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Improved Data Handling Techniques for Spectrometer Data
| Content Provider | Semantic Scholar |
|---|---|
| Copyright Year | 2000 |
| Abstract | A mathematical method to improve resolution and select solar emission lines in spectrometer data is presented. The method depends upon non-linear averaging, numerical band-pass filtering, and second differences. Spectra representing scans of the solar emission intensity from 40 to 400 i are computed. Line intensities as low as 35 counts per second above background and separated by 0.4 i or more are detected. Computer programs for the GSFC direct coupled IBM 7050/7094 have been written to execute the algorithms developed and are presented. |
| File Format | PDF HTM / HTML |
| Alternate Webpage(s) | https://ntrs.nasa.gov/archive/nasa/casi.ntrs.nasa.gov/19650023761.pdf |
| Language | English |
| Access Restriction | Open |
| Content Type | Text |
| Resource Type | Article |
