Search Publications

Interface Region Imaging Spectrograph (IRIS) Observations of the Fractal Dimension in the Solar Atmosphere
DOI: 10.3389/fspas.2022.999319 Bibcode: 2022FrASS...999319A

Aschwanden, Markus J.; Vilangot Nhalil, Nived

While previous work explored the fractality and self-organized criticality (SOC) of flares and nanoflares in wavelengths emitted in the solar corona (such as in hard X-rays, soft X-rays, and EUV wavelenghts), we focus here on impulsive phenomena in the photosphere and transition region, as observed with the {\sl Interface Region Imaging Spectrogra…

2022 Frontiers in Astronomy and Space Sciences
IRIS 1
Space Physics: The Need for a Wider Perspective
DOI: 10.3389/fspas.2022.937742 Bibcode: 2022FrASS...9.7742A

André, Mats

We argue that many studies in space physics would benefit from putting a detailed investigation into a wider perspective. Three examples of theoretical and observational studies are given. We argue that space physics should aim to be less of an isolated branch of science. Rather, by putting the scientific space results into a wider perspective the…

2022 Frontiers in Astronomy and Space Sciences
Cluster 1
Quaternionic Transform: A new Light on the Solar Power Spectrum
DOI: 10.3389/fspas.2022.931963 Bibcode: 2022FrASS...9.1963G

Garrido, Rafael; Ayala, Adrián; Pascual-Granado, Javier +2 more

Asteroseismology, that is, the use of the frequency content of a time series caused by variations in brightness or radial velocity of a stellar object, is based on the hypothesis that such a series is harmonic and therefore can be described by a sum of sines and cosines. If this were not the case (e.g., the oscillations of an ellipsoid of revoluti…

2022 Frontiers in Astronomy and Space Sciences
SOHO 0
Light Elements in the Universe
DOI: 10.3389/fspas.2021.616201 Bibcode: 2021FrASS...8....6R

Magrini, Laura; Randich, Sofia

Due to their production sites, as well as to how they are processed and destroyed in stars, the light elements are excellent tools to investigate a number of crucial issues in modern astrophysics: from stellar structure and non-standard processes at work in stellar interiors to age dating of stars; from pre-main sequence evolution to the star form…

2021 Frontiers in Astronomy and Space Sciences
Gaia 45
The Census of Exoplanets in Visual Binaries: population trends from a volume-limited Gaia DR2 and literature search
DOI: 10.3389/fspas.2021.625250 Bibcode: 2021FrASS...8...16F

Fontanive, Clémence; Bardalez Gagliuffi, Daniella

We present results from an extensive search in the literature and Gaia DR2 for visual, co-moving binary companions to stars hosting exoplanets and brown dwarfs within 200 pc. We found 218 planet hosts out of the 938 in our sample to be part of multiple-star systems, with 10 newly discovered binaries and 2 new tertiary stellar components. This repr…

2021 Frontiers in Astronomy and Space Sciences
Gaia 37
Highlights of Discoveries for δ Scuti Variable Stars From the Kepler Era
DOI: 10.3389/fspas.2021.653558 Bibcode: 2021FrASS...8...55G

Guzik, Joyce Ann

The NASAKeplerand follow-on K2 mission (2009–2018) left a legacy of data and discoveries, finding thousands of exoplanets, and also obtaining high-precision long time-series data for hundreds of thousands of stars, including many types of pulsating variables. Here we highlight a few of the ongoing discoveries fromKeplerdata on δ Scuti pulsating va…

2021 Frontiers in Astronomy and Space Sciences
Gaia 36
Drag-Based Model (DBM) Tools for Forecast of Coronal Mass Ejection Arrival Time and Speed
DOI: 10.3389/fspas.2021.639986 Bibcode: 2021FrASS...8...58D

Dumbović, Mateja; Temmer, Manuela; Veronig, Astrid +4 more

Forecasting the arrival time of coronal mass ejections (CMEs) and their associated shocks is one of the key aspects of space weather research. One of the commonly used models is the analytical drag-based model (DBM) for heliospheric propagation of CMEs due to its simplicity and calculation speed. The DBM relies on the observational fact that slow …

2021 Frontiers in Astronomy and Space Sciences
SOHO 31
The spiral structure in the Solar neighbourhood
DOI: 10.3389/fspas.2021.671670 Bibcode: 2021FrASS...8..103H

Hou, L. G.

The spiral structure in the solar neighborhood is an important issue in astronomy. In the past few years, there has been significant progress in observation. The distances for a large number of good spiral tracers, i.e., giant molecular clouds, high-mass star-formation region masers, HII regions, O-type stars, and young open clusters, have been ac…

2021 Frontiers in Astronomy and Space Sciences
Gaia 25
Plasma and Magnetic Field Turbulence in the Earth's Magnetosheath at Ion Scales
DOI: 10.3389/fspas.2020.616635 Bibcode: 2021FrASS...716635R

Rakhmanova, Liudmila; Riazantseva, Maria; Zastenker, Georgy

Crossing the Earth's bow shock is known to crucially affect solar wind plasma including changes in turbulent cascade. The present review summarizes results of more than 15 years of experimental exploration into magnetosheath turbulence. Great contributions to understanding turbulence development inside the magnetosheath was made by means of recent…

2021 Frontiers in Astronomy and Space Sciences
Cluster 23
Investigating Remote-sensing Techniques to Reveal Stealth Coronal Mass Ejections
DOI: 10.3389/fspas.2021.695966 Bibcode: 2021FrASS...8..109P

Nitta, Nariaki V.; Richardson, Ian G.; Srivastava, Nandita +7 more

Eruptions of coronal mass ejections (CMEs) from the Sun are usually associated with a number of signatures that can be identified in solar disc imagery. However, there are cases in which a CME that is well observed in coronagraph data is missing a clear low-coronal counterpart. These events have received attention during recent years, mainly as a …

2021 Frontiers in Astronomy and Space Sciences
PROBA-2 SOHO 20