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Solar wind
speed: 474.8 km/sec
density: 5.2 protons/cm3
explanation | more data
Updated: Today at 2349 UT
X-ray Solar Flares
6-hr max: C1
2144 UT Jan07
24-hr: C4
1151 UT Jan07
explanation | more data
Updated: Today at: 2300 UT
Daily Sun: 07 Jan 15
Decaying sunspot AR2253 has a 'beta-gamma' magnetic field that poses a waning threat for M-class solar flares. Credit: SDO/HMI

Sunspot number: 102
What is the sunspot number?
Updated 07 Jan 2015

Spotless Days
Current Stretch: 0 days
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%)

Update 07 Jan 2015


The Radio Sun
10.7 cm flux: 142 sfu
explanation | more data
Updated 07 Jan 2015

Current Auroral Oval:
Switch to: Europe, USA, New Zealand, Antarctica
Credit: NOAA/Ovation
Planetary K-index
Now: Kp= 3 quiet
24-hr max: Kp= 7
strong
explanation | more data
Interplanetary Mag. Field
Btotal: 12.7 nT
Bz: 3.4 nT north
explanation | more data
Updated: Today at 2348 UT
Coronal Holes: 07 Jan 15
Earth is exiting a stream of solar wind flowing from this large southern coronal hole. Credit: SDO/AIA.
Noctilucent Clouds As of Nov. 22, 2014, the season for southern hemisphere noctilucent clouds is underway. The south polar "daisy" pictured below is a composite of near-realtime images from NASA's AIM spacecraft.
Switch view: Ross Ice Shelf, Antarctic Penninsula, East Antarctica, Polar
Updated at: 01-06-2015 23:55:10
SPACE WEATHER
NOAA Forecasts
Updated at: 2015 Jan 07 2200 UTC
FLARE
0-24 hr
24-48 hr
CLASS M
50 %
50 %
CLASS X
10 %
10 %
Geomagnetic Storms:
Probabilities for significant disturbances in Earth's magnetic field are given for three activity levels: active, minor storm, severe storm
Updated at: 2015 Jan 07 2200 UTC
Mid-latitudes
0-24 hr
24-48 hr
ACTIVE
40 %
30 %
MINOR
25 %
10 %
SEVERE
05 %
01 %
High latitudes
0-24 hr
24-48 hr
ACTIVE
10 %
15 %
MINOR
20 %
30 %
SEVERE
65 %
40 %
 
Wednesday, Jan. 7, 2015
What's up in space
 

Learn to photograph Northern Lights like a pro. Sign up for Peter Rosen's Aurora Photo Courses in Abisko National Park.

 
Lapland tours

UNEXPECTED GEOMAGNETIC STORM: A strong G3-class geomagnetic storm erupted during the early hours of Jan. 7th, sparking bright auroras around Earth's poles. What happened? The interplanetary magnetic field (IMF) near our planet tipped south, opening a crack in Earth's magnetosphere. Solar wind poured in to fuel the strongest magnetic storm since Sept. 2014. NOAA analysts believe the fluctuation in IMF is related to the arrival of a CME originally expected to miss Earth. Browse the aurora gallery for pictures of the event. Aurora alerts: text, voice

BRIGHTENING, GORGEOUS COMET: Comet Lovejoy (C/2014 Q2) continues to brighten, and it can now be seen with the naked eye even from light-polluted urban areas. Science journalist and longtime comet watcher Mariano Ribas reports from the Planetario de Buenos Aires: "Last night, I could see Comet Lovejoy with my unaided eyes in the sky of Buenos Aires. Barely, and only using averted vision. But I saw it!"

"Comparing the comet to nearby background stars, I estimate the comet's visual magnitude to be about 4.2," he continues. "The comet was very bright with my 10x50 binoculars. Also, I could see a hint of its tail. The comet's atmosphere (or 'coma') looks clearly gray/green, and it appears more condensed than one week ago."

What is merely pleasing to the unaided eye transforms into something gorgeous in the focus of a mid-sized telescope. Gerald Rhemann took this picture using a remotely-controlled 12-inch 'scope in Farm Tivoli, Namibia:

The comet's blue tail is so long, only 1/3rd of it fits in the space provided above. The whole thing stretches more than 7 million km from end to end.

On Jan. 7th, Comet Lovejoy was at its closest to Earth: 0.47 astronomical units (70 million km) away. Although the comet will be moving away from us for the rest of the month, it will continue to grow in brightness because it is still moving closer to the sun.

"Surely," says Ribas, "the best is still to come!"

This week, observers can find Comet Lovejoy passing by the constellation Orion en route to Taurus. For accurate pointing of telescopes, an ephemeris from the Minor Planet Center is available.

Realtime Comet Photo Gallery

RADS ON A PLANE, CONTINUED: Many people think you have to go all the way to the Arctic Circle to experience space weather. Not so. All you have to do is step inside an airplane. Every day more than 8 million people fly somewhere on Earth. All of them are exposed to cosmic rays, a form of high-energy space radiation. To illustrate the point, on Jan. 5th, Dr. Tony Phillips of spaceweather.com carried a pair of ionizing radiation detectors onboard a US Airways flight from Reno to Phoenix. At cruising altitude (38,700 ft) he measured dose rates 42 times higher than at ground level:

At this rate, a passenger flying for 5 hours could be exposed to about as much radiation as a dental X-ray--not dangerous, but not negligible either.

The radiation comes from space. Cosmic rays are subatomic particles accelerated to nearly light speed by supernovas, active galactic nuclei, and solar flares. Earth is peppered with this kind of radiation, every day, from all directions. Cosmic rays penetrate our planet's atmosphere, producing a spray of secondary particles that air travelers routinely (and mostly unknowingly) absorb as they fly.

Cosmic rays are a genuine form of space weather. They fluctuate in response to solar storms--both up and down. For example, solar flares can accelerate energetic particles toward Earth, adding to the flux of cosmic rays. CMEs, on the other hand, sweep aside cosmic rays, causing radiation counts to dip. When you step on a plane, you're never quite sure what you're going to get.

Case in point: Phillips took the same flight from Reno to Phoenix on Nov. 11, 2014. He measured 40% more radiation then vs. now. The difference is not fully understood.

Here are the data from the Jan. 5th flight:

The two curves, orange and blue, trace data from two identical yet independent radiation detectors. Differences between the two curves are an indication of the measurement uncertainty. Using helium balloons, spaceweather.com and the students of Earth to Sky Calculus have flown these detectors to the stratosphere dozens of times to monitor the response of Earth's upper atmosphere to solar storms. They are sensitive to ionizing radiation such as X-rays and gamma-rays in the energy range 10 keV to 20 MeV.

It is important to note that these sensors sample only a fraction of the total radiation. In particular, they are not sensitive to neutrons, a key form of biologically effective radiation at aviation altitudes. Adding neutrons to the count could more than double the measured dose. Solar flare alerts: text, voice

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 Jan. 7, 2015, 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 January 7, 2015 there were potentially hazardous asteroids.
Recent & Upcoming Earth-asteroid encounters:
Asteroid
Date(UT)
Miss Distance
Size
2014 YE42
Jan 3
4.3 LD
88 m
2014 YP34
Jan 4
8.8 LD
26 m
2007 EJ
Jan 12
68.9 LD
1.1 km
1991 VE
Jan 17
40.6 LD
1.0 km
2004 BL86
Jan 26
3.1 LD
650 m
2008 CQ
Jan 31
4.8 LD
36 m
2000 EE14
Feb 27
72.5 LD
1.6 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.
  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
Space Weather Alerts
   
  more links...
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