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MMLU-Pro / 9572 / The solar constant, the power due to radiation from the sun falling on the…

Problem

Answer published by the source. Consult the official source to check your work against its answer.

question

The solar constant, the power due to radiation from the sun falling on the earth's atmosphere, is 1.35 kW \bullet m^-2. What are the magnitudes of E^\ding{217} and B^\ding{217} for the electromagnetic waves emitted from the sun at the position of the earth?

category

physics

options

  1. E = 1.21 × 10^3 V ⋅ m^-1, B = 4.05 × 10^-6 Weber ⋅ m^-2
  2. E = 0.68 × 10^3 V ⋅ m^-1, B = 1.15 × 10^-5 Weber ⋅ m^-2
  3. E = 0.71 × 10^3 V ullet m^-1, B = 2.39 × 10^-6 Weber ullet m^-2
  4. E = 1.42 × 10^3 V ullet m^-1, B = 4.78 × 10^-6 Weber ullet m^-2
  5. E = 2.03 × 10^3 V ⋅ m^-1, B = 6.80 × 10^-6 Weber ⋅ m^-2
  6. E = 1.35 × 10^3 V ⋅ m^-1, B = 4.52 × 10^-6 Weber ⋅ m^-2
  7. E = 0.71 × 10^2 V ullet m^-1, B = 2.39 × 10^-5 Weber ullet m^-2
  8. E = 0.51 × 10^3 V ⋅ m^-1, B = 1.70 × 10^-6 Weber ⋅ m^-2
  9. E = 0.35 × 10^3 V ullet m^-1, B = 1.20 × 10^-6 Weber ullet m^-2
  10. E = 0.85 × 10^2 V ⋅ m^-1, B = 2.84 × 10^-5 Weber ⋅ m^-2

src

stemez-Optics

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Source and history

upstream_id / Original problem ID
9572
task_id
ce335182-ddac-5765-b8f0-44d0fd1ccb40
task_key
default--test--9572
task_revision_id
1
config / split
default / test

Official source

initial import