Space Weather Update: 01/27/2017
By Spaceweather.com, 01/27/2017
THE SOLAR WIND HAS ARRIVED: Arriving a day earlier than expected, a stream of solar wind hit Earth’s magnetic field on Jan. 27th. This is causing intermittent G1-class geomagnetic storms and Northern Lights around the Arctic Circle. Rauno Pakarinen sends this photo from Pieksämäki in eastern Finland:
The solar wind responsible for this display is flowing from a hole in the sun’s atmosphere. It is expected to influence our planet for the next 2 to 3 days, with a 40% chance of continued geomagnetic storms on Jan. 27th and Jan. 28th. Arctic sky watchers should remain alert for auroras this weekend. Free: Aurora Alerts
ALTERNATE AURORAS: On Jan. 24th, photographer Dave Bell of Pinedale, Wyoming, witnessed a display of colorful lights in the sky. They looked liked auroras–but they were not.
They’re light pillars, caused by ice crystals in the air which intercept urban lights and spread them into colorful columns. Sometimes called “false auroras,” no solar activity is required for the phenomenon. The only ingredients are ice and light pollution.
“We had a really terrific snowstorm in Pinedale for 36 hours,” says Bell. “As the storm cleared and temperatures plummeted, fine crystals of ice filled the air and we were treated to a spectacular display of pillars. A friend recently commented that light pillars are like our version of the aurora borealis.”
FAR-OUT VALENTINE’S GIFT: To raise money for their cosmic ray ballooning program, the students of Earth to Sky Calculus have flown a payload-full of Valentine’s pendants to the edge of space–and you can have one for $89.95. Buy one this week and we will include a space rose free of charge.
Each glittering pendant comes with a greeting card showing the jewelry in flight and certifying that it has been to the stratosphere and back again.
More far-out Valentine’s gifts may be found in the Earth to Sky store. All proceeds support cosmic ray balloon flights and STEM education.
TWO BIG HOLES IN THE SUN’S ATMOSPHERE: NASA’s Solar Dynamics Observatory is now tracking two large holes in the sun’s atmosphere. One (on the right) is almost directly facing Earth, and the other (left) is still turning toward us:
These are “coronal holes” (CHs)–places in the sun’s atmosphere where the sun’s magnetic field opens up and allows solar wind to escape. Coronal holes turn the sun into a kind of gassy lighthouse. They strobe Earth with streams of solar wind every 27 days, the rotation period of the sun.
Earth will encounter solar wind streams from both of these holes. The first is due to arrive on Jan. 27th. (Update: it’s here!) The second, larger stream should reach our planet on or about Feb 1st. Arctic sky watchers, mark your calendars; auroras are in the offing.
All Sky Fireball Network
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 Jan. 26, 2017, the network reported 13 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]
Near Earth Asteroids
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 January 27, 2017 there were 1765 potentially hazardous asteroids.
Recent & Upcoming Earth-asteroid encounters:Asteroid
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
Readers, thank you for your patience while we continue to develop this new section of Spaceweather.com. We’ve been working to streamline our data reduction, allowing us to post results from balloon flights much more rapidly, and we have developed a new data product, shown here:
This plot displays radiation measurements not only in the stratosphere, but also at aviation altitudes. 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. These measurements are made by our usual cosmic ray payload as it passes through aviation altitudes en route to the stratosphere over California.
What is this all about? 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 12% since 2015:
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 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 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.
speed: 583.6 km/sec
density: 4.9 protons/cm3
more data: ACE, DSCOVR
Updated: Today at 1506 UTX-ray Solar Flares
6-hr max: B5 1045 UT Jan27
24-hr: B5 1045 UT Jan27
explanation | more data
Updated: Today at: 1500 UTDaily Sun: 27 Jan 17Not one of these sunspots pose a threat for strong solar flares. Credit: SDO/HMI
Sunspot number: 31
What is the sunspot number?
Updated 27 Jan 2017
Current Stretch: 0 days
2017 total: 10 days (40%)
2016 total: 32 days (9%)
2015 total: 0 days (0%)
2014 total: 1 day (<1%)
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%)
Updated 27 Jan 2017
Current Auroral Oval:
Switch to: Europe, USA, New Zealand, Antarctica
Credit: NOAA/OvationPlanetary K-index
Now: Kp= 3 quiet
24-hr max: Kp= 4 unsettled
explanation | more data
Interplanetary Mag. Field
Btotal: 3.6 nT
Bz: 2.8 nT north
more data: ACE, DSCOVR
Updated: Today at 1506 UTCoronal Holes: 27 Jan 17
Earth is inside a stream of solar wind flowing from the indicated coronal hole. Credit: NASA/SDO.Noctilucent Clouds The southern season for noctilucent clouds began on Nov. 17, 2016. Come back to this spot every day to see the “daily daisy” from NASA’s AIM spacecraft, which is monitoring the dance of electric-blue around the Antarctic Circle.
Switch view: Ross Ice Shelf, Antarctic Peninsula, East Antarctica, PolarUpdated at: 01-26-2017 16:55:02
Updated at: 2017 Jan 26 2200 UTC
Probabilities for significant disturbances in Earth’s magnetic field are given for three activity levels: active, minor storm, severe stormUpdated at: 2017 Jan 26 2200 UTCMid-latitudes