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Machine Learning for Predicting the Bz Magnetic Field Component From Upstream in Situ Observations of Solar Coronal Mass Ejections

Space Weather, 2021-12, Vol.19 (12), p.n/a

2021

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Heliospheric Evolution of Magnetic Clouds

The Astrophysical journal, 2019-06, Vol.877 (2), p.77

2019

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Using Gradient Boosting Regression to Improve Ambient Solar Wind Model Predictions

Space Weather, 2021-05, Vol.19 (5), p.n/a

2021

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ElEvoHI: A NOVEL CME PREDICTION TOOL FOR HELIOSPHERIC IMAGING COMBINING AN ELLIPTICAL FRONT WITH DRAG-BASED MODEL FITTING

The Astrophysical journal, 2016-06, Vol.824 (2), p.131-131

2016

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Automatic Detection of Interplanetary Coronal Mass Ejections in Solar Wind In Situ Data

Space Weather, 2022-10, Vol.20 (10), p.n/a

2022

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Prediction of Dst During Solar Minimum Using In Situ Measurements at L5

Space Weather, 2020-05, Vol.18 (5), p.n/a

2020

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Real-time Flare Detection in Ground-Based Hα Imaging at Kanzelhöhe Observatory

Solar physics, 2015-03, Vol.290 (3), p.951-977

2015

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COMBINED MULTIPOINT REMOTE AND IN SITU OBSERVATIONS OF THE ASYMMETRIC EVOLUTION OF A FAST SOLAR CORONAL MASS EJECTION

Astrophysical journal. Letters, 2014-07, Vol.790 (1), p.1-7

2014

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ERRATUM: "ElEvoHI: A NOVEL CME PREDICTION TOOL FOR HELIOSPHERIC IMAGING COMBINING AN ELLIPTICAL FRONT WITH DRAG-BASED MODEL FITTING" (ApJ, 824, 2, 131)

The Astrophysical journal, 2016-11, Vol.831 (2), p.210

2016

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Escape and evolution of Mars's CO2 atmosphere: Influence of suprathermal atoms

Journal of geophysical research. Planets, 2017-06, Vol.122 (6), p.1321-1337

2017

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The role of magnetic handedness in magnetic cloud propagation

Annales geophysicae (1988), 2010-05, Vol.28 (5), p.1075-1100

2010

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On Kelvin–Helmholtz instability due to the solar wind interaction with unmagnetized planets

Planetary and space science, 2007-10, Vol.55 (12), p.1811-1816

2007

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The Kelvin–Helmholtz instability in magnetohydrodynamics with finite Larmor radius effects and application to Venus

Planetary and space science, 2009-03, Vol.57 (3), p.426-427

Amerstorfer, U.V.

2009

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Ion loss on Mars caused by the Kelvin–Helmholtz instability

Planetary and space science, 2004-11, Vol.52 (13), p.1157-1167

2004

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Venus' atomic hot oxygen environment

Journal of Geophysical Research: Planets, 2010-12, Vol.115 (E12), p.n/a

2010

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Solar wind flow past Venus and its implications for the occurrence of the Kelvin–Helmholtz instability

Planetary and space science, 2007-10, Vol.55 (12), p.1793-1803

2007

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Shear driven waves in the induced magnetosphere of Mars

Plasma physics and controlled fusion, 2008-07, Vol.50 (7), p.074018

2008

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Machine Learning for Predicting the B z Magnetic Field Component From Upstream in Situ Observations of Solar Coronal Mass Ejections

Space weather, 2021-12, Vol.19 (12)

2021

Volltextzugriff (PDF)

Prediction of D s t During Solar Minimum Using In Situ Measurements at L5

Space weather, 2020-05, Vol.18 (5)

2020

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Estimation of the past and present Martian water-ice reservoirs by isotopic constraints on exchange between the atmosphere and the surface

International journal of astrobiology, 2003-07, Vol.2 (3), p.195-202

2003

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Shear driven waves in the induced magnetosphere of Mars: parameter dependence

Astrophysics and space sciences transactions, 2009, Vol.5 (1), p.39-42

2009

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Real-time Flare Detection in Ground-Based H[alpha] Imaging at Kanzelhöhe Observatory

Solar physics, 2015-03, Vol.290 (3), p.951

2015

Volltextzugriff (PDF)

Influence of a density increase on the evolution of the Kelvin–Helmholtz instability and vortices

Physics of plasmas, 2010-07, Vol.17 (7), p.072901-072901-8

2010

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Escape and evolution of Mars's CO 2 atmosphere: Influence of suprathermal atoms

Journal of geophysical research. Planets, 2017-06, Vol.122 (6), p.1321-1337

2017

Volltextzugriff (PDF)

The role of magnetic handedness in magnetic cloud propagation

Annales geophysicae (1988), 2010, Vol.28 (5), p.1075-1100

2010

Volltextzugriff (PDF)

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Machine Learning for Predicting the Bz Magnetic Field Component From Upstream in Situ Observations of Solar Coronal Mass Ejections

Heliospheric Evolution of Magnetic Clouds

Using Gradient Boosting Regression to Improve Ambient Solar Wind Model Predictions

ElEvoHI: A NOVEL CME PREDICTION TOOL FOR HELIOSPHERIC IMAGING COMBINING AN ELLIPTICAL FRONT WITH DRAG-BASED MODEL FITTING

Automatic Detection of Interplanetary Coronal Mass Ejections in Solar Wind In Situ Data

Prediction of Dst During Solar Minimum Using In Situ Measurements at L5

Real-time Flare Detection in Ground-Based Hα Imaging at Kanzelhöhe Observatory

COMBINED MULTIPOINT REMOTE AND IN SITU OBSERVATIONS OF THE ASYMMETRIC EVOLUTION OF A FAST SOLAR CORONAL MASS EJECTION

ERRATUM: "ElEvoHI: A NOVEL CME PREDICTION TOOL FOR HELIOSPHERIC IMAGING COMBINING AN ELLIPTICAL FRONT WITH DRAG-BASED MODEL FITTING" (ApJ, 824, 2, 131)

Escape and evolution of Mars's CO2 atmosphere: Influence of suprathermal atoms

The role of magnetic handedness in magnetic cloud propagation

On Kelvin–Helmholtz instability due to the solar wind interaction with unmagnetized planets

The Kelvin–Helmholtz instability in magnetohydrodynamics with finite Larmor radius effects and application to Venus

Ion loss on Mars caused by the Kelvin–Helmholtz instability

Venus' atomic hot oxygen environment

Solar wind flow past Venus and its implications for the occurrence of the Kelvin–Helmholtz instability

Shear driven waves in the induced magnetosphere of Mars

Machine Learning for Predicting the B z Magnetic Field Component From Upstream in Situ Observations of Solar Coronal Mass Ejections

Prediction of D s t During Solar Minimum Using In Situ Measurements at L5

Estimation of the past and present Martian water-ice reservoirs by isotopic constraints on exchange between the atmosphere and the surface

Shear driven waves in the induced magnetosphere of Mars: parameter dependence

Real-time Flare Detection in Ground-Based H[alpha] Imaging at Kanzelhöhe Observatory

Influence of a density increase on the evolution of the Kelvin–Helmholtz instability and vortices

Escape and evolution of Mars's CO 2 atmosphere: Influence of suprathermal atoms

The role of magnetic handedness in magnetic cloud propagation

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