Search Publications

Possible contribution of different energy sources to the production of organics in Titan's atmosphere
DOI: 10.1016/S0273-1177(01)00056-4 Bibcode: 2001AdSpR..27..261R

Coll, P.; Raulin, F.; Navarro-González, R. +1 more

A quantitative comparison of the products arising from the irradiation of a Titan's simulated atmosphere is presented. The energy sources used represent some of the main events that occur in the satellite's atmosphere. All of the compounds identified are classified in the hydrocarbon and nitrile chemical families. Almost all of the detected compou…

2001 Advances in Space Research
Huygens 29
Modulation of galactic and anomalous cosmic rays in the inner heliosphere
DOI: 10.1016/S0273-1177(01)00083-7 Bibcode: 2001AdSpR..27..451H

Heber, B.

Our knowledge on how galactic and anomalous cosmic rays are modulated in the inner heliosphere has been dramatically enlarged due to measurements provided by several missions launched in the past ten years. The current paradigma of singly charged anomalous cosmic rays has been confirmed by recent measurements from the SAMPEX and ACE satelite. Ulys…

2001 Advances in Space Research
Ulysses 14
Capability of the Cassini/Huygens PWA-HASI to measure electrical conductivity in Titan
DOI: 10.1016/S0273-1177(01)00585-3 Bibcode: 2001AdSpR..28.1511M

Rodrigo, R.; López-Moreno, J. J.; Molina-Cuberos, G. J. +1 more

The penetration of the Huygens probe through the atmosphere of Titan in 2004 will provide a unique opportunity to measure the electrical properties of its lower atmosphere. Many studies have been carried out to predict the density of electrons and the distribution of the major positive ions, but there is no recent analysis concerning the electrica…

2001 Advances in Space Research
Huygens 13
The transport of energetic particles and cosmic rays in the heliosphere
DOI: 10.1016/S0273-1177(01)00075-8 Bibcode: 2001AdSpR..27..461G

Giacalone, J.; Jokipii, J. R.

We discuss recent observations of energetic particles and cosmic rays lending insight into how these particles are influenced by the interplanetary magnetic field and what can be learned about the field itself by using the energetic particles as probes. Two recent observations on which we focus attention are those by Ulysses at high heliographic l…

2001 Advances in Space Research
Ulysses 10
Propagation of 3-10 MeV electrons in the inner heliosphere: Ulysses observations
DOI: 10.1016/S0273-1177(01)00078-3 Bibcode: 2001AdSpR..27..547H

Kunow, H.; Heber, B.; Ferrando, P. +3 more

Since the 1970's electrons in the MeV energy range, of Jovian origin, have been extensively studied near the ecliptic from close to the Sun to beyond the Kronian orbit. The Ulysses trajectory provides a unique opportunity to study the propagation of several MeV electrons in a wide range of heliographic latitudes. From the Ulysses launch up to the …

2001 Advances in Space Research
Ulysses 9
Propagation of electromagnetic waves in the lower ionosphere of Titan
DOI: 10.1016/S0273-1177(01)00584-1 Bibcode: 2001AdSpR..28.1505S

Rodrigo, R.; López-Moreno, J. J.; Molina-Cuberos, G. J. +6 more

Towards the end of 2004 during the descent of the HUYGENS probe the Permittivity, Wave and Altimetry instrument (PWA) as part of the HASI experiment will investigate electrical properties and electric field fluctuations in the atmosphere of Titan below 170 km. We have modelled the propagation of low frequency electromagnetic waves in the lower ion…

2001 Advances in Space Research
Huygens 9
Energetic ion (>∼50keV) and electron (>∼40keV) bursts observed by Ulysses near Jupiter
DOI: 10.1016/S0273-1177(01)00514-2 Bibcode: 2001AdSpR..28..903A

Anagnostopoulos, G. C.; Karanikola, I.; Marhavilas, P. K. +1 more

A careful analysis of data collected by the HISCALE experiment on board Ulysses suggests that the quasi-periodic (QP) modulation of several or tens of minutes in flux and/or anisotropy/spectral observations is an almost permanent characteristic of the energetic (>∼50 keV) ion population in the outer and the high latitude middle magnetosphere of…

2001 Advances in Space Research
Ulysses 7
Alfvén waves, magnetic decreases, and discontinuities in interplanetary space
DOI: 10.1016/S0273-1177(01)00507-5 Bibcode: 2001AdSpR..28..765T

Balogh, A.; Tsurutani, B. T.; Smith, E. J. +3 more

The Ulysses mission goes to the polar regions of the heliosphere and therefore is an ideal mission to study Alfvén waves and discontinuities. The polar region is dominated by a high speed solar wind with embedded outwardly propagating nonlinear (|Δ B|/ B0 ∼ 1 to 2) Alfvén waves. Rotational discontinuities are detected at the edges of Al…

2001 Advances in Space Research
Ulysses 5
ULF wave observations in Jupiter's magnetosphere
DOI: 10.1016/S0273-1177(01)00517-8 Bibcode: 2001AdSpR..28..909P

Dougherty, Michele K.; Petkaki, Panagiota

In previous work we have examined magnetometer data from the Ulysses Jupiter flyby, and in particular middle magnetosphere observations in the vicinity of the magnetodisk. Waves transverse to the background magnetic field were found in the heavy ion gyrofrequency regime, a signature of Ion Cyclotron (IC) waves. We examined the dayside and high lat…

2001 Advances in Space Research
Ulysses 5
Determination of physical properties of planetary sub-surface layers by artificial impacts and penetrometry
DOI: 10.1016/S0273-1177(01)00363-5 Bibcode: 2001AdSpR..28.1539K

Kargl, G.; Ball, A. J.; Kömle, N. I.

In recent years the exploration of planetary bodies by surface probes has entered a new phase of interest. The mechanical properties of the near-surface layers of cometary and planetary bodies, including their strength, texture and layering, are important parameters needed both for a proper physical understanding of these bodies and for the design…

2001 Advances in Space Research
Huygens 3