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Space Weather Update: 11/23/2015

By, 11/23/2015

FILAMENT ERUPTION PROBABLY MISSES EARTH: Yesterday, Nov. 22nd, a dark filament of magnetism erupted away from the sun's southeastern quadrant. NASA's Solar Dynamics Observatory recorded the blast:


SOHO has observed a faint coronal mass ejection (CME) emerging from the blast site: movie. NOAA forecasters are still computing a storm track for the CME. At first glance, however, it appears to be moving well off of the sun-Earth line. This eruption will probably miss our planet. Solar flare alerts: text or voice

Realtime Space Weather Photo Gallery

AURORAS, FOR NO PARTICULAR REASON: Nov. 21st was a day of quiet space weather. There were no intense solar flares, no CMEs, and no geomagnetic storms. The auroras appeared anyway. Liselotte Kahns saw them over Sweden's Abisko National Park:


"Despite the extremely low level of solar activity, Abisko's clear sky demonstrated a nice aurora display tonight," says Kahns. "[It's] a good illustration of why this place is rated as one of the best places on Earth to see auroras."

Indeed, it is not unusual for auroras to appear over Abisko even when the forecast calls for no magnetic activity. Aurora tour guides and photographers naturally gravitate toward the Park because of its frequently-green skies. The reason is Abisko's location beneath Earth's persistent auroral oval. A gentle rain of solar wind electrons, guided to Earth by our planet's curved magnetic field, creates a polar ringof Northern Lights that intersects the latitude of Abisko, more often than not. Browse the realtime gallery for more sightings:

Realtime Aurora Photo Gallery

FLY ME TO THE MOON: Observers of America's space program have often lamented that the International Space Station cannot go to the Moon. On Nov. 21st, it looks like it finally made the trip. Dennis Simmons sends this picture from Brisbane, Qld, Australia:


Unfortunately, it only looks like the ISS has re-traced the steps of Apollo. The giant spaceship is still in Earth orbit. It did, however, pass in front of the Moon as seen by observers in parts of Australia.

"The transit lasted just 0.49 seconds," says Simmons, who used a video camera to record the split-second passage. "This is a composite of video frames taken through a C9.25 telescope."

Elsewhere in Brisbane, astrophotographer Tom Harradine also took a spectacular picture of the transit. "I caught the ISS passing by the crater Copernicus," he says.

At the time of the transit, the ISS was 400 km from Earth and almost 400 thousandkm from the Moon. So it still has a ways to go. For now, lunar transits are the next best thing to being there.

Realtime Space Weather Photo Gallery

TRANSCONTINENTAL SPACE WEATHER BALLOON FLIGHT: On Nov. 21st, the students of Earth to Sky Calculus, in collaboration with and the University of New Hampshire, launched a pair of space weather balloons from opposite sides of the USA. Using cell phones to conduct a transcontinental countdown, they released the balloons at the same moment from California and New Hampshire:


Flying simultaneously, the balloons ascended to the stratosphere, sampling X-rays and gamma-rays at altitudes of interest to aviation, space tourism, and climate science. The goal of the experiment is to investigate a curious difference in radiation, which the group discovered during a previous transcontinental flight in July 2015. During the summer, radiation levels in the stratosphere above New Hampshire were more than 25% higher than California, a surprisingly wide gap considering the relatively small difference in latitude between the two launch sites. The Nov. 21st flight will confirm and expand upon the findings from July.

Update: Both payloads have parachuted back to Earth. The New Hampshire payload landed in Maine, and has since been recovered from the branches of a tall tree. The California payload landed in the Saline Valley, a desert area not far from Death Valley National Park. It will be recovered on Nov. 22nd. Stay tuned for results from the flight.

Realtime Space Weather Photo Gallery

Realtime Noctilucent Cloud Photo Gallery

Realtime Meteor Photo Gallery

 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

On Nov. 23, 2015, the network reported 20 fireballs.
(14 sporadics, 4 Leonids, 2 Northern Taurids)



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 November 23, 2015 there were potentially hazardous asteroids.

Recent & Upcoming Earth-asteroid encounters:Asteroid


Miss Distance


2005 UL5

Nov 20

5.9 LD

390 m

2015 WC1

Nov 20

9.7 LD

41 m

2015 VE66

Nov 21

7.5 LD

62 m

2015 WZ1

Nov 22

1.6 LD

6 m

2015 VO142

Nov 24

1 LD

7 m

2015 VH2

Nov 24

12.9 LD

14 m

2003 EB50

Nov 29

48.8 LD

2.2 km

2007 BG29

Dec 1

54.1 LD

1.1 km

2015 VZ145

Dec 8

9.2 LD

80 m

1998 WT24

Dec 11

10.9 LD

1.1 km

2011 YD29

Dec 24

9.7 LD

24 m

2003 SD220

Dec 24

28.4 LD

1.8 km

2008 CM

Dec 29

22.8 LD

1.5 km

2004 MQ1

Jan 2

55.4 LD

1.1 km

1999 JV6

Jan 6

12.6 LD

410 m

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

Situation Report -- Oct. 30, 2015Stratospheric 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)

These measurements are based on regular space weather balloon flights: learn more.

Approximately once a week, 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 cloudstrigger 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.

Current Conditions

Solar wind
speed: 334.5 km/sec
density: 2.7 protons/cm3

explanation | more data
Updated: Today at 1737 UTX-ray Solar Flares
6-hr max: C1 
1213 UT Nov23 
24-hr: C8 0228 UT Nov23 
explanation | more data
Updated: Today at: 1700 UTDaily Sun: 23 Nov 15Crackling with minor C-class solar flares, sunspot AR2454 remains the most active region on the solar disk. Credit: SDO/HMI

Sunspot number: 76 
What is the sunspot number?
Updated 23 Nov 2015

Spotless Days
Current Stretch: 0 days
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 23 Nov 2015

The Radio Sun
10.7 cm flux: 123 sfu

explanation | more data
Updated 23 Nov 2015

Current Auroral Oval:

Switch to: Europe, USA, New Zealand, Antarctica
Credit: NOAA/OvationPlanetary K-index
Now: Kp= 1 quiet
24-hr max: Kp= 1 
explanation | more data
Interplanetary Mag. Field
Btotal: 3.7 nT
Bz: 0.3 nT north 

explanation | more data
Updated: Today at 1737 UTCoronal Holes: 23 Nov 15 
There are no large coronal holes on the Earthside of the sun. Credit: SDO/AIA.Noctilucent Clouds The northern season for NLCs is finished. According to NASA's AIM spacecraft, the last clouds were observed over Greenland on Aug. 27th. Now the waiting begins for the southern season expected to begin in November.

Switch view: Ross Ice Shelf, Antarctic Peninsula, East Antarctica, PolarUpdated at: 11-22-2015 17:55:02

NOAA Forecasts

Updated at: 2015 Nov 22 2200 UTC


0-24 hr

24-48 hr


20 %

20 %


01 %

01 %

Geomagnetic Storms:
Probabilities for significant disturbances in Earth's magnetic field are given for three activity levels: activeminor stormsevere stormUpdated at: 2015 Nov 22 2200 UTCMid-latitudes

0-24 hr

24-48 hr


05 %

10 %


05 %

05 %


01 %

01 %

High latitudes

0-24 hr

24-48 hr


15 %

15 %


15 %

15 %


15 %

15 %