Add to ORKGRecent Ulysses observations from the Sun's equator to the poles reveal fundamental properties of the three-dimensional heliosphere at the maximum in solar activity. The heliospheric magnetic field originates from a magnetic dipole oriented nearly perpendicular to, instead of nearly parallel to, the Sun's rotation axis. Magnetic fields, solar wind, and energetic charged particles from low-latitude sources reach all latitudes, including the polar caps. The very fast high-latitude wind and polar coronal holes disappear and reappear together. Solar wind speed continues to be inversely correlated with coronal temperature. The cosmic ray flux is reduced symmetrically at all latitudes
[1] At the time of the solar flare on the Bastille Day of 2000, the Ulysses spacecraft was at 3.17 A...
Understanding the evolution of magnetic flux in the heliosphere remains an unresolved issue. The cur...
Observations from the second Ulysses fast latitude scan show that the global structure of solar wi...
Recent Ulysses observations from the Sun's equator to the poles reveal fundamental properties of the...
During solar maximum conditions, the heliosphere is highly structured on all spatial scales. It is t...
In 2000–2001 Ulysses passed from the south to the north polar regions of the Sun in the inner he...
International audienceThe Ulysses spacecraft is in a near-polar solar orbit with a period of 6.2 yea...
Abstract: Ulysses, the first spacecraft ever to fly over the poles of the Sun, plays a central role ...
Abstract. Observed properties of the magnetic field in the outer heliosphere are generally well desc...
Abstract This thesis studies the structure and evolution of the large scale heliospheric magnetic fi...
We present an overview of the data and models collected for the Whole Heliosphere Interval, an inter...
Ulysses, launched in October 1990, began its second out-of-ecliptic orbit in December 1997, and it...
The heliospheric magnetic field (HMF) is the extension of the coronal magnetic field carried out int...
The concept that open magnetic flux of the Sun (rooted with one and only one footpoint at the Sun) i...
Dissertation (Ph.D.) University of Alaska Fairbanks, 1985An improved kinematic method is used to per...
[1] At the time of the solar flare on the Bastille Day of 2000, the Ulysses spacecraft was at 3.17 A...
Understanding the evolution of magnetic flux in the heliosphere remains an unresolved issue. The cur...
Observations from the second Ulysses fast latitude scan show that the global structure of solar wi...
Recent Ulysses observations from the Sun's equator to the poles reveal fundamental properties of the...
During solar maximum conditions, the heliosphere is highly structured on all spatial scales. It is t...
In 2000–2001 Ulysses passed from the south to the north polar regions of the Sun in the inner he...
International audienceThe Ulysses spacecraft is in a near-polar solar orbit with a period of 6.2 yea...
Abstract: Ulysses, the first spacecraft ever to fly over the poles of the Sun, plays a central role ...
Abstract. Observed properties of the magnetic field in the outer heliosphere are generally well desc...
Abstract This thesis studies the structure and evolution of the large scale heliospheric magnetic fi...
We present an overview of the data and models collected for the Whole Heliosphere Interval, an inter...
Ulysses, launched in October 1990, began its second out-of-ecliptic orbit in December 1997, and it...
The heliospheric magnetic field (HMF) is the extension of the coronal magnetic field carried out int...
The concept that open magnetic flux of the Sun (rooted with one and only one footpoint at the Sun) i...
Dissertation (Ph.D.) University of Alaska Fairbanks, 1985An improved kinematic method is used to per...
[1] At the time of the solar flare on the Bastille Day of 2000, the Ulysses spacecraft was at 3.17 A...
Understanding the evolution of magnetic flux in the heliosphere remains an unresolved issue. The cur...
Observations from the second Ulysses fast latitude scan show that the global structure of solar wi...