output
20142025
most citedStatistical Postprocessing for Weather Forecasts -- Review, Challenges and Avenues in a Big Data World

205 citations

25 papers

astro-ph.EP2025★ 2 cited

Knobs and dials of retrieving JWST transmission spectra. II. Impacts of pipeline-level differences on retrieval posteriors

Simon Schleich, Sudeshna Boro Saikia, Quentin Changeat +3

Since the launch of JWST, observations of exoplanetary atmospheres have seen a revolution in data quality. Given that atmospheric parameter inferences depend heavily on the underly…

astro-ph.EP2024★ 13 cited

Knobs and dials of retrieving JWST transmission spectra. I. The importance of p-T profile complexity

Simon Schleich, Sudeshna Boro Saikia, Quentin Changeat +3

We investigate the impact of using multipoint p-T profiles of varying complexity on the retrieval of synthetically generated hot Jupiter transmission spectra modelled after state-o…

physics.space-ph2023★ 1 cited

Which Upstream Solar Wind Conditions Matter Most in Predicting Bz within Coronal Mass Ejections

Pete Riley, M. A. Reiss, C. Mostl

Accurately predicting the z-component of the interplanetary magnetic field, particularly during the passage of an interplanetary coronal mass ejection (ICME), is a crucial objectiv…

astro-ph.SR2022★ 12 cited

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

Hannah T. Rüdisser, Andreas Windisch, Ute V. Amerstorfer +4

Interplanetary coronal mass ejections (ICMEs) are one of the main drivers for space weather disturbances. In the past, different approaches have been used to automatically detect e…

astro-ph.SR2022★ 12 cited

Writhed Analytical Magnetic Flux Rope Model

Andreas J. Weiss, Teresa Nieves-Chinchilla, Christian Möstl +3

Observations of magnetic clouds, within interplanetary coronal mass ejections (ICMEs), are often well described by flux rope models. Most of these assume either a cylindrical or to…

physics.geo-ph2021★ 21 cited

Forecasting GICs and geoelectric fields from solar wind data using LSTMs: application in Austria

R. L. Bailey, R. Leonhardt, C. Möstl +4

The forecasting of local GIC effects has largely relied on the forecasting of dB/dt as a proxy and, to date, little attention has been paid to directly forecasting the geoelectric…

astro-ph.SR2021★ 52 cited

Multipoint interplanetary coronal mass ejections observed with Solar Orbiter, BepiColombo, Parker Solar Probe, Wind and STEREO-A

C. Möstl, A. J. Weiss, M. A. Reiss +12

We report the result of the first search for multipoint in situ and imaging observations of interplanetary coronal mass ejections (ICMEs) starting with the first Solar Orbiter (Sol…

physics.soc-ph2021★ 10 cited

Meteorological factors and non-pharmaceutical interventions explain local differences in the spread of SARS-CoV-2 in Austria

Katharina Ledebur, Michaela Kaleta, Jiaying Chen +12

The drivers behind regional differences of SARS-CoV-2 spread on finer spatio-temporal scales are yet to be fully understood. Here we develop a data-driven modelling approach based…

physics.space-ph2021★ 25 cited

Machine learning for predicting the Bz magnetic field component from upstream in situ observations of solar coronal mass ejections

Martin A. Reiss, Christian Möstl, Rachel L. Bailey +6

Predicting the Bz magnetic field embedded within ICMEs, also known as the Bz problem, is a key challenge in space weather forecasting. We study the hypothesis that upstream in situ…

cond-mat.mtrl-sci2021★ 15 cited

Re-entrant phenomenon in diffuse ferroelectric, : Local structural insights and FORC study

Akash Surampalli, Ramon Egli, Deepak Prajapat +2

From the phase diagram as proposed by Lei et.al., [J. App. Phys 101, 084105 (2007)] a is chosen showing a diffuse phase transition between cubic to rhom…

astro-ph.SR2021★ 34 cited

The Observational Uncertainty of Coronal Hole Boundaries in Automated Detection Schemes

Martin A. Reiss, Karin Muglach, Christian Möstl +16

Coronal holes are the observational manifestation of the solar magnetic field open to the heliosphere and are of pivotal importance for our understanding of the origin and accelera…

astro-ph.SR2021★ 41 cited

Multi point analysis of coronal mass ejection flux ropes using combined data from Solar Orbiter, BepiColombo and Wind

A. J. Weiss, C. Moestl, E. E. Davies +15

The recent launch of Solar Orbiter and BepiColombo opened a brief window in which these two spacecraft were positioned in a constellation that allows for the detailed sampling of a…

astro-ph.SR2021★ 19 cited

Why are ELEvoHI CME arrival predictions different if based on STEREO-A or STEREO-B heliospheric imager observations?

Jürgen Hinterreiter, Tanja Amerstorfer, Martin A. Reiss +9

Accurate forecasting of the arrival time and arrival speed of coronal mass ejections (CMEs) is a unsolved problem in space weather research. In this study, a comparison of the pred…

physics.ao-ph2020★ 4 cited

Assimilation of the SCATSAR-SWI with SURFEX: Impact of local observation errors in Austria

J. Vural, S. Schneider, B. Bauer-Marschallinger +1

The proper determination of soil moisture on different scales is important for applications in a variety of fields. We aim to develop a high-level soil moisture product with high t…

physics.space-ph2020★ 62 cited

In situ multi-spacecraft and remote imaging observations of the first CME detected by Solar Orbiter and BepiColombo

E. E. Davies, C. Möstl, M. J. Owens +20

On 2020 April 19 a coronal mass ejection (CME) was detected in situ by Solar Orbiter at a heliocentric distance of about 0.8 AU. The CME was later observed in situ on April 20th by…

astro-ph.SR2020★ 32 cited

Analysis of coronal mass ejection flux rope signatures using 3DCORE and approximate Bayesian Computation

Andreas J. Weiss, Christian Möstl, Tanja Amerstorfer +5

We present a major update to the 3D coronal rope ejection (3DCORE) technique for modeling coronal mass ejection flux ropes in conjunction with an Approximate Bayesian Computation (…

physics.space-ph2020★ 37 cited

Evaluation of CME Arrival Prediction Using Ensemble Modeling Based on Heliospheric Imaging Observations

Tanja Amerstorfer, Jürgen Hinterreiter, Martin A. Reiss +8

In this study, we evaluate a coronal mass ejection (CME) arrival prediction tool that utilizes the wide-angle observations made by STEREO's heliospheric imagers (HI). The unsurpass…

astro-ph.SR2020★ 62 cited

Prediction of the in situ coronal mass ejection rate for solar cycle 25: Implications for Parker Solar Probe in situ observations

Christian Möstl, Andreas J. Weiss, Rachel L. Bailey +7

The Parker Solar Probe (PSP) and Solar Orbiter missions are designed to make groundbreaking observations of the Sun and interplanetary space within this decade. We show that a part…

physics.space-ph2020★ 28 cited

Using gradient boosting regression to improve ambient solar wind model predictions

R. L. Bailey, M. A. Reiss, C. N. Arge +7

Studying the ambient solar wind, a continuous pressure-driven plasma flow emanating from our Sun, is an important component of space weather research. The ambient solar wind flows…

astro-ph.SR2020★ 19 cited

Prediction of Dst during solar minimum using in situ measurements at L5

R. L. Bailey, C. Möstl, M. A. Reiss +6

Geomagnetic storms resulting from high-speed streams can have significant negative impacts on modern infrastructure due to complex interactions between the solar wind and geomagnet…

physics.ao-ph2020★ 205 cited

Statistical Postprocessing for Weather Forecasts -- Review, Challenges and Avenues in a Big Data World

Stéphane Vannitsem, John Bjørnar Bremnes, Jonathan Demaeyer +21

Statistical postprocessing techniques are nowadays key components of the forecasting suites in many National Meteorological Services (NMS), with for most of them, the objective of…

astro-ph.EP2018

Hesperos: A geophysical mission to Venus

Robert-Jan Koopmans, Agata Białek, Anthony Donohoe +12

The Hesperos mission proposed in this paper is a mission to Venus to investigate the interior structure and the current level of activity. The main questions to be answered with th…

astro-ph.SR2017★ 105 cited

Time resolved 2 million year old supernova activity discovered in Earth's microfossil record

Peter Ludwig, Shawn Bishop, Ramon Egli +11

Massive stars, which terminate their evolution as core collapse supernovae, are theoretically predicted to eject more than 1E-5 solar masses of the radioisotope 60Fe. If such an ev…

q-bio.NC2015★ 86 cited

Conversion of the chemical concentration of odorous mixtures into odour concentration and odour intensity: a comparison of methods

C. Wu, J. Liu, P. Zhao +2

Continuous odour measurements both of emissions as well as ambient concentrations are seldom realised, mainly because of their high costs. They are therefore often substituted by c…