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Solar wind
speed: 420.6 km/sec
density: 14.8 protons/cm3
explanation | more data
Updated: Today at 2350 UT
X-ray Solar Flares
6-hr max: B2
1706 UT Sep10
24-hr: B2
0638 UT Sep10
explanation | more data
Updated: Today at: 2300 UT
Daily Sun: 10 Sep 15
None of these sunspots poses a threat for strong flares. Solar activity remains very low. Credit: SDO/HMI

Sunspot number: 49
What is the sunspot number?
Updated 10 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 10 Sep 2015


The Radio Sun
10.7 cm flux: 82 sfu
explanation | more data
Updated 10 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= 4
unsettled
explanation | more data
Interplanetary Mag. Field
Btotal: 13.6 nT
Bz: 2.6 nT south
explanation | more data
Updated: Today at 2342 UT
Coronal Holes: 10 Sep 15

Solar wind flowing from this wide equatorial coronal hole should reach Earth on Sept. 12-13. 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 10 2230 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 10 2230 UTC
Mid-latitudes
0-24 hr
24-48 hr
ACTIVE
35 %
35 %
MINOR
25 %
25 %
SEVERE
05 %
05 %
High latitudes
0-24 hr
24-48 hr
ACTIVE
10 %
10 %
MINOR
30 %
30 %
SEVERE
55 %
55 %
 
Thursday, Sep. 10, 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

VERY QUIET... Powered by fusion, the sun is a 1027-ton nuclear explosion contained in one place only by the awesome force of its own gravity. How quiet can such a thing be? Very. According to NOAA, solar activity has been very low all week long. No sunspots are flaring, and the sun's X-ray output has flatlined. The chance of a strong solar flare on Sept. 10th is no more than 1%. Solar flare alerts: text or voice

...BUT VERY PRETTY: The sun may be quiet, but that does not mean there is no space weather. On the contrary, northern skies have been filled with auroras for the past three days. Paul Nelson sends this example from Marquette, Michigan, on Sept. 9th:

"I was out most of the night enjoying and photographing the Northern Lights," says Nelson. "The display started to fade around 5:30 a.m. and then, just like in a fireworks display, the whole sky suddenly lit up. It was the Grand Finale! I captured the moment in the photo, above."

How can such a display occur while solar activity is so low? The answer has to do with the interplanetary magnetic field (IMF). On Sept. 7th, the IMF tilted south, opening a crack in Earth's magnetosphere. Solar wind (which exists even during times of quiet) poured in to fuel the auroras.

High-latitude sky watchers should remain alert for more on Sept. 10th. NOAA forecasters estimate a 70% chance of geomagnetic storms as the solar wind continues to blow. Aurora alerts: text or voice

Realtime Aurora Photo Gallery

THE MORNING PLANET SHOW: Planets are gathering in the morning sky. Venus and Jupiter have recently emerged as morning "stars," rising in the east ahead of the sun, joining Mars in an array of lights that lets early risers view 1/3rd of the solar system at a glance. The display will continue--and improve--as autumn unfolds. This morning Jean-Baptiste Feldmann of Nuits-Saint-Georges, France, got a preview of things to come:

On Sept. 10th the crescent Moon passed by Venus en route to Jupiter, adding its luster to that of the planets. "It was a beautiful view," says Feldmann, whose lists his camera settings here.

If you like what you see, and wish to see more, mark your calendar as follows: On Oct. 8th the crescent Moon will have another close encounter with Venus (sky map), followed on Oct. 9th by a near miss of Jupiter and Mars (sky map). Every morning after that, the planets will converge until Oct. 24th - Oct. 29th when they fit within a circle only 5o wide (sky maps: #1, #2, #3, #4, #5, #6). Typical binoculars can see a patch of sky about 6o or 7o degrees wide.  So when the triangle of planets shrinks to 5o, they will all fit inside a binoculars field of view. Imagine looking through the eyepiece and seeing three planets--all at once.

By the time October comes to an end, the planetary triangle will start breaking apart.  But there are still two dates of special interest:  Nov. 6th and 7th (sky maps: #1, #2).  On those increasingly wintry mornings, the crescent Moon will swoop in among the dispersing planets for a loose but beautiful conjunction.

Look east before sunrise. There's a lot to see.

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 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. 10, 2015, the network reported 44 fireballs.
(44 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]

  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 10, 2015 there were potentially hazardous asteroids.
Recent & Upcoming Earth-asteroid encounters:
Asteroid
Date(UT)
Miss Distance
Size
1991 CS
Sep 4
62.1 LD
1.4 km
2015 RG2
Sep 7
6.4 LD
20 m
2015 RC
Sep 8
10.5 LD
60 m
2014 KS76
Sep 14
8.7 LD
22 m
2004 TR12
Sep 15
58.8 LD
1.0 km
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
12 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
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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