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Estimates of Densities and Filling Factors from a Cooling Time Analysis of Solar Microflares Observed with RHESSI
Estimates Densities Filling Factors Solar Microflares
2011/10/12
We use more than 4,500 microflares from the Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) microflare data set (Christe et al., 2008, Ap. J., 677, 1385) to estimate electron densities a...
Study of Microflares through SOXS Mission
X-ray detectors coronal 100 ps solar flares microflares hard X-ray emission
2010/9/17
We present a study of 10 microflares observed in 4–30 keV by SOXS mission simultaneously with Hα observations made at NAOJ,Japan during the interval between February and August 2004. The X-ray and Hα ...
Microflares as Possible Sources for Coronal Heating
Solar flares microflares Fe-line feature coronal heating
2010/9/16
We present a preliminary study of 27 microflares observed by Solar X-ray Spectrometer (SOXS) mission during July 2003 to August 2006. We found that all 27 microflares show the Fe-line feature peaking ...
Study of Microflares through SOXS Mission
X-ray detectors coronal 100 ps solar flares microflares hard X-ray emission
2009/5/7
We present a study of 10 microflares observed in 4-30 keV by SOXS mission simultaneously with Hα observations made at NAOJ, Japan during the interval between February and August 2004. The X-ray a...
Microflares as Possible Sources for Coronal Heating
Solar flares: microflares, Fe line feature coronal heating
2009/5/6
We present a preliminary study of 27 microflares observed
by Solar X-ray Spectrometer (SOXS) mission during July 2003 to August
2006. We found that all 27 microflares show the Fe-line feature peakin...