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Solar wind
speed: 521.3 km/sec
density: 1.4 protons/cm3
explanation | more data
Updated: Today at 2348 UT
X-ray Solar Flares
6-hr max: C1
2006 UT Mar23
24-hr: C1
2006 UT Mar23
explanation | more data
Updated: Today at: 2300 UT
Daily Sun: 23 Mar 15
Sunspot AR2305 has a 'beta-gamma' magnetic field that harbors energy for M-class solar flares. Credit: SDO/HMI

Sunspot number: 88
What is the sunspot number?
Updated 23 Mar 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 23 Mar 2015


The Radio Sun
10.7 cm flux: 120 sfu
explanation | more data
Updated 23 Mar 2015

Current Auroral Oval:
Switch to: Europe, USA, New Zealand, Antarctica
Credit: NOAA/Ovation
Planetary K-index
Now: Kp= 2 quiet
24-hr max: Kp= 5
storm
explanation | more data
Interplanetary Mag. Field
Btotal: 4.8 nT
Bz: 0.1 nT north
explanation | more data
Updated: Today at 1942 UT
Coronal Holes: 22 Mar 15

There are no large equatorial coronal holes on the Earthside of the sun. Credit: SDO/AIA.
Noctilucent Clouds The southern season for NLCs has come to an end. The last clouds were observed by NASA's AIM spacecraft on Feb. 20, 2015. Now attention shifts to the northern hemisphere, where the first clouds of 2015 should appear in mid-May.
Switch view: Ross Ice Shelf, Antarctic Penninsula, East Antarctica, Polar
Updated at: 02-28-2015 02:55:03
SPACE WEATHER
NOAA Forecasts
Updated at: 2015 Mar 23 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: 2015 Mar 23 2200 UTC
Mid-latitudes
0-24 hr
24-48 hr
ACTIVE
40 %
35 %
MINOR
20 %
10 %
SEVERE
01 %
01 %
High latitudes
0-24 hr
24-48 hr
ACTIVE
10 %
15 %
MINOR
25 %
30 %
SEVERE
60 %
45 %
 
Monday, Mar. 23, 2015
What's up in space
 

Come to Tromsø and share Marianne's passion for rural photography: Chasethelighttours.co.uk invites you to experience "Heaven on Earth" with an aurora, fjord, fishing, whale watching, photography or sightseeing tour.

 
Chase the Light Tours

GEOMAGNETIC ACTIVITY: For the 5th day in a row, a high-speed (600 km/s) solar wind stream is buffeting Earth's magnetic field, sparking mild geomagnetic storms around the Arctic Circle. High-latitude sky watchers should remain alert for auroras on March 23rd. Aurora alerts: text, voice

INSIDE THE SHADOW OF THE MOON: Warning: The movie you are about to see could turn you into an eclipse-chaser. Last Friday, March 20th, the Moon passed directly in front of the sun, producing a total eclipse over the Arctic Ocean. For almost three minutes, the cool shadow of the Moon fell on Svalbard, also known as "the island of polar bears" because of its large population of Ursus maritimus. Nick James, who became an eclipse-chaser long ago, was in Longyearbyen, Svalbard, for the event, and he made this movie:

"This eclipse was one of my best," says James. "The weather was perfect and the corona was amazing in a very transparent deep blue sky. There were interesting prominences and dramatic shadow bands--both of which are shown in the movie. At totality, the temperature dropped below -20 C, which was a challenge for both the photographer and his cameras!"

Meanwhile in the ionosphere: The eclipse had a dramatic effect on the ionization of Earth's upper atmosphere. Normally, during the day, solar UV radiation breaks apart atoms and molecules, creating a layer of ionized gas hundreds of kilometers above Earth's surface. The Moon, however, blocked those UV rays. Subsequent changes to the ionization structure of the atmosphere altered the propagation of radio waves in a broad region around the eclipse zone. Take a look at these data from Rudolf Slošiar, who operates a VLF (very low frequency) radio monitoring station in Bojnice, Slovakia:

"During the solar eclipse, significant changes in the the D layer of the ionosphere affected the transmission of radio stations I record using my SID monitor," says Slošiarl. Signals from Iceland were boosted, while radio stations in France and Puerto Rico dropped out.

For more anecdotes from the eclipse, monitor Spaceweather.com's realtime photo gallery:

Realtime Space Weather Photo Gallery

SPACE YEAST: On March 17th, during the strongest geomagnetic storm of the current solar cycle, Spaceweather.com and the students of Earth to Sky Calculus launched a Space Weather Buoy to measure the effect of the CME's impact on cosmic rays in the stratosphere. Along with radiation detectors and other sensors, the payload carried some hitchhikers--brewer's and baker's yeast:

During their ascent to the stratosphere, the yeast experienced temperatures as low as -60 C, air pressures only 1% of sea level, and cosmic ray dose rates 40 times Earth-normal.

What can you do with Space Yeast? Bake space bread, brew space beer, or whip up any recipe that calls for yeast. Also, teachers and homeschoolers can conduct some cool classroom experiments.

If you would like a packet of space yeast, you can have one by making a donation of $49.95 to Earth to Sky Calculus. Every flown packet of baker's yeast comes with a control packet that remained behind on Earth during the flight, so you can conduct a properly-controlled scientific experiment. All proceeds support student space weather research. Contact Dr. Tony Phillips to place your order.

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 Mar. 23, 2015, the network reported 8 fireballs.
(8 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 23, 2015 there were potentially hazardous asteroids.
Recent & Upcoming Earth-asteroid encounters:
Asteroid
Date(UT)
Miss Distance
Size
2015 FK
Mar 19
3.6 LD
37 m
2015 FF
Mar 20
4.2 LD
20 m
2015 EG7
Mar 20
2.7 LD
15 m
2015 FM
Mar 23
6.1 LD
26 m
2015 FW33
Mar 23
9.5 LD
29 m
2015 FO34
Mar 23
6.4 LD
13 m
2015 FN34
Mar 25
8 LD
20 m
2015 FC
Mar 26
2.9 LD
20 m
2015 FP
Mar 28
9.6 LD
41 m
2015 FN33
Apr 6
9.8 LD
26 m
2063 Bacchus
Apr 7
76 LD
1.6 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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