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The heliospheric current sheet and plasma sheet during Parker Solar Probe's first orbit
We present heliospheric current sheet (HCS) and plasma sheet (HPS) observations during
Parker Solar Probe's (PSP) first orbit around the Sun. We focus on the eight intervals that …
Parker Solar Probe's (PSP) first orbit around the Sun. We focus on the eight intervals that …
Turbulence and wave transmission at an ICME-driven shock observed by the Solar Orbiter and Wind
Aims. An interplanetary coronal mass ejection (ICME) event was observed by the Solar
Orbiter at 0.8 AU on 2020 April 19 and by Wind at 1 AU on 2020 April 20. Futhermore, an …
Orbiter at 0.8 AU on 2020 April 19 and by Wind at 1 AU on 2020 April 20. Futhermore, an …
A Closer Look at Small-scale Magnetic Flux Ropes in the Solar Wind at 1 au: Results from Improved Automated Detection
Small-scale interplanetary magnetic flux ropes (SMFRs) are similar to ICMEs in magnetic
structure, but are smaller and do not exhibit coronal mass ejection plasma signatures. We …
structure, but are smaller and do not exhibit coronal mass ejection plasma signatures. We …
Plasma heating and Alfvénic turbulence enhancement during two steps of energy conversion in magnetic reconnection exhaust region of solar wind
The magnetic reconnection exhaust is a pivotal region with enormous magnetic energy
being continuously released and converted. The physical processes of energy conversion …
being continuously released and converted. The physical processes of energy conversion …
Characteristics of the heliospheric current sheets at the sector boundaries: wind observations from 1995–2020
We report results of a statistical study of 1197 heliospheric current sheet (HCS) events
associated with the sector boundaries observed by the Wind spacecraft between 1995 and …
associated with the sector boundaries observed by the Wind spacecraft between 1995 and …
Exploring the inner acceleration region of solar wind: A study based on coronagraphic UV and visible light data
This work combined coronagraphic visible light (VL) and UV data to provide with an
unprecedented view of the inner corona where the nascent solar wind is accelerated. The …
unprecedented view of the inner corona where the nascent solar wind is accelerated. The …
The structure and origin of switchbacks: parker solar probe observations
Switchbacks are rapid magnetic field reversals that last from seconds to hours. Current
Parker Solar Probe (PSP) observations pose many open questions in regard to the nature of …
Parker Solar Probe (PSP) observations pose many open questions in regard to the nature of …
Helium abundance and speed difference between helium ions and protons in the solar wind from coronal holes, active regions, and quiet Sun
Two main models have been developed to explain the mechanisms of release, heating, and
acceleration of the nascent solar wind, the wave-turbulence-driven (WTD) models and …
acceleration of the nascent solar wind, the wave-turbulence-driven (WTD) models and …
Modeling solar energetic particle transport in 3D background solar wind: Influences of the compression regions
In modeling the transport process of solar energetic particles (SEPs) in the heliosphere,
previous simulation works often simplify the solar wind velocity as radial and constant, and …
previous simulation works often simplify the solar wind velocity as radial and constant, and …
A link between high-speed solar wind streams and explosive extratropical cyclones
P Prikryl, K Iwao, DB Muldrew, V Rušin… - Journal of Atmospheric …, 2016 - Elsevier
A link between solar wind magnetic sector boundary (heliospheric current sheet) crossings
by the Earth and the upper-level tropospheric vorticity was discovered in the 1970s. These …
by the Earth and the upper-level tropospheric vorticity was discovered in the 1970s. These …