Solar-MACH: An open-source tool to analyze solar magnetic connection configurations
@article{Gieseler2022SolarMACHAO, title={Solar-MACH: An open-source tool to analyze solar magnetic connection configurations}, author={Jan Gieseler and Nina Dresing and Christian Palmroos and Johan L. Freiherr von Forstner and Daniel J. Price and Rami Vainio and Athanasios Kouloumvakos and L. Rodr'iguez-Garc'ia and Domenico Trotta and Vincent G'enot and Arnaud Masson and Markus Roth and Astrid Veronig}, journal={Frontiers in Astronomy and Space Sciences}, year={2022} }
The Solar MAgnetic Connection HAUS1 tool (Solar-MACH) is an open-source tool completely written in Python that derives and visualizes the spatial configuration and solar magnetic connection of different observers (i.e., spacecraft or planets) in the heliosphere at different times. For doing this, the magnetic connection in the interplanetary space is obtained by the classic Parker Heliospheric Magnetic Field (HMF). In close vicinity of the Sun, a Potential Field Source Surface (PFSS) model can…
One Citation
Solar energetic particle time series analysis with Python
- PhysicsFrontiers in Astronomy and Space Sciences
- 2022
Solar Energetic Particles (SEPs) are charged particles accelerated within the solar atmosphere or the interplanetary space by explosive phenomena such as solar flares or Coronal Mass Ejections…
References
SHOWING 1-10 OF 40 REFERENCES
The Solar Probe Plus Mission: Humanity’s First Visit to Our Star
- Physics
- 2016
Solar Probe Plus (SPP) will be the first spacecraft to fly into the low solar corona. SPP’s main science goal is to determine the structure and dynamics of the Sun’s coronal magnetic field,…
A magnetic flux rope configuration derived by optimization of two-spacecraft In-situ measurements
- PhysicsFrontiers in Physics
- 2022
Increasingly one interplanetary coronal mass ejection (ICME) structure can propagate across more than one spacecraft in the solar wind. This usually happens when two or more spacecraft are nearly…
PyThea: An open-source software package to perform 3D reconstruction of coronal mass ejections and shock waves
- PhysicsFrontiers in Astronomy and Space Sciences
- 2022
PyThea is a newly developed open-source Python software package that provides tools to reconstruct coronal mass ejections (CMEs) and shocks waves in three dimensions, using multi-spacecraft…
LONGITUDINAL PROPERTIES OF A WIDESPREAD SOLAR ENERGETIC PARTICLE EVENT ON 2014 FEBRUARY 25: EVOLUTION OF THE ASSOCIATED CME SHOCK
- Physics, Geology
- 2016
We investigate the solar phenomena associated with the origin of the solar energetic particle (SEP) event observed on 2014 February 25 by a number of spacecraft distributed in the inner heliosphere…
The Large Longitudinal Spread of Solar Energetic Particles During the 17 January 2010 Solar Event
- Physics
- 2012
We investigate multi-spacecraft observations of the 17 January 2010 solar energetic particle event. Energetic electrons and protons have been observed over a remarkable large longitudinal range at…
The Large Longitudinal Spread of Solar Energetic Particles During the 17 January 2010 Solar Event
- PhysicsSolar Physics
- 2012
We investigate multi-spacecraft observations of the 17 January 2010 solar energetic particle event. Energetic electrons and protons have been observed over a remarkable large longitudinal range at…
pfsspy: A Python package for potential field source surface modelling
- Physics, GeologyJ. Open Source Softw.
- 2020
The PFSS equations assume that there is zero electrical current in the domain of interest, leading to the equations for magnetic fields in solar and stellar atmospheres.
Statistical survey of widely spread out solar electron events observed with STEREO and ACE with special attention to anisotropies
- Physics, Geology
- 2014
Context. In February 2011, the two STEREO spacecrafts reached a separation of 180 degrees in longitude, offering a complete view of the Sun for the first time ever. When the full Sun surface is…
Solar differential rotation in the period 1964-2016 determined by the Kanzelhöhe data set
- Physics
- 2017
The main aim of this work is to determine the solar differential rotation by tracing sunspot groups during the period 1964-2016, using the Kanzelhohe Observatory for Solar and Environmental Research…
The first ground-level enhancement of solar cycle 25 on 28 October 2021
- PhysicsAstronomy & Astrophysics
- 2022
Aims. The first relativistic solar proton event of solar cycle 25 was detected on 28 October 2021 by neutron monitors (NMs) on the ground and particle detectors on board spacecraft in near-Earth…