Using Partial Solar Eclipse for the 14-Metre Radio Telescope Calibration

dc.contributorAalto-yliopistofi
dc.contributorAalto Universityen
dc.contributor.authorKallunki, J.
dc.contributor.departmentMetsähovi Radio Observatoryen
dc.contributor.organizationMetsähovi Radio Observatory
dc.date.accessioned2024-01-04T09:08:20Z
dc.date.available2024-01-04T09:08:20Z
dc.date.issued2023-12-01
dc.descriptionPublisher Copyright: © 2023 J. Kallunki, published by Sciendo.
dc.description.abstractA partial solar eclipse occurred on 25 October 2022, in the central and northern parts of Europe. The partial solar eclipse was observed at Aalto University Metsähovi Radio Observatory, Finland at the radio wavelength of 8 mm (37 GHz). In Finland, the magnitude of the partial solar eclipse was 62.7 %. Solar radio maps at the time cadence of about 9 minutes were observed over the whole eclipse. The solar eclipse observations could be used for instrument calibration purposes. This paper investigates the solar brightness temperature, the limb brightening effect, the height of the chromosphere and the location of radio brightening using the aforementioned partial solar eclipse observations. We got the confirmation that our earlier results are consistent, e.g., the solar brightness temperature matches with 8100 K ± 300 K. It was also possible to detect limb brightening effect. However, the prevailing solar activity might have distorted the final conclusions. The Moon should operate as a focusing element and the location of radio brightenings could be defined more carefully than in the normal conditions. We investigated this feature. Our results are in some parts unexpected and need further investigations.en
dc.description.versionPeer revieweden
dc.format.extent9
dc.format.mimetypeapplication/pdf
dc.identifier.citationKallunki, J 2023, 'Using Partial Solar Eclipse for the 14-Metre Radio Telescope Calibration', Latvian Journal of Physics and Technical Sciences, vol. 60, no. 6, pp. 54-62. https://doi.org/10.2478/lpts-2023-0036en
dc.identifier.doi10.2478/lpts-2023-0036
dc.identifier.issn0868-8257
dc.identifier.issn2255-8896
dc.identifier.otherPURE UUID: b95165f6-3231-48e9-ae59-4909c911e221
dc.identifier.otherPURE ITEMURL: https://research.aalto.fi/en/publications/b95165f6-3231-48e9-ae59-4909c911e221
dc.identifier.otherPURE FILEURL: https://research.aalto.fi/files/132104555/Kallunki_Using_partial_solar_eclipse.pdf
dc.identifier.urihttps://aaltodoc.aalto.fi/handle/123456789/125507
dc.identifier.urnURN:NBN:fi:aalto-202401041196
dc.language.isoenen
dc.publisherDe Gruyter
dc.relation.ispartofseriesLatvian Journal of Physics and Technical Sciencesen
dc.relation.ispartofseriesVolume 60, issue 6, pp. 54-62en
dc.rightsopenAccessen
dc.subject.keywordInstrument calibration
dc.subject.keywordpartial solar eclipse
dc.subject.keywordradio telescope
dc.subject.keywordsolar activity
dc.subject.keywordsolar radio observations
dc.titleUsing Partial Solar Eclipse for the 14-Metre Radio Telescope Calibrationen
dc.typeA1 Alkuperäisartikkeli tieteellisessä aikakauslehdessäfi
dc.type.versionpublishedVersion

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