Heat Radiation Calculator (Stefan-Boltzmann Law, Q=εσA·T⁴)

POST https://api.elysiatools.com/en/api/tools/heat-radiation-calculator

{
  "mcpServers": {
    "elysiatools-heat-radiation-calculator": {
      "name": "heat-radiation-calculator",
      "description": "Compute thermal radiation from a blackbody/grey body (Stefan-Boltzmann law): blackbody emissive power E_b = σ·T⁴ (W/m²), total radiated power Q_rad = ε·σ·A·T⁴ (W); with an optional surrounding temperature T₀ it also computes the net radiative exchange Q_net = ε·σ·A·(T⁴-T₀⁴) (W). σ = 5.670374419e-8 W/(m²·K⁴); ε is the emissivity (0 < ε ≤ 1, blackbody ε=1); T is the ABSOLUTE temperature (K) — °C and °F are first converted to K (this is an absolute temperature, not a difference); A is the radiating area. Area in m²/cm².",
      "baseUrl": "https://api.elysiatools.com/mcp/sse?toolId=heat-radiation-calculator",
      "command": "",
      "args": [],
      "env": {},
      "isActive": true,
      "type": "sse"
    }
  }
}

{
  "jsonrpc": "2.0",
  "id": 1,
  "method": "tools/list"
}

{
  "jsonrpc": "2.0",
  "id": 2,
  "method": "tools/call",
  "params": {
    "name": "heat-radiation-calculator",
    "arguments": {
  "emissivity": 1,
  "temperature": 300,
  "tempUnit": "K",
  "area": 1,
  "areaUnit": "m2",
  "coldTemperature": 0,
  "decimalPlaces": 4
}
  }
}