Search
Search Results
-
-
The Spectrometer Telescope for Imaging X-rays (STIX) on Solar Orbiter
The Spectrometer/Telescope for Imaging X-rays (STIX) is one of the ten instruments on board the scientific payload of ESA’s Solar Orbiter mission....
-
The Structure of the Large-Scale Heliosphere as Seen by Current Models
This review summarizes the current state of research aiming at a description of the global heliosphere using both analytical and numerical modeling...
-
Modeling Global Magnetic-Flux Emergence in Bipolar Solar-Active Regions
Active regions (ARs) appear in the solar atmosphere as a consequence of the emergence of magnetic-flux ropes (FR). In this study, we use Bayesian...
-
Solar Radio-Burst Forecast Based on a Convolutional Neural Network
A solar radio burst is the enhancement of radio emission during the release of solar magnetic energy. It is an important indicator of the level of...
-
Rate of Change of Large-Scale Solar-Wind Structure
Quantifying the rate at which the large-scale solar-wind structure evolves is important for both understanding the physical processes occurring in...
-
The Earth, the Moon, Mercury, Saturn and Its Rings, and Asteroids
The planets Earth and Saturn have dense atmosphere and strong intrinsic magnetic field and hence a sturdy magnetosphere. Therefore, both of these...
-
Oblique and rippled heliosphere structures from the Interstellar Boundary Explorer
Past analysis has shown that the heliosphere structure can be deduced from correlations between long-scale solar wind pressure evolution and...
-
Magnetic Properties of Source Regions of CMEs and DH Type II Radio Bursts
The Sun is a dynamic star that exhibits various phenomena, including solar flares, coronal mass ejections (CMEs), and Type II radio bursts. CMEs are...
-
-
The Magnetic-Field Calibration of the Full-Disk Magnetograph Onboard the Advanced Space Based Solar Observatory (ASO-S/FMG)
The full-disk magnetograph is a main scientific payload onboard the Advanced Space based Solar Observatory (ASO-S/FMG) that through Stokes-parameters...
-
-
Earth’s Exospheric X-Ray Emissions
In this chapter we explore solar wind charge exchange X-ray emission emitted from the Earth’s exosphere, following an interaction between heavy ions...
-
Coronal Mass Ejections
General properties of coronal mass ejections (CMEs), their kinematics, morphology, source regions, etc., are described. CMEs are giant clouds of...
-
Rapid Rotation of an Erupting Prominence and the Associated Coronal Mass Ejection on 13 May 2013
In this paper, we report the multiwavelength observations of an erupting prominence and the associated coronal mass ejection (CME) on 13 May 2013....
-
Direct observations of a complex coronal web driving highly structured slow solar wind
The solar wind consists of continuous streams of charged particles that escape into the heliosphere from the Sun, and is split into fast and slow...
-
Multiwavelength Observations of a Partial Filament Eruption on 13 June 2011
In this paper, we report the multiwavelength observations of the partial filament eruption associated with a C1.2 class flare in NOAA active region...
-
Observations of cross scale energy transfer in the inner heliosphere by Parker Solar Probe
The solar wind, a continuous flow of plasma from the sun, not only shapes the near Earth space environment but also serves as a natural laboratory to...
-
Estimating Total Open Heliospheric Magnetic Flux
Over the solar-activity cycle, there are extended periods where significant discrepancies occur between the spacecraft-observed total (unsigned) open...
-
Solar Activity in the Past and Its Impacts on Climate
Solar activity is suggested to impact the climate system through the influence of total solar irradiance (TSI), solar ultraviolet (UV), and galactic...