Search Publications

Exploring the Circular Polarisation of Low-Frequency Solar Radio Bursts with LOFAR
DOI: 10.1007/s11207-022-01976-9 Bibcode: 2022SoPh..297...47M

Kumari, Anshu; Zucca, Pietro; Vocks, Christian +9 more

The Sun is an active star that often produces numerous bursts of electromagnetic radiation at radio wavelengths. Low frequency radio bursts have recently been brought back to light with the advancement of novel radio interferometers. However, their polarisation properties have not yet been explored in detail, especially with the Low Frequency Arra…

2022 Solar Physics
PROBA-2 13
A Review of the Extended EUV Corona Observed by the Sun Watcher with Active Pixels and Image Processing (SWAP) Instrument
DOI: 10.1007/s11207-022-02063-9 Bibcode: 2022SoPh..297..136W

Berghmans, David; West, Matthew J.; Mierla, Marilena +7 more

The Sun Watcher with Active Pixels and Image Processing (SWAP) instrument onboard ESA's PRoject for On Board Autonomy 2 (PROBA2) has provided the first uncompressed, high-cadence, continuous, large field-of-view observations of the extended extreme-ultraviolet (EUV) corona for over a complete solar cycle. It has helped shape our understanding of t…

2022 Solar Physics
PROBA-2 SOHO 6
Observation of a Flare and Filament Eruption in Lyman-α on 8 September 2011 by the PRoject for OnBoard Autonomy/Large Yield Radiometer (PROBA2/LYRA)
DOI: 10.1007/s11207-022-01963-0 Bibcode: 2022SoPh..297...36W

Kretzschmar, M.; Dammasch, I. E.; Dominique, M. +3 more

The Large Yield Radiometer (LYRA) instrument onboard the PRoject for OnBoard Autonomy (PROBA2) observes the solar irradiance in four channels in the UV-EUV. One of these channels is centered around the hydrogen line at 121.6 nm. The solar Lyman-α emission line is an optically thick line mostly formed in the chromosphere. Although it is one of the …

2022 Solar Physics
PROBA-2 SOHO 6
Overexpansion-dominated coronal mass ejection formation and induced radio bursts
DOI: 10.1051/0004-6361/202244275 Bibcode: 2022A&A...666A.166W

Song, H. Q.; Cheng, X.; Ding, M. D. +1 more


Aims: Coronal mass ejections (CMEs) are the most fascinating explosions in the Solar System. Their formation is still not fully understood, however.
Methods: We investigated a well-observed CME on 2021 May 7 that showed a typical three-component structure and was continuously observed from 0 to 3 R by a combination of SDO/AIA…

2022 Astronomy and Astrophysics
PROBA-2 SolarOrbiter 5
Simultaneous High Dynamic Range Algorithm, Testing, and Instrument Simulation
DOI: 10.3847/1538-4357/ac33a1 Bibcode: 2022ApJ...924...63M

Chamberlin, Phillip C.; Jin, Meng; Woods, Thomas N. +4 more

Within an imaging instrument's field of view, there may be many observational targets of interest. Similarly, within a spectrograph's bandpass, there may be many emission lines of interest. The brightness of these targets and lines can be orders of magnitude different, which poses a challenge to instrument and mission design. A single exposure can…

2022 The Astrophysical Journal
PROBA-2 4
Formation of Coronal Mass Ejection and Posteruption Flow of Solar Wind on 2010 August 18 Event
DOI: 10.3847/1538-4357/ac5901 Bibcode: 2022ApJ...929..146S

Slemzin, Vladimir; Goryaev, Farid; Rodkin, Denis

The state of the space environment plays a significant role in the forecasting of geomagnetic storms produced by disturbances of the solar wind (SW). Coronal mass ejections (CMEs) passing through the heliosphere often have a prolonged (up to several days) trail with declining speed, which affects propagation of the subsequent SW streams. We studie…

2022 The Astrophysical Journal
PROBA-2 SOHO 3
Comparing the Sun Watcher Using Active Pixel System Detector and Image Processing Instrument to the Atmosphere Imaging Assembly Instrument Through Measurements of Polar Coronal Holes
DOI: 10.1007/s11207-022-01979-6 Bibcode: 2022SoPh..297...42K

West, Matthew J.; Pesnell, W. Dean; Kirk, Michael S. F. +2 more

The PRoject for OnBoard Autonomy 2/Sun Watcher using Active pixel system detector and image Processing (PROBA2/SWAP) instrument images the full-disk extreme ultraviolet (EUV) Sun using a complementary metal-oxide semiconductor active-pixel sensor (CMOS-APS) detector with a filter centered on a 174 Å passband at a cadence of one to two minutes. In …

2022 Solar Physics
PROBA-2 0
Correction to: Observation of a Flare and Filament Eruption in Lyman-α on 8 September 2011 by the PRoject for OnBoard Autonomy/Large Yield Radiometer (PROBA2/LYRA)
DOI: 10.1007/s11207-022-01978-7 Bibcode: 2022SoPh..297...39W

Kretzschmar, M.; Dammasch, I. E.; Dominique, M. +3 more

2022 Solar Physics
PROBA-2 0