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Digital TV Box Firmware is a type of software that is used to control the operation of a digital TV box. It is responsible for controlling the hardware components of the device, such as the processor, memory, and other peripherals. It also provides the user interface for the device, allowing users to access the various features and functions of the device.
The firmware is typically updated periodically to ensure that the device is running the latest version of the software. This is done to ensure that the machine is running the most up-to-date version of the software, which can help to improve the performance of the device.
In addition to providing the necessary instructions for the device to operate correctly, the firmware also provides security features to protect the device from malicious software. This includes features such as encryption, authentication, and access control. These features help to ensure that the device is secure and that only authorized users can access the device.
Digital TV Box Firmware is an essential component of a digital TV box. It is responsible for controlling the hardware components of the device, providing the user interface, and providing security features to protect the device from malicious software. By keeping the firmware up-to-date, users can ensure that their device is running the most up-to-date version of the software and is secure from malicious software.
The PWE covers frequency range from DC to 10 MHz for electric field, and from a few Hz to 100 kHz for magnetic field by the following receivers: Electric Field Detector (EFD) (Kasaba et al. 2017) for the measurement of electric field from DC to 256 Hz, Waveform Capture/Onboard Frequency Analyzer (WFC/OFA) for the measurement of electric field and magnetic field from a few Hz to 20 kHz, and the High-Frequency Analyzer (HFA) (Kumamoto et al. 2018) for the measurement of electric field from 10 kHz to 10 MHz and magnetic field from 10 to 100 kHz. Each receiver focuses on the measurements of the following issues (for more details, see Kasahara et al. 2018):
Raw waveforms (and some processed data) generated by the EWO receiver and the HFA receivers are stored to the ring buffer (long buffer and short buffer) on the CPU board. For the EWO receiver, sampling rates of EFD waveform and that of WFC waveform are 512 Hz and 65.536 kHz, respectively. The size of long and short buffers and the bit rates of data obtained by the each receiver are shown in Table 2.
The WFC measures the electric and magnetic field waveforms. All the components of \\(E_{\\mathrm{u}}\\), \\(E_{\\mathrm{v}}\\), \\(B_{\\alpha }\\), \\(B_{\\beta }\\), and \\(B_{\\gamma }\\) are nominally obtained by the WFC. The component measured by the WFC can be changed using commands for the purpose of emphasized observation of specific components and to reduce the processing time. We perform the synchronized observation of electric and magnetic field waveforms by the shared-packet exchange between the two CPUs. One CPU decides and sends the start time of a burst operation to the other CPU. Each CPU monitors generated time of data packets from the EWO receiver and starts burst operation when the target packet comes from the receiver.
For the test of the onboard calibration technique, we fed calibration signals into the input of the WPT-PRE(AC) and performed SWCAL procedure. We obtained complex spectra at the fundamental frequency and the odd (up to the \\(29{\\mathrm{th}}\\) order) harmonic frequencies of the square waves (source calibration signals). Then, we calculated the frequency response of the receiver by calculating Eq. (8). Figure 13 shows the pre-launch results of the SWCAL function. (The top and bottom panels show the amplitude and phase characteristics, respectively.) Each mark in Fig. 13 represents calculated frequency response by using each source calibration signal (initial frequency = 32 Hz, number of steps = 10, exponential step mode). The calculated frequency responses correspond reasonably well with the experimental data (not shown here).
We can select the changeable impedance by the telemetry command among \\(1\\,{\\mathrm{k}}\\Omega\\), \\(100\\,{\\mathrm{k}}\\Omega\\), \\(1\\,{\\mathrm{M}}\\Omega\\), and \\(10\\,{\\mathrm{M}}\\Omega\\). The calibration signal is affected by the relation of the selected resistance and the antenna impedance. Figure 15 shows the simulation result of the divided voltage at the point \\(V_\\mathrm{1}\\) in Fig. 14. Since the effect of the antenna impedance is ignored when \\(R_{{\\mathrm{CAL}}}\\) is selected to \\(1\\,{\\mathrm{k}}\\Omega\\), we can measure the end-to-end frequency response of the WFC receiver including the preamplifier [see Kasahara et al. (2018) in this issue]. On the other hand, observed signals by the WFC receiver include effects of the antenna impedance when \\(R_{\\mathrm{CAL}} >100\\,{\\mathrm{k}}\\Omega\\). We can calculate \\(R_{\\mathrm{S}}\\) and \\(C_{\\mathrm{S}}\\) by solving simultaneous equations of the two frequency responses of the circuit (under the two different \\(R_{{\\mathrm{CAL}}}\\) values).
The EWO receiver has programmable gain amplifiers (PGAs). We can select gains by telemetry commands from four (0, 20, 40, and 60 dB) for the electric field and from two (0 and 20 dB) for the magnetic field. We developed automatic gain control (AGC) system which performs automatic selection of appropriate gains for the electric and magnetic field measurements by monitoring peak values of instantaneous electric and magnetic field waveforms. The resolution of the A/D converters onboard the EWO receiver is 14 bit. We set the lower and higher thresholds at \\(128=(1000\\,0000)_2\\) and \\(4096=(1\\,0000\\,0000\\,0000)_2\\) A/D count value. If the level of instantaneous waveform becomes over the higher threshold level, the AGC system sends a telemetry command to switch to low gain. On the other hand, the level becomes less than the lower threshold level, the AGC system sends a telemetry command to switch to high gain. The AGC system obtains instantaneous waveforms and controls PGA gains every 7 spins. We can observe not only very weak events but also large amplitude events (e.g., large amplitude whistlers) by using the AGC system.
The onboard software of the PWE has a real-time operation mode for acquiring data that requires immediate attention, such as the extended operation of the WPT and MAST. In the real-time operation mode, the same data as those of OFA-SPEC are stored in the HK data packet at a cycle of once every 4 s. The number of frequency points \\(p_{\\mathrm{f}}\\) of the OFA-SPEC is synchronized with the relevant setting in the OFA.
After Arase was launched on December 20, 2016, we deployed antennas (WPT-S and MSC) and started nominal operation. In order to confirm that our onboard software satisfies technical and scientific requirements, we show initial results obtained by the PWE.
SM developed onboard software of the PWE and wrote whole of this paper. YK was a principal investigator of PWE. HK and YK were co-principal investigators of PWE. SY and MO developed MSC on board Arase. TI designed the concept of onboard software. YK and KI developed WPT-S on board Arase. AK and FT developed the HFA of PWE. MO and SK contributed processing of the data obtained by PWE. YM was a project scientist of the ERG project. MH developed onboard software of MDP/MDR. AM operated the MAST extension and provided DC magnetic field measurement data. IS was a project manager of the ERG project. All authors read and approved the final manuscript. 153554b96e
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