The ACE Magnetic Fields Experiment

@article{Smith1998TheAM,
  title={The ACE Magnetic Fields Experiment},
  author={C. W. Smith and Jacques L'Heureux and Norman F. Ness and Mario H. Acuna and L. F. Burlaga and J. L. Scheifele},
  journal={Space Science Reviews},
  year={1998},
  volume={86},
  pages={613-632}
}
The magnetic field experiment on ACE provides continuous measurements of the local magnetic field in the interplanetary medium. These measurements are essential in the interpretation of simultaneous ACE observations of energetic and thermal particles distributions. The experiment consists of a pair of twin, boom- mounted, triaxial fluxgate sensors which are located 165 inches (=4.19 m) from the center of the spacecraft on opposing solar panels. The electronics and digital processing unit (DPU… 
Spacecraft and interplanetary contributions to the magnetic environment on-board LISA Pathfinder
LISA Pathfinder (LPF) has been a space-based mission designed to test new technologies that will be required for a gravitational wave observatory in space. Magnetically driven forces play a key role
ACE Observations of Magnetic Waves Arising from Newborn Interstellar Pickup Helium Ions
We report low-frequency magnetic waves that were observed by the Advanced Composition Explorer (ACE) spacecraft on day-of-year (DOY) 180 of 1999 with characteristics consistent with the predictions
Evolution of low-altitude and ring current ENA emissions from a moderate magnetospheric storm: Continuous and simultaneous TWINS observations
[1] The moderate storm of 22 July 2009 is the largest measured during the extended solar minimum between December 2006 and March 2010. We present observations of this storm made by the two wide-angle
Science objectives of the magnetic field experiment onboard Aditya-L1 spacecraft
Abstract The Aditya-L1 is first Indian solar mission scheduled to be placed in a halo orbit around the first Lagrangian point (L1) of Sun-Earth system in the year 2018–19. The approved scientific
The interplanetary magnetic field environment at Mercury's orbit
Abstract Mercury is exposed to the most dynamic heliospheric space environment of any planet in the solar system. The magnetosphere is particularly sensitive to variations in the interplanetary
Spatial distributions of electromagnetic field variations and injection regions during the 20 November 2007 sawtooth event
Abstract. We report multi-spacecraft and ground-based observations of a "sawtooth" event on 20 November 2007. For this event, data from three THEMIS, two GOES, and four LANL spacecraft are available
The Magnetometer Instrument on MESSENGER
Abstract The Magnetometer (MAG) on the MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) mission is a low-noise, tri-axial, fluxgate instrument with its sensor mounted on a
Dual Spacecraft Observations of a Compression Event Within the Jovian Magnetosphere
Received 1 July 2003; revised 21 October 2003; accepted 29 October 2003; published 9 July 2004. [1] By using Cassini as an upstream solar wind monitor, we are able to infer increases in the
Interplanetary magnetic fluctuation anisotropy in the inertial range
[1] We have created a database of interplanetary magnetic field spectra from over 900 separate solar wind intervals at 1 AU using data from the Advanced Composition Explorer (ACE) spacecraft. These
Cluster observations of the heliospheric current sheet and an associated magnetic flux rope and comparisons with ACE
[1] Cluster and ACE magnetic field measurements from the 13 February 2001 are presented. On this day the four Cluster spacecraft made two crossings of the heliospheric current sheet (HCS) while in
...
1
2
3
4
5
...

References

SHOWING 1-10 OF 27 REFERENCES
The WIND magnetic field investigation
The magnetic field experiment on WIND will provide data for studies of a broad range of scales of structures and fluctuation characteristics of the interplanetary magnetic field throughout the
The main magnetic field of Jupiter
The main magnetic field of Jupiter has been measured by the Goddard Space Flight Center flux gate magnetometer on Pioneer 11, and analysis of the data yields a more detailed model than that obtained
Multiple spacecraft survey of the north‐south asymmetry of the interplanetary magnetic field
Twenty-three years of spacecraft observations spanning 22 AU of heliocentric distance have been used in an examination of the north-south asymmetry of the interplanetary magnetic field. Using the
Solar Wind Electron Proton Alpha Monitor (SWEPAM) for the Advanced Composition Explorer
The Solar Wind Electron Proton Alpha Monitor (SWEPAM) experiment provides the bulk solar wind observations for the Advanced Composition Explorer (ACE). These observations provide the context for
Measurement of the rugged invariants of magnetohydrodynamic turbulence in the solar wind
Measurements of the total energy, cross helicity, and magnetic helicity of the solar wind at 1, 2.8, and 5 AU are presented. These quantities are the three rugged invariants of three-dimensional
Origin and evolution of fluctuations in the solar wind: Helios observations and Helios-Voyager comparisons
Using hour-averaged data from the Helios and Voyager spacecraft, we have investigated the origin and evolution of low-frequency interplanetary fluctuations from 0.3 to 20 AU. Alfvenic fluctuations in
Cosmic ray modulation and the distant heliospheric magnetic field: Voyager 1 and 2 observations from 1986 to 1989
The changes in the cosmic ray intensity >70 MeV/nucleon observed by Voyager I (termed VI) near 30[degrees] heliographic latitude and by Voyager 2 (termed V2) near O[degrees] heliographic latitude
Fluxgate magnetometers for outer planets exploration
The exploration of the interplanetary medium and the magnetospheres of the outer planets requires the implementation of magnetic field measuring instrumentation with wide dynamic range, high
The role of coronal mass ejections and interplanetary shocks in interplanetary magnetic field statistics and solar magnetic flux ejection
We examine the role of coronal mass ejections (CMEs) and interplanetary shocks in modifying the large-scale winding of the interplanetary magnetic field (IMF) by extracting CME and shock observations
Large-Amplitude Alfvn Waves in the Interplanetary Medium'
An extensive study of the dynamic nonshock properties of the microscale fluctuations (scale lengths of 0.01 AU and less) in the interplanetary medium was made by using plasma and magnetic field data
...
1
2
3
...