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DOGS CAN SENSE MAGNETIC FIELDS: Add dogs to the list of lifeforms that can use magnetic fields to navigate. New research summarized in today's issue of Science magazine shows that at least some hunting dogs take shortcuts along N-S magnetic field lines--a strategy that helps them navigate unfamiliar terrain. This means dogs may be sensitive to the disturbing effects of space weather. FULL STORY.
THE SYNCHRONIC BANDS OF COMET NEOWISE: Comet NEOWISE (C/2020 F3) is doing something usually reserved for Great Comets. It has sprouted synchronic bands. Also known as "striae," these bands divide the comet's dust tail into linear regions of greater and lesser density. Chris Cook of Cape Cod, MA, captured the phenomenon on the evening of July 15th:

"Comet NEOWISE is now in its full glory for northern hemisphere observers," says Cook. "This image is a stack of thirty 25s exposures at ISO1600. It clearly shows the formation of synchronic bands within the dust tail."
Synchronic bands have been seen in comet tails for centuries, yet only recently have astronomers begun to understand what they are. The turning point came in 2007 when European and NASA spacecraft observed the formation of striae in Comet McNaught (C/2006 P1). Apparently, the process starts when a chunk of comet detaches itself from the nucleus. Boulder-sized chunks fragment into smaller and smaller pieces, a cascading process shaped into dusty striations by solar radiation pressure.

A few years ago, then-PhD student Ollie Price of University College London’s Mullard Space Science Laboratory was looking at old pictures of McNaught's striae and noticed some "weird goings-on." The bands were occasionally being bent and disrupted by some invisible force. "So I set out to investigate what might have happened to create this weird effect," he recalls.
Price and colleagues ultimately found the answer. The disruptions occured when Comet McNaught crossed the heliospheric current sheet (HCS)--a vast wavy structure in interplanetary space separating regions of opposite magnetic polarity. "It appears the dust may be electrically charged, and gets rearranged as it crosses the HCS boundary," says Karl Battams of the Naval Research Lab, a co-author of their 2018 paper.
Could the same thing happen to Comet NEOWISE? It's possible. Photographers monitoring NEOWISE are encouraged to keep a sharp eye on the striae. Changes may be in the offing. Sky maps: July 15, 16, 17.
Realtime Comet NEOWISE Photo Gallery
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A SURPRISE VISIT FROM STEVE: Even STEVE wants to see Comet NEOWISE. On July 14th, the geomagnetic phenomenon appeared over Canada, streaking the sky with mauve ribbons of light. Harlan Thomas of Calgary, Alberta, reports: "I was out shooting the comet when I noticed a mauve-looking cloud. Wow!" I thought. "STEVE has come to visit NEOWISE. How cool is that?"

STEVE is a recent discovery. It looks like an aurora, but it is not. The purple glow is caused by hot (3000°C) ribbons of gas flowing through Earth's magnetosphere at speeds exceeding 6 km/s (13,000 mph). It appears during some geomagnetic storms, often alongside a type of green aurora known as the "picket fence," also shown in Thomas's photo.
Statistics suggest that STEVE appears most often in spring and fall. What summoned STEVE in mid-summer? It may have been a CME that grazed Earth's magnetic field on July 13th. As our planet passed through the CME's magnetized wake on July 14th, hot currents and plasma waves rippled through Earth's magnetosphere. STEVE was the result.
Christy Turner saw it too:

"I was shooting the comet outside Calgary when STEVE started to form," she says. "It was a huge purple pillar--a total delight!"
Many observers across western Canada witnessed the display. During a normal summer, STEVE might have been overlooked, but with Comet NEOWISE drawing photographers outdoors, his visit was well documented. "Summertime STEVE" might be more common than previously thought.
Realtime STEVE Photo Gallery
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A FAR-OUT GIFT FOR TREKKIES: Mr. Sulu has been to the stratosphere. The helmsman of the starship Enterprise (NCC-1701) hitched a ride onboard an Earth to Sky Calculus cosmic ray balloon on May 21st. Here he is, floating 107,611 feet above the Sierra Nevada mountains of central California:

You can have him for $119.95. The students of Earth to Sky are selling Sulu bobbleheads to support their cosmic ray ballooning program. Each one comes with a greeting card showing Sulu in flight and telling the story of his journey to the edge of space and back again. This makes a great anniversary or birthday gift for fans of Star Trek.
Far Out Gifts: Earth to Sky Store
All sales support hands-on STEM education
Realtime Noctilucent Cloud Photo Gallery
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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 July 17, 2020, the network reported 12 fireballs.
(10 sporadics, 1 alpha Capricornid, 1 Northern June Aquilid)
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 July 17, 2020 there were 2037 potentially hazardous asteroids.
 |
Recent & Upcoming Earth-asteroid encounters: Asteroid | Date(UT) | Miss Distance | Velocity (km/s) | Diameter (m) |
2020 ML | 2020-Jul-12 | 11.4 LD | 4.4 | 23 |
2020 KJ7 | 2020-Jul-13 | 11.8 LD | 3.4 | 33 |
2009 OS5 | 2020-Jul-13 | 17.6 LD | 2.6 | 45 |
2020 MQ2 | 2020-Jul-14 | 17.1 LD | 8.3 | 44 |
2020 NM | 2020-Jul-16 | 10.6 LD | 5.7 | 20 |
2020 MX | 2020-Jul-17 | 15 LD | 5.3 | 52 |
2016 DY30 | 2020-Jul-19 | 9 LD | 15.1 | 3 |
2020 ME3 | 2020-Jul-19 | 14.8 LD | 4.6 | 24 |
2002 BF25 | 2020-Jul-21 | 9.4 LD | 6.8 | 129 |
2020 NO | 2020-Jul-22 | 2.1 LD | 7.7 | 15 |
2020 ND | 2020-Jul-24 | 14.5 LD | 13.6 | 167 |
2020 NN | 2020-Jul-25 | 16.3 LD | 10.1 | 47 |
2020 NZ | 2020-Jul-28 | 8.3 LD | 7.8 | 29 |
2020 MX3 | 2020-Jul-29 | 9.4 LD | 8.5 | 68 |
2018 PY7 | 2020-Jul-31 | 8.9 LD | 9.5 | 16 |
2007 RF1 | 2020-Jul-31 | 10.7 LD | 5 | 21 |
2018 BD | 2020-Aug-03 | 7.6 LD | 9.4 | 3 |
2009 PQ1 | 2020-Aug-05 | 10.8 LD | 13.5 | 112 |
2020 FA1 | 2020-Aug-23 | 18.4 LD | 1.9 | 20 |
2016 AH164 | 2020-Aug-26 | 15.7 LD | 5.6 | 4 |
2011 ES4 | 2020-Sep-01 | 0.3 LD | 8.2 | 30 |
465824 | 2020-Sep-06 | 19.4 LD | 14 | 162 |
2012 RM15 | 2020-Sep-12 | 14.9 LD | 9.8 | 45 |
2017 US | 2020-Sep-13 | 17.3 LD | 5.9 | 21 |
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 |
SOMETHING NEW! We have developed a new predictive model of aviation radiation. It's called E-RAD--short for Empirical RADiation model. We are constantly flying radiation sensors onboard airplanes over the US and and around the world, so far collecting more than 22,000 gps-tagged radiation measurements. Using this unique dataset, we can predict the dosage on any flight over the USA with an error no worse than 15%.
E-RAD lets us do something new: Every day we monitor approximately 1400 flights criss-crossing the 10 busiest routes in the continental USA. Typically, this includes more than 80,000 passengers per day. E-RAD calculates the radiation exposure for every single flight.
The Hot Flights Table is a daily summary of these calculations. It shows the 5 charter flights with the highest dose rates; the 5 commercial flights with the highest dose rates; 5 commercial flights with near-average dose rates; and the 5 commercial flights with the lowest dose rates. Passengers typically experience dose rates that are 20 to 70 times higher than natural radiation at sea level.
To measure radiation on airplanes, we use the same sensors we fly to the stratosphere onboard Earth to Sky Calculus cosmic ray balloons: neutron bubble chambers and X-ray/gamma-ray Geiger tubes sensitive to energies between 10 keV and 20 MeV. These energies span the range of medical X-ray machines and airport security scanners.
Column definitions: (1) The flight number; (2) The maximum dose rate during the flight, expressed in units of natural radiation at sea level; (3) The maximum altitude of the plane in feet above sea level; (4) Departure city; (5) Arrival city; (6) Duration of the flight.
SPACE WEATHER BALLOON DATA: 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 18% since 2015:

The data points in the graph above correspond to the peak of the Regener-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.
En route to the stratosphere, our sensors also pass through aviation altitudes:
In this plot, 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.
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.
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 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 |
| fun to read, but should be taken with a grain of salt! Forecasts looking ahead more than a few days are often wrong. |
| from the NOAA Space Environment Center |
| the underlying science of space weather |
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