J/A+A/491/561       Plasma filling factor of coronal bright points (Dere+, 2008)

The plasma filling factor of coronal bright points. Coronal bright points. Dere K.P. <Astron. Astrophys. 491, 561 (2008)> =2008A&A...491..561D 2008A&A...491..561D
ADC_Keywords: Sun Keywords: Sun: corona Abstract: We determine the volumetric plasma filling factor of coronal bright points. Rastered spectra of the regions of the quiet Sun were recorded by the Extreme ultraviolet Imaging Spectrometer (EIS) during operations with the Hinode satellite. Calibrated intensities of Fe XII lines were obtained and images of the quiet corona were constructed. From the imaged spectra, the emission measures and geometrical widths of coronal bright points were obtained. Electron densities were determined from density-sensitive line ratios. A comparison of the emission measure and bright point widths with the electron densities yielded the plasma-filling factor. Description: The data describe the observed and derived properties of a set of corona l bright points. The labeling allows the reader to correlate the data in Table 2 with their images in Figures 2 and 3. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 38 62 Observed and derived properties of a set of coronal bright points -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 A3 --- Label Bright point label 7- 9 A3 --- Raster Raster label 11- 18 E8.3 mW/m2/sr Int Bright point intensity 20- 24 F5.2 cm-3 LogNe Log (decimal) of the electron density 26- 30 F5.2 arcsec Width Observed bright point width 32- 38 E7.2 --- FillFactor Volumetric plasma filling factor -------------------------------------------------------------------------------- Acknowledgements: K.P. Dere, kdere(at)gmu.edu
(End) K.P. Dere [George Mason University], Patricia Vannier [CDS] 30-Sep-2008
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line