The solar activity varies in 11-year cycles. After a few very passive years, the curve on solar activity turns to a very steep rise.
For a long time, researchers have believed that there is not much of interest going on in the Sun during the passive period, therefore not worth studying. Now this assumption is showed to be false by Juha Kallunki, Merja Tornikoski and Irene Bj枚rklund, researchers at Mets盲hovi Radio Observatory, in their peer-reviewed research article published in Solar Physics. This is the first time that astronomers are systematically studying the phenomena of the solar minimum.
The researchers came to this conclusion by examining the solar radio maps of Mets盲hovi Radio Observatory and comparing them with satellite data on the same objects. The solar maps showed active areas, or radio brightenings, which can be observed on the maps as hotter areas than the rest of the solar surface. According to researchers, there are three explanations for radio brightenings.
The brightenings observed in the polar areas on the solar maps (on the left) could be identified as coronal holes. Particle flows, or solar winds, ejected by coronal holes can cause auroras in the Earth's atmosphere.
Secondly, the researchers observed brightenings from which, based on other observations, ejections of hot material from the surface of the sun could be detected.
In addition, radio brightenings were found in areas where, based on satellite observations, strong magnetic fields were detected.
Researchers also found radio brightenings in some areas where no explanatory factor was found on the basis of satellite observations.
鈥楾he other sources used did not explain the cause of the brightening. We don't know what causes those phenomena. We must continue our research鈥, Kallunki says.
Additional observations and research are also needed to predict whether the phenomena of the solar minimum indicate something about the next active period, about its onset and intensity, for example. Each one of the last four cycles has been weaker than the previous one. Researchers do not know why the activity curves do not rise as high as during the previous cycles.
鈥楽olar activity cycles do not always last exactly 11 years, either鈥, explains Docent Merja Tornikoski.
鈥楢 new activity period will not be identified until it is already ongoing. In any case, these observations of the quiet phase we are now analysing are clearly during a period when activity is at its lowest. Now we are waiting for a new rise in activity.鈥
On the Earth, the solar activity can be seen as, for example, auroras. Solar activity can even cause major damage, as solar storms caused by solar flares can damage satellites, electricity networks and radio frequency communications. The study will help to prepare for such damage.
鈥淚n solar storms, it takes 2鈥3 days before the particles hit the Earth. They reach satellites higher up in orbit much faster, so that would leave us even less time to prepare for damage,鈥 Kallunki points out.
Located in Kirkkonummi, Aalto University Mets盲hovi is the only astronomical radio observatory and continuously operational astronomical observation station in Finland. Mets盲hovi is internationally known for its unique, continuous datasets, including a solar monitoring programme spanning over 40 years that has collected data from scientifically very interesting high radio frequencies. This is possible thanks to the exceptionally precise mirror surface of the Mets盲hovi radio telescope.
Yli 40 vuoden ajalta ker盲tty radiodata Auringon aktiivisuudesta on kansainv盲lisesti yksi laajimmista. Avointa dataa hy枚dynt盲v盲t niin tutkijat, opiskelijat kuin taiteilijat.
Mets盲hovin Auringosta saatava datan m盲盲r盲 on valtava ja kasvaa uusilla havainnoilla p盲ivitt盲in.
Aurinko on meit盲 l盲hin t盲hti ja siten ensisijainen havainnointikohde t盲htien toiminnan ymm盲rt盲miseksi.
