Solar wind
speed: 281.4 km/sec
density: 5.2 protons/cm3
more data: ACE, DSCOVR
Updated: Today at 1023 UT
X-ray Solar Flares
6-hr max: B6
0317 UT Mar23
24-hr: B8
0004 UT Mar23
explanation | more data
Updated: Today at: 1000 UT
Daily Sun: 23 Mar 19
Departing sunspot AR2736 poses a continued threat for C-class solar flares. Credit: SDO/HMI

Sunspot number: 27
What is the sunspot number?
Updated 23 Mar 2019

Spotless Days
Current Stretch: 0 days
2019 total: 53 days (67%)
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 23 Mar 2019


Thermosphere Climate Index
today: 4.35
x1010 W Cold
Max: 49.4
x1010 W Hot (10/1957)
Min: 2.05
x1010 W Cold (02/2009)
explanation | more data
Updated 22 Mar 2019

The Radio Sun
10.7 cm flux: 82 sfu
explanation | more data
Updated 23 Mar 2019

Current Auroral Oval:
Switch to: Europe, USA, New Zealand, Antarctica
Credit: NOAA/Ovation
Planetary K-index
Now: Kp= 0 quiet
24-hr max: Kp= 0
quiet
explanation | more data
Interplanetary Mag. Field
Btotal: 3.8 nT
Bz: -1.1 nT south
more data: ACE, DSCOVR
Updated: Today at 1023 UT
Coronal Holes: 23 Mar 19


Solar wind flowing from this large coronal hole should reach Earth on March 26-27.
Credit: SDO/AIA

Noctilucent Clouds The southern season for noctilucent clouds (NLCs) is ending. NASA's AIM spacecraft is detecting a sharp decline in electric blue clouds at the edge of space over Antarctica.
Switch view: Europe, USA, Asia, Polar
Updated at: 03-02-2019 16:55:03
SPACE WEATHER
NOAA Forecasts
Updated at: 2019 Mar 22 2200 UTC
FLARE
0-24 hr
24-48 hr
CLASS M
10 %
10 %
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: 2019 Mar 22 2200 UTC
Mid-latitudes
0-24 hr
24-48 hr
ACTIVE
30 %
40 %
MINOR
40 %
30 %
SEVERE
20 %
05 %
High latitudes
0-24 hr
24-48 hr
ACTIVE
05 %
05 %
MINOR
20 %
20 %
SEVERE
75 %
70 %
 
Saturday, Mar. 23, 2019
What's up in space
       
 

Solar minimum is here - but even now strangely beautiful auroras are dancing around the poles. Deep inside the Arctic Circle, the expert guides of Aurora Holidays in Utsjoki, Finland, can help you chase them. Book now!

 

SPACE WEATHER PHOTO GALLERY TROUBLES: Many readers have noticed that our realtime photo gallery is malfunctioning. We apologize for the inconvenience. Troubleshooting is underway. Meanwhile, if you have any problem submitting your photos, feel free to email them directly to Dr. Tony Phillips.

GEOMAGNETIC STORM WARNING: NOAA forecasters say there is a 75% chance of geomagnetic storms on March 23rd when a coronal mass ejection (CME) is expected to sideswipe Earth's magnetic field. Storm levels could reach category G2, which is moderately strong. During G2-class storms, auroras may be seen in northern-tier US states as far south as New York and Idaho. Aurora alerts: SMS text, email.

COSMIC RAY BALLOON LAUNCH: For more than 4 years, Spaceweather.com and the students of Earth to Sky Calculus have been launching cosmic ray balloons to the stratosphere. Near-weekly launches have shown that radiation levels are increasing. Today, mindful that a CME is approaching Earth, the young scientists launched their 285th balloon laden with X-ray/gamma-ray sensors:

The balloon ascended 110,000 feet over the snow-capped Sierra Nevada mountains of central California, sampled cosmic rays, then parachuted back to Earth, landing in a remote area of Death Valley National Park. The purpose of the flight is to provide a BEFORE measurement--before the CME arrives, that is. If the CME strikes on March 23rd, as expected, an AFTER balloon will be launched to assess the affect of the solar storm cloud on atmospheric radiation.

It might surprise you to learn that a CME can cause radiation to go down. It's called a "Forbush Decrease," named after physicist Scott E. Forbush who first described it in the 20th century. Magnetic fields inside CMEs often sweep aside cosmic rays that would otherwise penetrate Earth's atmosphere. We may be able to measure this ironic effect of solar storms in the day ahead. stay tuned.

Realtime Aurora Photo Gallery

A GIFT FROM THE EDGE OF SPACE: Last month, the students of Earth to Sky Calculus launched the starship Enterprise to the stratosphere. Riding onboard a high-altitude cosmic ray balloon, the laser-etched crystal spaceship traveled 34.7 km (113,845 feet) above Earth's surface:

You can have it for $149.95. The students are selling the Enterprise to support their cosmic ray ballooning program. Each starship comes with a greeting card showing the item in flight and telling the story of its journey to the edge of space. Also included is a multi-colored LED illuminated stand (shown in the picture above). This creates a colorful visual effect and allows the Enterprise to be used as a far-out night light.

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


Realtime Space Weather Photo Gallery


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 Mar. 22, 2019, 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, 2019 there were 1967 potentially hazardous asteroids.
Recent & Upcoming Earth-asteroid encounters:
Asteroid
Date(UT)
Miss Distance
Velocity (km/s)
Diameter (m)
2019 DH1
2019-Mar-18
8.6 LD
5
21
2019 CL2
2019-Mar-18
10.2 LD
7.5
76
2019 CD5
2019-Mar-20
10.1 LD
17
146
2019 ES2
2019-Mar-20
7.6 LD
6.9
24
2019 DS
2019-Mar-21
17.3 LD
8.9
38
2019 EA2
2019-Mar-22
0.8 LD
5.4
24
2019 FF
2019-Mar-23
3.2 LD
8.6
20
2019 EK2
2019-Mar-23
4.7 LD
8.1
11
2019 ER2
2019-Mar-25
8.9 LD
4.8
23
2019 EN
2019-Mar-27
9.7 LD
15.2
207
2016 GE1
2019-Apr-04
3.9 LD
10.1
17
2014 UR
2019-Apr-09
13 LD
4.6
17
2016 GW221
2019-Apr-09
10.1 LD
5.3
39
2014 HD177
2019-Apr-10
6.1 LD
14
102
2012 XO134
2019-Apr-18
14.8 LD
11
56
522684
2019-Apr-19
19 LD
11.5
214
2018 KK1
2019-May-05
13.9 LD
13.9
71
2017 RC
2019-May-09
14.5 LD
10.6
9
2008 HS3
2019-May-09
14.6 LD
5.3
162
2018 VX8
2019-May-12
6.2 LD
15.5
118
2012 KT12
2019-May-18
3.3 LD
3.9
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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