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HAPPY SOLSTICE: Today is the June solstice--the longest day of the year in the northern hemisphere, and the shortest day in the south. The exact moment of the solstice is 11:54 am EDT, when the sun reaches its highest declination on the celestial sphere (+23.5o). Northern summer and southern winter are underway. Wherever you live, happy solstice!
THE SUN IS SO BLANK, IT LOOKS LIKE A BILLIARD BALL: The sun is blank--really blank. No sunspots have appeared for the past 33+ days, giving the sun the appearance of a giant orange billiard ball. This is a sign that Solar Minimum is underway. Earlier this year, a panel of experts from NOAA and NASA predicted that the solar cycle would reach its nadir sometime between July 2019 and Sept 2020. The current stretch of spotless suns is consistent with their forecast.
Above: The sun on June 21, 2019. Credit: NASA's Solar Dynamics Observatory
What happens when sunspots vanish? For one thing, solar flares stop happening. No big explosions means no shortwave radio blackouts and fewer geomagnetic storms. Also, the sun dims. Sunspots are sources of extreme ultraviolet radiation (EUV). Without sunspots, EUV levels decrease, causing Earth's upper atmosphere to cool and contract. Satellites and space junk stay in orbit longer as aerodynamic drag subsides.
During this phase of the solar cycle, the solar wind slows and the sun's magnetic field weakens--shields down! This allows extra cosmic rays from deep space to penetrate the solar system. Indeed, recent high altitude balloon flights show increased radiation in Earth's atmosphere. Extra cosmic rays can trigger lightning, alter the electro-chemistry of the upper atmosphere, and boost dose rates on commercial airplane flights.
Solar Minimum won't last forever. Forecasters expect sunspot numbers to increase after 2019-2020, climaxing in a new Solar Maximum around 2023-2026. Meanwhile, stay tuned for more blank suns.
Realtime Space Weather Photo Gallery
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GIANT 'PALM TREE' SPRITE: On Wednesday night in Texas, a flurry of red sprites exploded from the top of a powerful thunderstorm. One of the the red forms was so tall and bright, people saw it 200 miles away in Oklahoma. "My boys and I saw it with our unaided eyes," reports Paul Smith, who photographed the event from the shores of Lake Thunderbird, OK. This may be the first time that a sprite's reflection has been captured in water:
Naked-eye sightings of sprites are rare, mainly because they are so fleeting. But this one left an impression. "My eleven-year-old son Thomas described it as a 'huge orange-y-brown flash of lines high in the sky,'" says Smith. "My seven-year-old James just exclaimed 'what the heck was that?'"
At first glance, Smith's capture resembles a Gigantic Jet--that is, a type of "sprite on steroids." But lightning expert Oscar van der Velde of the Universitat Politècnica de Catalunya thinks it may be something else:
"In early days of sprite research, they were called 'palm trees' by researchers from the University of Alaska," van der Velde explains. "It is, basically, a bushy group of red sprites on top, with a secondary purple discharge hanging below. These types of events are quite rare. You need a big, active mesoscale convective system to produce them."
Palm tree sprites are a topic of cutting edge research. "We haven't even been able to confirm that they indeed originate from the thundercloud," says van der Velde.
"Last night was so much fun," adds Smith. "In addition to the sprites, my son Thomas photographed Jupiter and our Moon with the Nikon coolpix 80x zoom camera. We also saw a nice bolide exploding over the storms. The kid's reactions were priceless."
Realtime Sprite Photo Gallery
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APOLLO 11 PROOF SILVER DOLLAR: To celebrate the 50th anniversary of the Apollo 11 Moon landing, the United States Mint has created a commemorative 2019 Proof Silver Dollar. We decided to celebrate even more by flying the coins to the edge of space. On June 13th, the students of Earth to Sky Calculus launched this 99.9% silver dollar 99,022 feet above Earth's surface:
You can have it for $179.95. The students are selling the coins to support their cosmic ray ballooning program. The silver dollar is curved and reproduces the helmet of astronaut Buzz Aldrin. Reflected in Buzz's visor are Neil Armstrong, the United States flag, and the lunar lander. The opposite side of the coin shows Neil's first footprint on the Moon. Each of these coins comes with a greeting card showing the item in flight and a certificate of authenticity.
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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 Jun. 21, 2019, the network reported 3 fireballs.
(3 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]
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 June 21, 2019 there were 1983 potentially hazardous asteroids.
|
Recent & Upcoming Earth-asteroid encounters: Asteroid | Date(UT) | Miss Distance | Velocity (km/s) | Diameter (m) |
2019 LU | 2019-Jun-16 | 4.2 LD | 8 | 33 |
2019 LR | 2019-Jun-16 | 18.3 LD | 15 | 34 |
2019 LU4 | 2019-Jun-18 | 2 LD | 8.1 | 18 |
2019 LA5 | 2019-Jun-18 | 18.3 LD | 7.7 | 29 |
2019 LC1 | 2019-Jun-19 | 19.2 LD | 9.9 | 26 |
2019 LB2 | 2019-Jun-20 | 6.5 LD | 3.4 | 15 |
2019 LM1 | 2019-Jun-23 | 9.8 LD | 8.7 | 25 |
2019 LC5 | 2019-Jun-23 | 13.6 LD | 11.1 | 42 |
441987 | 2019-Jun-24 | 7.7 LD | 12.6 | 178 |
2008 KV2 | 2019-Jun-27 | 17.8 LD | 11.4 | 195 |
2016 NN15 | 2019-Jun-28 | 9.6 LD | 8.4 | 16 |
2019 LR4 | 2019-Jun-29 | 11.3 LD | 8.3 | 31 |
2019 LV1 | 2019-Jun-29 | 5.2 LD | 6.2 | 27 |
2015 XC352 | 2019-Jul-01 | 11.9 LD | 4.1 | 26 |
2016 OF | 2019-Jul-07 | 12.8 LD | 8.5 | 85 |
2016 NO56 | 2019-Jul-07 | 3.4 LD | 12.2 | 26 |
2019 KD3 | 2019-Jul-12 | 15.5 LD | 8 | 89 |
2016 NJ33 | 2019-Jul-12 | 15 LD | 4.5 | 32 |
2015 HM10 | 2019-Jul-24 | 12.2 LD | 9.5 | 68 |
2010 PK9 | 2019-Jul-26 | 8.2 LD | 16.5 | 155 |
2006 QQ23 | 2019-Aug-10 | 19.4 LD | 4.7 | 339 |
454094 | 2019-Aug-12 | 17 LD | 8.2 | 148 |
2018 PN22 | 2019-Aug-17 | 17.1 LD | 2.3 | 11 |
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 Reneger-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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