Signal self-adaptive interception method and system of solar radio observation system

A solar radio and observation system technology, applied in the field of signal processing, can solve the problems of large truncation error, unfavorable calibration, and increase the difficulty of data processing of the solar radio observation system, so as to achieve the effect of improving sensitivity and measurement accuracy, and improving sensitivity

Active Publication Date: 2020-11-13
SHANDONG UNIV
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Problems solved by technology

[0008] However, the inventors have found that in the existing truncation methods, direct truncation will produce a large truncation error; the compensation truncation method has a fixed number of truncation bits, so it has limitations in the observable power range; and based on the maximum The adaptive truncation method of absolute value cumulative average and grid comparison can realize the change of the range of observation power, but this method requires the observed signal to have certain characteristics, and different truncations are performed in sections, which is not conducive to the solar radio observation system The calibration of the observation signal value affects the later analysis of the spectrum data; the truncation after the introduction of the Dither signal increases the noise source of the observation signal and increases the difficulty of data processing in the later stage of the solar radio observation system

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  • Signal self-adaptive interception method and system of solar radio observation system

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Embodiment 1

[0034] The solar radio observation system studies solar activity phenomena through the observation and analysis of solar spectrum data. Solar radio includes three states, namely quiet solar radio, solar slow-changing radio and solar radio burst, solar radio burst and quiet solar radio The energies in the two states are different. Different frequencies and types of bursts have different energy multipliers compared with the calm state. For example, type II bursts have very high intensity, usually exceeding the quiet solar radio radiation by 100 to 1000 times.

[0035] like figure 1 The signal processing flow of the traditional solar radio observation system is shown, including: after the antenna receives the solar radio observation signal, the analog front-end performs amplification, filtering, mixing and other processing, and then the ADC converts the processed analog signal into a digital signal and transmits it to the FPGA In the FPGA, various digital signal processing such ...

Embodiment 2

[0054] This embodiment provides a signal adaptive truncation system of a solar radio observation system, including:

[0055] Initial module for setting initial truncation and comparison thresholds based on observed signals during quiet solar radio hours;

[0056] The processing module is used to take the average value of the observation signal of the solar radio burst time period after the maximum absolute value cumulative average processing as the upper limit value of the solar energy of the current time period;

[0057] The adjustment module is used to adjust the current truncation bit according to the comparison result of the solar energy upper limit value and the comparison threshold, so as to obtain the effective data bits required by the solar radio observation system, so as to observe the solar radio.

[0058] It should be noted here that the above-mentioned modules correspond to steps S1 to S3 in Embodiment 1, and the examples and application scenarios implemented by t...

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Abstract

The invention discloses a signal self-adaptive interception method and system of a solar radio observation system. The method comprises the following steps: setting an initial interception and a comparison threshold value according to an observation signal when the sun radiates quietly; taking an average value of the observation signals in the solar radio burst time period after maximum absolute value cumulative average processing as a solar energy upper limit value of the current time period; and according to a comparison result of the upper limit value of the solar energy quantity and the comparison threshold, adjusting the digit of the current interception bit to obtain an effective data bit required by the solar radio observation system so as to observe the solar radio. According to the energy difference, observed by a solar radio observation system, between a quiet solar radio state and a solar radio burst state, cut-off changes are controlled by comparing the upper limit value ofsolar energy in the current time period with a threshold value, so that high-precision observation of solar signals with different intensities is realized.

Description

technical field [0001] The invention relates to the technical field of signal processing, in particular to a signal adaptive truncation method and system for a solar radio observation system. Background technique [0002] The statements in this section merely provide background information related to the present invention and do not necessarily constitute prior art. [0003] The internal truncation methods of FPGA mainly include direct truncation, compensation truncation and adaptive truncation. Direct truncation means directly retaining the required effective data bits and directly discarding the remaining data bits. This method occupies the least resources and is simple to implement. It is the most commonly used truncation method when FPGA performs digital signal processing; but this method will generate truncation errors. , the data truncation error in digital signal processing is caused by the approximation method after truncation. For positive and negative numbers, the...

Claims

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Application Information

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Patent Type & Authority Applications(China)
IPC IPC(8): G06K9/00
CPCG06F2218/02
Inventor 严发宝刘洋尚自乾徐珂武昭苏艳蕊路光陈耀
Owner SHANDONG UNIV
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