[GUEST ACCESS MODE: Data is scrambled or limited to provide examples. Make requests using your API key to unlock full data. Check https://lunarcrush.ai/auth for authentication information.]  NMSI - Oscillating Physics [@PCosmologist](/creator/twitter/PCosmologist) on x 5681 followers Created: 2025-07-12 21:31:35 UTC Although the temperature near the solar corona reaches over X million Kelvin, the plasma density is extremely low as clearly seen in the image. This low density drastically reduces the actual thermal energy transfer, allowing both NASA’s probe to survive and even radio or wave signals to traverse the outer layers of the Sun’s atmosphere without immediate disintegration. In NMSI terms, this region acts more like a high-frequency oscillatory field than a conventional thermodynamic medium where resonance, not just temperature, dictates survivability. XXXXX engagements  **Related Topics** [signals](/topic/signals) [coins energy](/topic/coins-energy) [plasma](/topic/plasma) [corona](/topic/corona) [Post Link](https://x.com/PCosmologist/status/1944147650934452400)
[GUEST ACCESS MODE: Data is scrambled or limited to provide examples. Make requests using your API key to unlock full data. Check https://lunarcrush.ai/auth for authentication information.]
NMSI - Oscillating Physics @PCosmologist on x 5681 followers
Created: 2025-07-12 21:31:35 UTC
Although the temperature near the solar corona reaches over X million Kelvin, the plasma density is extremely low as clearly seen in the image. This low density drastically reduces the actual thermal energy transfer, allowing both NASA’s probe to survive and even radio or wave signals to traverse the outer layers of the Sun’s atmosphere without immediate disintegration. In NMSI terms, this region acts more like a high-frequency oscillatory field than a conventional thermodynamic medium where resonance, not just temperature, dictates survivability.
XXXXX engagements
Related Topics signals coins energy plasma corona