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Solar and Heliospheric Processes from Solar Wind Composition Measurements
DOI: 10.1098/rsta.1994.0126 Bibcode: 1994RSPTA.349..213G

Geiss, J.; Gloeckler, G.; von Steiger, R.

Composition measurements in the solar wind provide important information for solar system science and astrophysics. We show in this report how ion composition data are used to investigate chromospheric and coronal processes. Isotopic abundances in the Sun can best be derived from solar wind measurements. 3He/4He is an isotopi…

1994 Philosophical Transactions of the Royal Society of London Series A
Ulysses 34
The Heliosphere and the Ulysses Mission
DOI: 10.1098/rsta.1994.0127 Bibcode: 1994RSPTA.349..227B

Balogh, A.

The interplanetary medium consists primarily of the supersonic solar wind, carrying the frozen-in magnetic field extending from the solar corona. The properties of this medium are controlled by the state of the corona and by dynamic processes occurring in the medium itself. As a result, there are significant variations in those properties as a fun…

1994 Philosophical Transactions of the Royal Society of London Series A
Ulysses 4
Recent Magnetic Field Results from the Galileo and Ulysses Spacecraft: Discussion
Bibcode: 1994RSPTA.349..270M

Wallis, M. K.; Southwood, D. J.; Miller, S.

1994 Philosophical Transactions of the Royal Society of London Series A
Ulysses 0
Recent Magnetic Field Results from the Galileo and Ulysses Spacecraft
DOI: 10.1098/rsta.1994.0130 Bibcode: 1994RSPTA.349..261S

Southwood, D. J.

Both Galileo and Ulysses spacecraft have made important exploratory measurements before either start the main phase of their missions. Galileo has flown by several objects in the inner Solar System before its reaching Jupiter. The most notable results from the spacecraft magnetometer are the detection of magnetic field deflections in the vicinity …

1994 Philosophical Transactions of the Royal Society of London Series A
Ulysses 0