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Long-Lived Recurrent Fluxes of Energetic Ions from Coronal Holes on the Sun
AbstractResults are presented from studying the relative abundances and energy spectra of 4 He, C, O, and Fe suprathermal ions in particle fluxes...
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Spatially resolved imaging of the inner Fomalhaut disk using JWST/MIRI
Planetary debris disks around other stars are analogous to the asteroid and Kuiper belts in the Solar System. Their structure reveals the...
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Linking the Sun to the Heliosphere Using Composition Data and Modelling
Our understanding of the formation and evolution of the corona and the heliosphere is linked to our capability of properly interpret the data from...
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A Review of the Extended EUV Corona Observed by the Sun Watcher with Active Pixels and Image Processing (SWAP) Instrument
The Sun Watcher with Active Pixels and Image Processing (SWAP) instrument onboard ESA’s PRoject for On Board Autonomy 2 (PROBA2) has provided the...
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Sun-synchronous orbital dust ring to reduce climate change at the polar caps
As a geoengineering strategy to attenuate the solar insolation and offset the impacts of global warming at the polar regions, this study proposes a...
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Fluid Simulation of the Plasma Characteristics in an Inductively Coupled Plasma Source with Planar and Cylindrical Coils
AbstractInductively coupled plasma (ICP) source with planar and cylindrical coils is one of the effective methods to generate large-area uniform...
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Future Directions for the Investigation of Surface-Bounded Exospheres in the Inner Solar System
Surface-bounded exospheres result from complex interactions between the planetary environment and the rocky body’s surface. Different drivers...
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Solar Electron Beam Velocities That Grow Langmuir Waves in the Inner Heliosphere
Solar accelerated electron beams, a component of space weather, are emitted by eruptive events at the Sun. They interact with the ambient plasma to...
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Multi-source connectivity as the driver of solar wind variability in the heliosphere
The ambient solar wind that fills the heliosphere originates from multiple sources in the solar corona and is highly structured. It is often...
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Nonlinear Analysis of Radial Evolution of Solar Wind in the Inner Heliosphere
We analyzed the radial evolution of solar wind in the inner heliosphere using nonlinear time series tools such as correlation dimension
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IRAS 16293–2422 Source A
Rotational spectral line emission of OCS, CH \(_3\) OH,...
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The Kuiper Belt As An Evolved Circumstellar Disk
In the past decade, more than 400 objects have been discovered in orbit about the sun beyond Neptune. They constitute a vast ring of bodies the...
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Time Evolution of a Cometary Spear of the Sun
AbstractSome asteroids, comets, and planets (ACPs) are accelerated by giant planets and ejected from parent planetary systems with velocities of...
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The high-energy Sun - probing the origins of particle acceleration on our nearest star
As a frequent and energetic particle accelerator, our Sun provides us with an excellent astrophysical laboratory for understanding the fundamental...
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An indoor calibration light source of the transmissometers based on spatial light modulation
Aiming at the problem that the calibration results of the transmissometers cannot be traced to the meteorological optical range ( MOR ) defined by the...
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Transverse oscillations and an energy source in a strongly magnetized sunspot
The solar corona is two to three orders of magnitude hotter than the underlying photosphere, and the energy loss of coronal plasma is extremely...
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Study on thickness uniformity of Ta2O5 film evaporated on the inner-face of a hemispherical substrate
Theoretical analysis and experimental study on the thickness distribution of Ta 2 O 5 film evaporated on the inner-face of a hemispherical substrate are...
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Peering into the Milky Way by FAST: II. Ionized gas in the inner Galactic disk revealed by the piggyback line observations of the FAST GPPS survey
As one of the major components of the interstellar medium, the ionized gas in our Milky Way, especially the low-density diffuse component, has not...
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Possible Source and Mechanism of Origin of the Hot Component of the Kuiper Belt
Abstract—A mechanism for the origin of Kuiper belt (KB) bodies different from the hitherto known mechanisms is proposed. The distributions of the...
