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First Steps Towards K Indices from South Atlantic Observatories: Port Stanley Observatory

机译:南大西洋天文台向K指数迈出的第一步:斯坦利港天文台

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References(13) To enhance the quality and near real time production of K-based planetary magnetic activity indices, such as am, and longitude-sector indices, aλ, there is a requirement for local three-hourly K index values from the South Atlantic observatory at Port Stanley. We describe the computer algorithm used to estimate the solar regular variation, SR, and techniques used to establish the parameters required to derive the K indices. We analyse the results by comparing the distributions of K values with observatories at similar geomagnetic latitude and thus with likely similar levels of geomagnetic activity. We also look for biases by comparing the indices directly to those from nearby observatories. Both sets of results show a good overall agreement. However adjustment of input parameters will be necessary if improved agreement with the indices from the other observatories is required.
机译:参考文献(13)为了提高基于K的行星磁活动指数(例如am和经度扇区指数aλ)的质量和近实时性,南大西洋地区需要每小时三小时的本地K指数值斯坦利港的天文台。我们描述了用于估算太阳规律变化,SR的计算机算法,以及用于建立导出K指数所需参数的技术。我们通过将K值的分布与类似地磁纬度的观测站进行比较,从而对可能具有相似地磁活动水平的观测结果进行分析。我们还通过直接将索引与附近天文台的索引进行比较来寻找偏差。两组结果均显示出良好的整体一致性。但是,如果需要与其他天文台的索引更好地达成一致,则必须调整输入参数。

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