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Solar wind
speed: 432.8 km/sec
density: 4.0 protons/cm3
explanation | more data
Updated: Today at 2350 UT
X-ray Solar Flares
6-hr max: B3
2213 UT Sep13
24-hr: B6
0420 UT Sep13
explanation | more data
Updated: Today at: 2300 UT
Daily Sun: 13 Sep 15
Sunspot AR2414 has a 'beta-gamma' magnetic field that harbors energy for M-class solar flares. Credit: SDO/HMI

Sunspot number: 87
What is the sunspot number?
Updated 13 Sep 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 13 Sep 2015


The Radio Sun
10.7 cm flux: 99 sfu
explanation | more data
Updated 13 Sep 2015

Current Auroral Oval:
Switch to: Europe, USA, New Zealand, Antarctica
Credit: NOAA/Ovation
Planetary K-index
Now: Kp= 3 quiet
24-hr max: Kp= 3
quiet
explanation | more data
Interplanetary Mag. Field
Btotal: 5.1 nT
Bz: 3.6 nT north
explanation | more data
Updated: Today at 2350 UT
Coronal Holes: 13 Sep 15

Solar wind flowing from this broad northern coronal hole should reach Earth on Sept. 14. 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: Europe, USA, Asia, Polar
Updated at: 09-01-2015 09:00:00
SPACE WEATHER
NOAA Forecasts
Updated at: 2015 Sep 13 2200 UTC
FLARE
0-24 hr
24-48 hr
CLASS M
10 %
10 %
CLASS X
01 %
01 %
Geomagnetic Storms:
Probabilities for significant disturbances in Earth's magnetic field are given for three activity levels: active, minor storm, severe storm
Updated at: 2015 Sep 13 2200 UTC
Mid-latitudes
0-24 hr
24-48 hr
ACTIVE
30 %
30 %
MINOR
10 %
15 %
SEVERE
01 %
01 %
High latitudes
0-24 hr
24-48 hr
ACTIVE
15 %
15 %
MINOR
30 %
25 %
SEVERE
40 %
45 %
 
Sunday, Sep. 13, 2015
What's up in space
 

Learn to photograph Northern Lights like a pro. Sign up for Peter Rosen's Aurora Photo Courses in Abisko National Park, winner of the TripAdvisor Certificate of Excellence Award 2015.

 
Lapland tours

PARTIAL SOLAR ECLIPSE: Today, Sept. 13th at approximately 0700 UT, the Moon passed in front of the sun, off-center, producing a partial eclipse visible from the southern reaches of Africa and parts of Antarctica. Photographers with images of this remote eclipse are encouraged to share them here.

THE SUN IS STUBBORNLY QUIET: Despite the emergence of a new and unstable sunspot (AR2414), the sun remains stubbornly quiet. There hasn't been a strong flare in weeks, and the sun's X-ray output is very low. NOAA forecasters estimate a scant 10% chance of M-class solar flares on Sept. 13th. Solar flare alerts: text or voice

MORE AURORAS IN THE OFFING: So far, September has been a great month for auroras. A series of solar wind streams, mixed with one or two minor CMEs, has buffeted Earth's magnetic field almost non-stop for the past two weeks. The resulting G1- to G3-class geomagnetic storms have caused displays like this:

Minoru Yoneto took the picture on September 11th from Queenstown, New Zealand. "A big stream of solar wind gave us four lovely colors of Southern Lights," he says.

One reason for the recent spate of auroras is the coming change of seasons. For reasons that are not fully understood, auroras love equinoxes. At this time of year even gentle gusts of solar wind can spark a nice display of Northern or Southern Lights

Two gusts are on the way. NOAA forecasters expect streams of solar wind to reach Earth on Sept. 13th and Sept. 15th, sparking renewed displays of high-latitude auroras. Monitor the realtime photo gallery for updates. Aurora alerts: text or voice

Realtime Aurora Photo Gallery

EAST COAST GREEN FLASH: Last Monday, Sept. 7th, Spaceweather.com reader Don Koenigsberg woke up early to watch the sun rise from Atlantic City, NJ. He was vacationing on Labor Day. The holiday began with a flash of green:

"It was a great way to begin the day," says Koenigsberg. "I thought the video was interesting because green flashes can be difficult to see on the East Coast due to less than ideal atmospheric conditions."

Indeed, says atmospheric optics expert Les Cowley, "flashes from the west coast are MUCH more common. Mock-mirage green flashes - the type most frequently photographed - need temperature inversions.  These inversions are readily generated along the west coast by the combination of cold offshore ocean current and warm air from inland. Almost daily green flashes have sometimes been seen from San Francisco!"

Green flashes on the east coast tend to be of a different type: "the classical Omega flash," says Cowley. "This occurs when there is warm air immediately over the ocean and the air temperature gradient changes rapidly with height. For the flash to be visible the warm air layers must be below you. An 'Omega flash' is what Koenigsberg witnessed."

Mock-mirage flashes, Omega flashes, east coast flashes, west coast flashes: they are all beauties. As Jules Verne wrote in his 1882 novel "Le Rayon Vert" (The Green Ray), they display "a green which no artist could ever obtain on his palette, a green of which neither the varied tints of vegetation nor the shades of the most limpid sea could ever produce the like!" More of this special green may be found in the realtime photo gallery:

Realtime Space Weather Photo Gallery

WILDFIRE AT THE EDGE OF SPACE: On Sept. 6th, Spaceweather.com and the students of Earth to Sky Calculus launched a space weather balloon equipped with radiation sensors. It was a regular flight, part of their weekly program to monitor cosmic rays in the atmosphere. En route to the stratosphere, cameras on the payload looked back and observed an enormous wildfire. This is the view from 109,600 feet:

The massive plume of smoke, pictured right, is coming from the Rough Fire, an 86,000 acre inferno raging through King's Canyon National Park in central California. Smoke from the fire is choking much of the Sierra Nevada mountain range where our space weather balloons are launched.

We've been using balloons and Geiger tubes to monitor cosmic radiation for the past two years. This particular balloon flight attempted something new: using microbes to measure radiation. Five different strains of yeast were flown alongside conventional radiation sensors to calibrate the microbes' response to cosmic rays. This kind of experiment could lead to new and improved techniques for measuring the biological effectiveness of high-altitude radiation.

HEY THANKS! The students of Earth to Sky Calculus wish to thank Dr. Mark Casafrancisco, whose generous donation of $500 made this research flight possible. Here is his business card floating in the stratosphere:

"Sending my business card to space not only allows me to support your student research program, but also shows how proud I am of our out-of-this-world family of stellar staff and pediatric dentists at Monarch Pediatric Dental Centre in Vancouver, BC, Canada!" he says.

Readers, if you would like to sponsor a research flight and see your photo at the edge of space, please contact Dr. Tony Phillips to make arrangements.

Realtime Space Weather Photo Gallery


Realtime Sprite Photo Gallery


Realtime NLC 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 Spaceweather.com.

On Sep. 13, 2015, the network reported 13 fireballs.
(12 sporadics, 1 September epsilon Perseid)

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 September 13, 2015 there were potentially hazardous asteroids.
Recent & Upcoming Earth-asteroid encounters:
Asteroid
Date(UT)
Miss Distance
Size
2015 RG2
Sep 7
6.4 LD
20 m
2015 RC
Sep 8
10.5 LD
60 m
2015 RW35
Sep 13
2.1 LD
6 m
2014 KS76
Sep 14
8.7 LD
22 m
2004 TR12
Sep 15
58.8 LD
1.0 km
2015 RF36
Sep 30
14.5 LD
108 m
2015 RM35
Oct 2
11.7 LD
61 m
2000 SM10
Oct 2
11.7 LD
65 m
2000 FL10
Oct 10
65.7 LD
1.9 km
2011 QD48
Oct 17
67.5 LD
1.0 km
2014 UR
Oct 18
3.8 LD
21 m
2011 SE97
Oct 18
11.9 LD
50 m
2001 UY4
Oct 21
58.2 LD
1.0 km
2005 UL5
Nov 20
5.9 LD
390 m
2003 EB50
Nov 29
48.8 LD
2.2 km
2007 BG29
Dec 1
54.1 LD
1.1 km
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.
  Essential web links
NOAA Space Weather Prediction Center
  The official U.S. government space weather bureau
Atmospheric Optics
  The first place to look for information about sundogs, pillars, rainbows and related phenomena.
Solar Dynamics Observatory
  Researchers call it a "Hubble for the sun." SDO is the most advanced solar observatory ever.
STEREO
  3D views of the sun from NASA's Solar and Terrestrial Relations Observatory
Solar and Heliospheric Observatory
  Realtime and archival images of the Sun from SOHO.
Daily Sunspot Summaries
  from the NOAA Space Environment Center
Heliophysics
  the underlying science of space weather
Columbia Northern High School
  Web-based high school science course with free enrollment
Aspendell California
   
  more links...
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