Search Publications

Heliosheath Processes and the Structure of the Heliopause: Modeling Energetic Particles, Cosmic Rays, and Magnetic Fields
DOI: 10.1007/s11214-017-0354-8 Bibcode: 2017SSRv..212..193P

Wurz, P.; Fichtner, H.; Scherer, K. +11 more

This paper summarizes the results obtained by the team "Heliosheath Processes and the Structure of the Heliopause: Modeling Energetic Particles, Cosmic Rays, and Magnetic Fields" supported by the International Space Science Institute (ISSI) in Bern, Switzerland. We focus on the physical processes occurring in the outer heliosphere, especially at i…

2017 Space Science Reviews
Ulysses VenusExpress 70
The Global Solar Dynamo
DOI: 10.1007/s11214-015-0230-3 Bibcode: 2017SSRv..210..367C

Cameron, R. H.; Dikpati, M.; Brandenburg, A.

A brief summary of the various observations and constraints that underlie solar dynamo research are presented. The arguments that indicate that the solar dynamo is an alpha-omega dynamo of the Babcock-Leighton type are then shortly reviewed. The main open questions that remain are concerned with the subsurface dynamics, including why sunspots emer…

2017 Space Science Reviews
Ulysses 69
Radiative Diagnostics in the Solar Photosphere and Chromosphere
DOI: 10.1007/s11214-016-0294-8 Bibcode: 2017SSRv..210..109D

van Noort, M.; de la Cruz Rodríguez, J.

Magnetic fields on the surface of the Sun and stars in general imprint or modify the polarization state of the electromagnetic radiation that is leaving from the star. The inference of solar/stellar magnetic fields is performed by detecting, studying and modeling polarized light from the target star. In this review we present an overview of techni…

2017 Space Science Reviews
Hinode 62
Measurements of Photospheric and Chromospheric Magnetic Fields
DOI: 10.1007/s11214-015-0219-y Bibcode: 2017SSRv..210...37L

Gosain, Sanjay; Lagg, Andreas; Lites, Bruce +2 more

The Sun is replete with magnetic fields, with sunspots, pores and plage regions being their most prominent representatives on the solar surface. But even far away from these active regions, magnetic fields are ubiquitous. To a large extent, their importance for the thermodynamics in the solar photosphere is determined by the total magnetic flux. W…

2017 Space Science Reviews
Hinode SOHO 55
Achievements and Challenges in the Science of Space Weather
DOI: 10.1007/s11214-017-0390-4 Bibcode: 2017SSRv..212.1137K

Veronig, Astrid; Balogh, André; Koskinen, Hannu E. J. +3 more

In June 2016 a group of 40 space weather scientists attended the workshop on Scientific Foundations of Space Weather at the International Space Science Institute in Bern. In this lead article to the volume based on the talks and discussions during the workshop we review some of main past achievements in the field and outline some of the challenges…

2017 Space Science Reviews
Cluster Ulysses 48
Near-Earth Magnetic Field Effects of Large-Scale Magnetospheric Currents
DOI: 10.1007/s11214-016-0267-y Bibcode: 2017SSRv..206..521L

Le, Guan; Lühr, Hermann; Xiong, Chao +1 more

Magnetospheric currents play an important role in the electrodynamics of near-Earth space. This has been the topic of many space science studies. Here we focus on the magnetic fields they cause close to Earth. Their contribution to the geomagnetic field is the second largest after the core field. Significant progress in interpreting the magnetic f…

2017 Space Science Reviews
Cluster 47
Space Weather Effects Produced by the Ring Current Particles
DOI: 10.1007/s11214-017-0412-2 Bibcode: 2017SSRv..212.1315G

Jaynes, Allison; Ganushkina, Natalia; Liemohn, Michael

One of the definitions of space weather describes it as the time-varying space environment that may be hazardous to technological systems in space and/or on the ground and/or endanger human health or life. The ring current has its contributions to space weather effects, both in terms of particles, ions and electrons, which constitute it, and magne…

2017 Space Science Reviews
Cluster 44
Solar Magnetoconvection and Small-Scale Dynamo. Recent Developments in Observation and Simulation
DOI: 10.1007/s11214-015-0204-5 Bibcode: 2017SSRv..210..275B

Solanki, S. K.; Borrero, J. M.; Schüssler, M. +1 more

A number of observational and theoretical aspects of solar magnetoconvection are considered in this review. We discuss recent developments in our understanding of the small-scale structure of the magnetic field on the solar surface and its interaction with convective flows, which is at the centre of current research. Topics range from plage areas …

2017 Space Science Reviews
Hinode 39
The Scientific Foundations of Forecasting Magnetospheric Space Weather
DOI: 10.1007/s11214-017-0399-8 Bibcode: 2017SSRv..212.1221E

Eastwood, J. P.; Nakamura, R.; Turc, L. +2 more

The magnetosphere is the lens through which solar space weather phenomena are focused and directed towards the Earth. In particular, the non-linear interaction of the solar wind with the Earth's magnetic field leads to the formation of highly inhomogenous electrical currents in the ionosphere which can ultimately result in damage to and problems w…

2017 Space Science Reviews
Cluster 38
Aeronomy of the Venus Upper Atmosphere
DOI: 10.1007/s11214-017-0422-0 Bibcode: 2017SSRv..212.1617G

Pätzold, M.; López-Valverde, M. A.; Drossart, P. +3 more

We present aeronomical observations collected using remote sensing instruments on board Venus Express, complemented with ground-based observations and numerical modeling. They are mostly based on VIRTIS and SPICAV measurements of airglow obtained in the nadir mode and at the limb above 90 km. They complement our understanding of the behavior of Ve…

2017 Space Science Reviews
VenusExpress 33