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An Analytical Diffusion-Expansion Model for Forbush Decreases Caused by Flux Ropes

The Astrophysical journal, 2018-06, Vol.860 (1), p.71

2018

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On the Interaction of Galactic Cosmic Rays with Heliospheric Shocks During Forbush Decreases

Solar physics, 2020-02, Vol.295 (2), Article 28

2020

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Interplanetary Protons versus Interacting Protons in the 2017 September 10 Solar Eruptive Event

The Astrophysical journal, 2020-02, Vol.890 (1), p.13

2020

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Evolution of Coronal Mass Ejections and the Corresponding Forbush Decreases: Modeling vs. Multi-Spacecraft Observations

Solar physics, 2020-07, Vol.295 (7), Article 104

2020

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Modeling the Evolution and Propagation of 10 September 2017 CMEs and SEPs Arriving at Mars Constrained by Remote Sensing and In Situ Measurement

Space Weather, 2018-08, Vol.16 (8), p.1156-1169

2018

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On the Rigidity Spectrum of Cosmic-Ray Variations within Propagating Interplanetary Disturbances: Neutron Monitor and SOHO/EPHIN Observations at ∼1-10 GV

The Astrophysical journal, 2021-02, Vol.908 (1), p.5

2021

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Subsurface Radiation Environment of Mars and Its Implication for Shielding Protection of Future Habitats

Journal of geophysical research. Planets, 2020-03, Vol.125 (3), p.n/a

2020

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Global ionospheric flare detection system (GIFDS)

Journal of atmospheric and solar-terrestrial physics, 2016-02, Vol.138-139, p.233-242

2016

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A new model suite to determine the influence of cosmic rays on (exo)planetary atmospheric biosignatures

Astronomy and astrophysics (Berlin), 2019-11, Vol.631

2019

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Variations of dose rate observed by MSL/RAD in transit to Mars

Astronomy and astrophysics (Berlin), 2015-05, Vol.577, p.A58

2015

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Implementation and validation of the GEANT4/AtRIS code to model the radiation environment at Mars

Journal of space weather and space climate, 2019, Vol.9, p.A2

2019

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Catalogue of 55–80 MeV solar proton events extending through solar cycles 23 and 24

Journal of space weather and space climate, 2017, Vol.7, p.A14

2017

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Multi-point galactic cosmic ray measurements between 1 and 4.5 AU over a full solar cycle

Annales geophysicae (1988), 2019-09, Vol.37 (5), p.903-918

2019

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Galactic Cosmic Ray induced absorbed dose rate in deep space – Accounting for detector size, shape, material, as well as for the solar modulation

Journal of space weather and space climate, 2019, Vol.9, p.A14

2019

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The Electron Proton Helium INstrument as an example for a Space Weather Radiation Instrument

Journal of space weather and space climate, 2020, Vol.10, p.53

2020

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The mini-neutron monitor: a new approach in neutron monitor design

Journal of space weather and space climate, 2020, Vol.10, p.39

2020

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A new model describing Forbush Decreases at Mars: combining the heliospheric modulation and the atmospheric influence

Earth and planetary physics, 2020-01, Vol.4 (1), p.62-72

2020

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Matroshka DOSTEL measurements onboard the International Space Station (ISS)

Journal of space weather and space climate, 2015, Vol.5, p.A38

2015

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The Atmospheric Radiation Interaction Simulator (AtRIS): Description and Validation

Journal of geophysical research. Space physics, 2019-01, Vol.124 (1), p.50-67

2019

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From solar to stellar flare characteristics: On a new peak size distribution for G-, K-, and M-dwarf star flares

Astronomy and astrophysics (Berlin), 2019-01, Vol.621, p.A67

2019

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A New Trend in Forecasting Solar Radiation Hazards

Space weather, 2009-05, Vol.7 (5), p.n/a

2009

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The Dependence of the Peak Velocity of High‐Speed Solar Wind Streams as Measured in the Ecliptic by ACE and the STEREO satellites on the Area and Co‐latitude of Their Solar Source Coronal Holes

Journal of geophysical research. Space physics, 2018-03, Vol.123 (3), p.1738-1753

2018

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Characteristics of Low-latitude Coronal Holes near the Maximum of Solar Cycle 24

The Astrophysical journal, 2017-02, Vol.835 (2), p.268

2017

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Statistical Results for Solar Energetic Electron Spectra Observed over 12 yr with STEREO/SEPT

The Astrophysical journal, 2020-02, Vol.889 (2), p.143

2020

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Catalogue of >55 MeV Wide-longitude Solar Proton Events Observed by SOHO, ACE, and the STEREOs at ≈1 AU During 2009 – 2016

Solar physics, 2018-04, Vol.293 (4), p.1-53

2018

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An Analytical Diffusion-Expansion Model for Forbush Decreases Caused by Flux Ropes

On the Interaction of Galactic Cosmic Rays with Heliospheric Shocks During Forbush Decreases

Interplanetary Protons versus Interacting Protons in the 2017 September 10 Solar Eruptive Event

Evolution of Coronal Mass Ejections and the Corresponding Forbush Decreases: Modeling vs. Multi-Spacecraft Observations

Modeling the Evolution and Propagation of 10 September 2017 CMEs and SEPs Arriving at Mars Constrained by Remote Sensing and In Situ Measurement

On the Rigidity Spectrum of Cosmic-Ray Variations within Propagating Interplanetary Disturbances: Neutron Monitor and SOHO/EPHIN Observations at ∼1-10 GV

Subsurface Radiation Environment of Mars and Its Implication for Shielding Protection of Future Habitats

Global ionospheric flare detection system (GIFDS)

A new model suite to determine the influence of cosmic rays on (exo)planetary atmospheric biosignatures

Variations of dose rate observed by MSL/RAD in transit to Mars

Implementation and validation of the GEANT4/AtRIS code to model the radiation environment at Mars

Catalogue of 55–80 MeV solar proton events extending through solar cycles 23 and 24

Multi-point galactic cosmic ray measurements between 1 and 4.5 AU over a full solar cycle

Galactic Cosmic Ray induced absorbed dose rate in deep space – Accounting for detector size, shape, material, as well as for the solar modulation

The Electron Proton Helium INstrument as an example for a Space Weather Radiation Instrument

The mini-neutron monitor: a new approach in neutron monitor design

A new model describing Forbush Decreases at Mars: combining the heliospheric modulation and the atmospheric influence

Matroshka DOSTEL measurements onboard the International Space Station (ISS)

The Atmospheric Radiation Interaction Simulator (AtRIS): Description and Validation

From solar to stellar flare characteristics: On a new peak size distribution for G-, K-, and M-dwarf star flares

A New Trend in Forecasting Solar Radiation Hazards

The Dependence of the Peak Velocity of High‐Speed Solar Wind Streams as Measured in the Ecliptic by ACE and the STEREO satellites on the Area and Co‐latitude of Their Solar Source Coronal Holes

Characteristics of Low-latitude Coronal Holes near the Maximum of Solar Cycle 24

Statistical Results for Solar Energetic Electron Spectra Observed over 12 yr with STEREO/SEPT

Catalogue of >55 MeV Wide-longitude Solar Proton Events Observed by SOHO, ACE, and the STEREOs at ≈1 AU During 2009 – 2016

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