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SpaceWeather.com -- News and information about meteor showers, solar flares, auroras, and near-Earth asteroids
 
Solar wind
speed: 291.7 km/sec
density: 8.7 protons/cm3
more data: ACE, DSCOVR
Updated: Today at 2348 UT
X-ray Solar Flares
6-hr max: A2
1949 UT Nov26
24-hr: A2
1408 UT Nov26
explanation | more data
Updated: Today at: 2300 UT
Daily Sun: 26 Nov 18
Sunspot AR2728 is small and quiet--typical of Solar Minimum sunspots. Credit: SDO/HMI

Sunspot number: 15
What is the sunspot number?
Updated 26 Nov 2018

Spotless Days
Current Stretch: 0 days
2018 total: 194 days (59%)
2017 total: 104 days (28%)
2016 total: 32 days (9%)
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%)
2008 total: 268 days (73%)
2007 total: 152 days (42%)
2006 total: 70 days (19%)

Updated 26 Nov 2018


Thermosphere Climate Index
today: 3.87
x1010 W Cold
Max: 49.4
x1010 W Hot (10/1957)
Min: 2.05
x1010 W Cold (02/2009)
explanation | more data
Updated 26 Nov 2018

The Radio Sun
10.7 cm flux: 70 sfu
explanation | more data
Updated 26 Nov 2018

Current Auroral Oval:
Switch to: Europe, USA, New Zealand, Antarctica
Credit: NOAA/Ovation
Planetary K-index
Now: Kp= 0 quiet
24-hr max: Kp= 1
quiet
explanation | more data
Interplanetary Mag. Field
Btotal: 3.6 nT
Bz: -0.6 nT south
more data: ACE, DSCOVR
Updated: Today at 2347 UT
Coronal Holes: 26 Nov 18

Solar wind flowing from this large coronal hole could reach Earth's magnetic field on Nov. 30th or Dec. 1st. Credit: SDO/AIA
Noctilucent Clouds The season for noctilucent clouds (NLCs) in the northern hemisphere has come to an end. Images from NASA's AIM spacecraft show no NLCs around the north pole.
Switch view: Europe, USA, Asia, Polar
Updated at: 09-03-2018 14:55:02
SPACE WEATHER
NOAA Forecasts
Updated at: 2018 Nov 26 2200 UTC
FLARE
0-24 hr
24-48 hr
CLASS M
01 %
01 %
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: 2018 Nov 26 2200 UTC
Mid-latitudes
0-24 hr
24-48 hr
ACTIVE
20 %
10 %
MINOR
05 %
01 %
SEVERE
01 %
01 %
High latitudes
0-24 hr
24-48 hr
ACTIVE
20 %
15 %
MINOR
25 %
20 %
SEVERE
20 %
15 %
 
Monday, Nov. 26, 2018
What's up in space
       
 

Lights Over Lapland has a brand-new website full of exciting adventures in Abisko National Park, Sweden! Take a look at our aurora activities and book your once-in-a-lifetime trip with us today!

 

INSIGHT LANDS ON MARS: NASA's InSight Mars lander is safe on the Red Planet. InSight touched down in the plains of Elysium Planitia at 11:54 a.m. PST (2:54 p.m. EST) and has already sent back its first picture. A post-landing news briefing expected at 2 p.m. PST (5 p.m. EST). Stay tuned to NASA TV .

A LONG-LASTING HOLE IN THE SUN'S ATMOSPHERE: It's back. A hole in the sun's atmosphere that opened in June is turning to face Earth for the 6th time. NASA's Solar Dynamics Observatory photographed the structure, which stretches for more than 700,000 km across the sun's equator:

This is a "coronal hole"--a place where the sun's magnetic field opens up and allows solar wind to escape. An emerging stream of solar wind is expected to reach Earth on Nov. 30th or Dec. 1st.

The last time solar wind from this hole lashed Earth's magnetic field, on Nov. 4th, it sparked a G1-class geomagnetic storm with auroras photographed in northern-tier US States including Wyoming, Montana, Iowa, Washington, North Dakota and, of course, Alaska. Similar displays may be in the offing this weekend. Free: Aurora Alerts.

Realtime Space Weather Photo Gallery

COMET PLUNGES INTO THE SUN: Subtract one from the Solar System's total count of comets. On Saturday, Nov. 24th, a small unnamed comet dove into the sun and evaporated. Coronagrapbhs onboard the Solar and Heliospheric Observatory (SOHO) recorded the death plunge:

A subsequent movie shows the comet going in, but not coming out again. R.I.P.!

The doomed comet was a member of the Kreutz family. Kreutz sungrazers are fragments from the breakup of a single giant comet many centuries ago. They are seen falling into the sun dozens of times a year. This particular sungrazer measured a few tens of meters in diameter, too small to survive a close approach with the sun.

Realtime Space Weather Photo Gallery

A GIFT FROM THE EDGE OF SPACE: Are you looking for a far-out gift? Nothing says "Merry Christmas" like a moonstone from the edge of space. The students of Earth to Sky Calculus flew this moonstone wrapped in a hand-crafted sterling silver Celtic love knot 35.1 km (115,158 feet) above Earth's surface:

You can have it for $179.95. The students are selling these pendants to support their cosmic ray ballooning program. Each one comes with a greeting card showing the item in flight and telling the story of its journey to the edge of space. All sales support the Earth to Sky Calculus cosmic ray ballooning program and hands-on STEM research.

Far Out Gifts: Earth to Sky Store
All sales support hands-on STEM education


Realtime Aurora 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 Nov. 26, 2018, the network reported 29 fireballs.
(29 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 November 26, 2018 there were 1936 potentially hazardous asteroids.
Recent & Upcoming Earth-asteroid encounters:
Asteroid
Date(UT)
Miss Distance
Velocity (km/s)
Diameter (m)
2018 VQ6
2018-Nov-20
11.4 LD
7.9
21
2018 VP7
2018-Nov-20
7.7 LD
5.7
17
2018 WD
2018-Nov-24
4.5 LD
13.6
50
2009 WB105
2018-Nov-25
15.2 LD
18.9
71
2018 VT7
2018-Nov-25
8.2 LD
2.3
10
2008 WD14
2018-Nov-27
7.4 LD
9.3
93
2001 WO15
2018-Nov-28
13.6 LD
11.7
107
2018 VE4
2018-Nov-30
15 LD
4.8
30
2018 WN
2018-Dec-01
14.9 LD
4.4
17
2018 TG6
2018-Dec-02
3.9 LD
1.4
13
2013 VX4
2018-Dec-09
4.1 LD
6.6
65
2001 XG1
2018-Dec-10
7.9 LD
14.2
78
2018 VX6
2018-Dec-10
16.5 LD
11.2
69
2015 XX169
2018-Dec-13
17 LD
5.8
12
2018 VO9
2018-Dec-15
2.6 LD
2.9
16
2017 XQ60
2018-Dec-21
11.3 LD
15.6
47
163899
2018-Dec-22
7.4 LD
6.2
1232
418849
2018-Dec-23
16.6 LD
17.6
269
2014 AD16
2019-Jan-04
12.9 LD
9.4
12
2016 AZ8
2019-Jan-07
11.6 LD
9.1
224
2013 YM2
2019-Jan-09
7.3 LD
4.3
20
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.
  Cosmic Rays in the Atmosphere

SOMETHING NEW! We have developed a new predictive model of aviation radiation. It's called E-RAD--short for Empirical RADiation model. We are constantly flying radiation sensors onboard airplanes over the US and and around the world, so far collecting more than 22,000 gps-tagged radiation measurements. Using this unique dataset, we can predict the dosage on any flight over the USA with an error no worse than 15%.

E-RAD lets us do something new: Every day we monitor approximately 1400 flights criss-crossing the 10 busiest routes in the continental USA. Typically, this includes more than 80,000 passengers per day. E-RAD calculates the radiation exposure for every single flight.

The Hot Flights Table is a daily summary of these calculations. It shows the 5 charter flights with the highest dose rates; the 5 commercial flights with the highest dose rates; 5 commercial flights with near-average dose rates; and the 5 commercial flights with the lowest dose rates. Passengers typically experience dose rates that are 20 to 70 times higher than natural radiation at sea level.

To measure radiation on airplanes, we use the same sensors we fly to the stratosphere onboard Earth to Sky Calculus cosmic ray balloons: neutron bubble chambers and X-ray/gamma-ray Geiger tubes sensitive to energies between 10 keV and 20 MeV. These energies span the range of medical X-ray machines and airport security scanners.

Column definitions: (1) The flight number; (2) The maximum dose rate during the flight, expressed in units of natural radiation at sea level; (3) The maximum altitude of the plane in feet above sea level; (4) Departure city; (5) Arrival city; (6) Duration of the flight.

SPACE WEATHER BALLOON DATA: Approximately once a week, Spaceweather.com and the students of Earth to Sky Calculus fly space weather balloons to the stratosphere over California. These balloons are equipped with radiation sensors that detect cosmic rays, a surprisingly "down to Earth" form of space weather. Cosmic rays can seed clouds, trigger lightning, and penetrate commercial airplanes. Furthermore, there are studies ( #1, #2, #3, #4) linking cosmic rays with cardiac arrhythmias and sudden cardiac death in the general population. Our latest measurements show that cosmic rays are intensifying, with an increase of more than 18% since 2015:

The data points in the graph above correspond to the peak of the Reneger-Pfotzer maximum, which lies about 67,000 feet above central California. When cosmic rays crash into Earth's atmosphere, they produce a spray of secondary particles that is most intense at the entrance to the stratosphere. Physicists Eric Reneger and Georg Pfotzer discovered the maximum using balloons in the 1930s and it is what we are measuring today.

En route to the stratosphere, our sensors also pass through aviation altitudes:

In this plot, dose rates are expessed as multiples of sea level. For instance, we see that boarding a plane that flies at 25,000 feet exposes passengers to dose rates ~10x higher than sea level. At 40,000 feet, the multiplier is closer to 50x.

The radiation sensors onboard our helium balloons detect X-rays and gamma-rays in the energy range 10 keV to 20 MeV. These energies span the range of medical X-ray machines and airport security scanners.

Why are cosmic rays intensifying? The main reason is the sun. Solar storm clouds such as coronal mass ejections (CMEs) sweep aside cosmic rays when they pass by Earth. During Solar Maximum, CMEs are abundant and cosmic rays are held at bay. Now, however, the solar cycle is swinging toward Solar Minimum, allowing cosmic rays to return. Another reason could be the weakening of Earth's magnetic field, which helps protect us from deep-space radiation.

  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
NOAA 27-Day Space Weather Forecasts
  fun to read, but should be taken with a grain of salt! Forecasts looking ahead more than a few days are often wrong.
Aurora 30 min forecast
  from the NOAA Space Environment Center
Heliophysics
  the underlying science of space weather
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