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Solar wind
speed: 351.5 km/sec
density: 3.0 protons/cm3
explanation | more data
Updated: Today at 2347 UT
X-ray Solar Flares
6-hr max: C3
1725 UT Jun15
24-hr: M1
1139 UT Jun15
explanation | more data
Updated: Today at: 2300 UT
Daily Sun: 15 Jun 14
Earth-facing sunspot AR2087 has a 'beta-gamma' magnetic field that harbors energy for M-class solar flares. Credit: SDO/HMI
Sunspot number: 159
What is the sunspot number?
Updated 15 Jun2014

Spotless Days
Current Stretch: 0 days
2014 total: 0 days (0%)
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%)

Update
15 Jun 2014

The Radio Sun
10.7 cm flux: 153 sfu
explanation | more data
Updated 15 Jun 2014

Current Auroral Oval:
Switch to: Europe, USA, New Zealand, Antarctica
Credit: NOAA/POES
Planetary K-index
Now: Kp= 1 quiet
24-hr max: Kp= 2
quiet
explanation | more data
Interplanetary Mag. Field
Btotal: 5.0 nT
Bz: 1.1 nT north
explanation | more data
Updated: Today at 2347 UT
Coronal Holes: 15 Jun 14
There are no large equatorial coronal holes on the Earthside of the sun. Credit: SDO/AIA.

Spaceweather.com posts daily satellite images of noctilucent clouds (NLCs), which hover over Earth's poles at the edge of space. The data come from NASA's AIM spacecraft. The north polar "daisy" pictured below is a composite of near-realtime images from AIM assembled by researchers at the University of Colorado's Laboratory for Atmospheric and Space Physics (LASP).
Noctilucent Clouds
Switch view: Europe, USA, Asia, Polar
Updated at: 06-15-2014 14:55:02
SPACE WEATHER
NOAA Forecasts
Updated at: 2014 Jun 15 2200 UTC
FLARE
0-24 hr
24-48 hr
CLASS M
55 %
55 %
CLASS X
25 %
20 %
Geomagnetic Storms:
Probabilities for significant disturbances in Earth's magnetic field are given for three activity levels: active, minor storm, severe storm
Updated at: 2014 Jun 15 2200 UTC
Mid-latitudes
0-24 hr
24-48 hr
ACTIVE
20 %
20 %
MINOR
05 %
05 %
SEVERE
01 %
01 %
High latitudes
0-24 hr
24-48 hr
ACTIVE
15 %
15 %
MINOR
25 %
20 %
SEVERE
30 %
20 %
 
Sunday, Jun. 15, 2014
What's up in space
 

When is the best time to see auroras? Where is the best place to go? And how do you photograph them? These questions and more are answered in a new book, Northern Lights - a Guide, by Pal Brekke & Fredrik Broms.

 
Northern Lights - a Guide

HARSH SPACE WEATHER DOOMS LIFE ON RED DWARF PLANETS: Red dwarfs are by far the most numerous type of star in the Galaxy, accounting for as much as 80% of the stellar population of the Milky Way. Because of this, astronomers looking for potentially habitable worlds have targeted red dwarf stars. A new study, however, shows that harsh space weather might strip the atmosphere of any rocky planet orbiting in a red dwarf's habitable zone, dooming life as we would know it in a majority of the Galaxy's planetary systems. [full story]

SOLAR ACTIVITY: With several active sunspots rotating over the sun's western limb, departing for the farside, solar activity is quieting. The departure, however, is a riot. J. P. Brahic sends this picture from Uzès, France:

Brahic inserted an image of Earth for scale. The dark cores of the departing sunspots are about the size of our planet, and the surrounding tangle of magnetic filaments could swallow Earth with room to spare. Brahic took the picture through cirrus clouds using a 9 inch solar telescope.

These sunspots are leaving behind at least one region still capable of major flares: AR2087 is almost directly facing Earth and it has a 'beta-gamma' magnetic field that harbors energy for M-class eruptions. Any flares from AR2087 this weekend would hit Earth head on.  Solar flare alerts: text, voice

Realtime Space Weather Photo Gallery

TIME TO CHECK YOUR SOLARCANS: The northern summer solstice is just one week away. According to Jan Koeman of Philippus Lansbergen Observatory in Middelburg,the Netherlands, that means "it's time to check your solarcans." A solarcan, a.k.a. solargraph, is a pinhole camera made from a soda or beer can lined with a piece of photographic paper. Using such a simple device, it is possible to take extraordinarily long exposures of the daily sun--in this case, six months long. Yesterday, Koeman opened a solarcan he deployed in December, and this is what he found:

Normally, solarcans record the graceful tracks the sun makes across the sky as the seasons unfold--high tracks corresponding to summer, low tracks to winter. In this case, the tracks were interrupted because Koeman deployed his solarcan inside a lighthouse. "I worried that the powerful light from the lighthouse would overwhelm the sun. Luckily our sun is much stronger. However, the fresnel prisms in the lighthouse were chopping up the sunlight."

Got a solarcan? Open it up and submit your images.

6-month Solargraph How-to Guides: #1, #2, #3

Realtime Space Weather Photo Gallery


Realtime Aurora Photo Gallery


Realtime Comet 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 Spaceweather.com.

On Jun. 15, 2014, the network reported 5 fireballs.
( 5 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 June 15, 2014 there were 1483 potentially hazardous asteroids.
Recent & Upcoming Earth-asteroid encounters:
Asteroid
Date(UT)
Miss Distance
Size
2014 LL26
Jun 10
5.3 LD
38 m
2013 AG69
Jul 8
2.7 LD
15 m
2011 PU1
Jul 17
7.9 LD
43 m
2002 JN97
Aug 2
61.4 LD
2.0 km
2001 RZ11
Aug 17
34.2 LD
2.2 km
2013 WT67
Aug 17
16.1 LD
1.2 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
Space Weather Alerts
   
  more links...
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