en:data-outputs
Differences
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en:data-outputs [2017/01/05 18:33] – [Spectral records description] fluktuacia | en:data-outputs [2019/04/24 13:39] – [Records generation] fluktuacia | ||
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====== Bolidozor data outputs ====== | ====== Bolidozor data outputs ====== | ||
- | The data produced by the detection stations are sent to the [[en: | + | Data produced by detection stations are sent to the [[en: |
There are several types of files among the data records: | There are several types of files among the data records: | ||
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- | JS9 web viewer enables viewing only the first two records. A specialised application is required to see the rest of the records. The description of how the data files are sorted can be found on [[en: | + | JS9 web viewer enables viewing only the first two types of records. A specialised application is required to see the rest of the records. The description of how the data files are sorted can be found at [[en: |
===== Records generation ===== | ===== Records generation ===== | ||
- | The records are generated by a software running on the detection stations. Majority of data are produced by [[en: | + | The records are generated by a software running on detection stations. Majority of data are produced by [[en: |
===== Spectral records description ===== | ===== Spectral records description ===== | ||
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The lower portion of the record shows a head-echo - a signal, always beginning at higher frequencies than the meteor trail. Head-echo is a signal formed by the reflection from an ionised plasma at the front of the meteor during its fly-by. It is a moving object whose signal (due to a considerable speed up to tens of km/s) has a large doppler shift that passes through zero (at the point of the shortest sum of distances transmitter -> meteor -> receiver). Some meteors lack head-echo signal as the geometry of their fly-by does not allow the reflection to the receiver station. On the other side, other meteors have a head-echo extending even behind the point of the zero doppler shift. | The lower portion of the record shows a head-echo - a signal, always beginning at higher frequencies than the meteor trail. Head-echo is a signal formed by the reflection from an ionised plasma at the front of the meteor during its fly-by. It is a moving object whose signal (due to a considerable speed up to tens of km/s) has a large doppler shift that passes through zero (at the point of the shortest sum of distances transmitter -> meteor -> receiver). Some meteors lack head-echo signal as the geometry of their fly-by does not allow the reflection to the receiver station. On the other side, other meteors have a head-echo extending even behind the point of the zero doppler shift. | ||
- | Following the area of the head-echo signal there is an area of a static reflection from the meteor trail. Its intensity varies in time. The change in intensity is caused by a progressive recombination of the plasma trail of the meteor and the periodic changes in intensity are caused by a space modulation of the radar signal. | + | Following |
+ | |||
+ | ==== FITS header content ==== | ||
+ | |||
+ | |||
+ | SIMPLE | ||
+ | BITPIX | ||
+ | NAXIS | ||
+ | NAXIS1 | ||
+ | NAXIS2 | ||
+ | EXTEND | ||
+ | ORIGIN | ||
+ | DATE = ' | ||
+ | DATE-OBS= ' | ||
+ | CTYPE2 | ||
+ | CRPIX2 | ||
+ | CRVAL2 | ||
+ | CDELT2 | ||
+ | CTYPE1 | ||
+ | CRPIX1 | ||
+ | CRVAL1 | ||
+ | CDELT1 | ||
+ | END | ||
+ | |||
+ | |||
+ | |||
+ |
en/data-outputs.txt · Last modified: 2019/04/25 15:33 by fluktuacia