AURORA WATCH: Earth is entering a stream of fast solar wind, and this could spark auroras tonight at high latitudes. NOAA forecasters estimate a 30% chance of polar geomagnetic storms. Aurora alerts: text, voice.
COLORFUL SPRITES OVER NEBRASKA: "August 12th was another successful night in our sprites campaign," reports Jason Ahrns of the University of Alaska Fairbanks. With a team of researchers from NCAR, he has been flying over the midwestern USA onboard a Gulfstream V in search of exotic forms of lightning. As they were photographing a thunderstorm over Nebraska, these six sprites appeared:
These remarkably beautiful discharges were red on top and purple on the bottom. "I really can't explain the color change," says Ahrns. "That's one of the things we hope to investigate with this campaign by capturing high speed spectra."
First documented in 1989 by scientists from the University of Minnesota who photographed strange flashes coming out of the tops of thunderstorms, sprites remain a mystery today. Neither their basic physics nor their effect on the surrounding atmosphere is well understood. "Do sprites have a large scale impact on the middle atmosphere?" asks Ahrns. "Sprites clearly represent some kind of transfer of energy, but is it on a scale that has a significant effect on the weather and climate? We can't answer that without studying them."
The ephemeral nature of sprites (they typically last no more than a few milliseconds) makes them tricky to study. Researchers on the NCAR Gulfstream capture sprites using Phantom cameras running at 10,000 frames per second. "One of the Phantoms has a diffraction grating in front of it to capture high speed spectra, which I don't think has ever been done before," notes Ahrns.
The prettiest pictures, though, come from Arhns' own camera, a dSLR that he mounts in the window of the airplane to capture "beauty shots." The image above is an example. More may be found in Ahrns' personal blog.
Solar wind
speed: 647.0 km/sec
density: 0.6 protons/cm3
explanation | more data
Updated: Today at 0346 UT
X-ray Solar Flares
6-hr max: C2 2216 UT Aug15
24-hr: C2 2216 UT Aug15
explanation | more data
Updated: Today at: 2359 UT
Daily Sun: 15 Aug 13
Sunspots AR1817 and AR1818 pose a threat for M-class solar flares. Credit: SDO/HMI
Sunspot number: 129
What is the sunspot number?
Updated 15 Aug 2013
Spotless Days
Current Stretch: 0 days
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%)
Since 2004: 821 days
Typical Solar Min: 486 days
Update 15 Aug 2013
The Radio Sun
10.7 cm flux: 125 sfu
explanation | more data
Updated 15 Aug 2013
Current Auroral Oval:
Switch to: Europe, USA, New Zealand, Antarctica
Credit: NOAA/POES
Planetary K-index
Now: Kp= 4 unsettled
24-hr max: Kp= 4 unsettled
explanation | more data
Interplanetary Mag. Field
Btotal: 6.0 nT
Bz: 0.2 nT north
explanation | more data
Updated: Today at 0347 UT
Coronal Holes: 15 Aug 13
Solar wind flowing from this coronal hole should reach Earth on August 17-18. Credit: SDO/AIA.