ပို၍ စစ်ထုတ်မှုများ ထောင့်ကျဉ်းကင်မရာ စစ်ထုတ်မှု နာမည် လှိုင်းအလျား Spectrum အာရုံခံမှု ရှင်းလင်း 280–640 nm 50px | center | UV 280–370 nm 50px | center | ခရမ်း 350–450 nm 50px | center | အပြာ 430–530 nm 50px | center | ' ' 50px | center | ' အစိမ်း 530–640 nm 50px | center | ' '50px | center | ' လိမော် 590–640 nm 50px | center | ' ' 50px | center | ' ထောင့်ကျယ်ကင်မရာ စစ်ထုတ်မှု နာမည် လှိုင်းအလျား ရောင်စဉ် အာရုံခံမှု ရှင်းလင်း 280–640 nm 50px | center | ' ' 50px | center | ' ခရမ်းရောင် 350–450 nm 50px | center | အပြာ 430–530 nm 50px | center | CH4-U 536–546 nm 50px | center | အစိမ်း 530–640 nm 50px | center | Na-D 588–590 nm 50px | center | လိမော် 590–640 nm 50px | center | CH4-JST 614–624 nm 50px | center |ရေဒီယို သိပ္ပံစနစ်(RSS) Utilized the telecommunications system of the Voyager spacecraft to determine the physical properties of planets and satellites (ionospheres, atmospheres, masses, gravity fields, densities) and the amount and size distribution of material in Saturn's rings and the ring dimensions. ပို၍Infrared Interferometer Spectrometer (IRIS) Investigates both global and local energy balance and atmospheric composition. Vertical temperature profiles are also obtained from the planets and satellites as well as the composition, thermal properties, and size of particles in Saturn's rings. ပို၍ ခရမ်းလွန်ရောင်ခြည် ရောင်စဉ်စစ်ကိရိယာ (UVS) Designed to measure atmospheric properties, and to measure radiation. ပို၍ Triaxial Fluxgate Magnetometer (MAG) Designed to investigate the magnetic fields of Jupiter and Saturn, the interaction of the solar wind with the magnetospheres of these planets, and the magnetic field of interplanetary space out to the boundary between the solar wind and the magnetic field of interstellar space, if crossed. ပို၍ ပါလစမာ Spectrometer (PLS) Investigates the macroscopic properties of the plasma ions and measures electrons in the energy range from 5 eV to 1 keV. ပို၍ Low Energy Charged Particle Instrument (LECP) Measures the differential in energy fluxes and angular distributions of ions, electrons and the differential in energy ion composition. ပို၍ ကော့မစ်ရောင်ခြည် စနစ် (CRS) Determines the origin and acceleration process, life history, and dynamic contribution of interstellar cosmic rays, the nucleosynthesis of elements in cosmic-ray sources, the behavior of cosmic rays in the interplanetary medium, and the trapped planetary energetic-particle environment. ပို၍ Planetary Radio Astronomy Investigation (PRA) Utilizes a sweep-frequency radio receiver to study the radio-emission signals from Jupiter and Saturn. ပို၍ Polarimeter System (PPS) Utilized a telescope with a polarizer to gather information on surface texture and composition of Jupiter and Saturn and information on atmospheric scattering properties and density for both planets. ပို၍ Plasma Wave System (PWS) Provides continuous, sheath-independent measurements of the electron-density profiles at Jupiter and Saturn as well as basic information on local wave-particle interaction, useful in studying the magnetospheres. ပို၍ ဗွိုင်ယေဂျာ ရွှေအသံသွင်းဓာတ်ပြား ဗွိုင်ယေဂျာ ၁ နှင့် ၂ တို့ အသီးသီးတွင် ကမ္ဘာမြေရှိ ပုံများနှင့်အသံများဖမ်းယူထားသော ရွှေဓာတ်ပြားများထည့်သွင်းပေးထားသည်။