Marianne's Heaven On Earth Aurora Chaser Tours Chasethelighttours.co.uk invites you to join them in their quest to find and photograph the Aurora Borealis. Experience the winter wonderland in the Tromsø Area.
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LEONID METEOR SHOWER: Today and tomorrow, Earth will pass through a stream of dusty debris from Comet 55P/Tempel-Tuttle, source of the annual Leonid meteor shower. This is not a storm year for the Leonids. Forecasters expect a mild display of no more than 15 or 20 meteors per hour best seen during the dark hours before sunrise. Got clouds? You can listen to Leonid radar echoes on Space Weather Radio.
GLANCING-BLOW CME EXPECTED THIS WEEK: A magnetic filament on the sun erupted during the late hours of Nov. 15th, hurling inky-black fragments of itself into space. Shortly thereafter, a CME was observed racing away from the sun:
Storm track models from NOAA suggest that the CME will deliver a glancing blow to Earth's magnetic field on Nov. 18th or 19th. There is a 70% chance of polar geomagnetic storms when the CME arrives.
Actually, the arrival of the CME could be the second strike. A co-rotating interaction region (CIR) is also expected to hit Earth's magnetic field on Nov. 18th. CIRs are transition zones between fast- and slow-moving solar wind streams. Solar wind plasma piles up in these regions, producing density gradients and shock waves that do a good job of sparking auroras.
The double impact, CIR followed by CME, could produce a G1 or G2-class geomagnetic storm and bright auroras around the Arctic Circle. Observers in northern-tier US states from Maine to Washington should be alert for colorful lights in the midnight sky. Aurora alerts: text or voice
Realtime Aurora Photo Gallery
TRANSCONTINENTAL SPACE WEATHER BALLOON LAUNCH: The students of Earth to Sky Calculus, Spaceweather.com, and physicists from the University of New Hampshire are preparing their second transcontinental launch of space weather balloons. On Saturday morning, Nov. 21st, two identical balloons equipped with radiation detectors will lift off from opposite sides of the USA. The goal of the experiment is to explore how cosmic rays affect Earth's atmosphere on continental scales.
Flying simultaneously, the balloons will ascend all the way to the stratosphere, sampling X-rays and gamma-rays at altitudes of interest to aviation, space tourism, and climate science. The last time the teams did this, on July 20, 2015, they discovered an interesting difference between California and New Hampshire: Radiation levels above New Hampshire were more than 25% higher, a surprisingly wide gap considering their relatively small difference in latitude. The Nov. 21st flight will confirm and expand upon these findings.
Here are what the data looked like from the previous transcontinental flight:
The graph shows how radiation levels over California changed as the balloon ascended toward the stratosphere, then parachuted back to Earth. A California vs. New Hampshire plot highlights the extra radiation over the Granite State. Is it still there? Stay tuned!
Realtime Space Weather Photo Gallery
Realtime Taurid Photo Gallery
Realtime Meteor 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 Nov. 17, 2015, the network reported 38 fireballs.
(23 sporadics, 9 Northern Taurids, 3 Leonids, 2 November I Draconids, 1 omicron Eridanid)
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 November 17, 2015 there were 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.
| ||Cosmic Rays in the Atmosphere |
These measurements are based on regular space weather balloon flights: learn more.
|Situation Report -- Oct. 30, 2015 ||Stratospheric Radiation (+37o N) |
|Cosmic ray levels are elevated (+6.1% above the Space Age median). The trend is flat. Cosmic ray levels have increased +0% in the past month. |
|Sept. 06: 4.14 uSv/hr (414 uRad/hr) |
|Sept. 12: 4.09 uSv/hr (409 uRad/hr) |
|Sept. 23: 4.12 uSv/hr (412 uRad/hr) |
|Sept. 25: 4.16 uSv/hr (416 uRad/hr) |
|Sept. 27: 4.13 uSv/hr (413 uRad/hr) |
|Oct. 11: 4.02 uSv/hr (402 uRad/hr) |
|Oct. 22: 4.11 uSv/hr (411 uRad/hr) |
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. Our measurements show that someone flying back and forth across the continental USA, just once, can absorb as much ionizing radiation as 2 to 5 dental X-rays. Here is the data from our latest flight, Oct. 22nd:
Radiation levels peak at the entrance to the stratosphere in a broad region called the "Pfotzer Maximum." This peak is named after physicist George Pfotzer who discovered it using balloons and Geiger tubes in the 1930s. Radiation levels there are more than 80x sea level.
Note that the bottom of the Pfotzer Maximim is near 55,000 ft. This means that some high-flying aircraft are not far from the zone of maximum radiation. Indeed, according to the Oct 22th measurements, a plane flying at 45,000 feet is exposed to 2.79 uSv/hr. At that rate, a passenger would absorb about one dental X-ray's worth of radiation in about 5 hours.
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 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 |