Matzka, Jürgen; Bronkalla, Oliver; Kervalishvili, Guram; Rauberg, Jan; Yamazaki, Yosuke (2022): Geomagnetic Hpo index. V. 2.0. GFZ Data Services. https://doi.org/10.5880/Hpo.0002
Status
I N R E V I E W : Matzka, Jürgen; Bronkalla, Oliver; Kervalishvili, Guram; Rauberg, Jan; Yamazaki, Yosuke (2022): Geomagnetic Hpo index. V. 2.0. GFZ Data Services. https://doi.org/10.5880/Hpo.0002
This data publication includes the half-hourly Hp30 and ap30 indices as well as the hourly Hp60 and ap60 indices, collectively denoted as Hpo. This dataset is based on near real-time geomagnetic observatory data provided by 13 contributing observatories. It is derived and distributed by GFZ German Research Centre for Geosciences. When using the Hpo index, please cite this data publication as well as the accompanying publication Yamazaki et al. (2022), which serves as documentation of the Hpo.
The dataset is organised in yearly files, which, for the current year, are updated on a monthly basis. Typically, during the second week of a month, the data for the previous month is appended to the current year's file. The files are in ASCII files and start with header lines marked with # (hash).
The Hpo index was developed within the H2020 project SWAMI (grant agreement No 776287) and is produced by Geomagnetic Observatory Niemegk, GFZ German Research Centre for Geosciences. It derives from the same 13 geomagnetic observatories that also contribute to the Kp index (Matzka et al., 2021, https://doi.org/10.5880/Kp.0001). They are listed as contributors to this data publication.
With the introduction of the DOI for the Hpo index (Matzka et al, 2021, https://doi.org/10.5880/Hpo.0001), this DOI landing page and the associated HTTPS server linked to the DOI become the primary archive of Hpo (while the other established index distribution mechanisms at GFZ will be maintained in parallel). With the DOI, the dataset can grow with time, but a change of the data, once published, is not possible. If necessity arises in the future to correct already published values, then the corrected dataset will be published with a new DOI. Older DOIs and data sets will then still be available. For each DOI, an additional versioning mechanism will be available to document changes to the files such as header or format changes, which do not affect the integrity of the data. The DOI https://doi.org/10.5880/Hpo.0002 identifies the current version. A format description and a version history are provided in the data download folder.
Additional Information
Version history:
2022-05-13
----------
Addition of key reference (Yamazaki et al., 2022, https://doi.org/10.1029/2022GL098860) to the landing page, the data files and the format description
2022-03-26
----------
Publication of Version Hpo.0002. This version replaces version Hpo.0001.
The Hpo, like the Kp nowcast, is based on the FMI algorithm (see Matzka et al., 2021, https://doi.org/10.1029/2020SW002641) and goes through a rescaling procedure to be more similar to the definitive Kp values. The data in version Hpo.0001 from 2018 onwards suffered from a slight error in this rescaling algorithm, causing for example somewhat too few Hpo 0 values and somewhat too many Hpo 0.333 values. This error was corrected for version Hpo.0002. The values from 1995 to 2017 are identical for both versions.
2021-04-26
----------
Publication of Version Hpo.0001
Authors
Matzka, Jürgen;GFZ German Research Centre for Geosciences, Potsdam, Germany
Bronkalla, Oliver;GFZ German Research Centre for Geosciences, Potsdam, Germany
Kervalishvili, Guram;GFZ German Research Centre for Geosciences, Potsdam, Germany
Rauberg, Jan;GFZ German Research Centre for Geosciences, Potsdam, Germany
Yamazaki, Yosuke;GFZ German Research Centre for Geosciences, Potsdam, Germany
Contact
Matzka, Jürgen; GFZ German Research Centre for Geosciences, Potsdam, Germany;
Bronkalla, Oliver; GFZ German Research Centre for Geosciences, Potsdam, Germany;
Contributors
Baillie, Orsi; Blais, Charles; Calp, David; Clarke, Ellen; Claycomb, Abram; Haseloff, Jürgen; Lewis, Andrew; Morris, Jake; Morschhauser, Achim; Petersen, Tanja; Reay, Sarah; Schwarz, Gerhard; Tornow, Katrin; Willer, Anna Naemi; Worthington, Bill; Geomagnetic Observatory Canberra (CNB) maintained by: Geoscience Australia (Australia); Geomagnetic Observatory Brorfelde (BFE) maintained by: Technical University of Denmark (Denmark); Geomagnetic Observatory Eskdalemuir (ESK) maintained by: British Geological Survey (UK); Geomagnetic Observatory Eyrewell (EYR) maintained by: GNS Science (New Zealand); Geomagnetic Observatory Fredericksburg (FRD) maintained by: U.S. Geological Survey (US); Geomagnetic Observatory Hartland (HAD) maintained by: British Geological Survey (UK); Geomagnetic Observatory Lerwick (LER) maintained by: British Geological Survey (UK); Geomagnetic Observatory Meanook (MEA) maintained by: Natural Resources Canada (Canada); Geomagnetic Observatory Niemegk (NGK) maintained by: GFZ German Research Centre for Geosciences (Germany); Geomagnetic Observatory Ottawa (OTT) maintained by: Natural Resources Canada (Canada); Geomagnetic Observatory Sitka (SIT) maintained by: U.S. Geological Survey (US); Geomagnetic Observatory Uppsala (UPS) maintained by: Geological Survey of Sweden (Sweden); Geomagnetic Observatory Wingst (WNG) maintained by: GFZ German Research Centre for Geosciences (Germany)
Funders
H2020 European Research Council:
Space Weather Atmosphere Models and Indices (SWAMI) (776287)
Keywords
Hpo, Hpo index, Hp30, ap30, Hp60, ap60, Kp, Kp index, ap index, geomagnetism, space weather, space physics
CharacterString: This data publication includes the half-hourly Hp30 and ap30 indices as well as the hourly Hp60 and ap60 indices, collectively denoted as Hpo. This dataset is based on near real-time geomagnetic observatory data provided by 13 contributing observatories. It is derived and distributed by GFZ German Research Centre for Geosciences. When using the Hpo index, please cite this data publication as well as the accompanying publication Yamazaki et al. (2022), which serves as documentation of the Hpo.
The dataset is organised in yearly files, which, for the current year, are updated on a monthly basis. Typically, during the second week of a month, the data for the previous month is appended to the current year's file. The files are in ASCII files and start with header lines marked with # (hash).
The Hpo index was developed within the H2020 project SWAMI (grant agreement No 776287) and is produced by Geomagnetic Observatory Niemegk, GFZ German Research Centre for Geosciences. It derives from the same 13 geomagnetic observatories that also contribute to the Kp index (Matzka et al., 2021, https://doi.org/10.5880/Kp.0001). They are listed as contributors to this data publication.
With the introduction of the DOI for the Hpo index (Matzka et al, 2021, https://doi.org/10.5880/Hpo.0001), this DOI landing page and the associated HTTPS server linked to the DOI become the primary archive of Hpo (while the other established index distribution mechanisms at GFZ will be maintained in parallel). With the DOI, the dataset can grow with time, but a change of the data, once published, is not possible. If necessity arises in the future to correct already published values, then the corrected dataset will be published with a new DOI. Older DOIs and data sets will then still be available. For each DOI, an additional versioning mechanism will be available to document changes to the files such as header or format changes, which do not affect the integrity of the data. The DOI https://doi.org/10.5880/Hpo.0002 identifies the current version. A format description and a version history are provided in the data download folder.
pointOfContact
CI_ResponsibleParty
individualName
CharacterString: Matzka, Jürgen
organisationName
CharacterString: GFZ German Research Centre for Geosciences, Potsdam, Germany
CI_OnLineFunctionCode (codeList=http://www.isotc211.org/2005/resources/Codelist/gmxCodelists.xml#CI_OnLineFunctionCode codeListValue=http://www.isotc211.org/2005/resources/Codelist/gmxCodelists.xml#CI_OnLineFunctionCode_information): information