Japan Geoscience Union Meeting 2022

Presentation information

[E] Oral

P (Space and Planetary Sciences ) » P-CG Complex & General

[P-CG18] Future missions and instrumentation for space and planetary science

Mon. May 23, 2022 10:45 AM - 12:15 PM 303 (International Conference Hall, Makuhari Messe)

convener:Naoya Sakatani(Department of Physics, Rikkyo University), convener:Kazunori Ogawa(Japan Aerospace Exploration Agency), Kazuo Yoshioka(Graduate School of frontier Science, The University of Tokyo), convener:Shoichiro Yokota(Graduate School of Science, Osaka University), Chairperson:Kazuo Yoshioka(Graduate School of frontier Science, The University of Tokyo), Shoichiro Yokota(Graduate School of Science, Osaka University), Naoya Sakatani(Department of Physics, Rikkyo University), Kazunori Ogawa(Japan Aerospace Exploration Agency)

10:45 AM - 11:00 AM

[PCG18-01] Development of a space-borne electron impact ion source optimizing ionization rate

*Oya Kawashima1, Naho yanase1, Yoshifumi Saito2, Masafumi Hirahara3, Shoichiro Yokota4, Satoshi Kasahara1 (1.The University of Tokyo, 2.ISAS/JAXA, 3.Nagoya University, 4.Osaka University)


Keywords:Space exploration, Electron gun, Ion source

Mass spectrometer is one of the powerful tools to analyze elemental/isotopic compositions of planetary neutral atmosphere. In many previous missions, the instrument has been great help to understand the history and evolution of planets. In MAVEN mission, for example, mass spectrometer named NGIMS has successfully observed Martian neutral atmospheric escape rate to reconstruct Martian ancient atmosphere. For mass spectrometers in future missions, higher sensitivity is desired to measure trace components, such as noble gases and isotopic diversity. For the purpose, we are developing ionization source with increased ionization rates in this study.
In most of the previous planetary missions, ion sources are designed with electron impact ionization method for the simplicity of the technique.Although 3% Re-W alloy filaments are conventionally used and have a lot of flight-proven performance (e.g., Mahaffy et al., 2012), we selected Iridium filaments with Y2O3 coating for the low work function. Based on the Richardson equation, lower work-function materials enable more electrons to be emitted at the same temperature. Consequently, we confirmed 10-times higher electron emissions in safety with our new model (>2 mA) than that of the previous model (~200 μA, Mahaffy et al., 2012) in our laboratory experiments. Additionally, we established linear relationship between sample gas abundance and extracted ion current (~1×104 nA/Pa) within 1% accuracy for both tandem optics, which we mounted for the redundancy. Then we conducted endurance performance test (ON/OFF = 30min/1hour × 100cycle, 8hour/1hour × 100cycle), verifying the feasibility and robustness of the ion source with the repetitive operation by rapid switching.