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Rachel Weintraub
Associate TV Producer
Goddard Space Flight Center
301.286.0918

Dr. Tom Bridgman

Data Visualization Specialist
Goddard Space Flight Center

Walt Feimer

Animation Specialist
Goddard Space Flight Center  

 

 

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February 2003 - (date of web publication)


SCIENCE HIGHLIGHTS FROM NASA'S SUN-EARTH CONNECTION

A Year of Solar Fluctuations and New Explorers

 

image of the Sun

Image 1

 

2002 marked a period of surprises from our great star that should have been quieting down after its high point of the solar cycle of activity. Rather it was marked with flares and coronal mass ejections, comet sightings, a peak sunspot count last seen in 2000 and three new solar explorers.


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.

SUPER: 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.

SUPER: 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.

SUPER: 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.

SUPER: 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).

SUPER: 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.

SUPER: NASA

 


Breaking News

What is a CME?

 

coronal mass ejection

Image 8

 

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.

SUPER: NASA

 

Solar Fireworks

 

solar sunspots

Image 9

 

A group of sunspots measuring 15 Earths across produced some major solar activity the week of July 15 in the form of X-class flares, the most powerful designation.

SUPER: NASA / ESA


 


Spotting the Solar Fireworks

 

view of the Sun

Image 10

 

Sunspot group 'AR 30' (for "Active Region") located near the middle of the Sun had been producing flares and other solar events since July 12; here they stretch 15 Earth-diameters from end-to-end.


SUPER: NASA / ESA

 

A Solar Grand Slam

 

still of a solar flare

Image 11

 

As Tiger Woods attempted a golf grand slam in July, the Sun delivered a show of its own with four powerful X-class flares in just eight days.

SUPER: NASA / ESA

 

 

The First 'Keyhole' CME

 

"keyhole" coronal mass ejection

Image 12

 

"We've observed thousands of CMEs, but none ever looked like this one," said one scientist. A CME in October appeared to have a keyhole in the center of the explosion.

SUPER: NASA / ESA

 

 

 

A 'Corkscrew' CME

 

"corkscrew" shaped mass ejection

Image 13

 

This remarkable October CME vaguely resembles a corkscrew with twisted lines bursting from the Sun.

SUPER: NASA / ESA

 

 

 

A Prominent Prominence

 

image of a solar prominence

Image 14

 

Prominences occur when dense plasma at the solar surface becomes trapped in magnetic fields that are propelled high into the corona, or outer atmosphere of the Sun.

SUPER: NASA / ESA

 

 

 

Spectacular Solar Loop

 

looping solar prominence

Image 15

 

This prominence was large enough to encompass 40 Earths and likely reached about 107,000 degrees F, considerably cooler than the Sun's atmosphere of 1 million degrees.

SUPER: NASA / ESA

 

 

 

Solar Comet Hunter

 

SOHO catching a comet

Image 16

 

The SOHO spacecraft spotted its 500th comet on August 12, making it the most prolific comet hunter in history only six years after its launch.

SUPER: NASA / ESA

 

 

 

Dial-Up Comet Spotting

 

comet watching with SOHO

Image 17

 

In April 2002, an amateur astronomer in China discovered his 14th comet via real-time images of the Sun on the Internet in time for National Astronomy Day.

SUPER: NASA / ESA







Other Comet Discoveries

 

Comet Machholz passing by the Sun

Image 18

 

In January, Comet Machholz passed by the Sun at the same time a CME erupted on the opposite side, all captured by SOHO. Venus is also visible in the lower right.

SUPER: NASA / ESA

 

 

 

Alternate View of An Eclipse

 

SOHO sees the total solar eclipse

Image 19

 

The December 4, 2002 total eclipse was the last of the year. It is shown here in an image of the Sun from SOHO superimposed on a photograph of the eclipse.

SUPER: NASA / ESA / Jay Pasachoff / Williams College Eclipse Expedition

 

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