† Contributed equally to this project. Magnetic monopoles 1 -3 are hypothetical elementary particles exhibiting quantized magnetic charge = ±( ) ⁄ and quantized magnetic flux = ± / . In principle, such a magnetic charge can be detected by the quantized jump in magnetic flux it generates upon passage through a superconducting quantum interference device (SQUID) 4 . Naturally, with the theoretical discovery that a plasma of emergent magnetic charges should exist in several lanthanide-pyrochlore magnetic insulators 5,6 including Dy2Ti2O7, this SQUID technique was proposed for their direct detection 6 . Experimentally, this has proven challenging because of the high number density, and the generation-recombination (GR) fluctuations, of the monopole plasma. Recently, however, theoretical advances have allowed the spectral density of magnetic-flux noise ( , ) due to GR fluctuations of ± * magnetic charge pairs to be predicted 7 , 8 . Here we report development of a SQUID based flux-noise spectrometer, and consequent measurements of the frequency and temperature dependence of ( , ) for Dy2Ti2O7 samples. Virtually all the elements of ( , )predicted for a magnetic monopole plasma, including the existence of intense magnetization noise and its characteristic frequency and temperature dependence,