Search Publications

Solar orbiter: a short review of the mission and early science results
DOI: 10.1007/s10509-025-04400-3 Bibcode: 2025Ap&SS.370...12H

Müller, Daniel; Harra, Louise

On 9 February 2020 at 11:03 pm EST, an Atlas V 411 rocket launched the ESA/ NASA Solar Orbiter mission. This mission was the culmination of decades of work across many countries to achieve the goal of getting close to the Sun and measuring how the Sun creates and maintains the heliosphere. The mission's goal is to understand how the inner heliosph…

2025 Astrophysics and Space Science
SolarOrbiter Ulysses 0
The use of the Pearson differential equation to test energetic distributions in space physics as Kappa distributions; implication for Tsallis nonextensive entropy: II
DOI: 10.1007/s10509-021-04033-2 Bibcode: 2022Ap&SS.367....7S

Shizgal, Bernie D.

This paper presents a mathematical demonstration that particular observed energetic particle distributions of space physics in the particle velocity magnitude, v[0,

2022 Astrophysics and Space Science
Ulysses 5
The global modulation of Galactic and Jovian electrons in the heliosphere
DOI: 10.1007/s10509-018-3377-z Bibcode: 2018Ap&SS.363..156N

Potgieter, Marius S.; Nndanganeni, Rendani R.

A full three-dimensional, numerical model is used to study the modulation of Jovian and Galactic electrons from 1 MeV to 50 GeV, and from the Earth into the heliosheath. For this purpose the very local interstellar spectrum and the Jovian electron source spectrum are revisited. It is possible to compute the former with confidence at kinetic energi…

2018 Astrophysics and Space Science
Ulysses 12
Possible gamma-ray burst radio detections by the Square Kilometre Array. New perspectives
DOI: 10.1007/s10509-016-2866-1 Bibcode: 2016Ap&SS.361..279R

Capozziello, Salvatore; Ruggeri, Alan Cosimo

The next generation interferometric radio telescope, the Square Kilometre Array (SKA), which will be the most sensitive and largest radio telescope ever constructed, could greatly contribute to the detection, survey and characterization of Gamma Ray Bursts (GRBs). By the SKA, it will be possible to perform the follow up of GRBs even for several mo…

2016 Astrophysics and Space Science
INTEGRAL Ulysses 5
Quasi-Thermal Noise Diagnostics in Space Plasmas
DOI: 10.1023/A:1012281730151 Bibcode: 2001Ap&SS.277..309I

Issautier, K.; Moncuquet, M.; Meyer-Vernet, N. +2 more

We present the method of plasma diagnostics by quasi-thermal noise spectroscopy and show examples of application in the solar wind and the Earth's plasmasphere. Using only an electric antenna and a radio receiver, diagnostics of various space environments (magnetized or not) can be obtained in situ. Because of its accuracy, this technique can be u…

2001 Astrophysics and Space Science
Ulysses 27
The heliosphere after Ulysses
DOI: 10.1023/A:1012260014646 Bibcode: 2001Ap&SS.277..337M

Marsden, R. G.

Launched in October 1990, the ESA-NASA Ulysses mission has conducted the very first survey of the heliosphere within 5 AU of the Sun over the full range of heliolatitudes. With polar passes taking place in 1994 and 1995, the timing of the mission has enabled Ulysses to characterise the global structure of the heliosphere at solar minimum, when the…

2001 Astrophysics and Space Science
Ulysses 19
Acceleration and Transport of Energetic Charged Particles in Space
DOI: 10.1023/A:1012212417410 Bibcode: 2001Ap&SS.277...15J

Jokipii, J. R.

Energetic charged particles or cosmic rays are found in space wherever the ambient matter density is small enough to allow them to exist. Their observed kinetic energies vary from just above the local thermal energies to in excess of 1020 eV. The energy spectrum is quite smooth, suggesting that a common mechanism is responsible for part…

2001 Astrophysics and Space Science
Ulysses 12
Electron Temperature in the Solar Wind From a Kinetic Collisionless Model: Application to High-Latitude Ulysses Observations
DOI: 10.1023/A:1012206230015 Bibcode: 2001Ap&SS.277..189I

Issautier, Karine; Meyer-Vernet, Nicole; Pierrard, Viviane +1 more

We use a kinetic collisionless model of the solar wind to calculate the radial variation of the electron temperature and obtain analytical expressions at large radial distances. In order to be compared with Ulysses observations, the model, which initially assumed a radial magnetic field, has been generalized to a spiral magnetic field. We present …

2001 Astrophysics and Space Science
Ulysses 7
Magnetic Field Line Transport in the Heliosphere and Energetic Particle Propagation from Corotating Interaction Regions to High Heliographic Latitudes
DOI: 10.1023/A:1012223925955 Bibcode: 2001Ap&SS.277...97Z

Zimbardo, Gaetano; Veltri, Pierluigi; Pommois, Pierre

A numerical model of magnetic turbulence allows us to compute the diffusion coefficients for different degrees of anisotropy, and in particular for the cases corresponding to the solar wind. We consider here the problem of the propagation of the energetic particles accelerated by corotating interaction regions (CIRs) and observed by Ulysses at hig…

2001 Astrophysics and Space Science
Ulysses 2
Quasi-thermal Noise Spectra Measured by a Dipole Antenna in the Upper Hybrid frequency band
DOI: 10.1023/A:1012285814221 Bibcode: 2001Ap&SS.277..313C

Chugunov, Yury V.; Kazarova, Anna Yu.; Mareev, Eugene A. +3 more

Quasi-thermal noise (QTN) spectroscopy is one of the most effective tools for in situ diagnostics in space plasmas (Meyer-Vernet et al., 1998; Meyer-Vernet and Perche, 1989; Chugunov and Trakhtengerts, 1978). This method produces routine measurements of the bulk electron density and temperature; recently it has been extended to measure the ion bul…

2001 Astrophysics and Space Science
Ulysses 1