确定和测量C/A代码相互关系对跟踪的真实影响-在SBAS地质测量中的应用

L. Lestarquit, O. Nouvel
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引用次数: 7

摘要

本文将回顾由于相互关联(XC)而产生代码跟踪偏差的必要条件,重点关注当前的C/ a代码,并表明对于来自GPS卫星的信号确实不太可能,但对于来自具有低动态的卫星的信号,例如SBAS或IGSO卫星,可能会发生这种情况。对SBAS进行了测量活动,并发现了一个令人惊讶的结果:尽管测量的误差包线符合理论,但误差的性质是有噪声的,而它应该是一个偏差。原因是这样的解释:这是由于载波相位抖动对SBAS测距信号。我们将回顾相互相关误差的物理性质。它与多径效应有很多相似之处。将详细说明发生XC错误的条件。它们是:多普勒碰撞,数据信息相似,和XC峰的存在。XC跟踪错误发生的情况将会详细说明。由于卫星的高多普勒信号,GPS信号几乎不可能被接收,但低运动的SBAS卫星更有可能被接收。对于WAAS, 2颗卫星的报文帧大部分时间是相关的,相关指数在0.8 ~ 1之间;对于EGNOS,报文有时是相关的,但大部分时间是不相关的,这取决于卫星是否同时广播相同的报文类型。为了使XC误差最大,必须同时接收消息符号。如果有一个符号移位,即2毫秒或600公里的相对代码延迟,那么接收到的符号就变得不相关了。这解释了XC误差只会发生在一个非常狭窄的地带,只有几百公里宽。此外,在这个条带内,当多普勒碰撞发生时,用户必须被定位在对应于XC函数峰值的位置。一个测试活动是在这个地带进行的。发现观测到的误差包络与预测误差相匹配,但注意到一个重要的载波相位抖动达到了几个载波周期。这导致XC误差偏差变为随机误差。这允许过滤掉XC误差与载波平滑。存在一个矛盾的情况:如果改善载波相位抖动异常,则XC误差将成为无法用载波平滑滤波的偏置。如果使用SBAS信号进行测距,在接收端可以考虑XC误差。有多种可能性,一种是在多普勒碰撞的情况下忽略码测量,另一种可能是用误差模型来纠正它。
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Determining and measuring the true impact of C/A code cross-correlation on tracking—Application to SBAS georanging
This paper will review the necessary conditions for having a code tracking bias due to cross-correlation (XC), focussing on the current C/A code, and show that it will be indeed very unlikely for signals coming from GPS satellites, but it can happen for signals coming from satellites having a low dynamic, such as SBAS or IGSO satellites. Measurement campaigns on SBAS have been made and a surprising result has been found: even though the measured error envelope complies with the theory, the nature of the error is noisy whereas it should have been a bias. The reason for this was explained: this is due to carrier phase jitter on the SBAS ranging signal. The physics of the cross-correltion error will be reviewed. It has many analogies with the multipath effect. The condition for XC errors to happen will be detailed. They are : Doppler collision, data message similitude, and presence of a XC peak. The situation in which XC tracking error happen will be detailed. There are almost impossible for GPS signal due to the satellite high Doppler, but more likely for SBAS satellites with low motion. For WAAS, the message frames of the 2 satellites are most of the time correlated with a correlation index between 0.8 and 1, for EGNOS the messages are sometimes correlated, but most of the timre not, depending on whether the same message type are broadcast at the same time by the satellites. The message symbol have to be received at the same time for the XC error to be maximum. If there is a one symbol shift, that is a 2 ms or a 600km relative code delay, then the received symbols becomes uncorrelated. This explains that XC error can happen only on a very narrow strip, a few hundred km wide only. Additionnaly, within this strip the user must be positioned in a place corresponding to a XC function peak when the Doppler collision happens. A test campaign was made inside this strip. The observed error envelope was found to match the predicted error, but it was noticed an important carrier phase jitter that reached several carrier cycles. This caused the XC error bias to be changed into a random error. This allow to filter out the XC error with carrier smoothing. There is a paradoxal situation : if the carrier phase jitter anomaly was improved, the XC error would become a bias that couln't be filtered with carrier smoothing. If SBAS signal shall be used for ranging, XC error could be taken into account at the receiver level. There are many possibilities, one could be to ignore code measurement in case of Doppler collision, another could be to correct it with an error model.
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