Love Has Won

WE ARE HERE AS HUMANITY'S TEAM AND MIRRORS OF LOVE. SO TOGETHER WE CAN BRING BACK UNITY AND PEACE TO THIS PLANET, AND RETURN TO OUR NATURAL STATE. 

We Are The First Contact Ground Crew Team, who are preparing to take Humanity Home Into The Light.

Space Weather Update: 03/27/2017

By Spaceweather.com, 03/27/2017

SUNSPOT GENESIS: A large sunspot is growing in the sun's northern hemisphere. Only 24 hours ago it didn't exist, now the active region sprawls across more than 80,000 km of solar "terrain" and contains multiple dark cores as large as Earth. Watch this movie of sunspot genesis.

GEOMAGNETIC STORM: A G2-class (moderately strong) geomagnetic storm is underway on March 27th as Earth enters a stream of solar wind flowing from a canyon-shaped hole in the sun's atmosphere.  First contact with the stream sparked bright auroras around the South Pole visible as far away as New Zealand:

 

"It was just the most amazing display ever seen by myself and my friends," reports photographer Layton Findlater of Invercargill, New Zealand.

Activity was observed around the North Pole, too. In northern Norway, magnetometers detected a shaking of Earth's magnetic field in response to buffeting from the incoming solar wind stream. Instruments at the Polarlightcenter in Lofoton recorded the action:

 

"We detected significant variations in our local magnetic field and also electric currents flowing in theground," reports Rob Stammes, who operates the magnetic observatory.  Of the Northern Lights dancing overhead, he says "these could be the last of the season before the midnight sun returns in the near future."

More auroras around both poles are likely tonight as Earth moves deeper into the solar wind stream. This stream is threaded by negative-polarity (south-pointing) magnetic fields that do a good job connecting to Earth's magnetosphere and energizing geomagnetic storms. Free: Aurora Alerts

Realtime Aurora Photo Gallery

THE FLIGHT OF THE EASTERNAUTS: The cosmic ray monitoring program of Spaceweather.com and Earth to Sky Calculus is not supported by government grants or big corporate sponsors. Instead we rely on you. That is, you and the Easternauts:

 

On March 2nd, the student researchers flew a payload-full of Easter bunnies to the edge of space--and you can have one for $39.95. (Space helmet included!) They make great Easter gifts for young scientists, and all proceeds support STEM education.  Each bunny comes with a greeting card showing the Easternaut in flight and telling the story of its journey to the stratosphere and back again.

More far-out gifts may be found in the Earth to Sky store.

Realtime Space Weather Photo Gallery

Realtime Comet Photo Gallery

Realtime Venus 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. 27, 2017, the network reported 6 fireballs.
(6 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 27, 2017 there were 1782 potentially hazardous asteroids.

Recent & Upcoming Earth-asteroid encounters:

Asteroid

Date(UT)

Miss Distance

Size

2017 FZ2

Mar 23

1.7 LD

20 m

2015 TC25

Mar 26

7.6 LD

6 m

2017 FL63

Mar 26

4.2 LD

26 m

2017 FF3

Mar 27

5.7 LD

18 m

2017 FK3

Mar 27

9 LD

26 m

2017 FV

Apr 2

9 LD

60 m

2017 EB3

Apr 4

13.8 LD

43 m

2017 DC38

Apr 5

14.6 LD

54 m

2017 FU64

Apr 6

3.8 LD

80 m

2003 BD44

Apr 18

21.7 LD

1.9 km

2014 JO25

Apr 19

4.6 LD

1.0 km

1999 CU3

Apr 19

63.7 LD

1.9 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.

 Cosmic Rays in the Atmosphere

 

Readers, thank you for your patience while we continue to develop this new section of Spaceweather.com. We've been working to streamline our data reduction, allowing us to post results from balloon flights much more rapidly, and we have developed a new data product, shown here:

 

This plot displays radiation measurements not only in the stratosphere, but also at aviation altitudes. 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. These measurements are made by our usual cosmic ray payload as it passes through aviation altitudes en route to the stratosphere over California.

What is this all about? 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 cloudstrigger 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 12% since 2015:

 

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.

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.

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.

 

Current Conditions

Solar wind
speed: 612.2 km/sec
density: 6.3 protons/cm3
more data: ACEDSCOVR
Updated: Today at 1554 UT

X-ray Solar Flares
6-hr max: C3 1112 UT Mar27
24-hr: C3 1112 UT Mar27
explanation | more data
Updated: Today at: 1500 UT

 

Daily Sun: 27 Mar 17

New sunspot AR2644 is growing rapidly and crackling with C-class solar flares. Credit: SDO/HMI

 

Sunspot number: 20
What is the sunspot number?
Updated 27 Mar 2017

Spotless Days
Current Stretch: 0 days
2017 total: 27 days (32%)
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%)
Updated 27 Mar 2017

The Radio Sun
10.7 cm flux: 77 sfu
explanation | more data
Updated 27 Mar 2017

 

Current Auroral Oval:

 

Switch to: EuropeUSANew ZealandAntarctica
Credit: NOAA/Ovation

 

Planetary K-index
Now: Kp= 5 storm
24-hr max: Kp= 6 storm
explanation | more data

Interplanetary Mag. Field
Btotal: 9.9 nT
Bz: 2.3 nT south
more data: ACEDSCOVR
Updated: Today at 1553 UT

 

Coronal Holes: 27 Mar 17


Earth is entering a stream of solar wind flowing the indicated coronal hole. Credit: NASA/SDO.

 

Noctilucent Clouds The southern season for noctilucent clouds began on Nov. 17, 2016. Come back to this spot every day to see the "daily daisy" from NASA's AIM spacecraft, which is monitoring the dance of electric-blue around the Antarctic Circle.

 

Switch view: Ross Ice ShelfAntarctic PeninsulaEast AntarcticaPolar

Updated at: 02-24-2017 17:55:02

 

SPACE WEATHER
NOAA Forecasts

 

Updated at: 2017 Mar 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: activeminor stormsevere storm

Updated at: 2017 Mar 26 2200 UTC

Mid-latitudes

0-24 hr

24-48 hr

ACTIVE

40 %

30 %

MINOR

25 %

30 %

SEVERE

10 %

15 %

High latitudes

0-24 hr

24-48 hr

ACTIVE

15 %

35 %

MINOR

20 %

15 %

SEVERE

30 %

10 %

Space Weather Update: 03/26/2017

By Spaceweather.com, 03/26/2017

POTENT CORONAL HOLE FACES EARTH: A canyon-shaped hole in the sun's atmosphere is facing Earth, and it is spewing a stream of fast-moving solar wind toward our planet.  NASA's Solar Dynamics Observatory photographed the giant fissure on March 25th:

 

This is a "coronal hole" (CH) -- a vast region where the sun's magnetic field opens up and allows solar wind to escape.  A gaseous stream flowing from this coronal hole is expected to reach our planet on during the late hours of March 27th and could spark moderately-strong G2-class geomagnetic storms around the poles on March 28th or 29th. 

We've seen this coronal hole before.  In early March, it lashed Earth's magnetic field with a fast-moving stream that sparked several consecutive days of intense auroras around the poles. The coronal hole is potent because it is spewing solar wind threaded with "negative polarity" magnetic fields. Such fields do a good job connecting to Earth's magnetosphere and energizing geomagnetic storms.

Arctic sky watchers should be alert for auroras early next week. Free: Aurora Alerts

Realtime Aurora Photo Gallery

INFERIOR CONJUNCTION OF VENUS: This weekend, Venus is passing almost directly between Earth and the sun--an event astronomers call "inferior solar conjunction."  As Venus passes by with its night side facing Earth, all we can see of the 2nd planet is a slender 1% crescent. Shahrin Ahmad photographed the curve on March 25th from Tanjung Bidara, Melaka, Malaysia:

 

"Venus was a mere 8 degrees from the sun," says Ahmad. "This is my last view of Venus before it goes the other side of the sun and becomes a Morning Star."

Because Venus is so close to the sun, some observers are catching it very close to the horizon just after sunset. The turbulent low atmosphere of Earth has a disturbing effect on Venus' graceful curves.  Consider this picture taken by Helio Vital on March 24th fromRio de Janeiro, Brazil:

 

"Earth's turbulent atmosphere acts like a dynamic set of moving lenses and prisms that play with the point-like light from the stars, causing their apparent brightness, color and even position to fluctuate or 'twinkle'," says Vital. "This effect is usually negligible for planets because the multiple beams of light we receive from their extended disks tend to cancel out. However, the current situation with Venus is different.  Its crescent is so thin, each point along the crescent acts a bit like a star--twinkling colorfully as the planet sinks toward the horizon."

Realtime Venus Photo Gallery

THE FLIGHT OF THE EASTERNAUTS: The cosmic ray monitoring program of Spaceweather.com and Earth to Sky Calculus is not supported by government grants or big corporate sponsors. Instead we rely on you. That is, you and the Easternauts:

 

On March 2nd, the student researchers flew a payload-full of Easter bunnies to the edge of space--and you can have one for $39.95. (Space helmet included!) They make great Easter gifts for young scientists, and all proceeds support STEM education.  Each bunny comes with a greeting card showing the Easternaut in flight and telling the story of its journey to the stratosphere and back again.

More far-out gifts may be found in the Earth to Sky store.

Realtime Space Weather 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. 26, 2017, the network reported 4 fireballs.
(4 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 26, 2017 there were 1782 potentially hazardous asteroids.

Recent & Upcoming Earth-asteroid encounters:

Asteroid

Date(UT)

Miss Distance

Size

2017 FJ3

Mar 22

2.6 LD

5 m

2017 FZ2

Mar 23

1.7 LD

20 m

2015 TC25

Mar 26

7.6 LD

6 m

2017 FL63

Mar 26

4.2 LD

27 m

2017 FF3

Mar 27

5.7 LD

18 m

2017 FK3

Mar 27

9.1 LD

26 m

2017 FV

Apr 2

9 LD

60 m

2017 EB3

Apr 4

13.8 LD

43 m

2017 DC38

Apr 5

14.6 LD

54 m

2017 FU64

Apr 6

3.8 LD

80 m

2003 BD44

Apr 18

21.7 LD

1.9 km

2014 JO25

Apr 19

4.6 LD

1.0 km

1999 CU3

Apr 19

63.7 LD

1.9 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.

 Cosmic Rays in the Atmosphere

 

Readers, thank you for your patience while we continue to develop this new section of Spaceweather.com. We've been working to streamline our data reduction, allowing us to post results from balloon flights much more rapidly, and we have developed a new data product, shown here:

 

This plot displays radiation measurements not only in the stratosphere, but also at aviation altitudes. 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. These measurements are made by our usual cosmic ray payload as it passes through aviation altitudes en route to the stratosphere over California.

What is this all about? 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 cloudstrigger 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 12% since 2015:

 

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.

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.

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.

 

Current Conditions

Solar wind
speed: 368.6 km/sec
density: 5.2 protons/cm3
more data: ACEDSCOVR
Updated: Today at 1603 UT

X-ray Solar Flares
6-hr max: B1 1558 UT Mar26
24-hr: B4 0234 UT Mar26
explanation | more data
Updated: Today at: 1600 UT

 

Daily Sun: 26 Mar 17

Tiny sunspot AR2643 poses no threat for strong solar flares. Credit: SDO/HMI

 

Sunspot number: 11
What is the sunspot number?
Updated 26 Mar 2017

Spotless Days
Current Stretch: 0 days
2017 total: 27 days (32%)
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%)
Updated 26 Mar 2017

The Radio Sun
10.7 cm flux: 74 sfu
explanation | more data
Updated 26 Mar 2017

 

Current Auroral Oval:

 

Switch to: EuropeUSANew ZealandAntarctica
Credit: NOAA/Ovation

 

Planetary K-index
Now: Kp= 1 quiet
24-hr max: Kp= 2 quiet
explanation | more data

Interplanetary Mag. Field
Btotal: 1.6 nT
Bz: 0.4 nT north
more data: ACEDSCOVR
Updated: Today at 1603 UT

 

Coronal Holes: 26 Mar 17


A fast-moving stream of solar wind flowing from the indicated coronal hole could reach Earth as early as March 27th (although the 28th is more likely). Credit: NASA/SDO.

 

Noctilucent Clouds The southern season for noctilucent clouds began on Nov. 17, 2016. Come back to this spot every day to see the "daily daisy" from NASA's AIM spacecraft, which is monitoring the dance of electric-blue around the Antarctic Circle.

 

Switch view: Ross Ice ShelfAntarctic PeninsulaEast AntarcticaPolar

Updated at: 02-24-2017 17:55:02

 

SPACE WEATHER
NOAA Forecasts

 

Updated at: 2017 Mar 25 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: activeminor stormsevere storm

Updated at: 2017 Mar 25 2200 UTC

Mid-latitudes

0-24 hr

24-48 hr

ACTIVE

20 %

40 %

MINOR

10 %

25 %

SEVERE

05 %

10 %

High latitudes

0-24 hr

24-48 hr

ACTIVE

15 %

15 %

MINOR

20 %

20 %

SEVERE

30 %

30 %