The HESSI Challenge:

Making High Energy X-ray Pictures of the Sun



Rotating Grids



Human beings have limited sensitivity ranges in their five senses. For example, dogs have more sensitive noses for detecting faint odors. Bees can see in ultraviolet light while humans can not. Bats and dolphins can hear at much higher frequencies than humans.

In order to extend the senses, humans have made devices that expand our sensitivity ranges and report back in ways that we can perceive. HESSI is a device that attempts to extend our vision to the most energetic X-ray and gamma ray regions of the electomagnetic spectrum. The acronym HESSI stands for High Energy Solar Spetroscopic Imager. Scientists hope to give us X-ray pictures of the inner structrures of solar flares. [ This is a link to a previous mission proposal called HESI.] To understand the problems of achieving that goal click links 1. through 5. below:




Links to the Rest of the Story


1. The Human Eye

_2. Shorter Wavelengths of Light:
Ultraviolet (UV)

3. X-Rays: Even Shorter Wavelengths

4. Hard X-Rays and Gamma-Rays

5. How Are Hard X-Ray Images Made?





Web Author: George F. Smeller e-mail to: smeller@hesperia.gsfc.nasa.gov

Web Author: Dr. Brian Dennis e-mail to: dennis@stars.gsfc.nasa.gov

responsible NASA official:Dr. Edward Schmahl
Laboratory for Astronomy and Solar Physics. NASA/Goddard Space Flight Center
e-mail to: schmahl@hesperia.gsfc.nasa.gov



Links to other Goddard Web Sites


The Cybrary is a site which lists all known current mission related web sites at Goddard. They are listed alphabetically and under general categories.



Last revision was August 22, 1997