Abstract
Our aim is to prove that long time series of solar observations measured
with Metsähovi Radio Observatory's 1.8-meter solar radio telescope,
RT-1.8, at 11.2 GHz are reliable, and that the data can be used for
solar cyclicity studies. We give a detailed description of RT-1.8 and
its calibration. We compare 14 years of Metsähovi Radio
Observatory's solar data from solar cycles 23 and 24 to both Dominion
Radio Astrophysical Observatory (DRAO 2015), Penticton, Canada 2.8 GHz
and Nobeyama Solar Radio Observatory (NSRO 2015), Nobeyama, Japan 9.4
and 17.0 GHz data. Our results show high correlation between all data
sets.
| Original language | English |
|---|---|
| Article number | 33 |
| Pages (from-to) | 33 |
| Number of pages | 6 |
| Journal | Astrophysics and Space Science |
| Volume | 359 |
| DOIs | |
| Publication status | Published - 2015 |
| MoE publication type | A1 Journal article-refereed |
Keywords
- Solar activity
- Solar cyclicity
- Instrumentation
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Metsähovi Radio Observatory
Tammi, J. (Manager)
School of Electrical EngineeringFacility/equipment: Facility
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