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Solar wind
speed: 387.6 km/sec
density: 1.2 protons/cm3
explanation | more data
Updated: Today at 2346 UT
X-ray Solar Flares
6-hr max: C2
1900 UT Mar07
24-hr: C2
1900 UT Mar07
explanation | more data
Updated: Today at: 2300 UT
Daily Sun: 07 Mar 14
None of these sunspots poses a threat for strong flares. Solar activity is low. Credit: SDO/HMI
Sunspot number: 174
What is the sunspot number?
Updated 07 Mar 2014

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
07 Mar 2014

The Radio Sun
10.7 cm flux: 149 sfu
explanation | more data
Updated 07 Mar 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= 1
quiet
explanation | more data
Interplanetary Mag. Field
Btotal: 3.5 nT
Bz: 0.1 nT north
explanation | more data
Updated: Today at 2347 UT
Coronal Holes: 07 Mar 14
Streams of solar wind flowing from these widely-spaced coronal holes could sandwich Earth's magnetic field on March 9-10. 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: 02-28-2014 16:55:02
SPACE WEATHER
NOAA Forecasts
Updated at: 2014 Mar 07 2200 UTC
FLARE
0-24 hr
24-48 hr
CLASS M
30 %
30 %
CLASS X
05 %
05 %
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 Mar 07 2200 UTC
Mid-latitudes
0-24 hr
24-48 hr
ACTIVE
30 %
15 %
MINOR
05 %
05 %
SEVERE
01 %
01 %
High latitudes
0-24 hr
24-48 hr
ACTIVE
15 %
15 %
MINOR
30 %
25 %
SEVERE
35 %
25 %
 
Friday, Mar. 7, 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

ASTEROID BREAKUP: NASA's Hubble Space Telescope has recorded the never-before-seen break-up of an asteroid into as many as 10 smaller pieces. [full story]

STORM CLOUDS ON MARS: In April, Earth and Mars will converge for their closest approach of 2014. Opposition occurs on April 8th. That's when Mars rises in the east at sunset, almost perfectly opposite the sun, and soars overhead at midnight shining 8 times brighter than a 1st-magnitude star. Although closest approach is still more than a month away, astronomers are already enjoying great views of the Red Planet. Australian astrophotographer Anthony Wesley took this picture using a 16-inch telescope on March 6th:

His high-resolution image shows orographic clouds over the Elysium volcanoes just north of the Martian equator and an even brighter blue cloud over the Hellas impact basin in the southern hemisphere. Hellas is the lowest point on Mars, and some of the haze evident there could be icy fog.

Getting such Hubblesque results from a 16-inch telescope requires a combination of good seeing and long years of experience. Wesley, who is one of the world's top amateur astrophotographers, had both working for him on the morning of March 6th. "Skies were stable and clear," he says. "Using a Point Grey Research low-light Grasshopper3 camera, I recorded 2 minutes through red, green and blue filters with red @ 83fps, green@70fps and blue @50fps. I sorted all the frames according to image sharpness and stacked the best 2000 in each channel to make the color image, with additional wavelet sharpening in Registax, deconvolution in Astra Image and final color correction and touchups+captioning in the GIMP."

Observers with less experience can take good photos, too, especially as March gives way to April and Mars approaches Earth. Look for burnt-orange Mars rising in the east around around 10 p.m. about 5° from the blue 1st-magnitude star Spica. The Moon passes by Mars on March 19-20 and provides a convenient "landmark" for finding the Red Planet.

Realtime Mars Photo Gallery

CORONAL HOLE: In the sun's northern hemisphere, magnetic fields have opened up, allowing a stream of solar wind to escape into space. Such openings are called "coronal holes". NASA's Solar Dynamics Observatory took this picture of the structure during the early hours of March 6th:

A stream of solar wind flowing from this coronal hole should reach Earth on or about March 9th. Because the "spigot" is located in the sun's northern hemisphere, the stream will sail mostly north of our planet, delivering only a glancing blow to Earth's magnetic field.

A glancing blow, however, might be enough to spark polar auroras. For reasons that researchers don't fully understand, spring is aurora season. With the northern vernal equinox just around the corner, even small gusts of solar wind can stir up geomagnetic activity. Stay tuned for auroras. Aurora alerts: text, voice

Realtime Aurora Photo Gallery

HELIOPHYSICS SUMMER SCHOOL: Are you an undergraduate physics or astronomy instructor? There might be a seat waiting for you at the 2014 Heliophysics Summer School. The program's sponsor, UCAR, is looking for a number of qualified instructors to attend with most expenses paid. Apply here. The deadline has been extended to March 22nd.

Realtime Space Weather Photo Gallery


Realtime Comet 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 Mar. 6, 2014, the network reported 6 fireballs.
(6 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 March 7, 2014 there were 1458 potentially hazardous asteroids.
Recent & Upcoming Earth-asteroid encounters:
Asteroid
Date(UT)
Miss Distance
Size
2014 EL
Mar 2
3.2 LD
18 m
2014 DX110
Mar 5
0.9 LD
31 m
2014 EF
Mar 6
0.4 LD
7 m
2014 EC
Mar 6
0.2 LD
10 m
2000 EE14
Mar 6
64.6 LD
1.8 km
2014 CU13
Mar 11
8 LD
190 m
2014 DU22
Mar 14
7.9 LD
60 m
2014 EM
Mar 15
4.3 LD
41 m
2003 QQ47
Mar 26
49.9 LD
1.4 km
1995 SA
Apr 2
73.1 LD
1.6 km
2000 HD24
Apr 4
42.2 LD
1.3 km
2007 HB15
Apr 28
6.7 LD
12 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.
  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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