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2001 SPACE SCIENCE VIDEOTAPES

Tape Title

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Synopsis

2001 TOTAL SOLAR ECLIPSE G01-041A 06/21/01 00:22:11 Few people ever get the opportunity to see a total eclipse of the Sun. It only happens on the average of once every 400 years for any given spot on the Earth's surface and lasts only for one to two minutes. On June 21, 2001, and on the day of the summer solstice, this natural phenomenon will be visible within a very narrow path that begins in the Southern Atlantic Ocean and ending in the Indian Ocean. The total eclipse is not only beautiful to look at, but it provides a unique view of the Sun's outer atmosphere called the corona. Eclipses are so useful in helping us study the Sun that scientists built special cameras onboard the SOHO spacecraft to create a continuous artifical eclipse. From the unique vantage point in space, scientists have been able to monitor the explosions on the Sun that can impact us here on Earth.

TAPE CONTENTS:

ITEM (1):
 a) 
Solar Eclipse June 21, 2001
Courtesy: NASA / Exploratorium  

  b)  Eclipse Animations
 1.      The animation shows the path of the 
Moon's shadow on the Earth and illustrates the coronal flash that 
occurs when the eclipse reaches totality

2.      Global Image of the Path Animation

3.      Percentage of Coverage and Path Animation and Stills  

Courtesy: NASA 
  
ITEM (2): Aruba Eclipse of 1998 - These images were taken during the eclipse of February 26, 1998, as seen by scientists and students in Aruba. The images were produced as part of an interactive educational web cast produced by the Exploratorium and NASA's Sun-Earth Connection Educational Forum.

Courtesy: Exploratorium/NASA


ITEM (3): Satellite Views - Total Solar Eclipse From February 26, 1998 - This time-lapse sequence shows the shadow of the Moon as it first touches the Earth in the Pacific Ocean about 2000 miles south of the Hawaiian Islands. It then raced along the Pacific, over northern South America and across the Caribbean Sea before exiting in the Atlantic about 600 miles west of Morocco. The time-lapse image sequence is taken from the NOAA/National Weather Services Geostationary Operational Environment Satellite (GOES) 10. The sequence was enhanced and rendered at NASA Goddard Space Flight Center's Laboratory for Atmospheres. Courtesy: NASA/NOAA
ITEM (4): A Continuous Eclipse From a Million Miles in Space - The Large Angle and Spectrometric Coronograph onboard the SOHO (Solar and Heliospheric Observatory) satellie creates an artificial eclipse by using an occulting disk to block light coming from the Sun in order to see the tenuous region around the Sun called the corona. Note the intense activity captured in this time-lapse sequence from April 2001. The bright object that traverses the screen is the planet Mercury. Courtesy: NASA
ITEM (5): Solar Max/Solar Minimum Comparision - The Sun has been at its peak of its eleven-year cycle of activity. This is called the solar maximum and is the 2-3 year period when the Sun's activity is most complex and turbulent. Note the dramatic changes in the Sun from the solar minimum in 1996 to the solar maximum in 2000. These images were captured by the Solar and Heliospheric Observatory (SOHO) satellite, Extreme Ultraviolet Telescope (EIT) camera Courtesy: NASA
ITEM (6): Coronal Mass Ejection Animation - This animation depicts a powerful coronal mass ejection or CME, in which large explosions spew billions of tons of electrified gase into space, sometimes towards Earth, at speeds up to two million miles per hour. This event, known as space weather, can trigger major disturbances in Earth's magnetosphere.
   Courtesy:  NASA
ITEM (7): Summer Solstice Animation - Teh solar eclipse of 2001 falls on the day of the Summer Solstice; the longest day of the year when the Sun has climbed to its highest point in the sky. The four seasons of summer, fall, winter and spring, and the length of daylight changes, because the Sun's path through the sky is a result of the Earth's tilted axis. This tilt causes different parts of the globe to become oriented towards the Sun at diferent times of the year. Thus, summers are warming warmer because the days are longer, and the Sun's rays hit the Earth at a more direct angle.
Courtesy:  NASA
ITEM (8): Effects of Solar Storms -
a)  Power grids may fail 
 b) 
Spacecraft can be damaged, radio and satellite communications may be 
disrupted 
 c)  Data can become distorted as in this LASCO 
image 
 d)  Beautiful auroras

  
   Courtesy:  NASA
ITEM (9): SOHO Animation - The Solar and Heliospheric Observatory (SOHO) spacecraft operates at a special vantage point about one million miles out in space between the Sun and the Earth.
 
Courtesy:  NASA
ITEM (10): Eclipse Viewing Tips - This short video clip with NASA Astronomer Dr. Fred Espanek, gives viewers various eclipse viewing tips. It is VERY IMPORTANT to never attempt to observe the partial phases of any eclipse with the naked eye as permanent damage to the eyes can occur.
 Courtesy:  NASA
ITEM (11): Miscellaneous "B" Roll -
 a)  Solar scientists at work 
 b)  Satellites in Space Animation 
 c)  Leck 
Telescope in Hawaii 
 d)  SVS Visual of the Earth 
 e)  SVS visual of the United States 
 f)  SVS 
visual of Africa  
 Courtesy:  NASA
ITEM (12): Interview Excerpts With Fred Espenek, Astrophysicist, NASA/GSFC
 Courtesy:  NASA
ITEM (13): Reporters Package
 Courtesy:  NASA
 
 

[Partial Eclipse Movie][Shadow Movie] [20% Eclipse Path Movie]

NOTE: The material advertised on this page is a "Video File" and is strictly recommended for the media and production companies. This is NOT a finished production and contains no narration.

 

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