Name | VHM_FGM, Vector Helium Magnetometer - Flux Gate Magnetometer |
Mission | Ulysses |
URL | http://ufa.esac.esa.int/ufa/ |
DOI | https://doi.org/10.5270/esa-x56kgc1 |
Abstract | The Ulysses magnetometer uses two sensors, one a Vector Helium Magnetometer (VHM), the other a Fluxgate Magnetometer (FGM). Onboard data processing yields measurements of the magnetic field vector with a time resolution up to 1 vector/second and a sensitivity of about 10 pT. |
Description | High resolution samples at about one-second intervals of the interplanetary magnetic field. Field vector components are given in units of nanoteslas and in RTN coordinates, where R is the Sun-spacecraft axis, T is the cross product of the solar rotation axis and R, and N is the cross product of R and T. The field magnitudes in nT are averages of scalar magnitudes at higher time resolution. One minute and one day averages are also available. |
Publication | Balogh, A., et al., The magnetic field investigation on the Ulysses mission: Instrumentation and preliminary scientific results , Astron. Astrophys. Suppl., 92gwt-uid-105, 221, 1992; link to publication |
Temporal Coverage | 1990.10.06 - 2009.30.06 |
Mission Description | The joint ESA-NASA Ulysses deep-space mission conducted the first-ever out-of-ecliptic study of the heliosphere - the region of space influenced by the Sun and its magnetic field. The European-built Ulysses spacecraft was launched by the space shuttle Discovery on the 6th of October 1990, and remained operative until the 30th of June 2009, covering almost a full 22-year solar magnetic cycle. Wenzel, K.P., Marsden, R.G., Page, D.E., Smith, E.J., The ULYSSES Mission, Astron. Astrophys. Suppl., 92, 2, 207-219, 1992; link to publication |
Creator Contact | Prof. A. Balogh, Principal Investigator, Imperial College, United Kingdom, a.balogh@imperial.ac.uk |
Publisher And Registrant | European Space Agency |
Credit Guidelines | When publishing any works related to this experiment, please cite the DOI found herein. |