Prominences and filaments are manifestations of magnetized, levitated plasma within the
solar coronal atmosphere. Their structure is assumed to be driven by the ambient magnetic …

High-frequency wave phenomena present a great deal of interest as one of the possible
candidates to contribute to the energy input required to heat the corona as a part of the …

Abstract From 2022 March 18 to 21, NOAA Active Region (AR) 12967 was tracked
simultaneously by Solar Orbiter at 0.35 au and Hinode/EIS at Earth. During this period …

Despite the growing importance of planetary Space Weather forecasting and radiation
protection for science and robotic exploration and the need for accurate Space Weather …

The characteristics of a hydrogenated amorphous silicon (a-Si: H) detector are presented
here for monitoring in space solar flares and the evolution of strong to extreme energetic …

Context. The identification of proton core, proton beam, and alpha particles in solar wind ion
measurements is usually performed by applying specific fitting procedures to the particle …

The unexpected observation of a sudden expulsion of mass through the solar corona in
1971 opened up a new field of interest in solar and stellar physics. The discovery came from …

Aims. We present first science observations taken during the commissioning activities of the
Spectral Imaging of the Coronal Environment (SPICE) instrument on the ESA/NASA Solar …

Recent literature indicates that the diffractive sail concept is an interesting alternative to the
more conventional reflective solar sail, which converts solar radiation pressure into a (deep …

Abstract The Laser Interferometer Space Antenna (LISA) of the European Space Agency will
be the first interferometer for low-frequency (10-4–10-1 Hz) gravitational wave detection in …