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1
Published in 2017 at "Social Work"
DOI: 10.1002/2016sw001565
Abstract: There has long been interest in knowing the shape and location of the Earth's magnetopause and of the standing fast-mode bow shock upstream of the Earth's magnetosphere. This quest for knowledge spans both the research…
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Keywords:
nowcasting forecasting;
bow shock;
forecasting magnetopause;
status ... See more keywords
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1
Published in 2017 at "Geophysical Research Letters"
DOI: 10.1002/2017gl073175
Abstract: A Hot Flow Anomaly (HFA) is created when an interplanetary current sheet interacts with a planetary bow shock. Previous studies have reported observing HFAs at Earth, Mercury, Venus, Mars and Saturn. During Juno's approach to…
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Keywords:
jupiter;
hot flow;
flow anomaly;
hfa ... See more keywords
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1
Published in 2018 at "Journal of Geophysical Research"
DOI: 10.1029/2019ja027290
Abstract: The properties of whistler waves near lower‐hybrid frequencies within Earth's quasiperpendicular bow shock are examined using data from the Magnetospheric Multiscale (MMS) mission. These waves appear as right‐hand polarized wave packets propagating upstream obliquely to…
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Keywords:
bow shock;
whistler waves;
within earth;
shock ... See more keywords
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3
Published in 2023 at "Geophysical Research Letters"
DOI: 10.1029/2022gl101734
Abstract: The typical subsolar stand‐off distance of Mars' bow shock is of the order of a solar wind ion convective gyroradius, making it highly non‐planar to incident ions. Using spacecraft observations and a test particle model,…
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Keywords:
shock;
bow shock;
foreshock structures;
transient foreshock ... See more keywords
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0
Published in 2025 at "Geophysical Research Letters"
DOI: 10.1029/2025gl118868
Abstract: We conduct a statistical analysis of multiple bow shock (BS) crossings at Mars. Data from the magnetometer (MAG) and Solar Wind Ion Analyzer (SWIA) onboard the Mars Atmosphere and Volatile Evolution (MAVEN) spacecraft from its…
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Keywords:
multiple bow;
analysis multiple;
statistical analysis;
bow shock ... See more keywords
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Published in 2025 at "Nature Communications"
DOI: 10.1038/s41467-025-65011-8
Abstract: Bow shock, where the solar wind first encounters the Martian environment, reflects the complex interplay between the solar wind and Martian upper atmosphere and crustal fields. However, a comprehensive understanding of Martian bow shock dynamics…
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Keywords:
wind;
solar wind;
shock oscillations;
bow shock ... See more keywords
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1
Published in 2020 at "Astronomy and Astrophysics"
DOI: 10.1051/0004-6361/202037873
Abstract: In this work, we study the X-ray bow-shock nebula powered by the mature pulsar PSR B1929+10 using data from XMM-Newton, with an effective exposure of $\sim$ 300 ks, offering the deepest investigation of this system…
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Keywords:
nebula;
bow shock;
psr b1929;
pulsar ... See more keywords
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2
Published in 2023 at "Physics of Plasmas"
DOI: 10.1063/5.0129084
Abstract: Observations by Magnetospheric Multiscale have demonstrated that magnetic reconnection occurs at Earth's bow shock, typically at thin current sheets arising from plasma instabilities and turbulence in the shock transition region. Observational surveys of both the…
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Keywords:
bow shock;
reconnection;
current sheets;
hybrid simulations ... See more keywords
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1
Published in 2018 at "Publications of the Astronomical Society of the Pacific"
DOI: 10.1088/1538-3873/aace3e
Abstract: V341 Arae is a 10th-magnitude variable star in the southern hemisphere, discovered over a century ago by Henrietta Leavitt but relatively little studied since then. Although historically considered to be a Cepheid, it is actually…
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Keywords:
v341;
v341 ara;
spectroscopy;
nebula ... See more keywords
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Published in 2025 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/staf344
Abstract: New multi-wavelength Karl G. Jansky VLA observations of CKR02A, the compact radio source in the center of the compact HII region NGC 6334A, are presented. The observations were carried out in five epochs and included…
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Keywords:
ngc 6334a;
massive stars;
radio;
source ... See more keywords
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1
Published in 2018 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/sty2525
Abstract: When a pulsar is moving through a partially ionized medium, a fraction of neutral Hydrogen atoms penetrate inside the pulsar wind and can be photo-ionized by the nebula UV radiation. The resulting protons remains attached…
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Keywords:
pulsar;
numerical simulations;
tails bow;
pulsar wind ... See more keywords