Ulysses at the Sun's North Pole
15 January 2008
On 14 January, almost a year after last visiting the south solar pole, the European-built Ulysses spaceprobe arrived over the Sun's northern polar cap, thereby completing the third rapid south-to-north transit to date. "This important milestone for the joint ESA-NASA mission also coincides with the start of a new cycle of solar activity," explains Richard Marsden, ESA's Ulysses Mission Manager, "It's been calm on the space weather front recently and so we are looking forward to some solar fireworks over the coming months as the number of sunspots increases."
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Ulysses's third solar orbit |
Although the Sun has been relatively quiet during the past year, this hasn't meant that the spacecraft operations team has been able to sit back and relax. On the contrary, the rapid transit from south to north through perihelion is one of the most nerve-racking periods in the 6.2-year orbit of Ulysses, now in its 18th year of operations. This is because the spacecraft experiences a dynamic disturbance as it comes closer to the Sun, causing the spinning probe to wobble, a motion called nutation. "We have to keep the nutation under control," said Marsden, "otherwise we could lose contact with the spacecraft. Fortunately, the operations team has developed a robust strategy to tackle this problem, and there haven't been too many scary moments this time around!" In fact, this strategy is so effective that the scientific measurements have hardly been affected. The nutation is expected to die away over the next few weeks as Ulysses once again heads away from the Sun.
Ulysses's unique long-term observations
A long-standing scientific puzzle that has been under investigation during the recent south-to-north transit is the clear N-S asymmetry in the structure of the heliosphere that was found when Ulysses visited the polar caps for the first time in 1994-95, also near solar minimum. At that time, the magnetic equator separating positive and negative magnetic fields was pushed 10° southward with respect to the Sun's rotational equator. The reason for the offset is still not fully understood, and preliminary indications are that the recent data show much less of an effect than previously. Further study is needed before firm conclusions can be drawn, however, as the Ulysses measurements are not conducted in each hemisphere simultaneously and temporal changes cannot be ruled out. Nevertheless, investigations of this kind demonstrate the value of long-term out-of-ecliptic observations that only Ulysses can supply.
Contact
Nigel Angold
ESA - Mission Operations Manager
Email: Nigel.Angold
jpl.nasa.gov
Richard Marsden
ESA - Ulysses Mission Manager & Project Scientist
Email: Richard.Marsdenesa.int
