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Dyne per Hour per Centimeter [dyne/(h·cm)]


The unit dyne per hour per centimeter, written as dyne/(h·cm), measures force per unit length over time, often used in contexts such as viscous drag, material creep, or very slow mechanical processes in cgs (centimeter-gram-second) units.


A dyne is the cgs unit of force, defined as the force required to accelerate 1 gram of mass by 1 cm/s². Therefore, 1 dyne = 10⁻⁵ newtons in SI units. The additional division by centimeter represents a per-unit-length measure, and division by hour accounts for time rate.


Mathematically, the quantity can be expressed as:


Frate=FLtF_\text{rate} = \frac{F}{L \cdot t}

where F is force in dynes, L is length in cm, and t is time in hours.


Applications include:



  • Creep or stress studies in materials under very small forces over long periods



  • Lubrication or viscous flow measurements in cgs-based engineering studies



  • Experimental mechanics where small forces per unit length are measured over extended time



Conversion to SI units:


1dyne/(h\cdotpcm)2.78×109N/(m\cdotps)1 \, \text{dyne/(h·cm)} \approx 2.78 \times 10^{-9} \, \text{N/(m·s)}

This unit is largely of historical or specialized interest but provides a precise cgs-based measure for extremely slow, small-force phenomena.




Joule per Second per Square Meter [J/(s·m²)]


The unit joule per second per square meter, written as J/(s·m²), is a measure of heat flux density or radiant flux. Since 1 joule per second equals 1 watt, this unit is equivalent to watt per square meter (W/m²). It represents the amount of energy transferred or radiated through 1 square meter of surface every second.


This unit is widely used in physics, thermodynamics, meteorology, and solar energy studies. Examples include:



  • Measuring solar radiation incident on the Earth’s surface



  • Evaluating heat transfer through walls, roofs, and other surfaces



  • Calculating power density in radiant heating or cooling systems



Mathematically, the heat flux is expressed as:


q=QAtq = \frac{Q}{A \cdot t}

where q is the flux in J/(s·m²), Q is energy in joules, A is area in m², and t is time in seconds.


For example, solar constant outside Earth’s atmosphere is approximately 1361 J/(s·m²), indicating the power received per square meter from the Sun.


Using J/(s·m²) or W/m² provides a standardized, SI-compliant measure for energy transfer per unit area, replacing older units like cal/cm²·s or Btu/ft²·h in modern engineering and scientific applications.



No conversions available for heat-flux-density.

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