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Solar wind
speed: 268.3 km/sec
density: 2.8 protons/cm3
explanation | more data
Updated: Today at 2347 UT
X-ray Solar Flares
6-hr max: B8
2109 UT Apr28
24-hr: C2
1522 UT Apr28
explanation | more data
Updated: Today at: 2300 UT
Daily Sun: 28 Apr 14
None of these magnetically-simple sunspots poses a threat for strong solar flares. Credit: SDO/HMI
Sunspot number: 84
What is the sunspot number?
Updated 28 Apr 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
28 Apr 2014

The Radio Sun
10.7 cm flux: 118 sfu
explanation | more data
Updated 28 Apr 2014

Current Auroral Oval:
Switch to: Europe, USA, New Zealand, Antarctica
Credit: NOAA/POES
Planetary K-index
Now: Kp= 0 quiet
24-hr max: Kp= 3
quiet
explanation | more data
Interplanetary Mag. Field
Btotal: 1.7 nT
Bz: 0.8 nT south
explanation | more data
Updated: Today at 2347 UT
Coronal Holes: 28 Apr 14
There are no large 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: 02-28-2014 16:55:02
SPACE WEATHER
NOAA Forecasts
Updated at: 2014 Apr 28 2200 UTC
FLARE
0-24 hr
24-48 hr
CLASS M
15 %
15 %
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: 2014 Apr 28 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
20 %
20 %
MINOR
30 %
30 %
SEVERE
30 %
30 %
 
Monday, Apr. 28, 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

CONTINUED QUIET: Solar activity remains low. Only a few sunspots are facing Earth, and none has the kind of complex magnetic field that harbors energy for strong explosions. NOAA forecasters estimate a 10% chance of M-class flares and only a 1% chance of X-flares on April 28th. Solar flare alerts: text, voice

MYSTERIOUS SUN PILLAR ECHOS: Many of us have witnessed sun pillars--columns of light that lance upwards from the horizon just as the sun is rising or setting. They are caused by plate-shaped ice crystals in clouds that bend the rays of the low-hanging sun. While sun pillars are frequently seen, in all seasons and at all latitudes, elusive companions of sun pillars may have been frequently overlooked. They are called sun pillar "echos":


Image credit: Jon Inghram. Larger images: #1, #2

Atmospheric optics expert Les Cowley explains: "13 years ago in Finland, three halo experts saw peculiar 'echoes' straddling an otherwise ordinary sun pillar. They could not be explained and there the matter rested for want of confirmation by another observation. Then, last week, Jon Inghram sent me several sun pillar images. He too had noticed faint 'echoes' on each side of his pillar – the mysterious ice halo was at last confirmed!"

"More details and pictures may be found in an article here. But we still cannot explain them. The Finland observers, Jon and I have each tried simulations using the flattened pyramid crystals invoked to account for elliptical halos. They do not work at all well. We need many more observations! Take plenty of pictures of each pillar. The echoes are easily overlooked or mistaken for cloud patches and have probably been seen many times. Observations under different conditions could help unravel their mystery."

Realtime Space Weather Photo Gallery

WINGED SUNSPOT: Yesterday, for less than a second, the sunspot number surged. Kamila Mazurkiewicz of Michów, Poland, photographed the addition, which looked a lot like a spaceship:

"It was the International Space Station," says Mazurkiewicz.

Traveling faster than 17,000 mph, the ISS flitted across the sun in only 0.81 seconds, so quickly that Mazurkiewicz barely caught it. "The clouds parted just in time. There were storm clouds and thunder attending the transit. I squealed and jumped up when I saw the space station's silhouette."

Would you like to know when the sunspot number will spike again? Space station transit predictions are available from CalSky.com. Solar flare alerts: text, voice

Realtime Space Weather Photo Gallery


Realtime Mars Photo Gallery


Realtime Aurora 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 Apr. 27, 2014, the network reported 7 fireballs.
(7 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 April 28, 2014 there were potentially hazardous asteroids.
Recent & Upcoming Earth-asteroid encounters:
Asteroid
Date(UT)
Miss Distance
Size
2014 HP2
Apr 24
3.8 LD
15 m
2014 HU2
Apr 25
3.7 LD
22 m
2014 HM4
Apr 25
1.6 LD
18 m
2014 HW
Apr 27
2.1 LD
10 m
2007 HB15
Apr 28
6.7 LD
12 m
2014 HL2
Apr 28
8.8 LD
26 m
2014 HE5
Apr 29
9.7 LD
36 m
2014 HV2
Apr 29
1.4 LD
28 m
2014 HT46
May 4
7 LD
21 m
2010 JO33
May 17
4 LD
43 m
2005 UK1
May 20
36.7 LD
1.1 km
1997 WS22
May 21
47.1 LD
1.5 km
2002 JC
May 24
48.7 LD
1.4 km
2014 HQ124
Jun 8
3.2 LD
860 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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