• DOI:10.1051/swsc/2022031
• Corpus ID: 252527851

Interplanetary medium monitoring with LISA: lessons from LISA Pathfinder

@article{Cesarini2022InterplanetaryMM,
  title={Interplanetary medium monitoring with LISA: lessons from LISA Pathfinder},
  author={Andrea Cesarini and Catia Grimani and Michele Fabi and Federico Sabbatini and M.L. Villani and Simone Benella and Daniele Telloni},
  journal={Journal of Space Weather and Space Climate},
  year={2022}
}

• A. Cesarini, C. Grimani, +4 authors D. Telloni
• Published 25 September 2022
• Physics
• Journal of Space Weather and Space Climate

The Laser Interferometer Space Antenna (LISA) of the European Space Agency (ESA) will be the first low-frequency gravitational-wave observatory orbiting the Sun at 1 AU. 

The LISA Pathfinder (LPF) mission, aiming at testing of the instruments to be located on board the LISA spacecraft (S/C), hosted, among the others, fluxgate magnetometers and a particle detector as parts of a diagnostics subsystem. 

These instruments allowed us for the estimate of the magnetic and Coulomb spurious forces acting on the test masses that constitute the  mirrors of the interferometer. 

With these instruments we also had the possibility to study the galactic cosmic-ray short term-term variations as a function of the particle energy and the associated interplanetary disturbances.

Platform magnetometers and particle detectors will be also placed on board each LISA S/C.

This work reports about an empirical method that allowed us to disentangle the interplanetary and onboard-generated components of the magnetic field by using the LPF magnetometer measurements.

Moreover, we estimate the number and fluence of solar energetic particle events expected to be observed with the ESA Next Generation Radiation Monitor during the  mission lifetime. An additional cosmic-ray detector, similar to that designed for LPF, in combination with magnetometers, would permit to observe the evolution of recurrent and non-recurrent galactic cosmic-ray variations and associated increases of the interplanetary magnetic field at the transit of high-speed solar wind streams and interplanetary counterparts of coronal mass ejections.