Sodankylä Geophysical Observatory |
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The following three images are the instantaneous all-sky power, the estimated quiet-sky power and the derived radio absorption. Units are decibels. The plots are updated approximately once per minute.
To the left is an interferometric riometry keogram. This shows the radio absorption on the KAIRA meridian, at a frequency of approx. 38.1 MHz. The plot is generated by the realtime monitoring system. It is updated approximately every four hours, as data are moved from the KAIRA site to Sodankylä and then processed to generate all-sky images and from there to determine the absorption. Quiet-sky power is also determined as part of this process. The keogram is generated on a different timescale to the real-time, all-sky images above. This means it is generated less often, but is more robust in its calibration and is displayed with higher resolution. |
The following are references for interferometric riometry (technique and science) carried out by KAIRA.
McKay, D., "KAIRA - The Kilpisjärvi Atmospheric Imaging Receiver Array", Avhandling, UiT - The Arctic University of Norway, Tromsø, Norway, 2018 https://hdl.handle.net/10037/13716 (UiT Munin archive).
McKay, D., R. Fallows, M. Norden, A. Aikio, J. Vierinen, F. Honary, S. Marple, and T. Ulich (2015), All-sky interferometric riometry, Radio Sci., 50, 1050-1061, doi:10.1002/2015RS005709. http://onlinelibrary.wiley.com/doi/10.1002/2015RS005709/full
McKay, D., Partamies, N., and Kauristie, K.: Acquisition of optical and riometric keograms for studying auroral electron precipitation, in: XVIII Geofysiikan Päivät, Geofysiikan seura r.y., 35-38, available at: https://geofysiikanseura.yhdistysavain.fi/@Bin/174016/GFP2017_kirja.pdf (last access: 13 January 2018), 2017.
McKay, D., Partamies, N., and Vierinen, J.: Pulsating aurora and cosmic noise absorption associated with growth-phase arcs, Ann. Geophys., 36, 59-69, https://doi.org/10.5194/angeo-36-59-2018, 2018. https://www.ann-geophys.net/36/59/2018/