activity
20072024
most citedCME Propagation Characteristics from Radio Observations

74 citations · 159 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.SR2024★ 1 cited

Two-Part Interplanetary Type II Solar Radio Bursts

Silja Pohjolainen

Two similar-looking, two-part interplanetary type II burst events from 2003 and 2012 are reported and analysed. The 2012 event was observed from three different viewing angles, ena…

astro-ph.SR2023

Separating the effects of earthside and far side solar events. A case study

Silja Pohjolainen, Nasrin Talebpour Sheshvan, Christian Monstein

On 8 November 2013 a halo-type coronal mass ejection (CME) was observed, together with flares and type II radio bursts, but the association between the flares, radio bursts, and th…

astro-ph.IM2023★ 3 cited

Magnetic Energy Powers the Corona: How We Can Understand its 3D Storage & Release

Amir Caspi, Daniel B. Seaton, Roberto Casini +12

The coronal magnetic field is the prime driver behind many as-yet unsolved mysteries: solar eruptions, coronal heating, and the solar wind, to name a few. It is, however, still poo…

astro-ph.SR2021★ 6 cited

Formation of Isolated Radio Type II Bursts at Low Frequencies

Silja Pohjolainen, Nasrin Talebpour Sheshvan

The first appearance of radio type II burst emission at decameter-hectometer (DH) waves typically occurs in connection, and often simultaneously, with other types of radio emission…

astro-ph.SR2019★ 6 cited

Cut-off features in interplanetary solar radio type IV emission

Silja Pohjolainen, Nasrin Talebpour Sheshvan

Solar radio type IV bursts can sometimes show directivity, so that no burst is observed when the source region in located far from the solar disk center. This has recently been ver…

astro-ph.SR2018★ 8 cited

Visibility and Origin of Compact Interplanetary Radio Type IV Bursts

Nasrin Talebpour Sheshvan, Silja Pohjolainen

We have analysed radio type IV bursts in the interplanetary (IP) space at decameter-hectometer (DH) wavelengths, to find out their source origin and a reason for the observed direc…