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SpaceWeather.com -- News and information about meteor showers, solar flares, auroras, and near-Earth asteroids
 
Solar wind
speed: 310.5 km/sec
density: 9.3 protons/cm3
more data: ACE, DSCOVR
Updated: Today at 2345 UT
X-ray Solar Flares
6-hr max: A7
1552 UT Mar09
24-hr: A8
0011 UT Mar09
explanation | more data
Updated: Today at: 1913 UT
Daily Sun: 10 Mar 20
Sunspot AR2758 is rapidly disintegrating. Credit: SDO/HMI

Sunspot number: 12
What is the sunspot number?
Updated 10 Mar 2020

Spotless Days
Current Stretch: 0 days
2020 total: 50 days (71%)
2019 total: 281 days (77%)
2018 total: 221 days (61%)
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 10 Mar 2020


Thermosphere Climate Index
today: 3.60
x1010 W Cold
Max: 49.4
x1010 W Hot (10/1957)
Min: 2.05
x1010 W Cold (02/2009)
explanation | more data: gfx, txt
Updated 10 Mar 2020

The Radio Sun
10.7 cm flux: 71 sfu
explanation | more data
Updated 10 Mar 2020

Cosmic Rays Solar minimum is underway. The sun's magnetic field is weak, allowing extra cosmic rays into the solar system. Neutron counts from the University of Oulu's Sodankyla Geophysical Observatory show that cosmic rays reaching Earth in 2019 are near a Space Age peak.

Oulu Neutron Counts

Percentages of the Space Age average:
today: +9.7% High
7-day change: -0.1%
Max: +11.7% Very High
(12/2009)
Min: -32.1% Very Low (06/1991)
explanation | more data
Updated 10 Mar 2020 @ 1600 UT

Current Auroral Oval:
Switch to: Europe, USA, New Zealand, Antarctica
Credit: NOAA/Ovation
Planetary K-index
Now: Kp= 0 quiet
24-hr max: Kp= 2
quiet
explanation | more data
Interplanetary Mag. Field
Btotal: 1.5 nT
Bz: -0.2 nT south
more data: ACE, DSCOVR
Updated: Today at 2345 UT
Coronal Holes: 10 Mar 20

Solar wind flowing from this polar crown coronal hole could brush Earth's magnetic field on March 11th.
Credit: SDO/AIA

Noctilucent Clouds The southern hemisphere season for noctilucent clouds began on Nov. 15th--the earliest start in recorded history. Check here for daily images from NASA's AIM spacecraft.
Switch view: Europe, USA, Asia, Polar
Updated at: 03-02-2020 17:55:02 UT
SPACE WEATHER
NOAA Forecasts
Updated at: 2020 Mar 10 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: 2020 Mar 10 2200 UTC
Mid-latitudes
0-24 hr
24-48 hr
ACTIVE
20 %
15 %
MINOR
05 %
01 %
SEVERE
01 %
01 %
High latitudes
0-24 hr
24-48 hr
ACTIVE
15 %
15 %
MINOR
25 %
20 %
SEVERE
25 %
20 %
 
Tuesday, Mar. 10, 2020
What's up in space
       
 

Marianne’s Arctic tours: Operating in small groups of 7 to 14 persons--all needs supplied for safety, comfort and pleasure. Night & day photography or non-photographic landscape - wildlife tours. Click for details!

 

A 'RADIO-ACTIVE' SUNSPOT: New-cycle sunspot AR2758 announced itself with a roar on March 8th when it bubbled up from beneath the sun's surface and emitted a series of strong shortwave radio bursts. One of the static-y outbursts was very strong, rivaling bursts typically recorded during Solar Maximum. Listen to it here.

A QUIET WAVE IN EARTH'S MAGNETOSPHERE: On March 8th, a low hum rippled through Earth's magnetic field. It lasted for more than 2 hours, and caused compass needles in the Arctic to wave back and forth a tenth of a degree. Rob Stammes recorded the event from his magnetic observatory at the Polarlightcenter in Lofoten, Norway:

"When Earth's magnetic field is quiet (as it has been lately) sometimes very interesting things can be seen on my instruments," says Stammes. "In this case we recorded pulsations with a remarkably low frequency--about 7 minutes between pulses."

What are these waves? Imagine blowing across a piece of paper, making it flutter with your breath. Solar wind can have a similar effect on magnetic fields. The waves Stammes recorded are essentially flutters propagating down the flanks of Earth's magnetosphere excited by the breath of the sun.

Researchers call such waves "pulsations continuous" or "Pc" for short. Pc waves are classified into 5 types depending on their period. These fall into the range 150 to 600 seconds--that is, Pc5. Slow Pc5 waves have been linked to a loss of particles from the van Allen radiation belts. Energetic electrons can actually surf these waves down into Earth's atmosphere, where they dissipate harmlessly.

Detecting these delicate waves requires extraordinary quiet--like sitting in a silent room and hearing a pin drop. Solar Minimum makes this possible. At the moment, Earth's magnetic field is so still, magnetometers can pick up delicate waves that would otherwise be drowned out by the normal hub-bub of geomagnetic activity.

Realtime Space Weather Photo Gallery
Free:
Spaceweather.com Newsletter

A BLACK PEARL IN THE STRATOSPHERE: It came from Tahiti--and now it's been to the edge of space. On Feb. 27, 2020, this genuine Black Tahitian South Sea Cultured Pearl flew to the stratosphere onboard an Earth to Sky Calculus cosmic ray balloon, soaring more than 100,000 feet above the Sierra Nevada mountains of central California:

You can have it for $219.95. The students are selling these exotic space pearls to fund their cosmic ray monitoring program. Measuring 10 mm in diameter, the pearl has an 18K white gold clasp and is suspended from a matching 925 Sterling Silver chain. Each pearl comes with a greeting card showing the pendant in flight and telling the story of its journey to the edge of space.

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

Realtime Aurora Photo Gallery
Free:
Spaceweather.com Newsletter

  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. 10, 2020, the network reported 13 fireballs.
(13 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 10, 2020 there were 2018 potentially hazardous asteroids.
Recent & Upcoming Earth-asteroid encounters:
Asteroid
Date(UT)
Miss Distance
Velocity (km/s)
Diameter (m)
2020 EA
2020-Mar-06
18 LD
8.3
44
2018 RF6
2020-Mar-10
11.2 LD
12.6
36
2020 EE
2020-Mar-10
4.8 LD
7.9
14
2020 CA3
2020-Mar-10
13.7 LD
6.3
32
2020 ED
2020-Mar-11
7.6 LD
8.5
15
2008 UB95
2020-Mar-11
18.5 LD
7.6
41
2018 GY
2020-Mar-15
6.2 LD
9.5
39
2020 EF
2020-Mar-19
16.8 LD
4.5
18
2020 DP4
2020-Mar-22
3.5 LD
8.1
33
2012 XA133
2020-Mar-27
17.4 LD
23.7
235
2010 GD35
2020-Mar-29
15.3 LD
12
43
2006 FH36
2020-Mar-30
11.3 LD
5.1
93
2019 GM1
2020-Apr-02
9 LD
4.2
14
2015 FC35
2020-Apr-04
10.5 LD
13.8
148
2020 DT3
2020-Apr-05
17.6 LD
11.8
192
2019 HM
2020-Apr-10
7.2 LD
3.2
23
363599
2020-Apr-11
19.2 LD
24.5
224
2019 HS2
2020-Apr-26
13.6 LD
12.6
17
2019 GF1
2020-Apr-27
18.7 LD
3.2
12
52768
2020-Apr-29
16.4 LD
8.7
2457
2020 DM4
2020-May-01
18.6 LD
6.3
161
438908
2020-May-07
8.9 LD
12.8
282
2016 HP6
2020-May-07
4.3 LD
5.7
31
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 Regener-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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