Come to Tromsø and share Marianne's passion for rural photography: Chasethelighttours.co.uk invites you to experience "Heaven on Earth" with an aurora, fjord, fishing, whale watching, photography or sightseeing tour.
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SOLAR WIND SPARKS GEOMAGNETIC STORM: A high-speed (600 km/s) solar wind stream is buffeting Earth's magnetic field, sparking mild-to-moderate geomagnetic storms around the Arctic Circle. High-latitude sky watchers should remain alert for auroras on March 22-23. Aurora alerts: text, voice
SNAPSHOTS FROM THE ECLIPSE: What are the odds? On March 20th, just as the Moon was passing in front of the Sun, producing a deep solar eclipse over Europe, the International Space Station flew directly through the eclipse zone. Thierry Legault photographed the split-second transit from Fregenal de la Sierra, Spain:
"I had to drive a lot to find clear skies," says Legault, "but I managed to catch the ISS during the eclipse. The duration of the visible part of the transit was only 0.6s." See the Youtube video!
Meanwhile in the ionosphere.... The eclipse had a dramatic effect on the ionization of Earth's upper atmosphere. Normally, during the day, solar UV radiation breaks apart atoms and molecules, creating a layer of ionized gas hundreds of kilometers above Earth's surface. The Moon, however, blocked those UV rays. Subsequent changes to the ionization structure of atmosphere altered the propagation of radio waves in the eclipse zone. Take a look at these data from Rudolf Slošiar, who operates a VLF (very low frequency) radio monitoring station in Bojnice, Slovakia:
"During the solar eclipse, significant changes in the the D layer of the ionosphere affected the transmission of radio stations I record using my SID monitor, " says Slošiarl. Signals from Iceland were boosted, while radio stations in France and Puerto Rico dropped out.
For more anecdotes from the eclipse, monitor Spaceweather.com's realtime photo gallery:
Realtime Space Weather Photo Gallery
SPACE YEAST: On March 17th, during the strongest geomagnetic storm of the current solar cycle, Spaceweather.com and the students of Earth to Sky Calculus launched a Space Weather Buoy to measure the effect of the CME's impact on cosmic rays in the stratosphere. Along with radiation detectors and other sensors, the payload carried some hitchhikers--brewer's and baker's yeast:
During their ascent to the stratosphere, the yeast experienced temperatures as low as -60 C, air pressures only 1% of sea level, and cosmic ray dose rates 40 times Earth-normal.
What can you do with Space Yeast? Bake space bread, brew space beer, or whip up any recipe that calls for yeast. Also, teachers and homeschoolers can conduct some cool classroom experiments.
If you would like a packet of space yeast, you can have one by making a donation of $49.95 to Earth to Sky Calculus. Every flown packet of baker's yeast comes with a control packet that remained behind on Earth during the flight, so you can conduct a properly-controlled scientific experiment. All proceeds support student space weather research. Contact Dr. Tony Phillips to place your order.
Realtime Aurora Photo Gallery
Realtime Comet Photo Gallery
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. 22, 2015, the network reported 5 fireballs.
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]
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 22, 2015 there were 1561 potentially hazardous asteroids. 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.
| ||The official U.S. government space weather bureau |
| ||The first place to look for information about sundogs, pillars, rainbows and related phenomena. |
| ||Researchers call it a "Hubble for the sun." SDO is the most advanced solar observatory ever. |
| ||3D views of the sun from NASA's Solar and Terrestrial Relations Observatory |
| ||Realtime and archival images of the Sun from SOHO. |
| ||from the NOAA Space Environment Center |
| ||the underlying science of space weather |