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Rachel Weintraub
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Dr. Tom Bridgman

Data Visualization Specialist
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Walt Feimer

Animation Specialist
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The Top Story Archive listing can be found by clicking on this link.

All stories found on a Top Story page or the front page of this site have been archived from most to least current on this page.

For a list of recent press releases, click here.

January 2004 - (date of web publication)


SCIENCE HIGHLIGHTS FROM NASA'S SUN-EARTH CONNECTION

The Flare That Got Everyone's Attention

 

image of the Sun

Image 1

 

In 2003 the Sun produced the most powerful flare ever seen. It was entering the quiet period of its 11-year cycle of activity, so scientists likened the event to a blizzard in the middle of summer. Large sunspots in late October/early November unleashed 11 flares in only 14 days -- equaling the total number observed during the previous year. The largest was ranked a record-breaking X-28; X-6 flares are considered large.


Star of the Show

Multi-mission view of the sun

 

Image 2

 

In this new view, images from 7 instruments on 3 separate satellites are combined in one frame. With so many coordinated spacecraft datasets and so many diverse assignments, this visualization is striking in that it lines up the data to provide a radical view of one solar event from sunspot to flare to the X-rays pinpointed on that flare to the CME billowing out into space.

Credit: NASA / ESA / LMSAL

Full-disk View

 

full disk view of the Sun

Image 3

 

Millions of miles away, CMEs from the Sun blast billions of tons of plasma into our magnetosphere with the potential to disturb space systems, power grids and communications.

Credit: NASA / ESA

 

 

Amazing Changing Sun

 

Sun in solar minimum and maximum

Image 4

 

Solar maximum is the 2-3 year peak period (2000-2001 marked the peak of this cycle) when activity is most complex and turbulent, and the space around Earth is most disturbed.

Credit: NASA/ESA

 

Fountains of Fire

 

Trace coronal loops on the Sun

Image 5

 

Close-up images reveal an active surface with coronal loops emerging and disappearing all over the Sun's surface and can span a length of about 250,000 miles, or about 30 times the diameter of Earth.

Credit: NASA / LMSAL


Sunspots

 

sunspot

Image 6

 

Sunspots appear dark because they are cooler than the solar surface and can last for weeks and can be as large as 80,000 km (over 6 planet Earths).

Credit: NASA / ESA

 

How Do Active Regions Form?

 

active regions on the Sun

Image 7

 

Peering beneath the surface of AR 9393 revealed regions comprised of many small magnetic structures that rise quickly from deep within the Sun.

Credit: NASA

 


Breaking News

What is the Aurora?

 

Earth's magnetic field

Image 8

 

Plasma from solar storms hit the Earth’s magnetic field, ejecting oxygen ions from upper atmosphere. The ions flow along Earth's field lines until pressure from solar wind stretches the field toard the night-side of the Earth like a rubber band and snaps back.

Credit: NASA

 

Why Do we See Reds in the Sky?

 

animation showing collisions of molecules

Image 9

 

.Collisions between fast-moving electrons and the oxygen and nitrogen in Earth’s upper atmosphere create aurora. The electrons from the magnetosphere transfer energy to the gases, making them “excited.” As they “calm down” and return to their normal state, they emit small bursts of energy in the form of light. Oxygen produces a greenish-yellow or red light; nitrogen generally gives off a blue light.

Credit: NASA


What Shields The Earth?

 

Earth's magnetic field

Image 10

 

Solar wind shapes and impacts Earth’s magnetic field. The magnetosphere extends out about 65,000 km (40,000 miles) on the Sun side, and more than ten times that distance on the opposite side, well beyond the Moon’s orbit.

Credit: NASA


Storm of the Solar Cycle (And More!)

What is a CME?

 

image of a coronal mass ejection

Image 11

 

The largest explosions in the solar system, CMEs launch up to 10 billion tons of ionized gas into space at speeds of one to two million miles an hour.

Credit: NASA

 

The One-Two Punch

 

image of a large flare

Image 12

 

On Oct. 28 spacecraft tracked an X-17.2 sized flare – the second largest ever observed by SOHO – and arrived early the next day, meaning it was unusually fast as well. That same day that one arrived, an X-10 flare set off another round of particles and another fast-moving CME.

Credit: NASA / LMSAL

 

The Record Breaking Flare

 

 

animated GIF of the flare from Nov. 4, 2003

Image 13

 

The same spot blasted off one more flare Nov. 4 as the Sun rotated away. This one was X-28, making it the most powerful X-ray flare ever recorded. Only part of the associated CME (traveling at 2300 km/second) was directed toward Earth, resulting in few aurora.

Credit: NASA / E

 

Polar Sees Aurora Arrival

 

 

The Polar spacecraft is currently flying around the south pole and saw this aurora form after a CME brushed past Earth. The Polar spacecraft is currently flying around the south pole and saw this aurora form after a CME brushed past Earth. The Polar spacecraft is currently flying around the south pole and saw this aurora form after a CME brushed past Earth.

Image 14

Click on each earth image above to view movie.

The same spot rotated back and hurled a CME into space resulting in aurora as far south as Florida on Nov. 20. The Polar spacecraft was flying around the South Pole and saw this aurora australis (also known as the Southern Lights).

Credit: NASA / University of Iowa


IMAGE Spacecraft Spots Glow

 

IMAGE spacecraft spotted a glow at the South Pole

Image 15

 

Also in the South Pole, the IMAGE spacecraft caught these views Nov. 20. This strong aurora australis reached above the island of Tasmania.


Credit: NASA / UC Berkeley

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