Plancksches Strahlungsspektrum
About points...
We associate a certain number of points with each exercise.
When you click an exercise into a collection, this number will be taken as points for the exercise, kind of "by default".
But once the exercise is on the collection, you can edit the number of points for the exercise in the collection independently, without any effect on "points by default" as represented by the number here.
That being said... How many "default points" should you associate with an exercise upon creation?
As with difficulty, there is no straight forward and generally accepted way.
But as a guideline, we tend to give as many points by default as there are mathematical steps to do in the exercise.
Again, very vague... But the number should kind of represent the "work" required.
When you click an exercise into a collection, this number will be taken as points for the exercise, kind of "by default".
But once the exercise is on the collection, you can edit the number of points for the exercise in the collection independently, without any effect on "points by default" as represented by the number here.
That being said... How many "default points" should you associate with an exercise upon creation?
As with difficulty, there is no straight forward and generally accepted way.
But as a guideline, we tend to give as many points by default as there are mathematical steps to do in the exercise.
Again, very vague... But the number should kind of represent the "work" required.
About difficulty...
We associate a certain difficulty with each exercise.
When you click an exercise into a collection, this number will be taken as difficulty for the exercise, kind of "by default".
But once the exercise is on the collection, you can edit its difficulty in the collection independently, without any effect on the "difficulty by default" here.
Why we use chess pieces? Well... we like chess, we like playing around with \(\LaTeX\)-fonts, we wanted symbols that need less space than six stars in a table-column... But in your layouts, you are of course free to indicate the difficulty of the exercise the way you want.
That being said... How "difficult" is an exercise? It depends on many factors, like what was being taught etc.
In physics exercises, we try to follow this pattern:
Level 1 - One formula (one you would find in a reference book) is enough to solve the exercise. Example exercise
Level 2 - Two formulas are needed, it's possible to compute an "in-between" solution, i.e. no algebraic equation needed. Example exercise
Level 3 - "Chain-computations" like on level 2, but 3+ calculations. Still, no equations, i.e. you are not forced to solve it in an algebraic manner. Example exercise
Level 4 - Exercise needs to be solved by algebraic equations, not possible to calculate numerical "in-between" results. Example exercise
Level 5 -
Level 6 -
When you click an exercise into a collection, this number will be taken as difficulty for the exercise, kind of "by default".
But once the exercise is on the collection, you can edit its difficulty in the collection independently, without any effect on the "difficulty by default" here.
Why we use chess pieces? Well... we like chess, we like playing around with \(\LaTeX\)-fonts, we wanted symbols that need less space than six stars in a table-column... But in your layouts, you are of course free to indicate the difficulty of the exercise the way you want.
That being said... How "difficult" is an exercise? It depends on many factors, like what was being taught etc.
In physics exercises, we try to follow this pattern:
Level 1 - One formula (one you would find in a reference book) is enough to solve the exercise. Example exercise
Level 2 - Two formulas are needed, it's possible to compute an "in-between" solution, i.e. no algebraic equation needed. Example exercise
Level 3 - "Chain-computations" like on level 2, but 3+ calculations. Still, no equations, i.e. you are not forced to solve it in an algebraic manner. Example exercise
Level 4 - Exercise needs to be solved by algebraic equations, not possible to calculate numerical "in-between" results. Example exercise
Level 5 -
Level 6 -
Question
Solution
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\(\LaTeX\)
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Exercise:
minipagec.textwidth includegraphicswidthtextwidth#image_path:planck-spektrum# minipage hfill minipagec.textwidth Die meisten Festkörper nen bei celsius zu glühen. enumerate itema Berechne die Wellenlänge der Strahlung von der bei dieser Temperatur am meisten abgestrahlt wird. hfill pawnB itemb Berechne die Wärmestromdichte eines schwarzen Körpers mit dieser Temperatur an der Oberfläche. hfill pawnB enumerate Links ist das Plancksche Strahlungsspektrum abgebildet. enumerate itemc Was zeigt dieses Spektrum auf was das Stefan-Boltzmann-Gesetz und das Wiensche Verschiebungsgesetz alleine nicht aufzeigen? itemd Zeichne die in a und b berechneten Grössen im Spektrum links ein. enumerate minipage
Solution:
abclist abc newqtyT.K solqtyLmfracbTncbn/Tnm al lambda Lmf fracncbT Lm approx LmIII abc solqtyJvarepsilonsigma T^ncSn*Tn**wattpersquaremeter al J Jf ncSqtyT^ J approx JIII abc Es zeigt auf wie viel Wärme von jeder Wellenlänge bei einer bestimmten Temperatur abgestrahlt wird. abclist
minipagec.textwidth includegraphicswidthtextwidth#image_path:planck-spektrum# minipage hfill minipagec.textwidth Die meisten Festkörper nen bei celsius zu glühen. enumerate itema Berechne die Wellenlänge der Strahlung von der bei dieser Temperatur am meisten abgestrahlt wird. hfill pawnB itemb Berechne die Wärmestromdichte eines schwarzen Körpers mit dieser Temperatur an der Oberfläche. hfill pawnB enumerate Links ist das Plancksche Strahlungsspektrum abgebildet. enumerate itemc Was zeigt dieses Spektrum auf was das Stefan-Boltzmann-Gesetz und das Wiensche Verschiebungsgesetz alleine nicht aufzeigen? itemd Zeichne die in a und b berechneten Grössen im Spektrum links ein. enumerate minipage
Solution:
abclist abc newqtyT.K solqtyLmfracbTncbn/Tnm al lambda Lmf fracncbT Lm approx LmIII abc solqtyJvarepsilonsigma T^ncSn*Tn**wattpersquaremeter al J Jf ncSqtyT^ J approx JIII abc Es zeigt auf wie viel Wärme von jeder Wellenlänge bei einer bestimmten Temperatur abgestrahlt wird. abclist
Meta Information
Exercise:
minipagec.textwidth includegraphicswidthtextwidth#image_path:planck-spektrum# minipage hfill minipagec.textwidth Die meisten Festkörper nen bei celsius zu glühen. enumerate itema Berechne die Wellenlänge der Strahlung von der bei dieser Temperatur am meisten abgestrahlt wird. hfill pawnB itemb Berechne die Wärmestromdichte eines schwarzen Körpers mit dieser Temperatur an der Oberfläche. hfill pawnB enumerate Links ist das Plancksche Strahlungsspektrum abgebildet. enumerate itemc Was zeigt dieses Spektrum auf was das Stefan-Boltzmann-Gesetz und das Wiensche Verschiebungsgesetz alleine nicht aufzeigen? itemd Zeichne die in a und b berechneten Grössen im Spektrum links ein. enumerate minipage
Solution:
abclist abc newqtyT.K solqtyLmfracbTncbn/Tnm al lambda Lmf fracncbT Lm approx LmIII abc solqtyJvarepsilonsigma T^ncSn*Tn**wattpersquaremeter al J Jf ncSqtyT^ J approx JIII abc Es zeigt auf wie viel Wärme von jeder Wellenlänge bei einer bestimmten Temperatur abgestrahlt wird. abclist
minipagec.textwidth includegraphicswidthtextwidth#image_path:planck-spektrum# minipage hfill minipagec.textwidth Die meisten Festkörper nen bei celsius zu glühen. enumerate itema Berechne die Wellenlänge der Strahlung von der bei dieser Temperatur am meisten abgestrahlt wird. hfill pawnB itemb Berechne die Wärmestromdichte eines schwarzen Körpers mit dieser Temperatur an der Oberfläche. hfill pawnB enumerate Links ist das Plancksche Strahlungsspektrum abgebildet. enumerate itemc Was zeigt dieses Spektrum auf was das Stefan-Boltzmann-Gesetz und das Wiensche Verschiebungsgesetz alleine nicht aufzeigen? itemd Zeichne die in a und b berechneten Grössen im Spektrum links ein. enumerate minipage
Solution:
abclist abc newqtyT.K solqtyLmfracbTncbn/Tnm al lambda Lmf fracncbT Lm approx LmIII abc solqtyJvarepsilonsigma T^ncSn*Tn**wattpersquaremeter al J Jf ncSqtyT^ J approx JIII abc Es zeigt auf wie viel Wärme von jeder Wellenlänge bei einer bestimmten Temperatur abgestrahlt wird. abclist
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Plancksches Strahlungsspektrum by TeXercises