QuoteThe National Transportation Safety Board (NTSB) in the US has issued its report into the blaze on the bridge (pictured) of the crude tanker S-Trust 12 months ago. Investigators determined that the probable cause of the fire was the thermal runaway of one of the cells in a lithium-ion battery for a UHF handheld radio.
The S-Trust carried 20 ultra-high frequency (UHF) handheld radios for the crew to use to communicate during vessel operations. The two radios assigned to the bridge were a Motorola DP4400e radio (pictured), which used a lithium-ion battery, and a Motorola GP328 radio, which used a nickel-metal hydride battery.
Investigators found the remains of three batteries – one nickel-metal hydride and two lithium-ion – on the communications table. The single nickel-metal hydride battery was intact; one of the lithium-ion batteries was found intact in the remains of the chargers. Investigators only found components of the second lithium-ion battery.
Lithium-ion battery cell explosions are typically caused by a thermal runaway. An initial orange flash and puff of smoke caught on video feed at the time of the accident (see below) was likely the result of one of the missing lithium-ion cells exploding due to a thermal runaway.
QuoteThe Earth's ionosphere is the ionized upper part of the atmosphere, and it's also the most dynamic as it swells and ebbs depending on whether it's exposed to the Sun or not. It's the ionosphere that enables radio frequency communications to reach beyond the horizon, its thickness and composition also affects the range and quality of these transmissions. Using this knowledge, a group of ham radio operators used the October 14 solar eclipse to crowdsource an experiment, as part of the Ham Science Citizen Investigation (HamSCI) community.
A solar eclipse is an interesting consideration with ionospheric RF transmissions, as it essentially creates a temporary period of night time, which is when the ionosphere is the least dense, and thus weakening these transmissions and their total range. As with previous solar eclipses, they turned it into a kind of game, where each ham operator attempts to contact as many others as possible within the least amount of time. Using the collected data points on who was able to talk to whom on the globe, the event's effect on RF transmissions could be plotted over time. For the August 21, 2017 solar eclipse, the results were published in a 2018 paper by N. A. Frissell et al. in Geophysical Research Letters.
One points which they wished to examine during the 2023 solar eclipse were the plasma bubbles that form near the Earth's magnetic equator, in regions like Brazil. These plasma bubbles cause a lot of interference, which in the preliminary data can be seen as a clear Doppler shift of the signal due to the diffusion of the ionosphere as the eclipse's effect took hold. For the next lunar eclipse in April 2024 another experiment is scheduled, which will give even more ham radio operators the chance to sign up and contribute to ionospheric science.
Quote1. When any cell is full, the BMS stops the chargerfrom stackexchange
2. While the charger is off, the BMS removes some charge from the cell with the highest voltage
3. After that voltage drops sufficiently, the BMS restarts the charger
QuoteDuring the American solar eclipses of October 2023 and April 2024, hundreds of radio amateurs will take to the airwaves. Their goal is to help scientists investigate what happens to radio signals when the Moon blocks the Sun.