A four-parameter model which assumes a Gaussian dependence of both temperature and pressure on distance from center is used to fit the compact part of coronal active regions as observed in X-ray photographs from a rocket experiment. The four parameters are the maximum temperature TM, the maximum pre
An investigation of the structure of coronal active regions
โ Scribed by J. H. Parkinson
- Publisher
- Springer
- Year
- 1973
- Tongue
- English
- Weight
- 333 KB
- Volume
- 28
- Category
- Article
- ISSN
- 0038-0938
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โฆ Synopsis
The temperature and density structure of a 'typical' coronal active region is deduced from X-ray observations of several active regions. Observations of the limb transits of three regions from OSO-5 indicate that the X-ray emission originates between 2 x 104 km and 1.5 โข 105 km. An emission measure-temperature distribution is deduced from high resolution X-ray spectra obtained with a rocket observation of two similar regions. These observations are combined to give a model of a 'typical' active region, the temperature varying from 2 to 6 โข 106 K with corresponding densities between 2 โข 109 and 101~ cms -8.
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