimmed by low-hanging clouds, which made it possible to photograph these two large sunspots," he explains. "I was located on the grounds of the University of Girona."

These sunspots are large, but not very active.  Their magnetic fields are simple and stable, and thus pose little threat for explosive flares. Nevertheless they are photogenic. Warning: Even when the sun is dimmed by low-hanging clouds or smoke, it can still hurt your eyes. If you chose to photograph the low sun, as Soltanolkotabi did, use the camera's LCD screen for safe viewfinding. Never look into the eyepiece of an unfiltered camera or telescope when the sun is in the field of view.

Realtime Space Weather Photo Gallery


Realtime Aurora 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 Mar. 30, 2017, the network reported 7 fireballs.
(7 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 March 30, 2017 there were 1781 potentially hazardous asteroids.
Recent & Upcoming Earth-asteroid encounters:
Asteroid
Date(UT)
Miss Distance
Size
2017 FL63
Mar 26
4.2 LD
26 m
2017 FF3
Mar 27
5.7 LD
18 m
2017 FK3
Mar 27
9 LD
25 m
2017 FY101
Mar 29
1.3 LD
14 m
2017 FR91
Mar 29
3.5 LD
18 m
2017 FJ101
Mar 30
0.8 LD
10 m
2017 FX90
Apr 1
2.4 LD
26 m
2017 FV
Apr 2
9 LD
60 m
2017 EB3
Apr 4
13.8 LD
43 m
2017 FA102
Apr 4
14.2 LD
34 m
2017 FQ91
Apr 4
14.9 LD
36 m
2017 FM101
Apr 4
7 LD
21 m
2017 FX101
Apr 5
9.9 LD
39 m
2017 DC38
Apr 5
14.6 LD
54 m
2017 FU64
Apr 6
3.7 LD
74 m
2017 FN101
Apr 7
10.3 LD
47 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
  fun to read, but should be taken with a grain of salt! Forecasts looking ahead more than a few days are often wrong.
Aurora 30 min forecast
  from the NOAA Space Environment Center
Heliophysics
  the underlying science of space weather
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