Long term drifts in baselines of ground magnetic observatories. (May 2017)

• Record Type: Journal Article
• Authors: Iype, Anil; Deshmukh, A.T.; Veenadhari, B.
• Is Part Of: Measurement. Volume 102(2017)
• Page Start: 33
• Page End: 41
• Publication Date: 2017-05
• Subjects: Long term baseline stability -- Magnetic observatory -- Gradient field variation -- Baseline drift; Weights and measures -- Periodicals; Measurement -- Periodicals; Measurement; Weights and measures; Periodicals; 530.8
• DOI: 10.1016/j.measurement.2017.01.047
• Languages: English
• ISSNs: 0263-2241

Abstract

Highlights: The data quality of a magnetic observatory can be judged by the straightness of its baseline. Spatial magnetic gradient in the observatory premises need not be a constant and can vary over time. This variable gradient can introduce an error in the recorded data in the form of baseline drift. dF, dI are the difference in total field F, Inclination between the variometer room and absolute room. The baseline drift can be corrected by a formula which includes the terms dF and dI. Abstract: The stability of baseline is the most important criterion for evaluating the data quality of a ground magnetic observatory. Theoretically, a baseline should be a straight line, provided, there are no error factors affecting the absolute instruments, the variometer and the observational procedure. But in practice, we observe that the baselines are affected by some errors in the form of random errors and long term baseline drifts. It is known that temperature, pier tilts, aging of electronic components, etc. can affect the long term stability of baselines, but in this paper we discuss a new type of error which affects the baseline in the form of long term drifts due to the variation in the gradient field between the absolute room and the variometer room. Even though, a site is selected with the least magnetic gradient for the establishment of an observatory, in many cases, it is found that the magnetic gradient patterns are not permanent and changes over the time. This slow gradient changes can distort the actual temporal magnetic variations and thus affecting the purity of data recorded at a geomagnetic observatory. We have analytically shown that an ideal baseline has to be a horizontal straight line and the RHS of the fundamental equation of an observatory should be a constant. We have further shown that baseline instabilities are caused by variation in gradient field between the absolute and variometer pillars in addition to the measurement errors from absolute observations and variometer recording. This variation in the gradient field causes long term drifts in baselines. We have derived the correction factor which can filter out the signals arising out of variation in the gradient field. Finally we present how far the data quality can be improved by applying this correction.