High Energy K X-Ray Satellites

High Energy K X-Ray Satellites

Zewdu Alamineh Fetene

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Abstract

This study focus on High Energy K X-ray satellites which are a particular category of characteristic X-ray. They are emitted when an atom that has undergone multiple ionization de excites. Simultaneous single ionization in the K-shell and multiple ionization in the L-shell gives rise to K α X-ray satellites. These can be studied only by high energy resolution instruments like crystal spectrometry. Experimental investigations were carried out in this field by several workers using photon, electron, and ion excitation modes. The theoretical models to predict their energies and intensities were developed. And also this work can show a clear discrepancy between theoretical and experimental results in the case of satellites formation from different shells. In case of experimental instrumentation, WDXRF is the most accurate for determining the energy and intensity of X-ray satellites. The basic source of data was literature done by different scholars.

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Funding

No external funding was declared for this work.

Conflict of Interest

The authors declare no conflict of interest.

Ethical Approval

No ethics committee approval was required for this article type.

Data Availability

Not applicable for this article.

How to Cite This Article

Zewdu Alamineh Fetene. 2015. \u201cHigh Energy K X-Ray Satellites\u201d. Global Journal of Science Frontier Research - A: Physics & Space Science GJSFR-A Volume 15 (GJSFR Volume 15 Issue A2).

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GJSFR Volume 15 Issue A2

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Journal Specifications

Crossref Journal DOI 10.17406/GJSFR

Print ISSN 0975-5896

e-ISSN 2249-4626

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GJSFR-A Classification FOR Code: 090108

Submission ReceivedFebruary 5, 2015
Peer Review Double Blind
Handling Editor
Accepted March 3, 2015
Published March 17, 2015

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v1.2

Issue date

May 6, 2015

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Article Matrices

Total Score: 71

Country: Ethiopia

Subject: Global Journal of Science Frontier Research - A: Physics & Space Science

Authors: Zewdu Alamineh Fetene (PhD/Dr. count: 0)

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