Kopsavilkums
We analyze calibration errors that occur during the single-dish observations at the Irbene RT-32 radio telescope when calibration is done using noise diode. Only frequencyswitched mode of spectral line observations is considered. The purpose of the article is to find possible values of noise diode temperature Tcal and period of switching oscillator frequency 2tq. For this, we have analyzed the formula for calculating the antenna temperature of the source. It is shown that noise diode temperature affects the standard deviation of source antenna temperature σTs and the error of source antenna temperature δTs caused by instability of system temperature. tq affects the stability of the characteristics of the receiving system. In this article, the dependencies between Tcal, tq, σTs and δTs were found and analyzed. Based on these dependencies, possible values of Tcal and tq are found.
| Oriģinālvaloda | Angļu |
|---|---|
| Lapas (no-līdz) | 23-38 |
| Lapu skaits | 16 |
| Žurnāls | Astronomical and Astrophysical Transactions |
| Sējums | 32 |
| Izdevuma numurs | 1 |
| Publikācijas statuss | Publicēts - 2020 |
| Ārēji publicēts | Jā |
Nospiedums
Uzziniet vairāk par pētniecības tēmām “Estimation of errors at the calibration of spectral data at the irbene RT-32 radio telescope”. Kopā tie veido unikālu nospiedumu.Citēt šo
- APA
- Author
- BIBTEX
- Harvard
- Standard
- RIS
- Vancouver