Abstract

AbstractThe geomagnetic Kp index is one of the most extensively used indices of geomagnetic activity, both for scientific and operational purposes. This article reviews the properties of the Kp index and provides a reference for users of the Kp index and associated data products as derived and distributed by the GFZ German Research Centre for Geosciences. The near real‐time production of the nowcast Kp index is of particular interest for space weather services and here we describe and evaluate its current setup.

Highlights

  • The near real-time production of the nowcast Kp index is of particular interest for space weather services and here we describe and evaluate its current setup

  • Geomagnetic variation consists of quiet variation, which is regular in appearance and mostly of solar electromagnetic radiation origin, and geomagnetic disturbance, which is irregular in appearance and mostly driven by the solar wind

  • The concept of K-variation, referred to as geomagnetic activity or disturbance, predates the discovery of the solar wind and historically, K-variation was seen as the effect of 'solar particle radiation' (e.g. Bartels, 1957a)

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Summary

Introduction

Geomagnetic variation consists of quiet variation, which is regular in appearance and mostly of solar electromagnetic radiation origin, and geomagnetic disturbance, which is irregular in appearance and mostly driven by the solar wind. Kp is capped to a certain value (i.e., 9) for events with extreme geomagnetic disturbance In this regard, new Kp-like but open-ended indices with 30 and 60 min time resolution have been developed as part of the European Union (EU) project Space Weather Atmosphere Models and Indices (SWAMI; Jackson et al, 2020). We use italics for the letters denoting indices, we skip the hyphen in the index names (we use, e.g., “K index” and “Kp index”)

Derivation of K
Associations and Institutions Involved
Changes of Rules Affecting K and Kp
Introduction of Algorithm-Derived K Indices
Changes to the Network
Fundamental Properties of Kp
Distance of the Kp-Stations to the Auroral Zone
Nowcast Kp at GFZ
Summary and Conclusions
Findings
Data Availability Statement
Full Text
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