picam ion sensor  (Akatsuki Technology)

Journal: Space Science Reviews

Article Title: SERENA: Particle Instrument Suite for Determining the Sun-Mercury Interaction from BepiColombo

doi: 10.1007/s11214-020-00787-3

Figure Lengend Snippet: SERENA scientific performances

Article Snippet: The ratio between Fe and H, i.e., the so-called First Ionization Potential (FIP) bias, used to determine the location of SW source based on the abundance of the elements, can be measured by the PICAM and MIPA ion sensors of the SERENA package; measurements of plasma composition, of SW ion flux & density, and of magnetic fields in the vicinity of Venus and Mercury during flybys; coordinated science observations together with other spacecraft in Earth orbit and in the inner Solar System, e.g., Akatsuki, Parker Solar Probe, SDO, Proba-2, Hisaki, SOHO, Solar Orbiter and JUICE, to provide new measurements and/or additional vantage points; observations of InterPlanetary Scintillations (IPS) coordinated with Earth-based measurements to provide information on SW density.

Techniques: Clinical Proteomics

Journal: Space Science Reviews

Article Title: SERENA: Particle Instrument Suite for Determining the Sun-Mercury Interaction from BepiColombo

doi: 10.1007/s11214-020-00787-3

Figure Lengend Snippet: Serena HK telemetry (bit/s)

Article Snippet: The ratio between Fe and H, i.e., the so-called First Ionization Potential (FIP) bias, used to determine the location of SW source based on the abundance of the elements, can be measured by the PICAM and MIPA ion sensors of the SERENA package; measurements of plasma composition, of SW ion flux & density, and of magnetic fields in the vicinity of Venus and Mercury during flybys; coordinated science observations together with other spacecraft in Earth orbit and in the inner Solar System, e.g., Akatsuki, Parker Solar Probe, SDO, Proba-2, Hisaki, SOHO, Solar Orbiter and JUICE, to provide new measurements and/or additional vantage points; observations of InterPlanetary Scintillations (IPS) coordinated with Earth-based measurements to provide information on SW density.

Techniques:

Journal: Space Science Reviews

Article Title: SERENA: Particle Instrument Suite for Determining the Sun-Mercury Interaction from BepiColombo

doi: 10.1007/s11214-020-00787-3

Figure Lengend Snippet: SERENA nominal peak power operational scenario ***

Article Snippet: The ratio between Fe and H, i.e., the so-called First Ionization Potential (FIP) bias, used to determine the location of SW source based on the abundance of the elements, can be measured by the PICAM and MIPA ion sensors of the SERENA package; measurements of plasma composition, of SW ion flux & density, and of magnetic fields in the vicinity of Venus and Mercury during flybys; coordinated science observations together with other spacecraft in Earth orbit and in the inner Solar System, e.g., Akatsuki, Parker Solar Probe, SDO, Proba-2, Hisaki, SOHO, Solar Orbiter and JUICE, to provide new measurements and/or additional vantage points; observations of InterPlanetary Scintillations (IPS) coordinated with Earth-based measurements to provide information on SW density.

Techniques: Diagnostic Assay

Journal: Space Science Reviews

Article Title: SERENA: Particle Instrument Suite for Determining the Sun-Mercury Interaction from BepiColombo

doi: 10.1007/s11214-020-00787-3

Figure Lengend Snippet: SERENA Instrument modes reduced set

Article Snippet: The ratio between Fe and H, i.e., the so-called First Ionization Potential (FIP) bias, used to determine the location of SW source based on the abundance of the elements, can be measured by the PICAM and MIPA ion sensors of the SERENA package; measurements of plasma composition, of SW ion flux & density, and of magnetic fields in the vicinity of Venus and Mercury during flybys; coordinated science observations together with other spacecraft in Earth orbit and in the inner Solar System, e.g., Akatsuki, Parker Solar Probe, SDO, Proba-2, Hisaki, SOHO, Solar Orbiter and JUICE, to provide new measurements and/or additional vantage points; observations of InterPlanetary Scintillations (IPS) coordinated with Earth-based measurements to provide information on SW density.

Techniques: Clinical Proteomics