Search Publications

Science with a Small Two-Band UV-Photometry Mission I: Mission Description and Follow-up Observations of Stellar Transients
DOI: 10.1007/s11214-024-01048-3 Bibcode: 2024SSRv..220...11W

Behar, E.; Chang, Hsiang-Kuang; Merc, J. +33 more

This is the first in a collection of three papers introducing the science with an ultra-violet (UV) space telescope on an approximately 130 kg small satellite with a moderately fast re-pointing capability and a real-time alert communication system approved for a Czech national space mission. The mission, called Quick Ultra-Violet Kilonova surveyor…

2024 Space Science Reviews
eHST 15
Searching for Strong Gravitational Lenses
DOI: 10.1007/s11214-024-01042-9 Bibcode: 2024SSRv..220...23L

Hezaveh, Yashar; Courbin, Frédéric; Leung, Calvin +9 more

Strong gravitational lenses provide unique laboratories for cosmological and astrophysical investigations, but they must first be discovered - a task that can be met with significant contamination by other astrophysical objects and asterisms. Here we review strong lens searches, covering various sources (quasars, galaxies, supernovae, FRBs, GRBs, …

2024 Space Science Reviews
Gaia eHST 13
Magnetic Reconnection at Planetary Bodies and Astrospheres
DOI: 10.1007/s11214-023-01017-2 Bibcode: 2024SSRv..220....7G

Stawarz, Julia E.; Phan, Tai D.; Harada, Yuki +11 more

Magnetic reconnection is a fundamental mechanism for the transport of mass and energy in planetary magnetospheres and astrospheres. While the process of reconnection is itself ubiquitous across a multitude of systems, the techniques used for its analysis can vary across scientific disciplines. Here we frame the latest understanding of reconnection…

2024 Space Science Reviews
Cluster 10
Global-Scale Processes and Effects of Magnetic Reconnection on the Geospace Environment
DOI: 10.1007/s11214-024-01067-0 Bibcode: 2024SSRv..220...34F

Eastwood, J. P.; Lavraud, B.; Nakamura, R. +14 more

Recent multi-point measurements, in particular from the Magnetospheric Multiscale (MMS) spacecraft, have advanced the understanding of micro-scale aspects of magnetic reconnection. In addition, the MMS mission, as part of the Heliospheric System Observatory, combined with recent advances in global magnetospheric modeling, have furthered the unders…

2024 Space Science Reviews
Cluster 9
The Interplay Between Collisionless Magnetic Reconnection and Turbulence
DOI: 10.1007/s11214-024-01124-8 Bibcode: 2024SSRv..220...90S

Hasegawa, H.; Khotyaintsev, Yu. V.; Graham, D. B. +13 more

Alongside magnetic reconnection, turbulence is another fundamental nonlinear plasma phenomenon that plays a key role in energy transport and conversion in space and astrophysical plasmas. From a numerical, theoretical, and observational point of view there is a long history of exploring the interplay between these two phenomena in space plasma env…

2024 Space Science Reviews
Cluster 4
Mars Express: 20 Years of Mission, Science Operations and Data Archiving
DOI: 10.1007/s11214-024-01059-0 Bibcode: 2024SSRv..220...25C

Johnstone, A.; Geiger, B.; Määttänen, A. +27 more

Launched on 2 June 2003 and arriving at Mars on 25 December 2003 after a 7-month interplanetary cruise, Mars Express was the European Space Agency's first mission to arrive at another planet. After more than 20 years in orbit, the spacecraft and science payload remain in good health and the mission has become the second oldest operational planetar…

2024 Space Science Reviews
MEx 4
The Composition of Saturn's Rings
DOI: 10.1007/s11214-024-01104-y Bibcode: 2024SSRv..220...70M

Nicholson, Philip D.; Johnson, Robert E.; Hedman, Matthew M. +13 more

The origin and evolution of Saturn's rings is critical to understanding the Saturnian system as a whole. Here, we discuss the physical and chemical composition of the rings, as a foundation for evolutionary models described in subsequent chapters. We review the physical characteristics of the main rings, and summarize current constraints on their …

2024 Space Science Reviews
eHST 3
Dynamical Phenomena in the Martian Atmosphere Through Mars Express Imaging
DOI: 10.1007/s11214-024-01047-4 Bibcode: 2024SSRv..220...16S

Sánchez-Lavega, A.; Tirsch, D.; Spiga, A. +5 more

This review describes the dynamic phenomena in the atmosphere of Mars that are visible in images taken in the visual range through cloud formation and dust lifting. We describe the properties of atmospheric features traced by aerosols covering a large range of spatial and temporal scales, including dynamical interpretations and modelling when avai…

2024 Space Science Reviews
MEx 3
Airglow and Aurora in the Martian Atmosphere: Contributions by the Mars Express and ExoMars TGO Missions
DOI: 10.1007/s11214-024-01077-y Bibcode: 2024SSRv..220...42G

Montmessin, Franck; Fedorova, Anna; Gérard, Jean-Claude +6 more

The study of atmospheric emissions from orbit to probe the middle and upper atmosphere of Mars, which started with the Mariner missions, is living a golden era thanks to the European Space Agency (ESA) Mars Express mission and other subsequent missions built upon its success, including the ESA ExoMars Trace Gas Orbiter (TGO) mission. Here we summa…

2024 Space Science Reviews
ExoMars-16 MEx 2
The Ionosphere of Mars After 20 Years of Mars Express Contributions
DOI: 10.1007/s11214-024-01078-x Bibcode: 2024SSRv..220...41P

Pätzold, Martin; González-Galindo, Francisco; Holmström, Mats +6 more

The Martian ionosphere originates from the ionization of the planetary neutral atmosphere by solar radiation. This conductive layer is embedded within the thermosphere and exosphere of Mars where it forms a highly variable interaction region with the solar wind. The Martian ionosphere has been continuously observed by the three plasma instruments …

2024 Space Science Reviews
MEx 2