The words "Reuven Ramaty High Energy Solar Spectroscopic Imager" are a
mouthful and quite intimidating to someone not familiar with the terminology.
Basically, RHESSI took
images and spectra of the Sun in the high energy portion of the electromagnetic
spectrum: X-rays and Gamma-rays. The features of the Sun that create these high
energy emissions, primarily solar flares, occur in the Sun's outer layers,
called the corona. There are still many unanswered questions about how solar flares work, which this
mission is currently exploring.
These nuggets display scientific results related to RHESSI observations on the Web. The nuggets are in principle helpful and explanatory, with links for further information, ideally written in such a way that any technically competent person can follow them. New nuggets are posted as they become available. Go to the nuggets page by clicking here. RHESSI can also study astronomical objects other than the Sun.
In order to understand the RHESSI mission, it's important to know something about
the scientific topics below. Each link will take you to a list of
resources that will provide you with background information helpful in understanding the
RHESSI mission. Our materials and links will have easier, more general
sources of information listed first (some of which are intended for students,
but are fine for adults), and more difficult and specific sources will follow.
RHESSI Science Nuggets
Non-Solar Science
For more information about what non-solar science
RHESSI can do, click
here.
Last updated 01/29/2010 © UC Regents