STATISTICALLY DERIVED FLARING CHROMOSPHERIC-CORONAL DENSITY STRUCTURE FROM NON-THERMAL X-RAY OBSERVATIONS OF THE SUN
نویسندگان
چکیده
منابع مشابه
Chromospheric magnetic field and density structure measurements using hard X-rays in a flaring coronal loop
Aims. A novel method of using hard X-rays as a diagnostic for chromospheric density and magnetic structures is developed to infer sub-arcsecond vertical variation of magnetic flux tube size and neutral gas density. Methods. Using Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) X-ray data and the newly developed X-ray visibilities forward fitting technique we find the FWHM and cent...
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ژورنال
عنوان ژورنال: The Astrophysical Journal
سال: 2010
ISSN: 0004-637X,1538-4357
DOI: 10.1088/0004-637x/721/2/1933