1.7.6 · D1 · HinglishThermodynamics

FoundationsHeat transfer — conduction (Fourier's law k), convection, radiation (Stefan-Boltzmann σT⁴)

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1.7.6 · D1 · Physics › Thermodynamics › Heat transfer — conduction (Fourier's law k), convection, ra

Yeh page har woh symbol build karta hai jis par parent note depend karta hai, ek aisi reader ke liye shuru karke jisne kabhi ek bhi symbol nahi dekha. Har entry tumhe teen cheezein deta hai: seedha matlab → picture → topic ko yeh kyun chahiye. Upar se neeche padho; ladder ki har seedhi apne neeche wali par tikhi hai.


0. Heat aakhir hai kya? (ground floor)

Ek jar mein chhote balls (atoms) imagine karo jo kabhi ruk nahi rahe. Thande jar mein woh barely kaampte hain; garam jar mein woh hinsak tarike se hilte hain.

Figure — Heat transfer — conduction (Fourier's law k), convection, radiation (Stefan-Boltzmann σT⁴)
  • Seedha matlab: atoms ki average jiggle energy measure karta hai.
  • Picture: left jar = slow, chhote arrows; right jar = fast, bade arrows.
  • Topic ko yeh kyun chahiye: yahan ki har single formula temperature ke difference se drive hoti hai. ke bina koi "hot" aur "cold" nahi, aur heat ke paas flow karne ki koi direction nahi.

1. Temperature measure karne ke do tarike: Celsius aur Kelvin

Figure — Heat transfer — conduction (Fourier's law k), convection, radiation (Stefan-Boltzmann σT⁴)
  • Picture: ek vertical thermometer jisme do rulers side by side lage hain; tick marks ek line mein hain lekin har ek ka zero alag jagah par hai. Ticks ke beech ki spacing bilkul same hai.
  • Topic ko yeh kyun chahiye — crucial subtlety: kyunki ticks same size ke hain, ek difference dono scales par same hota hai: Lekin ek single value nahi hoti: , na ki K.
Recall Temperature kab Celsius mein chhod sakta hoon?

Sirf jab woh ek difference ke roop mein aaye (jaise Fourier's law mein). Koi bhi single value ya ki koi bhi power (jaise radiation mein ) zaroor kelvin mein honi chahiye. ::: Differences OK in °C; single values aur powers must be K.


2. Rate of change: ka matlab kya hai

Yeh tool kyun, bas "" kyun nahi? Ek wall total joules ki parwah nahi karti — woh flow speed ki parwah karti hai. "Har second kitne joules?" poochna exactly wahi hai jo ek rate answer karta hai, aur "per second, instant by instant" ke liye physics symbol derivative hai.

  • Picture: ek tap se nikalta paani. bucket mein total litres hain; yeh hai ki stream abhi is waqt kitni tezi se chal rahi hai.
  • Is rate ka is topic mein ek naam hai: heat current .

3. Temperature gradient

Figure — Heat transfer — conduction (Fourier's law k), convection, radiation (Stefan-Boltzmann σT⁴)
  • Picture: ek wall jo temperature ki ramp ki tarah draw ki gayi hai — left par hot face upar, right par cold face neeche. Us ramp ki slope hi hai. Steep ramp = bada gradient = heat ke liye strong push.
  • Sign negative kyun hota hai: jab tum direction mein (cold ki taraf) chalte ho, neeche jaata hai, isliye ek negative number hai. Heat opposite direction mein flow karti hai — ki taraf — isliye Fourier's law mein hai taaki positive rahe.
  • Topic ko yeh kyun chahiye: conduction raw temperatures se nahi, drop ki steepness se drive hoti hai. Gradient wohi steepness hai.

4. Area aur thickness — wall ki shape

  • Picture: ek slab (ek brik). = woh flat front jise tum paint karoge; = brik front-to-back kitni gehri hai.
  • Topic ko dono kyun chahiye: zyada chauda face () parallel mein zyada heat nikalne deta hai; zyada gehra brik () heat ko zyada travel karwata hai, use slow karta hai. Fourier's law mein yeh dono geometry ke knobs hain.

5. Material constants: , , ,

Transfer ka har mode apna "kitni aasaani se?" ek constant ke andar chhupata hai. Inse milo.


6. Power aur 4th power

Figure — Heat transfer — conduction (Fourier's law k), convection, radiation (Stefan-Boltzmann σT⁴)
  • Picture: chaar curves , , , origin se upar udhte hue — baakiyon se bahut upar rocket karta hai. Wohi steepness hai kyun temperature mein thodi si rise radiated power mein badi uchhaal laati hai.
  • Topic ko yeh kyun chahiye: radiation follow karta hai, isliye high temperature par yeh dominant loss channel ban jaata hai (ek filament, Sun) bhaale room temperature par tiny ho.

7. Thermal ↔ electrical analogy

Parent heat ko electricity par map karta hai. Dono pictures ko line up karo:

Heat picture Electrical twin Dekho
temperature difference voltage
heat current current
thermal resistance resistance Electrical resistance Ohm's law
  • Topic yeh kyun borrow karta hai: tum series/parallel resistor rules pehle se jaante ho; composite walls ke liye unhe reuse karna naya maths invent karne se bachata hai. High se "downhill flow" karne wali heat exactly high voltage se current flow jaisi hai.

Prerequisite map

Temperature T

Temperature difference delta T

Celsius and Kelvin scales

Absolute T needed for T to the 4th

Rate d by dt

Heat current H in watts

Gradient dT by dx

Fouriers law conduction

Area A and thickness delta x

Material constant k

Convection Newton cooling

Convection coefficient h

Stefan Boltzmann radiation

Emissivity e

Constant sigma

Thermal resistance analogy

Heat transfer topic


Equipment checklist

Reveal karne se pehle har jawab zor se bolo.

Main temperature aur heat ka fark explain kar sakta hoon
= atoms kitni tezi se hilte hain (ek level); = transfer hui jiggle-energy ki miqdar (joules).
Main Celsius aur Kelvin ke beech convert kar sakta hoon
; differences dono scales par equal hote hain.
Main jaanta hoon kab Celsius allowed hai aur kab sirf Kelvin chalega
Differences °C mein reh sakte hain; single values aur ki koi bhi power kelvin mein honi chahiye.
Main aur ko seedhe alfazon mein padh sakta hoon
"heat per second" (ek rate) aur "wall ke andar per metre temperature change" (ek slope).
Main jaanta hoon Fourier's law mein minus sign kyun hai
direction mein cold ki taraf jaane par girta hai, isliye ; ko flow direction mein positive rakhta hai.
Main jaanta hoon aur heat flow ko kya karte hain
Bada → zyada flow (parallel); bada → kam flow (travel karne ke liye zyada door).
Main charon constants aur unki units naam le sakta hoon
(W m⁻¹ K⁻¹) conduction, (W m⁻² K⁻¹) convection, (dimensionless 0–1) emissivity, W m⁻² K⁻⁴ radiation.
Main jaanta hoon high temperature par radiation ko kyun explode karta hai
bahut tezi se badhta hai — double karne par power se multiply ho jaati hai.
Main heat quantities ko unke electrical twins se match kar sakta hoon
voltage, current, resistance.