High resolution X-ray spectroscopy of comets

Statistics – Computation

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Scientific paper

Remote plasma diagnostics is an important tool for astrophysical studies. In order to fully utilize its power, a detailed knowledge of the properties of the atomic processes which give rise to the observable emission is essential. However, retrieving this information to the necessary accuracy, either by theoretical computation or by laboratory experiments, is often a challenging task. In this context, the X-ray emission of comets provides a welcome opportunity for checking and improving our knowledge of basic atomic quantities. Cometary X-ray emission is the result of charge exchange processes between highly ionized heavy atoms in the solar wind and neutrals in the cometary coma - a textbook example of an interaction between a highly ionized plasma and cold gas far from thermal equilibrium, which takes place in a huge, clean 'laboratory' fairly nearby. Thus, cometary X-ray spectra do not only provide information about the elusive properties of the heavy ion content of the solar wind over the solar cycle and in three dimensions, but are also valuable for plasma diagnostics in general.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

High resolution X-ray spectroscopy of comets does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with High resolution X-ray spectroscopy of comets, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High resolution X-ray spectroscopy of comets will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1192312

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.