Search Publications

Defining the Middle Corona
DOI: 10.1007/s11207-023-02170-1 Bibcode: 2023SoPh..298...78W

Giordano, Silvio; Andretta, Vincenzo; Reeves, Katharine K. +39 more

The middle corona, the region roughly spanning heliocentric distances from 1.5 to 6 solar radii, encompasses almost all of the influential physical transitions and processes that govern the behavior of coronal outflow into the heliosphere. The solar wind, eruptions, and flows pass through the region, and they are shaped by it. Importantly, the reg…

2023 Solar Physics
PROBA-2 SOHO 32
The Thermosphere Is a Drag: The 2022 Starlink Incident and the Threat of Geomagnetic Storms to Low Earth Orbit Space Operations
DOI: 10.1029/2022SW003330 Bibcode: 2023SpWea..2103330B

Berger, T. E.; Dominique, M.; Thiemann, E. +6 more

On 03 February 2022, SpaceX launched 49 Starlink satellites, 38 of which re-entered the atmosphere on or about 07 February 2022 due to unexpectedly high atmospheric drag. We use empirical model (NRLMSIS, JB08, and HASDM) outputs as well as solar extreme ultraviolet occultation and high-fidelity accelerometer data to show that thermospheric density…

2023 Space Weather
PROBA-2 20
Rapid Rotation of an Erupting Prominence and the Associated Coronal Mass Ejection on 13 May 2013
DOI: 10.1007/s11207-023-02126-5 Bibcode: 2023SoPh..298...35Z

Zhang, Qingmin; Ji, Haisheng; Zhou, Yuhao

In this paper, we report the multiwavelength observations of an erupting prominence and the associated coronal mass ejection (CME) on 13 May 2013. The event occurs behind the western limb in the field of view of the Atmospheric Imaging Assembly (AIA) on board the Solar Dynamics Observatory (SDO) spacecraft. The prominence is supported by a highly …

2023 Solar Physics
PROBA-2 SOHO 8
Global Energetics of Solar Powerful Events on 2017 September 6
DOI: 10.1088/1674-4527/acd592 Bibcode: 2023RAA....23i5017L

Lu, Lei; Dresing, Nina; Wang, Jincheng +9 more

Solar flares and coronal mass ejections (CMEs) are thought to be the most powerful events on the Sun. They can release energy as high as ~1032 erg in tens of minutes, and also can release solar energetic particles (SEPs) into interplanetary space. We explore global energy budgets of solar major eruptions that occurred on 2017 September …

2023 Research in Astronomy and Astrophysics
Hinode PROBA-2 6
The SWAP Filter: A Simple Azimuthally Varying Radial Filter for Wide-Field EUV Solar Images
DOI: 10.1007/s11207-023-02183-w Bibcode: 2023SoPh..298...92S

Berghmans, David; Rachmeler, Laurel A.; West, Matthew J. +5 more

We present the SWAP Filter: an azimuthally varying, radial normalizing filter specifically developed for EUV images of the solar corona, named for the Sun Watcher with Active Pixels and Image Processing (SWAP) instrument on the Project for On-Board Autonomy 2 (PROBA2) spacecraft. We discuss the origins of our technique, its implementation and key …

2023 Solar Physics
PROBA-2 3
Lower-ionosphere electron density and effective recombination coefficients from multi-instrument space observations and ground VLF measurements during solar flares
DOI: 10.1016/j.jastp.2023.106074 Bibcode: 2023JASTP.24706074Z

Dominique, Marie; Žigman, Vida; Grubor, Davorka +2 more

A new model to predict the electron density and effective recombination coefficient of the lower ionosphere under solar flare conditions is presented. This model relies on space-borne solar irradiance measurements in coincidence with ground recorded active transmissions of Very Low Frequency (VLF), (<30 kHz) signals. Use is made of the irradian…

2023 Journal of Atmospheric and Solar-Terrestrial Physics
PROBA-2 3
A Revised Graduated Cylindrical Shell Model and its Application to a Prominence Eruption
DOI: 10.1088/1674-4527/acee4d Bibcode: 2023RAA....23l5004Z

Zhang, Qing-Min; Hou, Zhen-Yong; Bai, Xian-Yong

In this paper, the well-known graduated cylindrical shell (GCS) model is slightly revised by introducing longitudinal and latitudinal deflections of prominences originating from active regions (ARs). Subsequently, it is applied to the three-dimensional (3D) reconstruction of an eruptive prominence in AR 13110, which produced an M1.7 class flare an…

2023 Research in Astronomy and Astrophysics
PROBA-2 SOHO 2
High-Cadence Observations of Magnetic Field Dynamics and Photospheric Emission Sources in the Eruptive Near-the-Limb X4.9 Solar Flare on 25 February, 2014: Evidences for Two-Stage Magnetic Reconnection during the Impulsive Phase
DOI: 10.1134/S0010952523090010 Bibcode: 2023CosRe..61..265S

Zimovets, I. V.; Sharykin, I. N.; Radivon, A. V.

We present an analysis of the pre-limb eruptive X4.9 solar flare on February 25, 2014, by means of which we confirm a hypothesis of the two-stage energy release corresponding to two magnetic reconnection regimes in the flare impulsive phase. This flare is selected, firstly, because of its morphological peculiarities suggesting the presence of the …

2023 Cosmic Research
PROBA-2 1