X-Ray Spectroscopy of the Sun in Time: a Study of Coronal Physics of Solar-Type Stars at Different Ages

Details X-Ray Spectroscopy of the Sun in Time: a Study of Coronal Physics of Solar-Type Stars at Different Ages X-Ray Spectroscopy of the Sun in Time: a Study of Coronal Physics of Solar-Type Stars at Different Ages

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000cxo..prop..556g&link_type=abstract

Chandra Proposal ID #02200379

Physics

Chandra Proposal Id #02200379

Scientific paper

A comprehensive project on the ``Sun in Time'' has been set up over the last few years, aiming at studying the physical properties, phenomenology, and fundamental parameters of a solar-type star (G0-5 V) throughout its main-sequence life. We propose a spectroscopic study with the LETGS/HRC-S to investigate in detail coronal temperature and emission measure structuring, coronal densities, elemental abundances, possible mass flows, and variability in selected targets. We propose three stars regularly distributed in log(rotation period) over the possible range, to be complemented by one GTO target that we will have access to. This will provide a gross overview over the range of solar-type coronae. It is anticipated that additional targets will be requested in later AOs.

Affiliated with

Also associated with

No associations

Rating

X-Ray Spectroscopy of the Sun in Time: a Study of Coronal Physics of Solar-Type Stars at Different Ages 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 X-Ray Spectroscopy of the Sun in Time: a Study of Coronal Physics of Solar-Type Stars at Different Ages, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and X-Ray Spectroscopy of the Sun in Time: a Study of Coronal Physics of Solar-Type Stars at Different Ages will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1525088